Assigned ID: 810
----- Attempting Submission 1 (Fri Feb 25 23:57:46 GMT 2011) -----
added requirements for single star guiding to selected visits
updated PI email
----- Attempting Submission 1 (Thu Jun 30 16:50:52 GMT 2011) -----
----- Attempting Submission 2 (Thu Jun 30 18:55:08 GMT 2011) -----
----- Attempting Submission 3 (Tue Sep 27 18:17:49 GMT 2011) -----
Near-IR Imaging of the Most Distant Spectroscopically-Confirmed Galaxies in the Subaru Deep Field
The last decade saw great progress in our understanding of the distant Universe as a number of objects at z > 6 were discovered. In particular, with the power of the HST WFC3/IR camera, galaxies and galaxy candidates at z > 6 (up to 10) are being routinely found. However, we still know very little about their physical properties due to a lack of a large and bright galaxy sample with secure redshifts. Here we propose to carry out HST/WFC3 near-IR imaging of a large sample of spectroscopically-confirmed galaxies at 5.7 < z < 7 in the Subaru Deep Field (SDF). SDF is unique: it covers more than 800 sq arcmin; it has the deepest optical images among all ground-based imaging data; it has the largest sample of spectroscopically-confirmed galaxies at z >= 6 so far; it also has deep IRAC (~6 hours) coverage from our Spitzer programs. From the proposed observations and our previous HST programs, we will obtain high-quality near-IR data (rest-frame UV) for about 60 galaxies. The near-IR data is the key to measure the properties of young stellar populations, while the IRAC data constrains mature populations. Using SED modeling with spectroscopic redshifts, we will be able to fully characterize the physical properties of these galaxies and obtain accurate information of age and stellar mass etc. We will also address the physical difference or similarity between Lyman alpha emitters and Lyman break galaxies at z >= 6. All these help us to understand the earliest galaxy formation and evolution and the galaxy contribution to cosmic reionization. Our WFC3 data will enable many other sciences, such as galaxy morphology at z >= 6 and search of bright galaxies at z > 7.
Our observing strategy is straightforward (simply broad-band photometry). We will observe more than 40 spectroscopically confirmed galaxies at z >= 6 in the Subaru Deep Field (13h274m, 27d30m) with 12 HST pointings. Each pointing will be observed in two WFC3 bands F125W and F160W, with one or two orbits per band. According to our existing WFC3 data, these galaxies likely span a large magnitude range of 25 < J_AB < 27, but WFC3 is able to detect the faintest ones with two-orbit integration. The integration of each object per band will be broken into four individual exposures with sub-pixel dithering, to improve PSF and to remove bad pixels and CRs. These galaxies were chosen so that all of them can be observed within 12 HST pointings regardless of rolling angles (with fixed coordinates). We do not have any scheduling constraints or special requirements.
None.
None.
None.
COSMOLOGY
12
false
0.0
0.0
false
false
false
false
SUPPORTED
GALAXY
HIGH REDSHIFT GALAXY
J2000
J2000
J = 25-27 AB mag
GALAXY
HIGH REDSHIFT GALAXY
J2000
J2000
J = 25-27 AB mag
GALAXY
HIGH REDSHIFT GALAXY
J2000
J2000
J = 25-27 AB mag
GALAXY
HIGH REDSHIFT GALAXY
J2000
J2000
J = 25-27 AB mag
GALAXY
HIGH REDSHIFT GALAXY
J2000
J2000
J = 25-27 AB mag
GALAXY
HIGH REDSHIFT GALAXY
J2000
J2000
J = 25-27 AB mag
GALAXY
HIGH REDSHIFT GALAXY
J2000
J2000
J = 25-27 AB mag
GALAXY
HIGH REDSHIFT GALAXY
J2000
J2000
J = 25-27 AB mag
GALAXY
HIGH REDSHIFT GALAXY
J2000
J2000
J = 25-27 AB mag
GALAXY
HIGH REDSHIFT GALAXY
J2000
J2000
J = 25-27 AB mag
GALAXY
HIGH REDSHIFT GALAXY
J2000
J2000
J = 25-27 AB mag
GALAXY
HIGH REDSHIFT GALAXY
J2000
J2000
J = 25-27 AB mag
WFC3/IR
Imaging
No
No
F125W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F125W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F125W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F125W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F125W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F125W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F125W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F125W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F125W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F125W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F125W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F125W
WFC3/IR
Imaging
No
No
F160W
POS-TARG
DITHER
0.572
LINE
0.365
false
false
74.653
4
18.528
WFC3-IR-DITHER-BOX-MIN
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:visit-id "10"
:obset-id "10"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 12616
:visit-id "10"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2840
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3257
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 12616
:visit-id "10"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2840
:al-overhead-at-end 0
:internal-dur-at-end 540
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3257
:pcs-gap 0
)
false
2
0
The scheduling data was generated by CASM 19.3.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 12616
:visit-id "11"
:proposal-version -1
:trans-version "20110509"
:date "30-Jun-2011 09:37:49.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 2089056
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 12616
:visit-id "11"
:obset-id "11"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 12616
:visit-id "11"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2840
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3257
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 12616
:visit-id "11"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2840
:al-overhead-at-end 0
:internal-dur-at-end 540
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3257
:pcs-gap 0
)
true
2
0
The scheduling data was generated by CASM 19.3.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 12616
:visit-id "12"
:proposal-version -1
:trans-version "20110509"
:date "30-Jun-2011 09:38:25.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 2089056
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 12616
:visit-id "12"
:obset-id "12"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 12616
:visit-id "12"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2840
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3257
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 12616
:visit-id "12"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2840
:al-overhead-at-end 0
:internal-dur-at-end 540
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3257
:pcs-gap 0
)
true
2
0