0
Assigned ID: 912
----- Attempting Submission 1 (Fri Apr 08 22:19:03 GMT 2016) -----
HST Phase I Proposal 912 (hst_wfc3_f140_q2343_c24.apt) successfully submitted.
Receipt: # 912-1
----- Attempting Submission 2 (Fri Apr 08 23:42:18 GMT 2016) -----
HST Phase I Proposal 912 (hst_wfc3_f140_q2343_c24_10point.apt) successfully submitted.
Receipt: # 912-2
----- Attempting Submission 3 (Fri Apr 08 23:54:01 GMT 2016) -----
HST Phase I Proposal 912 (hst_wfc3_f140_q2343_c24_10point.apt) successfully submitted.
Receipt: # 912-3
----- Attempting Submission 4 (Fri Apr 08 23:56:36 GMT 2016) -----
0
PATTERN POSITION OUTSIDE APERTURE
Be very careful mixing POS TARG and Center_Pattern = Yes
PATTERN POSITION OUTSIDE APERTURE
Be very careful mixing POS TARG and Center_Pattern = Yes
PATTERN POSITION OUTSIDE APERTURE
Be very careful mixing POS TARG and Center_Pattern = Yes
PATTERN POSITION OUTSIDE APERTURE
Be very careful mixing POS TARG and Center_Pattern = Yes
Be very careful mixing POS TARG and Center_Pattern = Yes
Be very careful mixing POS TARG and Center_Pattern = Yes
PATTERN POSITION OUTSIDE APERTURE
Be very careful mixing POS TARG and Center_Pattern = Yes
PATTERN POSITION OUTSIDE APERTURE
Be very careful mixing POS TARG and Center_Pattern = Yes
PATTERN POSITION OUTSIDE APERTURE
Be very careful mixing POS TARG and Center_Pattern = Yes
PATTERN POSITION OUTSIDE APERTURE
Be very careful mixing POS TARG and Center_Pattern = Yes
PATTERN POSITION OUTSIDE APERTURE
Be very careful mixing POS TARG and Center_Pattern = Yes
PATTERN POSITION OUTSIDE APERTURE
Be very careful mixing POS TARG and Center_Pattern = Yes
PATTERN POSITION OUTSIDE APERTURE
Be very careful mixing POS TARG and Center_Pattern = Yes
Be very careful mixing POS TARG and Center_Pattern = Yes
PATTERN POSITION OUTSIDE APERTURE
Be very careful mixing POS TARG and Center_Pattern = Yes
PATTERN POSITION OUTSIDE APERTURE
Be very careful mixing POS TARG and Center_Pattern = Yes
PATTERN POSITION OUTSIDE APERTURE
Be very careful mixing POS TARG and Center_Pattern = Yes
PATTERN POSITION OUTSIDE APERTURE
Be very careful mixing POS TARG and Center_Pattern = Yes
PATTERN POSITION OUTSIDE APERTURE
Be very careful mixing POS TARG and Center_Pattern = Yes
PATTERN POSITION OUTSIDE APERTURE
Be very careful mixing POS TARG and Center_Pattern = Yes
This version has new orients and POS Targs for Visits 12 and 15 based on guide star restrictions.
834533538
----- Attempting Submission 1 (Mon Jul 18 19:26:03 GMT 2016) -----
HST Phase II Proposal 14620 (c24_phase2_v1.apt) successfully submitted.
Receipt: # 14620-1
----- Attempting Submission 2 (Wed Jul 20 20:09:50 GMT 2016) -----
The warnings all relate to the mosaic layout, which includes several pointings outside the center aperture. I also used a POS TARG with Center_Pattern=Yes in order to dither the exposures at each mosaic pointing, which are centered away from the nominal target location.
QSO and Galaxy Growth Probed by Faint Lya-Emitters
We propose deep imaging of the stellar continuum of 84 faint Lyman-alpha-emitting galaxies (LAEs) surrounding a hyperluminous QSO at z=2.57. We have shown that these QSOs boost the Lyman-alpha emission of their nearby galaxies (a process known as fluorescence), allowing the direct characterization of the QSO ionizing field and the potential detection of galaxies independently of their stellar luminosities. However, the relative contributions of stellar and fluorescent Lyman-alpha emission are currently masked by the poorly-constrained stellar populations of these faint galaxies (R ~ 27; log(M*) ~ 8-9.5; L ~ 0.1 L*). Unlike typical broadband filters, the WFC3 F140W passband samples the stellar continuum at this redshift with minimal contamination by bright emission lines, and these wide-field images will allow us to map the stellar contribution to total luminosity out to large QSO-centric radii. Faint LAEs also exhibit characteristics that vastly expand the parameter space of galaxies selected by continuum colors alone: LAEs have weaker outflowing winds, less optically-thick gas, and a higher escape fraction of UV photons than continuum-selected galaxies. Robust measurements of the stellar masses and sizes of these galaxies are essential for understanding the efficiency and scaling of stellar feedback, star formation, and ionizing photon emission at low galaxy masses, and their morphologies will reveal how this feedback affects galaxy-scale structures and the observed anisotropic distributions of escaping gas and photons. Comparison to 182 continuum-selected galaxies (z~2-3) in the same field will reveal these properties as a function of stellar mass and galaxy structure.
We have proposed mosaiced imaging with the F140W filter, corresponding to rest-frame optical wavelengths ~4000 A at the typical redshift of our narrowband-selected LAEs (z = 2.57). Our objective is to obtain high-resolution images of the stellar continuum emission, so we request 4 dithered exposures at each pointing in order to maximize the sampling of the PSF and the resulting resolution. We have estimated that the typical LAE
in our sample has an AB magnitude H ~ 26.5 by stacking ground-based images of individual objects based on the location of their detected Ly-alpha emission. Previous deep imaging with WFC3/F160W in portions of the KBSS fields demonstrates that the typical sizes of the LAEs are 0.1-0.8" in diameter. In order to measure morphologies, we desire to reach S/N > 5 per 0.2" square region (~5x5 pixels), which requires ~5500 seconds divided into 4 four dithered exposures according to the HST/WFC3 ETC. Our field has a visibility of 54 minutes per orbit, so we request two orbits per pointing to fulfill these requirements. This exposure time is sufficient to set a 3-sigma limit of 28.15 mag (AB) for undetected point sources.
We request a total of 10 pointings to obtain a mosaic covering the entire field, including 84 LAEs and 182 LBGs. This request stems from a desire to 1) sample the full range of QSO-centric projected radii and ionizing field strengths, and 2) capture a census of the diverse LAE sizes, stellar masses, and morphologies in order to correlate these quantities with parameters derived from spectra and ground-based imaging. These requirements set our total request of 20 orbits.
Galaxies
Intergalactic Medium and Cosmology
12
false
false
false
false
false
0
0
0
0
0
false
SUPPORTED
CLUSTER OF GALAXIES
HIGH REDSHIFT CLUSTER
Foreground star H-band brightnesses are estimated from the 2MASS point source catalog.
J2000
J2000
Objects have Lya line fluxes ~1e-17 erg/s/cm^2 (not in band); continuum magnitudes are mAB ~ 26-27. Two foreground stars have H=12.0 and 12.9 (Vega).
WFC3/IR
Imaging
No
No
F140W
WFC3/IR
Imaging
No
No
F140W
WFC3/IR
Imaging
No
No
F140W
POS-TARG
DITHER
DITHER
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5.183
WFC3-IR-DITHER-LINE
false
true
0.636
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41.859
POS-TARG
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true
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Hst Same orient constraint links visits (11 13 14 16 17 18 19 20)
The scheduling data was generated by CASM 24.2.
CASM was run in Phase II mode.
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true
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Hst Same orient constraint links visits (11 13 14 16 17 18 19 20)
The scheduling data was generated by CASM 24.2.
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Hst Same orient constraint links visits (11 13 14 16 17 18 19 20)
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