WFC3 sample sequence changed from MIF to SPARS50
----- Attempting Submission 1 (Wed Jul 02 16:22:16 GMT 2008) -----
Phase II Proposal 11735 (lsdp2.apt) successfully submitted.
----- Attempting Submission 2 (Thu Jul 03 09:19:57 GMT 2008) -----
Phase II Proposal 11735 (lsdp2.apt) successfully submitted.
----- Attempting Submission 3 (Fri May 29 11:37:41 GMT 2009) -----
Assigned ID: 196
----- Attempting Submission 1 (Thu Mar 06 21:04:06 GMT 2008) -----
Phase I Proposal 196 (lsd.apt) successfully submitted.
----- Attempting Submission 2 (Fri Mar 07 14:41:52 GMT 2008) -----
Phase I Proposal 196 (lsd.apt) successfully submitted.
----- Attempting Submission 3 (Fri Mar 07 16:55:42 GMT 2008) -----
The LSD project: dynamics, merging and stellar populations of a sample of well-studied LBGs at z~3
A large observational effort with the ground-based ESO/VLT telescopes allowed us to obtain deep, spatially-resolved, near-IR spectra of complete sample of 11 Lyman-Break Galaxies at z~3.1. These observations were used to obtain, for the first time, the metallicity and the dynamical properties of a sample of objects that, albeit small, is representative of the total population of the LBGs.
We propose to use HST to obtain high-resolution optical and near-IR images of this sample of LBGs in order to study the broad-band morphology and the stellar light distribution of these galaxies. These images, exploiting the superior spatial resolution of HST images and the low-background : 1- will allow a precise measure of the dynamical mass from the velocity field derived with spectroscopy; 2- will permit a comparison of the distribution of star formation (from the line emission) with the underlying stellar population, and, 3- will be used to check if the complex velocity field and the multiple line-emitting regions detected in most targets can be ascribed to on-going mergers. This accurate study will shed light on a number of unsolved problems still affecting the knowledge of the LBGs.
We want to obtain rest-frame UV and optical images of a sample of galaxies at z~3.1.
Each galaxy will be observed with ACS/WFC in the F625W filter and with WFC3-IR with F160W. The filter F625W is preferred to the F775W filter requested during phase I as a slightly better sensitivity can be obtained.
In both cases, we will use the standard 4-position dither patter, with default values of spacing. All galaxies, except one, will require 1 orbit per instrument. For the faintest galaxy we split the 4 position dither into two orbits.
For the ACS observation, by using the ETC we estimated that 1 orbit (38 min each, assuming 53 minutes of orbits and overheads of 15 min) is enough to obtain S/N~30 within and aperture of 1"for 7 out of 8 of our targets, having Vega R-band
magnitudes between 23.0 and 24.3. Assuming a flat distribution of the light, this implies a S/N of 3-4 for each resolution element of 0.1"x0.1", which is adequate to obtain a reliable morphological study. Only one target, having R=24.8, requires 2 orbits to reach the same SNR. Two targets already have deep ACS or WFPC2 archive images, and will not be observed. As a consequence, the total number of requested orbits with ACS is 8.
The requested exposure time for WFC3-IR can be estimated with a reasonable approximation as the total, integrated H-band magnitude is known for most of the objects, and average R-H colors can be used for the remaining objects. The vega H-band magnitudes are between 21.7 and 22.5 for 10 out the 11 targets, while one object is fainter (H=22.9). In this case, a total S/N=30 within 1", corresponding to
S/N=5-6 per 0.2"x0.2" resolution element, is obtained in 1 orbit for the brighter objects, and 2 orbits for the faintest one.
COSMOLOGY
12
false
0.0
0.0
false
false
false
false
false
SUPPORTED
GALAXY
HIGH REDSHIFT GALAXY
R=23.9 z=3.104
J2000
22 17 19.2800
+00 15 44.70
J2000
GALAXY
HIGH REDSHIFT GALAXY
R=23.1,24.5 z=3.098,3.093
J2000
22 17 40.9200
+00 11 26.90
J2000
GALAXY
HIGH REDSHIFT GALAXY
R=24.9 z=3.117
J2000
22 17 47.0600
+00 04 25.70
J2000
GALAXY
HIGH REDSHIFT GALAXY
R=24.2 z=2.616
J2000
22 39 21.0800
+11 48 27.70
J2000
GALAXY
HIGH REDSHIFT GALAXY
R=24.1 z=3.240
J2000
03 04 35.0400
-00 11 18.30
J2000
GALAXY
HIGH REDSHIFT GALAXY
R=23.8 z=3.416
J2000
03 04 45.7000
-00 13 40.60
J2000
GALAXY
HIGH REDSHIFT GALAXY
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J2000
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-00 08 23.20
J2000
GALAXY
HIGH REDSHIFT GALAXY
R=23.5 z=3.285
J2000
22 17 30.8500
+00 12 51.00
J2000
GALAXY
HIGH REDSHIFT GALAXY
R=23.8,24.4 z=3.288,3.079
J2000
22 17 18.3000
+00 18 39.10
J2000
ACS/WFC
Imaging
No
No
F775W
WFC3/IR
Imaging
No
No
F160W
ACS/WFC
Imaging
No
No
F775W
WFC3/IR
Imaging
No
No
F160W
ACS/WFC
Imaging
No
No
F775W
WFC3/IR
Imaging
No
No
F160W
ACS/WFC
Imaging
No
No
F775W
WFC3/IR
Imaging
No
No
F160W
ACS/WFC
Imaging
No
No
F775W
WFC3/IR
Imaging
No
No
F160W
ACS/WFC
Imaging
No
No
F775W
WFC3/IR
Imaging
No
No
F160W
ACS/WFC
Imaging
No
No
F775W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F160W
POS-TARG
DITHER
0.265
LINE
0.187
false
false
69.05
4
20.67
ACS-WFC-DITHER-BOX
1
false
POS-TARG
DITHER
0.572
LINE
0.365
false
false
74.653
4
18.528
WFC3-IR-DITHER-BOX-MIN
2
false
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:internal-dur-at-end 349
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3236
:pcs-gap 0
)
true
2
0
The scheduling data was generated by CASM 17.2.
CASM was run in Phase II mode.
/private/tmp/OPVisit59047.xml
C5 WFC3
(Tic-Visit
:proposal-id 11735
:visit-id "L2"
:proposal-version -1
:trans-version "20090130"
:date "29-May-2009 13:34:41.0"
: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 1044528
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 11735
:visit-id "L2"
:obset-id "L2"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 11735
:visit-id "L2"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2710
: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 3236
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 11735
:visit-id "L2"
:orbit-number 2
:pcs-time 195
:si-vis-utilization 2710
:al-overhead-at-end 0
:internal-dur-at-end 231
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3236
:pcs-gap 0
)
true
2
0