Galaxy Transformation in the Infall Regions of Clusters
The rise in the number of S0's in dense environments since z = 0.5, and the corresponding decline in spiral galaxies, points strongly to S0's being a product of the hierarchical processes that build structure. However, the physical mechanism responsible for the transformation from spiral to lenticular is hotly debated and several viable candidates exist. We propose a survey of the infall regions of clusters, as traced using our existing wide field spectroscopic survey of groups and clusters at 0.4 < z < 0.8 out to ~3 virial radii, to discriminate between these mechanisms, whose effectiveness varies with environment. By determining where S0's form, rather than where they are ultimately found in great numbers (i.e. massive clusters), and by examining whether the bulge populations of these infalling systems are young, we will determine what processes are responsible for creating the large stellar bulges in these systems. By reaching out to at least 3 virial radii, we will be studying the regions from which over 90% of the galaxies that reside in today's clusters come from, as such we are guaranteed to be observing galaxies before, during, and after this transformation.
The observing program is straightforward. We will obtain ACS/WFC images at specific positions in the outskirts of intermediate redshift galaxy clusters that are chosen to maximize the number of cluster-associated galaxies. Parallel exposures in WFC3/UVIS provide additional coverage of the cluster outskirts. Both cameras will use F814W and F606W each for 1 orbit per position.
We have chosen the same 4-pt dither pattern as in the Brown et al. example proposal (-0.1976,-0.016) (0.2223,0.018) (0.1729, 0.2363) (0.0,0.1729) arcsec. This will give 0.5 pixel sampling on ACS/WFC and nearly 0.5 pixel sampling on WFC3/UVIS, because 4 ACS pixels are approximately 5 WFC3 pixels.
UNRESOLVED STELLAR POPULATIONS AND GALAXY STRUCTURE
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(Tic-Orbit
:proposal-id 13393
:visit-id "12"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2774
:al-overhead-at-end 70
:internal-dur-at-end 668
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "Y"
:pcs-visibility 3178
:pcs-gap 400
)
(Tic-Orbit
:proposal-id 13393
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:orbit-number 2
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:al-overhead-at-end 60
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "Y"
:pcs-visibility 3178
:pcs-gap 400
)
false
2
0
The scheduling data was generated by CASM 21.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 13393
:visit-id "13"
:proposal-version -1
:trans-version "20130502"
:date "13-Jun-2013 11:24:13.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "29"
:si-bright-earth-limb-angle 40.0
:data-volume 4583776
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 13393
:visit-id "13"
:obset-id "13"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 13393
:visit-id "13"
:orbit-number 1
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:si-vis-utilization 2774
:al-overhead-at-end 70
:internal-dur-at-end 668
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "Y"
:pcs-visibility 3178
:pcs-gap 400
)
(Tic-Orbit
:proposal-id 13393
:visit-id "13"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2777
:al-overhead-at-end 60
:internal-dur-at-end 1015
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "Y"
:pcs-visibility 3178
:pcs-gap 400
)
true
2
0
The scheduling data was generated by CASM 21.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 13393
:visit-id "14"
:proposal-version -1
:trans-version "20130502"
:date "13-Jun-2013 11:24:18.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "29"
:si-bright-earth-limb-angle 40.0
:data-volume 4583776
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 13393
:visit-id "14"
:obset-id "14"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 13393
:visit-id "14"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2774
:al-overhead-at-end 70
:internal-dur-at-end 668
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "Y"
:pcs-visibility 3178
:pcs-gap 400
)
(Tic-Orbit
:proposal-id 13393
:visit-id "14"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2777
:al-overhead-at-end 60
:internal-dur-at-end 1015
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "Y"
:pcs-visibility 3178
:pcs-gap 400
)
true
2
0
The scheduling data was generated by CASM 21.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 13393
:visit-id "15"
:proposal-version -1
:trans-version "20130502"
:date "13-Jun-2013 11:24:23.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "29"
:si-bright-earth-limb-angle 40.0
:data-volume 4583776
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 13393
:visit-id "15"
:obset-id "15"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 13393
:visit-id "15"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2774
:al-overhead-at-end 70
:internal-dur-at-end 668
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "Y"
:pcs-visibility 3178
:pcs-gap 400
)
(Tic-Orbit
:proposal-id 13393
:visit-id "15"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2777
:al-overhead-at-end 60
:internal-dur-at-end 1015
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "Y"
:pcs-visibility 3178
:pcs-gap 400
)
true
2
0