0Assigned ID: 4464
----- Attempting Submission 1 (Wed May 24 17:59:50 GMT 2023) -----ORBITAL VISIBILITY OVERRUN
GS ACQ SCENARIO REQUESTED INCONSISTENT WITH VISIT GYRO MODE
The specified GS Acq Scenario is not in the current list of valid scenarios.
GS ACQ SCENARIO REQUESTED INCONSISTENT WITH VISIT GYRO MODE
ORBITAL VISIBILITY OVERRUN
The specified GS Acq Scenario is not in the current list of valid scenarios.
GS ACQ SCENARIO REQUESTED INCONSISTENT WITH VISIT GYRO MODE
ORBITAL VISIBILITY OVERRUN
The specified GS Acq Scenario is not in the current list of valid scenarios.
GS ACQ SCENARIO REQUESTED INCONSISTENT WITH VISIT GYRO MODE
ORBITAL VISIBILITY OVERRUN
The specified GS Acq Scenario is not in the current list of valid scenarios.
GS ACQ SCENARIO REQUESTED INCONSISTENT WITH VISIT GYRO MODE
ORBITAL VISIBILITY OVERRUN
The specified GS Acq Scenario is not in the current list of valid scenarios.
ORBITAL VISIBILITY OVERRUN
GS ACQ SCENARIO REQUESTED INCONSISTENT WITH VISIT GYRO MODE
The specified GS Acq Scenario is not in the current list of valid scenarios.
ORBITAL VISIBILITY OVERRUN
GS ACQ SCENARIO REQUESTED INCONSISTENT WITH VISIT GYRO MODE
The specified GS Acq Scenario is not in the current list of valid scenarios.
GS ACQ SCENARIO REQUESTED INCONSISTENT WITH VISIT GYRO MODE
ORBITAL VISIBILITY OVERRUN
The specified GS Acq Scenario is not in the current list of valid scenarios.
GS ACQ SCENARIO REQUESTED INCONSISTENT WITH VISIT GYRO MODE
ORBITAL VISIBILITY OVERRUN
The specified GS Acq Scenario is not in the current list of valid scenarios.
ORBITAL VISIBILITY OVERRUN
GS ACQ SCENARIO REQUESTED INCONSISTENT WITH VISIT GYRO MODE
The specified GS Acq Scenario is not in the current list of valid scenarios.
ORBITAL VISIBILITY OVERRUN
GS ACQ SCENARIO REQUESTED INCONSISTENT WITH VISIT GYRO MODE
The specified GS Acq Scenario is not in the current list of valid scenarios.
GS ACQ SCENARIO REQUESTED INCONSISTENT WITH VISIT GYRO MODE
ORBITAL VISIBILITY OVERRUN
The specified GS Acq Scenario is not in the current list of valid scenarios.
GS ACQ SCENARIO REQUESTED INCONSISTENT WITH VISIT GYRO MODE
ORBITAL VISIBILITY OVERRUN
The specified GS Acq Scenario is not in the current list of valid scenarios.
GS ACQ SCENARIO REQUESTED INCONSISTENT WITH VISIT GYRO MODE
ORBITAL VISIBILITY OVERRUN
The specified GS Acq Scenario is not in the current list of valid scenarios.
GS ACQ SCENARIO REQUESTED INCONSISTENT WITH VISIT GYRO MODE
ORBITAL VISIBILITY OVERRUN
The specified GS Acq Scenario is not in the current list of valid scenarios.This submission is the fifth revision for RGM. The only change from the previous version is a small tweak to the schedule window for Visit 42.-3443298----- Attempting Submission 1 (Thu Sep 14 19:06:51 GMT 2023) -----
HST Phase II Proposal 17510 successfully submitted.
Receipt: # 17510-1
----- Attempting Submission 2 (Wed Oct 04 04:22:39 GMT 2023) -----
----- Attempting Submission 3 (Mon Nov 13 17:18:17 GMT 2023) -----
----- Attempting Submission 4 (Thu Jun 27 05:07:42 GMT 2024) -----
HST Phase II Proposal 17510 successfully submitted.
Receipt: # 17510-4
----- Attempting Submission 5 (Tue Jul 02 23:03:27 GMT 2024) -----
HST Phase II Proposal 17510 successfully submitted.
Receipt: # 17510-5
----- Attempting Submission 6 (Wed Aug 21 20:34:50 GMT 2024) -----
HST Phase II Proposal 17510 successfully submitted.
Receipt: # 17510-6
----- Attempting Submission 7 (Fri Nov 01 05:23:31 GMT 2024) -----
HST Phase II Proposal 17510 successfully submitted.
Receipt: # 17510-7
----- Attempting Submission 8 (Tue Nov 12 19:10:54 GMT 2024) -----Target charts have been previously verified at the first submission; no change to target coords.
The 45 warnings are for the completed visits done prior to RGM, which is generating all the warnings.
All of the unexecuted visits are clean.The Origin of the Virgo Intergalactic PopulationThe intracluster light (ICL) is a major component of galaxy clusters, and contains a record of the
galaxies destroyed during hierarchical assembly of the cluster. This proposal addresses three
issues critical to understanding the origin and evolution of intergalactic populations, using
resolved star WFC3/IR photometry of intergalactic fields in the Virgo cluster. Foremost, we will
probe the age distribution of Virgo's intracluster stars via the period distribution of bright AGB
variable stars, a tool successfully deployed to study stellar populations in elliptical galaxies.
By spreading the observations over 8 epochs and two HST cycles (4+4), we can determine periods and
reveal the age spread of the intracluster stars, opening a new window on their origin and evolution.
Second, IR color magnitude diagrams from the stacked imaging will establish the metallicity
distribution function of the ICL, constraining the luminosity function and abundances of the
galaxies that have been dismembered in assembling the intracluster population. Third, by observing
five fields around the core of the cluster, we will trace how spatially well-mixed the ICL
population is and how its age and metallicity vary across diverse environments, and thus measure its
evolutionary state. While JWST will extend photometric work on the Virgo ICL, period determination
of LPVs with JWST is very difficult because of its restricted visibility window in Virgo. It is
therefore critical to begin these multi-cycle observations while time permits before the end of
HST's lifetime.WFC3/IR will image five intergalactic fields in F110W and F160W. The
observations will be spread over 8 one-orbit visits and two HST cycles
(four visits in each cycle) to detect and phase variable stars with
periods up to at least 750d. The data will be taken with SPARS50,
dividing each orbit into 3 F110W and 3 F160W exposures. These will be
dithered in each visit to mitigate the effect of the IR blobs, and
then with tight dithers between each visit for bad pixels.
The visits will occur in two orients, ~300deg and ~120deg to achieve
optimum spacing of the epochs for phasing. Using just two orients
180deg apart preserves the field coverage between epochs, as well as
maximizes the depth of the parallel fields.
We request SAA-free orbits because of the sensitivity of the IR
detectors to SAA passage. We realize this is a limited resource, but
since one goal is to make as deep a CMD as possible, and having
reliable photometry at each epoch is necessary for the detection and
phasing of the variables, SAA-free time ensures the success of the
project. Our single orbit visits facilitate this scheduling.
During the WFC3/IR observations, ACS/WFC will be in the intergalactic
reaches of Virgo and can contribute further valuable data to the study
of the ICL and Virgo population. We will obtain F606W and F814W
images, to maximize depth and be compatible with other deep imaging
done with HST in Virgo. The images will be 1 F606W exposure and 2
F814W in each epoch for the parallelsDr. Michael Gregg has extensive expertise in planning and executing large HST programs, in reducing
WFC3 and ACS data using drizzling, and in the PSF photometry analysis of the resulting images. He
has a background in galaxy clusters, tidal disruption of galaxies, globular clusters in early type
galaxies, ultra-compact dwarf galaxies, and resolved star photometry of extragalactic red giant
branch populations. He will take main responsibility for planning the Phase II proposal and the
drizzling reductions, plus collaborate in all subsequent aspects of the photometry and
interpretation of the color magnitude diagrams and period distribution functions.
Dr. Chris Mihos is the PI of the Burrell Schmidt deep imaging survey of Virgo intracluster light, and an expert
on both observations and simulations of diffuse light in galaxy groups and clusters. He also is PI on
two recent HST projects studying the resolved stellar populations in M101 and galaxies in Virgo.
Dr. Dante Minniti has a background in stellar astrophysics, stellar populations, star clusters, and
variable stars. His expertise is in spectroscopy and multivavelength photometry, and he is currently PI of
the VISTA survey of the Galactic Plane, which includes discovery and phasing of variable stars.
Dr. Marina Rejkuba is an expert in extragalactic stellar populations, especially early type
galaxies. Of particular relevance here, she has led a major programs with the VLT and HST to study
the red and asymptotic giant branch populations around NGC5128, including phasing of the long period
variables over multi-year epochs of observations.
Dr. Doug Welch is an expert in variable star identification and period determination.
Dr. Michael West is an expert on galaxy formation and evolution, clusters of galaxies, and the
environmental impact of the large-scale structure of the universe on galaxies and galaxy clusters.
All of the Co-I's will contribute significantly to most components of this research, especially the
analysis and interpretation of the resulting color magnitude diagrams and period distribution
functions, and the implications for theory of cluster formation.Large Scale Structure of the UniverseStellar Populations and the Interstellar Medium0falsefalsefalsefalsefalsefalsefalsetruePRIMARY0.00.0falseSUPPORTEDEXT-STARK III-ILONG PERIOD VARIABLEM III-IJ2000J2000EXT-STARK III-ILONG PERIOD VARIABLEM III-IJ2000J2000EXT-STARK III-ILONG PERIOD VARIABLEM III-IJ2000J2000EXT-STARK III-ILONG PERIOD VARIABLEM III-IJ2000J2000EXT-STARK III-ILONG PERIOD VARIABLEM III-IJ2000J2000WFC3/IRImagingNoNoF160WWFC3/IRImagingNoNoF110WWFC3/IRImagingNoNoF160WWFC3/IRImagingNoNoF110WWFC3/IRImagingNoNoF160WWFC3/IRImagingNoNoF110WWFC3/IRImagingNoNoF160WWFC3/IRImagingNoNoF110WWFC3/IRImagingNoNoF160WWFC3/IRImagingNoNoF110WACS/WFCImagingNoNoF475WACS/WFCImagingNoNoF814WACS/WFCImagingNoNoF475WACS/WFCImagingNoNoF814WACS/WFCImagingNoNoF475WACS/WFCImagingNoNoF814WACS/WFCImagingNoNoF475WACS/WFCImagingNoNoF814WACS/WFCImagingNoNoF475WACS/WFCImagingNoNoF814WTiming link suitability includes constraints ([12 After 11 by 51.0 to 53.0 days] [13 After 11 by 118.0 to 122.0 days])Hst Same orient constraint links visits (11 12 14 A4)The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./private/var/folders/8t/mg1bkfyj20xf2vfc_9vyhfs80006z1/T/OPVisit1710999299245949330.xml1702464850000300.0(Tic-Visit
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