In this resubmission, I have added visit 44 which repeats the failed visit 04 and visit 22 which repeats failed visit 12 (approved by the TTRB). Our other repeat visit 55 is still there with just a slight change in the orient range. I had to create a new targets (NGC 2014 A,B,C) for the repeat visits. The scheduling window doesn't open until Feb 2, constraining us to orients about 30 degrees off from the rest of the mosaic, so the new dither patterns approximate the same sky coverage to "fill the holes". We'd appreciate getting these scheduled on the early end to avoid additional delay. -- Max Mutchler
889017861
----- Attempting Submission 5 (Tue Sep 17 18:35:56 GMT 2019) -----
----- Attempting Submission 6 (Mon Nov 04 21:05:27 GMT 2019) -----
----- Attempting Submission 7 (Mon Nov 25 16:39:35 GMT 2019) -----
----- Attempting Submission 8 (Mon Jan 06 17:09:54 GMT 2020) -----
----- Attempting Submission 9 (Mon Jan 13 18:57:13 GMT 2020) -----
Our total allocation has been increased from 36 to 43 orbits so we can repeat 3 failed visits.
WFC3 mosaic of NGC 2020 and NGC 2014
We will utilize WFC3 to create a large mosaic of NGC 2020 and NGC 2014 in the Large Magellanic Cloud.
We request 36 orbits to make a large WFC3 mosaic of NGC 2020 and NGC 2014 in the Large Magellanic Cloud (LMC). With a 4x3 mosaic and three HST orbits per tile, we will obtain deep narrow band imaging with two filters (F502N, F657N). We will also include shorter broadband exposures (F475W, F814W) both for continuum subtraction and to obtain colors for the many stars in this crowded LMC field. We will perform an expanded 3-step WFC3 gap dither for excellent rejection of cosmic rays and detector artifacts. The gap shift is exaggerated to make each tile a half-mosaic step that can be done in one visit (with the same guide stars). This modified gap dither helps to stretch the mosaic to fully cover NGC 2020 and the nebulosity around NGC 2014. It also helps mitigate saturation and ghosting which we expect due to the crowded LMC star field. These observations can be executed at the desired ORIENT angle range of 21-32 degrees in early January 2020, and could easily be converted to one-gyro mode if necessary. Our desired orient is optimal for standard three-gyro mode, but is not required. Switching to one-gyro mode would mainly require us to reduce exposure times, in which case we might consider switching to a smaller mosaic to maintain the desired signal-to-noise. We understand that the orientations of some mosaic tiles may need to vary a bit for schedulability, and we will work with our Program Coordinator to adjust the orients and tile overlaps to ensure continuous coverage.
Visits 04, 05, and 12 failed due to guide star acquisition errors, and will be repeated as visits 44, 55, and 22 (which has been approved by the TTRB). These repeat visits must be done a month later and therefore at an orientation about 30 degrees rotated from the original, requiring dithers that can cover a similar area to avoid missing data in the mosaic. These repeat visits require that separate target specifications (NGC 2014 A,B,C)) be specified.
Joel Green contributed to the target selection and observing plan, and is the overall content manager for the project in the STScI Office of Public Outreach (OPO). Max Mutchler contributed to the target selection and observing plan, prepared the Phase I proposal, and will lead the Phase II implementation, drizzling of the resulting data into mosaics, and delivery of data products to MAST as HLSP. Joe DePasquale contributed to the target selection and observing plan, and will process the mosaics into color composite images for press release and related visualizations. Christine Pulliam contributed to the target selection and observing plan, and is the JWST News Chief. Ray Villard contributed to the target selection and observing plan, and is the HST News Chief. Cheryl Gundy is the OPO News Production Lead. Emma Marcucci is the OPO Branch Manager for Science Communications and Engagement and plays an outreach advisory role on the overall project. Brandon Lawton plays an outreach advisory role on the overall project. Alex Lockwood plays an outreach advisory role on the overall project, and is a JWST liaison. Denise Smith is the OPO Deputy Division Head. Frank Summers will provide 3D visualization of the resulting mosaics. John Godfrey will design outreach products resulting from the mosaics.
Stellar Physics
6
false
SUPPORTED
ISM
HII REGION
STAR FORMING REGION
YES
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
ISM
HII REGION
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
ISM
HII REGION
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
ISM
HII REGION
STAR FORMING REGION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
WFC3/UVIS
Imaging
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F475W
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Imaging
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