Please find attached our Phase II submission for GO 11734.
Most of our visits are 3 orbits visits with either ACS/WFC or WFC3. For this purpose we use 2 exposures per orbit and have defined a new 6 point dither
pattern (essentially two line dithers). We believe that these patterns should be close to optimal for each instrument.
Finally, we have currently set the aperture as simply IR for the WFC3 observations. Depending on the initial post-installation (flat fields etc)
results we would like to move this aperture away from the amplifier boundry in an optimal way. However, if any of these targets are scheduled too
early in the cycle for this to be possible then we would simply introduce an arbitary 3" POS-TARG shift in each axis to ensure that our small
targets are not spread across the amplifier gap.
Many thanks!
use FGS3 on visit 2 -AV
----- Attempting Submission 1 (Thu Jul 03 14:52:14 GMT 2008) -----
----- Attempting Submission 2 (Mon Jul 07 17:43:31 GMT 2008) -----
A. J. Levan: z>3 GRB host galaxy imaging survey
Assigned ID: 626
----- Attempting Submission 1 (Fri Mar 07 21:51:56 GMT 2008) -----
Phase I Proposal 626 (hostnew.apt) successfully submitted.
----- Attempting Submission 2 (Fri Mar 07 22:28:17 GMT 2008) -----
The hosts of high redshift gamma-ray bursts
Gamma-ray bursts are the most luminous explosive events known, acting as beacons to the high redshift universe. Long duration GRBs have their origin in the collapse of massive stars and thus select star forming galaxies across a wide range of redshift. Due to their bright afterglows we can study the details of GRB host galaxies via absorption spectroscopy, providing redshifts, column densities and metallicities for galaxies far too faint to be accessible directly with current technology. We have already obtained deep ground based observations for many hosts and here propose ACS/WFC and WFC3 observations of the fields of bursts at z>3 which are undetected in deep ground based images. These observations will study the hosts in emission, providing luminosities and morphologies and will enable the construction of a sample of high-z galaxies with more detailed physical properties than has ever been possible before.
We will aim to obtain deep optical and nIR observations of a sample of high redshift (z>3, z_mean = 4, z_max = 5.5) GRB host galaxies with the aim of detecting hosts in emission for which detailed properties are known in absorption. The aim is to detect the host galaxies, and characterise the luminosities and morphologies.
Our standard observations will utilize a 3 orbit vist in either F814W (z<4) or F110W (z>4) for which we will use a 6 point dither pattern, obtaining two exposures in each orbit. We will offset the position of the target slightly from the apex of the WFC3 in order to avoid placing the target at the join of the amplifiers. These observations will allow us to reach 3-sigma limiting magnitudes of I~28.4, J~28.0.
For GRB 060927 we will undertake a 5 orbit observation, utlising a 4 point dither pattern and a 2-point sub-pattern. This will take 4 of the orbits, the final orbit will simply repeat two points of the pattern again.
COSMOLOGY
12
false
0.0
0.0
false
false
false
false
false
SUPPORTED
GALAXY
HIGH REDSHIFT GALAXY
R>26.5 (Vega)
J2000
03 40 49.5600
-17 07 48.40
J2000
GALAXY
HIGH REDSHIFT GALAXY
This object was generated by the targetselector and retrieved from the NED database.
R > 26.5 (Vega)
J2000
14 08 17.1000
-03 46 16.00
J2000
GALAXY
HIGH REDSHIFT GALAXY
This object was generated by the targetselector and retrieved from the NED database.
R ~ 27.5 (Vega)
J2000
01 21 50.8000
-12 57 18.00
J2000
GALAXY
HIGH REDSHIFT GALAXY
This object was generated by the targetselector and retrieved from the NED database.
R>27.0 (Vega)
J2000
03 36 8.2000
+17 20 44.00
J2000
GALAXY
HIGH REDSHIFT GALAXY
This object was generated by the targetselector and retrieved from the NED database.
R > 26.5 (Vega)
J2000
21 31 45.0000
+02 53 10.35
J2000
GALAXY
HIGH REDSHIFT GALAXY
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R > 26.5 (Vega)
J2000
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+00 17 5.00
J2000
GALAXY
HIGH REDSHIFT GALAXY
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R~27.0 (Vega)
J2000
21 28 37.3000
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J2000
GALAXY
HIGH REDSHIFT GALAXY
This object was generated by the targetselector and retrieved from the NED database.
H > 26 (AB)
J2000
21 58 11.9300
+05 21 50.32
J2000
GALAXY
HIGH REDSHIFT GALAXY
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J2000
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J2000
GALAXY
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J2000
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J2000
GALAXY
HIGH REDSHIFT GALAXY
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J2000
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J2000
WFC3/IR
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F110W
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F814W
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Imaging
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ACS/WFC
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ACS/WFC
Imaging
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No
F814W
ACS/WFC
Imaging
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ACS/WFC
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F814W
ACS/WFC
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POS-TARG
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POS-TARG
BOX
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POS-TARG
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WFC3-IR-DITHER-LINE
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The scheduling data was generated by CASM 17.2.
CASM was run in Phase II mode.
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