Science Keywords: Select from 2 to 5 items.
Science Keywords is a required field.
The total number of Primary Orbits used in all Cycles must equal the total number of Primary Orbits specified on all the Observations. (Compare totals reported on the first and second pages of the PDF Preview.)
Small GO Proposals are not allowed in Cycle 26 unless they are Joint Programs.
At least one target must be specified in Phase I
At least one observation must be specified
0
Assigned ID: 36
----- Attempting Submission 1 (Thu Aug 02 13:15:05 GMT 2018) -----
Joint Chandra/HST
Removed F160W observation from Visit 05, reset F110W and F140W exposures to nominal SNAP duration.
-1815057638
----- Attempting Submission 1 (Tue Oct 23 20:13:20 GMT 2018) -----
----- Attempting Submission 2 (Tue May 14 08:13:46 GMT 2019) -----
Your proposal could not be saved.
Submission aborted.
----- Attempting Submission 3 (Tue May 14 21:08:40 GMT 2019) -----
----- Attempting Submission 4 (Thu May 16 21:41:54 GMT 2019) -----
----- Attempting Submission 5 (Fri May 31 18:29:39 GMT 2019) -----
HST Phase II Proposal 15608 (GO-15608.apt) successfully submitted.
Receipt: # 15608-5
----- Attempting Submission 6 (Tue Jun 04 21:16:18 GMT 2019) -----
HST Phase II Proposal 15608 (GO-15608rev.apt) successfully submitted.
Receipt: # 15608-6
----- Attempting Submission 7 (Wed Jun 05 17:17:37 GMT 2019) -----
----- Attempting Submission 8 (Wed Jul 24 22:25:05 GMT 2019) -----
Visit planner WAS run for the only remaining visit (#5)
Characterizing the most X-ray luminous galaxy clusters at z=0.5-1
We propose moderately deep ACIS-I observations, as well as HST snapshots, of 11 exceptionally X-ray luminous clusters at z=0.5-0.9 discovered by the eMACS project. Confirmed as massive by velocity dis- persions exceeding 1100 km/s and the presence of strong-lensing features in existing HST images, nine of these systems were nonetheless missed by Planck. By yielding robust measurements of X-ray luminosity, ICM temperature, and X-ray morphology, the proposed observations will extend the redshift baseline for statistical studies of cluster growth beyond the MACS regime, identify physical biases in the eMACS and Planck cluster samples, and reveal exceptional opportunities for in-depth studies of the distribution and dynamics of luminous and dark matter in the era of JWST and 30m telescopes.
We follow the observing strategy of GO-15132 to complete SNAP observations of all targets in the same four passbands.
Cosmology
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