This DD proposal is being submmitted at the request of Neill Reid. Title updated 1179350414 Assigned ID: 2521 ----- Attempting Submission 1 (Wed Sep 10 14:03:49 GMT 2014) ----- HST Phase I Proposal 2521 (phase1-windsofchange_v1.apt) successfully submitted. ----- Attempting Submission 2 (Wed Sep 10 15:59:53 GMT 2014) ----- FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser POS TARG & PATTERN should be used carefully with WFC3 quad filters to avoid placing the target on the vignetted part of the field of view or moving it to another quadrant. FLASH level may be too low for this exposure or a short subexposure. See extended explanation in the diagnostic browser PLease contact both Simon and Wong if there are questions. -1904183879 ----- Attempting Submission 1 (Sun Sep 14 23:35:45 GMT 2014) ----- ----- Attempting Submission 2 (Sat Nov 08 00:44:44 GMT 2014) ----- ----- Attempting Submission 3 (Fri Jun 19 13:19:44 GMT 2020) ----- Settings determined from previous programs and are appropriate for these targets Long time base observations of the outer planets are critical in understanding the atmospheric dynamics and evolution of the gas giants. We propose yearly monitoring of each giant planet for the remainder of Hubble's lifetime to provide a lasting legacy of increasingly valuable data for time-domain studies. The Hubble Space Telescope is a unique asset to planetary science, allowing high spatial resolution data with absolute photometric knowledge. For the outer planets, gas/ice giant planets Jupiter, Saturn, Uranus and Neptune, many phenomena happen on timescales of years to decades, and the data we propose are beyond the scope of a typical GO program. Hubble is the only platform that can provide high spatial resolution global studies of cloud coloration, activity, and motion on a consistent time basis to help constrain the underlying mechanics. Here we show the orbits for Cycle 28. Global mapping for each of the four outer planets. Orbits spaced to allow complete longitude coverage for two rotations. Jupiter and Saturn orbits (when applicable) shuld be contiguous, and small incursions into the SAA may be ok. Uranus and Neptune orbits are spaced to give complete longitude coverage. CC: the PI and Co-I Wong on all correspondence SOLAR SYSTEM 0 false AVAILABLE SOLAR SYSTEM Observe when Jupiter is less than 168 degrees from the Sun. HST has a thermal constraint that it cannot point >168 degrees from the Sun for longer than 10 hours at a time. Also, after any pointing at >168, HST must spend at least 3 hours pointed at <168 before returning to any pointing >168. The Jupiter series of visits in this program would violate that constraint if they are attempted when Jupiter is >168 degrees from the Sun PLANET Global Jupiter maps STD=JUPITER NOT OCC OF JUPITER BY IO FROM EARTH, NOT OCC OF JUPITER BY EUROPA FROM EARTH, NOT OCC OF JUPITER BY GANYMEDE FROM EARTH, NOT OCC OF JUPITER BY CALLISTO FROM EARTH, SEP OF JUPITER SUN FROM EARTH LT 168D EARTH SOLAR SYSTEM Observe when Saturn is less than 168 degrees from the Sun. HST has a thermal constraint that it cannot point >168 degrees from the Sun for longer than 10 hours at a time. Also, after any pointing at >168, HST must spend at least 3 hours pointed at <168 before returning to any pointing >168. The Saturn series of visits in this program would violate that constraint if they are attempted when Saturn is >168 degrees from the Sun. PLANET Global Saturn Maps STD=SATURN NOT ECL P PARTIAL OF SATURN-MAPS BY TITAN FROM EARTH, SEP OF SATURN-MAPS RHEA FROM EARTH GT 10", SEP OF SATURN-MAPS TITAN FROM EARTH GT 10", SEP OF SATURN SUN FROM EARTH LT 168D EARTH SOLAR SYSTEM PLANET Global Uranus maps STD=URANUS EARTH SOLAR SYSTEM PLANET Global Neptune Maps STD=NEPTUNE EARTH WFC3/UVIS Imaging No No F631N WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F343N WFC3/UVIS Imaging No No F395N WFC3/UVIS Imaging No No F502N WFC3/UVIS Imaging No No FQ727N WFC3/UVIS Imaging No No FQ750N WFC3/UVIS Imaging No No FQ889N WFC3/UVIS Imaging No No FQ937N WFC3/UVIS Imaging No No F547M WFC3/UVIS Imaging No No F467M WFC3/UVIS Imaging No No F658N WFC3/UVIS Imaging No No F631N WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F343N WFC3/UVIS Imaging No No F395N WFC3/UVIS Imaging No No F502N WFC3/UVIS Imaging No No FQ727N WFC3/UVIS Imaging No No FQ750N WFC3/UVIS Imaging No No FQ889N WFC3/UVIS Imaging No No FQ937N WFC3/UVIS Imaging No No F467M WFC3/UVIS Imaging No No F547M WFC3/UVIS Imaging No No F631N WFC3/UVIS Imaging No No FQ619N WFC3/UVIS Imaging No No FQ727N WFC3/UVIS Imaging No No FQ750N WFC3/UVIS Imaging No No FQ889N WFC3/UVIS Imaging No No FQ906N WFC3/UVIS Imaging No No FQ924N WFC3/UVIS Imaging No No FQ937N WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F658N WFC3/UVIS Imaging No No F621M WFC3/UVIS Imaging No No F763M WFC3/UVIS Imaging No No F845M WFC3/UVIS Imaging No No F467M WFC3/UVIS Imaging No No F547M WFC3/UVIS Imaging No No F631N WFC3/UVIS Imaging No No FQ619N WFC3/UVIS Imaging No No FQ727N WFC3/UVIS Imaging No No FQ750N WFC3/UVIS Imaging No No FQ889N WFC3/UVIS Imaging No No FQ906N WFC3/UVIS Imaging No No FQ924N WFC3/UVIS Imaging No No FQ937N WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F658N WFC3/UVIS Imaging No No F621M WFC3/UVIS Imaging No No F763M WFC3/UVIS Imaging No No F845M POS-TARG DITHER 0.145 LINE false false 2 46.84 WFC3-UVIS-DITHER-LINE 2 false POS-TARG DITHER 0.725 LINE false false 2 46.84 WFC3-UVIS-DITHER-LINE 3 false 1592571392374 Timing link suitability includes constraints ([02 After 01 by 0.1 to 0.2 days] [08 After 01 by 1.3 to 1.3 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. Uranus opposition (2020-OCT-31) +/- 30 days preferred. 8 orbits. Visit 8 after visit 1 by 19 orbits. All visits spaced out as evenly as possible, with either 1-orbit or 2-orbit gaps between then. 3-orbit gaps are too big, consecutive orbits are too tight. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. 1602156058000 252.55951427019733 (Tic-Visit :proposal-id 16266 :visit-id "01" :proposal-version -1 :trans-version "20200518" :date "19-Jun-2020 08:56:31.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 263584 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "01" :orbit-number 1 :pcs-time 301 :si-vis-utilization 2636 :al-overhead-at-end 0 :internal-dur-at-end 325 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) false 1 0 1592571393569 Timing link suitability includes constraints ([02 After 01 by 0.1 to 0.2 days] [03 After 02 by 0.1 to 0.2 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. Uranus opposition (2020-OCT-31) +/- 30 days preferred. 8 orbits. Visit 8 after visit 1 by 19 orbits. All visits spaced out as evenly as possible, with either 1-orbit or 2-orbit gaps between then. 3-orbit gaps are too big, consecutive orbits are too tight. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. 1602173216000 252.56796061698526 (Tic-Visit :proposal-id 16266 :visit-id "02" :proposal-version -1 :trans-version "20200518" :date "19-Jun-2020 08:56:33.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 263584 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "02" :orbit-number 1 :pcs-time 301 :si-vis-utilization 2636 :al-overhead-at-end 0 :internal-dur-at-end 325 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) false 1 0 1592571394677 Timing link suitability includes constraints ([03 After 02 by 0.1 to 0.2 days] [04 After 03 by 0.1 to 0.2 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. Uranus opposition (2020-OCT-31) +/- 30 days preferred. 8 orbits. Visit 8 after visit 1 by 19 orbits. All visits spaced out as evenly as possible, with either 1-orbit or 2-orbit gaps between then. 3-orbit gaps are too big, consecutive orbits are too tight. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. 1602190375000 252.57657200596952 (Tic-Visit :proposal-id 16266 :visit-id "03" :proposal-version -1 :trans-version "20200518" :date "19-Jun-2020 08:56:34.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 263584 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "03" :orbit-number 1 :pcs-time 301 :si-vis-utilization 2636 :al-overhead-at-end 0 :internal-dur-at-end 325 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) false 1 0 1592571395773 Timing link suitability includes constraints ([04 After 03 by 0.1 to 0.2 days] [05 After 04 by 0.1 to 0.2 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. Uranus opposition (2020-OCT-31) +/- 30 days preferred. 8 orbits. Visit 8 after visit 1 by 19 orbits. All visits spaced out as evenly as possible, with either 1-orbit or 2-orbit gaps between then. 3-orbit gaps are too big, consecutive orbits are too tight. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. 1602201814000 252.5824064060489 (Tic-Visit :proposal-id 16266 :visit-id "04" :proposal-version -1 :trans-version "20200518" :date "19-Jun-2020 08:56:35.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 263584 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "04" :orbit-number 1 :pcs-time 301 :si-vis-utilization 2636 :al-overhead-at-end 0 :internal-dur-at-end 325 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) false 1 0 1592571396831 Timing link suitability includes constraints ([05 After 04 by 0.1 to 0.2 days] [06 After 05 by 0.1 to 0.2 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. Uranus opposition (2020-OCT-31) +/- 30 days preferred. 8 orbits. Visit 8 after visit 1 by 19 orbits. All visits spaced out as evenly as possible, with either 1-orbit or 2-orbit gaps between then. 3-orbit gaps are too big, consecutive orbits are too tight. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. 1602213253000 252.58831732188384 (Tic-Visit :proposal-id 16266 :visit-id "05" :proposal-version -1 :trans-version "20200518" :date "19-Jun-2020 08:56:36.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 263584 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "05" :orbit-number 1 :pcs-time 301 :si-vis-utilization 2636 :al-overhead-at-end 0 :internal-dur-at-end 325 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) false 1 0 1592571397885 Timing link suitability includes constraints ([06 After 05 by 0.1 to 0.2 days] [07 After 06 by 0.1 to 0.2 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. Uranus opposition (2020-OCT-31) +/- 30 days preferred. 8 orbits. Visit 8 after visit 1 by 19 orbits. All visits spaced out as evenly as possible, with either 1-orbit or 2-orbit gaps between then. 3-orbit gaps are too big, consecutive orbits are too tight. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. 1602230486000 244.0 (Tic-Visit :proposal-id 16266 :visit-id "06" :proposal-version -1 :trans-version "20200518" :date "19-Jun-2020 08:56:37.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 263584 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "06" :orbit-number 1 :pcs-time 301 :si-vis-utilization 2636 :al-overhead-at-end 0 :internal-dur-at-end 325 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) false 1 0 1592571399409 Timing link suitability includes constraints ([07 After 06 by 0.1 to 0.2 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. Uranus opposition (2020-OCT-31) +/- 30 days preferred. 8 orbits. Visit 8 after visit 1 by 19 orbits. All visits spaced out as evenly as possible, with either 1-orbit or 2-orbit gaps between then. 3-orbit gaps are too big, consecutive orbits are too tight. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. 1602247576000 231.79175787568596 (Tic-Visit :proposal-id 16266 :visit-id "07" :proposal-version -1 :trans-version "20200518" :date "19-Jun-2020 08:56:39.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 263584 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "07" :orbit-number 1 :pcs-time 301 :si-vis-utilization 2636 :al-overhead-at-end 0 :internal-dur-at-end 325 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) false 1 0 1592571400464 Timing link suitability includes constraints ([08 After 01 by 1.3 to 1.3 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. Uranus opposition (2020-OCT-31) +/- 30 days preferred. 8 orbits. Visit 8 after visit 1 by 19 orbits. All visits spaced out as evenly as possible, with either 1-orbit or 2-orbit gaps between then. 3-orbit gaps are too big, consecutive orbits are too tight. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. 1602264738000 231.79000320386382 (Tic-Visit :proposal-id 16266 :visit-id "08" :proposal-version -1 :trans-version "20200518" :date "19-Jun-2020 08:56:40.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 263584 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "08" :orbit-number 1 :pcs-time 301 :si-vis-utilization 2636 :al-overhead-at-end 0 :internal-dur-at-end 325 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) false 1 0 1623758717485 Using ephemeris for target 16266-09-JUPITER-MAPS Timing link suitability includes constraints ([10 After 09 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 52 /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v09.xml 13 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 OR 7 - 8 is acceptable. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Jupiter opposition (2021-AUG-19) +/- 30 days preferred. 1630715813000 76.2839934557552 (Tic-Visit :proposal-id 16266 :visit-id "09" :proposal-version -1 :trans-version "20200619" :date "15-Jun-2021 08:05:17.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 633488 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "09" :obset-id "09" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "09" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2436 :al-overhead-at-end 0 :internal-dur-at-end 344 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3120.0 :pcs-gap 0 ) true 1 0 1623758796138 Using ephemeris for target 16266-10-JUPITER-MAPS Timing link suitability includes constraints ([10 After 09 by 0.1 to 0.1 days] [11 After 10 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 46 /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v10.xml 13 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 OR 7 - 8 is acceptable. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Jupiter opposition (2021-AUG-19) +/- 30 days preferred. 1630721532000 76.2859094109341 (Tic-Visit :proposal-id 16266 :visit-id "10" :proposal-version -1 :trans-version "20200619" :date "15-Jun-2021 08:06:35.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 563088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "10" :obset-id "10" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "10" :orbit-number 1 :pcs-time 393 :si-vis-utilization 1834 :al-overhead-at-end 0 :internal-dur-at-end 652 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2760.0 :pcs-gap 0 ) true 1 0 1623758765217 Using ephemeris for target 16266-11-JUPITER-MAPS Timing link suitability includes constraints ([11 After 10 by 0.1 to 0.1 days] [12 After 11 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 52 /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v11.xml 13 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 OR 7 - 8 is acceptable. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Jupiter opposition (2021-AUG-19) +/- 30 days preferred. 1630727252000 76.28782464523351 (Tic-Visit :proposal-id 16266 :visit-id "11" :proposal-version -1 :trans-version "20200619" :date "15-Jun-2021 08:06:05.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 633488 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "11" :obset-id "11" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "11" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2436 :al-overhead-at-end 0 :internal-dur-at-end 344 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3120.0 :pcs-gap 0 ) true 1 0 1623758870419 Using ephemeris for target 16266-12-JUPITER-MAPS Timing link suitability includes constraints ([12 After 11 by 0.1 to 0.1 days] [13 After 12 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 46 /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v12.xml 13 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 OR 7 - 8 is acceptable. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Jupiter opposition (2021-AUG-19) +/- 30 days preferred. 1630732971000 42.517479886294694 (Tic-Visit :proposal-id 16266 :visit-id "12" :proposal-version -1 :trans-version "20200619" :date "15-Jun-2021 08:07:50.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 563088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "12" :orbit-number 1 :pcs-time 393 :si-vis-utilization 1834 :al-overhead-at-end 0 :internal-dur-at-end 652 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2760.0 :pcs-gap 0 ) true 1 0 1623758766538 Using ephemeris for target 16266-13-JUPITER-MAPS Timing link suitability includes constraints ([13 After 12 by 0.1 to 0.1 days] [14 After 13 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 52 /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v13.xml 13 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 OR 7 - 8 is acceptable. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Jupiter opposition (2021-AUG-19) +/- 30 days preferred. 1630738691000 40.0 (Tic-Visit :proposal-id 16266 :visit-id "13" :proposal-version -1 :trans-version "20200619" :date "15-Jun-2021 08:06:06.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 633488 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "13" :obset-id "13" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "13" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2436 :al-overhead-at-end 0 :internal-dur-at-end 344 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3120.0 :pcs-gap 0 ) true 1 0 1623758872490 Using ephemeris for target 16266-14-JUPITER-MAPS Timing link suitability includes constraints ([14 After 13 by 0.1 to 0.1 days] [15 After 14 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 46 /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v14.xml 13 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 OR 7 - 8 is acceptable. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Jupiter opposition (2021-AUG-19) +/- 30 days preferred. 1630744410000 40.0 (Tic-Visit :proposal-id 16266 :visit-id "14" :proposal-version -1 :trans-version "20200619" :date "15-Jun-2021 08:07:52.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 563088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "14" :obset-id "14" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "14" :orbit-number 1 :pcs-time 393 :si-vis-utilization 1834 :al-overhead-at-end 0 :internal-dur-at-end 652 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2760.0 :pcs-gap 0 ) true 1 0 1623758767825 Using ephemeris for target 16266-15-JUPITER-MAPS Timing link suitability includes constraints ([15 After 14 by 0.1 to 0.1 days] [16 After 15 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 52 /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v15.xml 13 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 OR 7 - 8 is acceptable. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Jupiter opposition (2021-AUG-19) +/- 30 days preferred. 1630750130000 40.0 (Tic-Visit :proposal-id 16266 :visit-id "15" :proposal-version -1 :trans-version "20200619" :date "15-Jun-2021 08:06:07.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 633488 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "15" :obset-id "15" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "15" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2439 :al-overhead-at-end 0 :internal-dur-at-end 344 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3120.0 :pcs-gap 0 ) true 1 0 1623758874406 Using ephemeris for target 16266-16-JUPITER-MAPS Timing link suitability includes constraints ([16 After 15 by 0.1 to 0.1 days] [17 After 16 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 46 /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v16.xml 13 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 OR 7 - 8 is acceptable. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Jupiter opposition (2021-AUG-19) +/- 30 days preferred. 1630755850000 40.0 (Tic-Visit :proposal-id 16266 :visit-id "16" :proposal-version -1 :trans-version "20200619" :date "15-Jun-2021 08:07:54.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 563088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "16" :obset-id "16" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "16" :orbit-number 1 :pcs-time 393 :si-vis-utilization 1834 :al-overhead-at-end 0 :internal-dur-at-end 652 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2760.0 :pcs-gap 0 ) true 1 0 1623758769103 Using ephemeris for target 16266-17-JUPITER-MAPS Timing link suitability includes constraints ([17 After 16 by 0.1 to 0.1 days] [18 After 17 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 52 /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v17.xml 13 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 OR 7 - 8 is acceptable. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Jupiter opposition (2021-AUG-19) +/- 30 days preferred. 1630761569000 55.0 (Tic-Visit :proposal-id 16266 :visit-id "17" :proposal-version -1 :trans-version "20200619" :date "15-Jun-2021 08:06:08.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 633488 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "17" :obset-id "17" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "17" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2439 :al-overhead-at-end 0 :internal-dur-at-end 344 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3120.0 :pcs-gap 0 ) true 1 0 1623758876290 Using ephemeris for target 16266-18-JUPITER-MAPS Timing link suitability includes constraints ([18 After 17 by 0.1 to 0.1 days] [19 After 18 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 46 /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v18.xml 13 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 OR 7 - 8 is acceptable. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Jupiter opposition (2021-AUG-19) +/- 30 days preferred. 1630767289000 74.26649240909501 (Tic-Visit :proposal-id 16266 :visit-id "18" :proposal-version -1 :trans-version "20200619" :date "15-Jun-2021 08:07:56.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 563088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "18" :obset-id "18" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "18" :orbit-number 1 :pcs-time 393 :si-vis-utilization 1834 :al-overhead-at-end 0 :internal-dur-at-end 652 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2760.0 :pcs-gap 0 ) true 1 0 1623758770355 Using ephemeris for target 16266-19-JUPITER-MAPS Timing link suitability includes constraints ([19 After 18 by 0.1 to 0.1 days] [20 After 19 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 52 /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v19.xml 13 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 OR 7 - 8 is acceptable. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Jupiter opposition (2021-AUG-19) +/- 30 days preferred. 1630773027000 74.26840473710311 (Tic-Visit :proposal-id 16266 :visit-id "19" :proposal-version -1 :trans-version "20200619" :date "15-Jun-2021 08:06:10.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 633488 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "19" :obset-id "19" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "19" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2439 :al-overhead-at-end 0 :internal-dur-at-end 344 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3120.0 :pcs-gap 0 ) true 1 0 1623758878171 Using ephemeris for target 16266-20-JUPITER-MAPS Timing link suitability includes constraints ([20 After 19 by 0.1 to 0.1 days] [21 After 20 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 46 /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v20.xml 13 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 OR 7 - 8 is acceptable. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Jupiter opposition (2021-AUG-19) +/- 30 days preferred. 1630778977000 74.27038649134201 (Tic-Visit :proposal-id 16266 :visit-id "20" :proposal-version -1 :trans-version "20200619" :date "15-Jun-2021 08:07:57.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 563088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "20" :obset-id "20" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "20" :orbit-number 1 :pcs-time 393 :si-vis-utilization 1834 :al-overhead-at-end 0 :internal-dur-at-end 652 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2760.0 :pcs-gap 0 ) true 1 0 1623758771608 Using ephemeris for target 16266-21-JUPITER-MAPS Timing link suitability includes constraints ([21 After 20 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 52 /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v21.xml 13 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 OR 7 - 8 is acceptable. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Jupiter opposition (2021-AUG-19) +/- 30 days preferred. 1630784836000 74.2723367092386 (Tic-Visit :proposal-id 16266 :visit-id "21" :proposal-version -1 :trans-version "20200619" :date "15-Jun-2021 08:06:11.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 633488 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "21" :obset-id "21" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "21" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2439 :al-overhead-at-end 0 :internal-dur-at-end 344 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3120.0 :pcs-gap 0 ) true 1 0 1592571410310 Timing link suitability includes constraints ([23 After 22 by 0.1 to 0.2 days] [29 After 22 by 1.2 to 1.3 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 52 Neptune Opposition (2021-SEP-14) +/- 30 days preferred. 8 orbits, with mostly 2-orbit gaps between most visits (4-6x 2-orbit gaps, 1-3x 1-orbit gaps). If shifting needed (for SAA avoidance or observatory constraints), can reduce a 3rd gap to 1 orbits (no more than 3 1-orbit gaps overall). We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. 1630910794000 239.10418831057854 (Tic-Visit :proposal-id 16266 :visit-id "22" :proposal-version -1 :trans-version "20200518" :date "19-Jun-2020 08:56:50.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 325232 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "22" :obset-id "22" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "22" :orbit-number 1 :pcs-time 301 :si-vis-utilization 2512 :al-overhead-at-end 0 :internal-dur-at-end 392 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3120.0 :pcs-gap 0 ) false 1 0 1592571411189 Timing link suitability includes constraints ([23 After 22 by 0.1 to 0.2 days] [24 After 23 by 0.1 to 0.2 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 52 Neptune Opposition (2021-SEP-14) +/- 30 days preferred. 8 orbits, with mostly 2-orbit gaps between most visits (4-6x 2-orbit gaps, 1-3x 1-orbit gaps). If shifting needed (for SAA avoidance or observatory constraints), can reduce a 3rd gap to 1 orbits (no more than 3 1-orbit gaps overall). We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. 1630927955000 239.1045671156554 (Tic-Visit :proposal-id 16266 :visit-id "23" :proposal-version -1 :trans-version "20200518" :date "19-Jun-2020 08:56:50.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 325232 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "23" :obset-id "23" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "23" :orbit-number 1 :pcs-time 301 :si-vis-utilization 2512 :al-overhead-at-end 0 :internal-dur-at-end 392 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3120.0 :pcs-gap 0 ) false 1 0 1592571412086 Timing link suitability includes constraints ([24 After 23 by 0.1 to 0.2 days] [25 After 24 by 0.1 to 0.2 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 52 Neptune Opposition (2021-SEP-14) +/- 30 days preferred. 8 orbits, with mostly 2-orbit gaps between most visits (4-6x 2-orbit gaps, 1-3x 1-orbit gaps). If shifting needed (for SAA avoidance or observatory constraints), can reduce a 3rd gap to 1 orbits (no more than 3 1-orbit gaps overall). We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. 1630945115000 270.9527062387973 (Tic-Visit :proposal-id 16266 :visit-id "24" :proposal-version -1 :trans-version "20200518" :date "19-Jun-2020 08:56:51.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 325232 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "24" :obset-id "24" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "24" :orbit-number 1 :pcs-time 301 :si-vis-utilization 2512 :al-overhead-at-end 0 :internal-dur-at-end 392 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3120.0 :pcs-gap 0 ) false 1 0 1592571412979 Timing link suitability includes constraints ([25 After 24 by 0.1 to 0.2 days] [26 After 25 by 0.1 to 0.2 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 52 Neptune Opposition (2021-SEP-14) +/- 30 days preferred. 8 orbits, with mostly 2-orbit gaps between most visits (4-6x 2-orbit gaps, 1-3x 1-orbit gaps). If shifting needed (for SAA avoidance or observatory constraints), can reduce a 3rd gap to 1 orbits (no more than 3 1-orbit gaps overall). We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. 1630962275000 270.95308588964957 (Tic-Visit :proposal-id 16266 :visit-id "25" :proposal-version -1 :trans-version "20200518" :date "19-Jun-2020 08:56:52.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 325232 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "25" :obset-id "25" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "25" :orbit-number 1 :pcs-time 301 :si-vis-utilization 2512 :al-overhead-at-end 0 :internal-dur-at-end 392 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3120.0 :pcs-gap 0 ) false 1 0 1592571413872 Timing link suitability includes constraints ([26 After 25 by 0.1 to 0.2 days] [27 After 26 by 0.1 to 0.2 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 52 Neptune Opposition (2021-SEP-14) +/- 30 days preferred. 8 orbits, with mostly 2-orbit gaps between most visits (4-6x 2-orbit gaps, 1-3x 1-orbit gaps). If shifting needed (for SAA avoidance or observatory constraints), can reduce a 3rd gap to 1 orbits (no more than 3 1-orbit gaps overall). We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. 1631013755000 252.0 (Tic-Visit :proposal-id 16266 :visit-id "26" :proposal-version -1 :trans-version "20200518" :date "19-Jun-2020 08:56:53.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 325232 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "26" :obset-id "26" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "26" :orbit-number 1 :pcs-time 301 :si-vis-utilization 2512 :al-overhead-at-end 0 :internal-dur-at-end 392 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3120.0 :pcs-gap 0 ) false 1 0 1592571414753 Timing link suitability includes constraints ([27 After 26 by 0.1 to 0.2 days] [28 After 27 by 0.1 to 0.2 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 52 Neptune Opposition (2021-SEP-14) +/- 30 days preferred. 8 orbits, with mostly 2-orbit gaps between most visits (4-6x 2-orbit gaps, 1-3x 1-orbit gaps). If shifting needed (for SAA avoidance or observatory constraints), can reduce a 3rd gap to 1 orbits (no more than 3 1-orbit gaps overall). We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. 1631030915000 252.0 (Tic-Visit :proposal-id 16266 :visit-id "27" :proposal-version -1 :trans-version "20200518" :date "19-Jun-2020 08:56:54.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 325232 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "27" :obset-id "27" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "27" :orbit-number 1 :pcs-time 301 :si-vis-utilization 2512 :al-overhead-at-end 0 :internal-dur-at-end 392 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3120.0 :pcs-gap 0 ) false 1 0 1592571415980 Timing link suitability includes constraints ([28 After 27 by 0.1 to 0.2 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 52 Neptune Opposition (2021-SEP-14) +/- 30 days preferred. 8 orbits, with mostly 2-orbit gaps between most visits (4-6x 2-orbit gaps, 1-3x 1-orbit gaps). If shifting needed (for SAA avoidance or observatory constraints), can reduce a 3rd gap to 1 orbits (no more than 3 1-orbit gaps overall). We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. 1631048204000 252.0 (Tic-Visit :proposal-id 16266 :visit-id "28" :proposal-version -1 :trans-version "20200518" :date "19-Jun-2020 08:56:55.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 325232 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "28" :obset-id "28" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "28" :orbit-number 1 :pcs-time 301 :si-vis-utilization 2512 :al-overhead-at-end 0 :internal-dur-at-end 392 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3120.0 :pcs-gap 0 ) false 1 0 1592571416869 Timing link suitability includes constraints ([29 After 22 by 1.2 to 1.3 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. 52 Neptune Opposition (2021-SEP-14) +/- 30 days preferred. 8 orbits, with mostly 2-orbit gaps between most visits (4-6x 2-orbit gaps, 1-3x 1-orbit gaps). If shifting needed (for SAA avoidance or observatory constraints), can reduce a 3rd gap to 1 orbits (no more than 3 1-orbit gaps overall). We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. 1631065234000 252.0 (Tic-Visit :proposal-id 16266 :visit-id "29" :proposal-version -1 :trans-version "20200518" :date "19-Jun-2020 08:56:56.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 325232 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "29" :obset-id "29" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "29" :orbit-number 1 :pcs-time 301 :si-vis-utilization 2512 :al-overhead-at-end 0 :internal-dur-at-end 392 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3120.0 :pcs-gap 0 ) false 1 0 1630517185589 Using ephemeris for target 16266-30-SATURN-MAPS Timing link suitability includes constraints ([31 After 30 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/0c/5011wfl508g14lx4917hgxmr0006vr/T/OPVisit11738814821368977706.xml 12 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 is acceptable, or a gap between 5-6, 6-7, or 7-8. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Saturn opposition (2021-AUG-02) +/- 30 days OPAL Saturn filters: 225, 275, 343, 395, 467, 502, 631, 727, 763, 889 If orbital visibility requires a cut, remove F467M first IF only a few second are needed, F889N can be trimmed to as short as 30S, but all exposures should be trimmed by the same amount (Tic-Visit :proposal-id 16266 :visit-id "30" :proposal-version -1 :trans-version "20210514" :date "01-Sep-2021 13:26:25.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 526768 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "30" :obset-id "30" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "30" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2421 :al-overhead-at-end 0 :internal-dur-at-end 612 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2782 :pcs-gap 0 ) true 1 1 1625745054907 Using ephemeris for target 16266-31-SATURN-MAPS Timing link suitability includes constraints ([31 After 30 by 0.1 to 0.1 days] [32 After 31 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v31.xml 47 12 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 is acceptable, or a gap between 5-6, 6-7, or 7-8. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Saturn opposition (2021-AUG-02) +/- 30 days OPAL Saturn filters: 225, 275, 343, 395, 467, 502, 631, 727, 763, 889 If orbital visibility requires a cut, remove F467M first (Tic-Visit :proposal-id 16266 :visit-id "31" :proposal-version -1 :trans-version "20210514" :date "08-Jul-2021 07:50:54.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 526768 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "31" :obset-id "31" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "31" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2373 :al-overhead-at-end 0 :internal-dur-at-end 612 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2782 :pcs-gap 0 ) true 1 0 1626786565326 Using ephemeris for target 16266-32-SATURN-MAPS Timing link suitability includes constraints ([32 After 31 by 0.1 to 0.1 days] [33 After 32 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v32.xml 12 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 is acceptable, or a gap between 5-6, 6-7, or 7-8. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Saturn opposition (2021-AUG-02) +/- 30 days OPAL Saturn filters: 225, 275, 343, 395, 467, 502, 631, 727, 763, 889 If orbital visibility requires a cut, remove F467M first (Tic-Visit :proposal-id 16266 :visit-id "32" :proposal-version -1 :trans-version "20210514" :date "20-Jul-2021 09:09:25.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 544176 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "32" :obset-id "32" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "32" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2576 :al-overhead-at-end 0 :internal-dur-at-end 631 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) false 1 0 1625745058848 Using ephemeris for target 16266-33-SATURN-MAPS Timing link suitability includes constraints ([33 After 32 by 0.1 to 0.1 days] [34 After 33 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v33.xml 47 12 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 is acceptable, or a gap between 5-6, 6-7, or 7-8. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Saturn opposition (2021-AUG-02) +/- 30 days OPAL Saturn filters: 225, 275, 343, 395, 467, 502, 631, 727, 763, 889 If orbital visibility requires a cut, remove F467M first (Tic-Visit :proposal-id 16266 :visit-id "33" :proposal-version -1 :trans-version "20210514" :date "08-Jul-2021 07:50:58.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 526768 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "33" :obset-id "33" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "33" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2373 :al-overhead-at-end 0 :internal-dur-at-end 612 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2782 :pcs-gap 0 ) true 1 0 1625745059911 Using ephemeris for target 16266-34-SATURN-MAPS Timing link suitability includes constraints ([34 After 33 by 0.1 to 0.1 days] [35 After 34 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v34.xml 12 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 is acceptable, or a gap between 5-6, 6-7, or 7-8. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Saturn opposition (2021-AUG-02) +/- 30 days OPAL Saturn filters: 225, 275, 343, 395, 467, 502, 631, 727, 763, 889 If orbital visibility requires a cut, remove F467M first (Tic-Visit :proposal-id 16266 :visit-id "34" :proposal-version -1 :trans-version "20210514" :date "08-Jul-2021 07:50:59.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 561584 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "34" :obset-id "34" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "34" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2742 :al-overhead-at-end 0 :internal-dur-at-end 650 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 1625745060866 Using ephemeris for target 16266-35-SATURN-MAPS Timing link suitability includes constraints ([35 After 34 by 0.1 to 0.1 days] [36 After 35 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v35.xml 47 12 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 is acceptable, or a gap between 5-6, 6-7, or 7-8. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Saturn opposition (2021-AUG-02) +/- 30 days OPAL Saturn filters: 225, 275, 343, 395, 467, 502, 631, 727, 763, 889 If orbital visibility requires a cut, remove F467M first (Tic-Visit :proposal-id 16266 :visit-id "35" :proposal-version -1 :trans-version "20210514" :date "08-Jul-2021 07:51:00.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 526768 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "35" :obset-id "35" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "35" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2373 :al-overhead-at-end 0 :internal-dur-at-end 612 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2782 :pcs-gap 0 ) true 1 0 1625745061896 Using ephemeris for target 16266-36-SATURN-MAPS Timing link suitability includes constraints ([36 After 35 by 0.1 to 0.1 days] [37 After 36 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v36.xml 12 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 is acceptable, or a gap between 5-6, 6-7, or 7-8. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Saturn opposition (2021-AUG-02) +/- 30 days OPAL Saturn filters: 225, 275, 343, 395, 467, 502, 631, 727, 763, 889 If orbital visibility requires a cut, remove F467M first (Tic-Visit :proposal-id 16266 :visit-id "36" :proposal-version -1 :trans-version "20210514" :date "08-Jul-2021 07:51:01.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 561584 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "36" :obset-id "36" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "36" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2742 :al-overhead-at-end 0 :internal-dur-at-end 650 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 1625745065048 Using ephemeris for target 16266-37-SATURN-MAPS Timing link suitability includes constraints ([37 After 36 by 0.1 to 0.1 days] [38 After 37 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v37.xml 47 12 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 is acceptable, or a gap between 5-6, 6-7, or 7-8. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Saturn opposition (2021-AUG-02) +/- 30 days OPAL Saturn filters: 225, 275, 343, 395, 467, 502, 631, 727, 763, 889 If orbital visibility requires a cut, remove F467M first (Tic-Visit :proposal-id 16266 :visit-id "37" :proposal-version -1 :trans-version "20210514" :date "08-Jul-2021 07:51:04.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 526768 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "37" :obset-id "37" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "37" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2421 :al-overhead-at-end 0 :internal-dur-at-end 612 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2782 :pcs-gap 0 ) true 1 1 1628084909594 Using ephemeris for target 16266-38-SATURN-MAPS Timing link suitability includes constraints ([38 After 37 by 0.1 to 0.1 days] [39 After 38 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v38.xml 12 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 is acceptable, or a gap between 5-6, 6-7, or 7-8. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Saturn opposition (2021-AUG-02) +/- 30 days OPAL Saturn filters: 225, 275, 343, 395, 467, 502, 631, 727, 763, 889 If orbital visibility requires a cut, remove F467M first (Tic-Visit :proposal-id 16266 :visit-id "38" :proposal-version -1 :trans-version "20210514" :date "04-Aug-2021 09:48:29.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 561584 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "38" :obset-id "38" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "38" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2742 :al-overhead-at-end 0 :internal-dur-at-end 650 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 1628084912401 Using ephemeris for target 16266-39-SATURN-MAPS Timing link suitability includes constraints ([39 After 38 by 0.1 to 0.1 days] [40 After 39 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v39.xml 47 12 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 is acceptable, or a gap between 5-6, 6-7, or 7-8. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Saturn opposition (2021-AUG-02) +/- 30 days OPAL Saturn filters: 225, 275, 343, 395, 467, 502, 631, 727, 763, 889 If orbital visibility requires a cut, remove F467M first (Tic-Visit :proposal-id 16266 :visit-id "39" :proposal-version -1 :trans-version "20210514" :date "04-Aug-2021 09:48:32.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 526768 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "39" :obset-id "39" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "39" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2421 :al-overhead-at-end 0 :internal-dur-at-end 612 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2782 :pcs-gap 0 ) true 1 1 1630517294465 Using ephemeris for target 16266-40-SATURN-MAPS Timing link suitability includes constraints ([40 After 39 by 0.1 to 0.1 days] [41 After 40 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/0c/5011wfl508g14lx4917hgxmr0006vr/T/OPVisit3180179494632882418.xml 12 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 is acceptable, or a gap between 5-6, 6-7, or 7-8. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Saturn opposition (2021-AUG-02) +/- 30 days OPAL Saturn filters: 225, 275, 343, 395, 467, 502, 631, 727, 763, 889 If orbital visibility requires a cut, remove F467M first (Tic-Visit :proposal-id 16266 :visit-id "40" :proposal-version -1 :trans-version "20210514" :date "01-Sep-2021 13:28:14.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 526768 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "40" :obset-id "40" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "40" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2373 :al-overhead-at-end 0 :internal-dur-at-end 612 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2782 :pcs-gap 0 ) true 1 0 1628084919124 Using ephemeris for target 16266-41-SATURN-MAPS Timing link suitability includes constraints ([41 After 40 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /System/Volumes/Data/solaris/user1/aroman/work/hst/OP-cache/16266-v41.xml 47 12 orbits, should be contiguous, if possible. A gap of 1 or 2 orbits between 6 - 7 is acceptable, or a gap between 5-6, 6-7, or 7-8. Impingement into SAA is OK if the above timing gaps cannot prevent it. We can tolerate gyro bias updates to ease the contiguous orbit constraints, and will work with our program contacts to fit them in. 3-gyro mode may be necessary as this is a moving target. Saturn opposition (2021-AUG-02) +/- 30 days OPAL Saturn filters: 225, 275, 343, 395, 467, 502, 631, 727, 763, 889 If orbital visibility requires a cut, remove F467M first (Tic-Visit :proposal-id 16266 :visit-id "41" :proposal-version -1 :trans-version "20210514" :date "04-Aug-2021 09:48:38.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 526768 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16266 :visit-id "41" :obset-id "41" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16266 :visit-id "41" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2421 :al-overhead-at-end 0 :internal-dur-at-end 612 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2782 :pcs-gap 0 ) false 1 1