0
Assigned ID: 374
----- Attempting Submission 1 (Fri Apr 10 06:18:22 GMT 2015) -----
HST Phase I Proposal 374 (Cycle23_LAE_lens_apt.apt) successfully submitted.
Receipt: # 374-1
----- Attempting Submission 2 (Fri Apr 10 16:38:40 GMT 2015) -----
HST Phase I Proposal 374 (Cycle23_LAE_lens_apt.apt) successfully submitted.
Receipt: # 374-2
----- Attempting Submission 3 (Fri Apr 10 19:09:05 GMT 2015) -----
Changing to UVIS2-C1K1C-CTE aperture; everything else is the same.
-1029276332
----- Attempting Submission 1 (Thu Jul 16 22:07:04 GMT 2015) -----
----- Attempting Submission 2 (Thu Oct 29 19:43:42 GMT 2015) -----
Target confirmation tool hangs/crashes APT for me.
Quantifying Cold Dark Matter Substructure with a Qualitatively New Gravitational Lens Sample
We propose WFC3 UVIS imaging of a new sample of 21 gravitationally lensed Lyman-alpha emitting galaxies (LAEs) discovered within the million-galaxy spectroscopic database of the Baryon Oscillation Spectroscopic Survey (BOSS) of the third Sloan Digital Sky Survey (SDSS-III). These systems consist of massive galaxies at redshifts of approximately 0.55 strongly lensing LAEs at redshifts from 2 to 3. Monte Carlo simulation of our survey selection function indicates that these LAEs will all be strongly lensed and highly magnified. This represents the first statistically significant sample of strong galaxy-galaxy lenses with high-redshift LAEs as their background sources. Viewed in rest-frame far-UV continuum light with WFC3 imaging, these LAEs have much more compact sizes than the lower-redshift lensed galaxies discovered by previous surveys (few 100 parsec versus few kiloparsec). This compactness makes lensed LAEs an ideal probe of dark substructures within the halos of the lensing galaxies, through observable perturbations to the predictions of smooth lensing mass models. We will use the constraints from substructure lensing in this new sample to make the most precise experimental measurement yet of the mass function and overall abundance of sub-halos in galaxy-scale parent halos, which will test a fundamental and robust prediction of the Lambda-CDM model on subgalactic scales. We request zero proprietary period in order to make these important data available immediately to all scientists pursuing lensing measurements of dark-matter substructure.
Targets are relatively small. Each one is to be observed with one orbit of WFC3-UVIS imaging through the F606W filter.
For all observations, I want to center the target in one of the two WFC3-UVIS apertures and execute a 4-position dither box.
COSMOLOGY
0
false
false
false
false
SUPPORTED
GALAXY
GRAVITATIONAL LENS
J2000
J2000
i = 19.2
GALAXY
GRAVITATIONAL LENS
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J2000
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GALAXY
GRAVITATIONAL LENS
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J2000
i = 19.4
GALAXY
GRAVITATIONAL LENS
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J2000
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GALAXY
GRAVITATIONAL LENS
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J2000
i = 19.2
GALAXY
GRAVITATIONAL LENS
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GALAXY
GRAVITATIONAL LENS
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J2000
i = 20.5
GALAXY
GRAVITATIONAL LENS
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J2000
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GALAXY
GRAVITATIONAL LENS
J2000
J2000
i = 19.4
GALAXY
GRAVITATIONAL LENS
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J2000
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GALAXY
GRAVITATIONAL LENS
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J2000
i = 19.9
GALAXY
GRAVITATIONAL LENS
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J2000
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GALAXY
GRAVITATIONAL LENS
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J2000
i = 19.4
GALAXY
GRAVITATIONAL LENS
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J2000
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GALAXY
GRAVITATIONAL LENS
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J2000
i = 19.3
GALAXY
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GALAXY
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J2000
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GALAXY
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GALAXY
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J2000
i = 19.9
GALAXY
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J2000
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GALAXY
GRAVITATIONAL LENS
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J2000
i = 19.6
WFC3/UVIS
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F606W
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F606W
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F606W
WFC3/UVIS
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F606W
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F606W
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F606W
WFC3/UVIS
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F606W
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F606W
WFC3/UVIS
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F606W
WFC3/UVIS
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No
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F606W
WFC3/UVIS
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No
F606W
POS-TARG
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LINE
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:number-of-orbits 1
:saa-model "29"
:si-bright-earth-limb-angle 20.0
:data-volume 1154992
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14189
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)
(Tic-Orbit
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:orbit-number 1
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:si-vis-utilization 3016
:al-overhead-at-end 116
:internal-dur-at-end 668
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3352
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
(Tic-Visit
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:visit-id "18"
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:tdrss-contact-duration 0
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)
(Tic-Obset
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)
(Tic-Orbit
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:orbit-number 1
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:si-vis-utilization 2972
:al-overhead-at-end 116
:internal-dur-at-end 668
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3307
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 14189
:visit-id "19"
:proposal-version -1
:trans-version "20150609"
:date "29-Oct-2015 13:36:47.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "29"
:si-bright-earth-limb-angle 20.0
:data-volume 1154992
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14189
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)
(Tic-Orbit
:proposal-id 14189
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:orbit-number 1
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:si-vis-utilization 2884
:al-overhead-at-end 116
:internal-dur-at-end 668
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3218
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 14189
:visit-id "20"
:proposal-version -1
:trans-version "20150609"
:date "29-Oct-2015 13:36:47.0"
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:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "29"
:si-bright-earth-limb-angle 20.0
:data-volume 1154992
:tdrss-contact-duration 0
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)
(Tic-Obset
:proposal-id 14189
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:pcs-mode "FGS"
)
(Tic-Orbit
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:orbit-number 1
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:si-vis-utilization 2876
:al-overhead-at-end 116
:internal-dur-at-end 668
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3210
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 14189
:visit-id "21"
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:number-of-orbits 1
:saa-model "29"
:si-bright-earth-limb-angle 20.0
:data-volume 1154992
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 14189
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)
(Tic-Orbit
:proposal-id 14189
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:orbit-number 1
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:al-overhead-at-end 116
:internal-dur-at-end 668
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3210
:pcs-gap 0
)
true
1
0