Modified slightly angle for subdither patterns (again) to be 138.141 in subpattern.
----- Attempting Submission 2 (Mon Sep 05 14:18:32 GMT 2011) -----
----- Attempting Submission 3 (Thu Sep 08 01:04:03 GMT 2011) -----
New Constraints on Intragroup Light and the Baryon Budget in Galaxy Groups
We propose a focused WFC3/IR imaging program targeting galaxy groups at z=0.3-0.5 to better understanding why the partitionings between baryon phases (gas vs. stars) and stellar components (within vs. outside galaxies) show such strong variation from groups to rich clusters. We will 1) obtain the first complete census of stars both in and out of group galaxies for a representative sample of groups and 2) use the luminosity distribution and colors of the intragroup stellar populations to constrain the galactic population from which the stars were stripped. As demonstrated by our Cycle 16 program on the Bullet Cluster, WFC3 offers a major step forward for studies of such diffuse stellar populations, enabling a vast improvement over previous ground-based studies of intracluster/intragroup light and total baryon content in groups and clusters. We will use the sample from this program in conjunction with the clusters from the CLASH Multicycle Treasury Program to quantify the total stellar baryon content in clusters and groups spanning more than a dex in mass. We will also unambiguously determine the progenitor galaxy population from which the ICL is assembled.
We are targeting a total of eight galaxy groups at 0.3<z<0.5 to map out the intragroup light in these systems. We are using the F105W and F160W filters, with the expectation of recovering the color gradient in these filters out to 140 kpc in each group. The F105W filter is somewhat less sensitive for this program than F110W, but the greater wavelength baseline nonetheless makes it the preferred option. To be precise, we expect to lose 0.2 mag/sq arcsec depth but gain 0.2 mag in color leverage. This still enables us to get out to r~140kpc from the center of each group, which is our intended reach. Low sky is critical for this program because one of the two key limiting factors will be uncertainty in the background sky level (the other being low order flatfielding variations). We note that all fields remain schedulable outside the Nov 11, 2011 - March 1, 2012 window with the low sky requirement.
We are observing six of the systems for 5 orbits each, with 4 orbits allocated for each of the two lower redshift groups. With the 5 orbit observations the split is 2 orbits in F160W and 3 orbits in F105W. For dithering we are using the IR-DITHER-BLOB pattern with a 2 point line sub-pattern for F160W and IR-DITHER-BLOB with a 3 point line pattern for F105W, with the goal of optimizing the subpixel sampling while also obtaining good (blob-free) data at all locations. With the 4 orbit observations every orbit is split between the two filters. We are again using IR-DITHER-BLOB with a 2 point dither patter in this instance, but taking both filters at each position during a single dither pattern (as opposed to executing a dither pattern separately for each filter as in the 5 orbit case).
There are parallel orbits associated with four of the targets in this program (each 5 orbits). These parallel images with ACS are designed to provide morphological information on galaxies in the infall region around the supergroup SG1120. We have no constraints on orientation associated with these parallel observations.
Please note that we have substituted in two new targets (the XMMXCS groups) to replace the XLSSC groups. This substitution has been approved.
UNRESOLVED STELLAR POPULATIONS AND GALAXY STRUCTURE
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)
(Tic-Orbit
:proposal-id 12575
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true
4
0
The scheduling data was generated by CASM 19.3.
CASM was run in Phase II mode.
/private/var/folders/RW/RW6WBQcRGYGrMOW0jgtCgk+++TI/-Tmp-/OPVisit5400942275427035296.xml
XMMXCS J022045.1-032555
(Tic-Visit
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:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 4
:saa-model "30"
:si-bright-earth-limb-angle 40.0
:data-volume 3133568
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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)
(Tic-Orbit
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)
(Tic-Orbit
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(Tic-Orbit
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(Tic-Orbit
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true
4
0