0Assigned ID: 142
----- Attempting Submission 1 (Thu Feb 23 06:14:33 GMT 2012) -----
HST Phase I Proposal 142 (HST_kepler11.apt) successfully submitted.
----- Attempting Submission 2 (Thu Feb 23 18:49:15 GMT 2012) -----
HST Phase I Proposal 142 (HST_kepler11.apt) successfully submitted.
----- Attempting Submission 3 (Thu Feb 23 21:49:22 GMT 2012) -----
HST Phase I Proposal 142 (HST_kepler11.apt) successfully submitted.
Submission failed communicating with the submission server:
java.rmi.ConnectException: Connection refused to host: clotho.stsci.edu; nested exception is:
java.net.ConnectException: Operation timed out
Submission failed communicating with the submission server:
java.rmi.UnknownHostException: Unknown host: clotho.stsci.edu; nested exception is:
java.net.UnknownHostException: clotho.stsci.edu
Submission failed communicating with the submission server:
java.rmi.UnknownHostException: Unknown host: clotho.stsci.edu; nested exception is:
java.net.UnknownHostException: clotho.stsci.edu
----- Attempting Submission 4 (Fri Feb 24 21:42:29 GMT 2012) -----Cut 10 exposures from visits 08 and 09 to allow scheduling
Cut 6 exposures from visit 15, expanded link. Added 5 exposures to visits 10-14
Expanded visits 03 and 16-20 to SCHED 30 length again1576682900----- Attempting Submission 1 (Wed Jul 04 04:18:00 GMT 2012) -----
----- Attempting Submission 2 (Wed May 08 19:28:32 GMT 2013) -----
----- Attempting Submission 3 (Wed Jul 31 12:22:17 GMT 2013) -----
----- Attempting Submission 4 (Fri Aug 09 18:35:46 GMT 2013) -----
----- Attempting Submission 5 (Fri Aug 09 22:08:28 GMT 2013) -----
----- Attempting Submission 6 (Thu Aug 15 14:59:22 GMT 2013) -----
----- Attempting Submission 7 (Tue Aug 20 14:40:17 GMT 2013) -----in-house processingComparing Planet Formation Signatures in two SystemsFollowing the discovery of exoplanet systems with multiple transiting planets - unique laboratories for studying planet formation and evolution - we propose to characterize and compare the exoplanet atmospheric composition in the compact solar system analog Kepler-11. We propose WFC3/G141 transmission spectroscopy of three low-density super-Earth/Neptune planets in the six-planet system. The proposed grism spectroscopy targets the strong 1.4-micron water band and the distinct 1.6-micron methane features, thus probing the principal thermochemical reservoirs of oxygen and carbon for the planets we will observe. The carbon and oxygen abundance and their ratio are key diagnostics of planet formation and evolution, and the proposed observations will provide a unique observational constraint because comparing planets in the same exoplanet system removes the variables that influence inter-system comparative exoplanetology. Together with the only other multi-planet system observation (PI Desert), the proposed observations aim at starting the process of observationally differentiating inter-system and intra-system parameters that influence the composition of individual planets. In so doing, we will improve our understanding of whether our own solar system is typical or exceptional.We will observe the spectroscopic time series of the transit [aka primary eclipse] of three super-Earth planets in the Kepler-11 system. Each of the different transits is implemented as a separate visit [3 visits in total]. Each visit targets a different planet, respectively Kepler-11d, Kepler-11e, and Kepler-11f. For each of the transits, we use the WFC3/G141 setup and the light output of the Kepler-11 system will be monitored over 7, 6, and 7 Hubble orbits respectively, to be executed continuously per transit event. The objective is to measure the spectroscopic change in the amount of light during transit versus out-of-transit for each of the targeted planets.
The observations are time sensitive because they have to measure the transit events. The timing of the transits is well known with minute precision and the transit timing is implemented with a period and zero phase. Each visit starts with a wavelength calibration direct image followed by a series of G141 spectra. Except for the first direct image, the 7, 6 and 7 Hubble orbits are filled with continuous time series of G141 spectroscopy. To time the observations correctly, the first image of the series [the wavelength calibration image] is timed such that the remainder orbits cover the transit and sufficient out of transit data to make a robust difference. The timing is implemented by providing a phase range. For APT reasons, the visits got split up in different sub-visits, one per Hubble orbit. Trying to put all observations in one visit did not work with the APT because the computing time required grew exponentially to beyond capability. Each visit now has 7, 6 and 7 sub-visits respectively. Each of the sub-visits is timed to start immediately after the startup visit (name Kepler11d, Kepler11e, and Kepler11f respectively). The sub-visits are named with Kepler11d_X with X being the orbit number. We request no role angle moves during a visit to optimize the stability.EXTRA-SOLAR PLANETS12falsefalse0.00.0falsefalsefalseSUPPORTEDSTAREXTRA-SOLAR PLANETARY SYSTEMThis object was generated by the targetselector and retrieved from the SIMBAD database.J2000J2000J = 12.55, H = 12.24, K = 12.18WFC3/IRSpectroscopicNoNoG141WFC3/IRSpectroscopicNoNoG141WFC3/IRSpectroscopicNoNoG141Timing link suitability includes constraints ([04 After 01 by at most 0.1 days])Hst Same orient constraint links visits (01 04 05 06 07 08 09)The scheduling data was generated by CASM 21.2.CASM was run in Phase II mode.observe the primary eclipse [aka transit] of Kepler-11d (7 orbits total)(Tic-Visit
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