0
Assigned ID: 179
----- Attempting Submission 1 (Thu Apr 09 09:13:04 GMT 2015) -----
HST Phase I Proposal 179 (qsopairs.apt) successfully submitted.
Receipt: # 179-1
----- Attempting Submission 2 (Fri Apr 10 16:30:07 GMT 2015) -----
HST Phase I Proposal 179 (qsopairs.apt) successfully submitted.
Receipt: # 179-2
----- Attempting Submission 3 (Fri Apr 10 17:03:48 GMT 2015) -----
We have added a CR_SPLIT in the direct image to mitigate the high density of CR hit in the direct images seen in the first two exposures taken. Exposure times have been adjusted accordingly to fill the available orbital time.
1760806441
----- Attempting Submission 1 (Wed Jul 22 11:51:31 GMT 2015) -----
----- Attempting Submission 2 (Thu Oct 01 16:37:45 GMT 2015) -----
Warnings refer to Phase 1 targets that have been replaced in Phase 2 and for which there is no corresponding visit.
First Measurement of the Small Scale Structure of Circumgalactic Gas via Grism Spectra of Close Quasar Pairs
In our current structure formation paradigm, the supply of cool gas in the circumgalactic medium (CGM) provides the primary fuel for galaxy formation. Hydrodynamic simulations predict that the cool CGM will self-shield, and hence be easily detectable in absorption as optically-thick Lyman limit systems (LLSs). Several decades of absorption line spectroscopy have established the abundance and properties of these LLSs, however their relationship to populations of galaxies and to our theoretical picture of structure formation remains a mystery. We propose to solve these puzzles with WFC3/G280 grism spectra of 55 quasar pairs at small separation, to simultaneously pierce LLSs with two sightlines at small impact parameters (10-500 kpc). This novel experiment will resolve the small-scale structure of optically thick gas in the CGM, and provide the first measurement of the two-point correlation function of LLS pairs. This new observable will place LLSs in the clustering hierarchy to finally determine their relationship to observed populations of distant galaxies. These efforts are complemented by existing ancillary ground-based spectroscopy, which reveals the kinematics of related metal-line absorption, providing unprecedented constraints on the infalling and outflowing gas kinematics around galaxies hosting LLSs. Our experiment will also provide new insights into the small-scale variations of metal enrichment in the halos of distant galaxies. Direct comparison to our state-of-the-art hydrodynamic simulations will provide a new quantitative test of the current galaxy formation picture, including galactic outflows and the existence of cold accretion.
This program will utilize the low-resolution grism spectroscopic mode of WFC3/UVIS on HST to obtain spectra of 55 close separation pairs of quasars at z~2-3. These spectra aim to reveal the small-scale structure of the circumgalactic medium (CGM) by measuring strong hydrogen absorption (Lyman limit systems, or LLS). The program will determine the presence of LLS by their characteristic strong absorption break feature in the spectra. Additionally, the program will produce a variety of stacked spectra to provide a new measurement of the spectral energy distribution of quasars between z~2-3. The program will also perform a survey of galaxies in the extended fields around the quasar pairs that the WFC3 data provides simultaneously with the quasar spectra.
For each target, we aim to acquire spectra for two quasars in the field, which are separated by angular separations between 1-20". Our observing strategy aims to observe each pair in a single visit. For each visit, one of the two members of the pair (generally the fainter one) will be positioned at the center of chip #2 by means of y-offset. The telescope roll angle will be constrained to lie within +/- 5 deg of the pair position angle, so that both quasars lie along the y-axis (orthogonal to the dispersion axis). Occasionally, however, the presence of other UV-bright sources aligned with the pair will require additional changes in the telescope roll angle (or y-offsets), to remove these sources from chip #2 or to avoid overlap of traces. Each visit will start with a direct image in the F300X filter, using the G280-REF aperture. The exposure time of 120s (240s for the faintest targets) is sufficient to image the targeted quasars with high SN (>20), avoiding at the same time saturation of the brightest sources. For the direct image, a postflash of 12e will be applied. Next, we will acquire 2 exposures (with CR-SPLIT = 2) with the G280 grism in the UVIS aperture. These two exposures will be of approximately 1200s each, with the exact length chosen to maximise the exposure time in one orbit.
QUASAR ABSORPTION LINES AND IGM
12
false
true
false
false
false
false
SUPPORTED
GALAXY
QUASAR
Lense: second image V = 19.80
HE0230-2130
J2000
J2000
GALAXY
QUASAR
Lense: second image V = 19.97
SDSSJ074653.03+440351.3
J2000
J2000
GALAXY
QUASAR
Lense: second image V = 19.95
SDSSJ1216+3529
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 19.40
Added in P2
J2000
GALAXY
QUASAR
Lense: second image V = 19.58
Q1017-207
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.94
Added in P2
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.50
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 18.72
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 18.23
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 18.68
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 19.99
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.62
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.58
Added in P2
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.35
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 19.97
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g=19.85
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.21
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 18.87
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.34
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.67
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 19.99
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 18.90
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.42
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 19.82
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.63
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 19.36
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 19.20
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 19.56
Added in P2
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.16
J2000
J2000
GALAXY
QUASAR
Quasar pair (maybe lense): second object g = 18.54
Added in P2
J2000
GALAXY
QUASAR
Quasar pair: second object g =20.13
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.31
Added in P2
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.11
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.62
Added in P2
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.52
Added in P2
J2000
GALAXY
QUASAR
Quasar pair: second object g = 18.92
Added in P2
J2000
GALAXY
QUASAR
Quasar pair: second image g = 19.88
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 19.82
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 19.15
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.67
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 18.94
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.44
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.29
Added in P2
J2000
GALAXY
QUASAR
Quasar pair: second object g = 19.40
Added in P2
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.06
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 19.37
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 19.35
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 19.93
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.37
Added in P2
J2000
GALAXY
QUASAR
Quasar pair: second object g = 19.10
Added in P2
J2000
GALAXY
QUASAR
Quasar pair: second object g = 19.29
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.57
Added in P2
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.36
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 19.87
J2000
J2000
GALAXY
QUASAR
Quasar pair: second object g = 20.25
J2000
J2000
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
WFC3/UVIS
Spectroscopic
No
No
G280
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
1448888172000
19.0
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true
1
0
Lock PA for lense
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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true
1
0
Lock PA for lense
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
1456658945000
223.84425446537819
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true
1
0
MR: PA change - to improve parallel lines? From 213-223 to 217-225
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
1459402504000
115.0
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:pcs-visibility 3218
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)
true
1
0
Observed at inclined angle to avoid overlap with nearby sources
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
1457800141000
43.0
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true
1
0
Lock PA for lense. Possible G star in the way [one beam safe].
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
1468501781000
105.0
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true
1
0
MR: PA change to avoid star u=21.55, g=1.60 from 83-93 and 263-273 to 95-105 and 275-285
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
1464432644000
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true
1
0
Object aligned is G5 star, which should not contribute to UV emission (WFC3UVIS.sp.718799)
To be safe, add small tilt from PA.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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true
1
0
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
1462809635000
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true
1
0
Object in SE with potential overlap - but more than 1/4 CCD so should be ok.
MR: Played with packing to maximize exposure time and still get visibility
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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:low-sky "N"
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)
true
1
0
Close separation - lock PA
Bright star off chip 2
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 14127
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:low-sky "N"
:pcs-visibility 3307
:pcs-gap 0
)
true
1
0
Bright G star nearby - should be ok with current angle (5 deg tilt from PA).
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
(Tic-Visit
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(Tic-Orbit
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:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3403
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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140.0
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(Tic-Orbit
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:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
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)
true
1
0
Observed off PA for increased scheduling
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
(Tic-Visit
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:max-dark-utilization 1920
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)
true
1
0
Observed off PA to avoid overlap with F star of comparable magnitude
MR: PA change to avoid Star (u=25,g=22) and galaxy (u=24, g=22.45). From 275-280 and 95-100 to 218-228 with slightly less packed orbit for visibility.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
(Tic-Visit
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(Tic-Orbit
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:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3229
:pcs-gap 0
)
true
1
0
Overlapping object u > 25 mag
MR: PA change from 226-236 to 220-226 to avoid galaxy u=24 g=22. Reduces visibility to 11 days in 2017.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
(Tic-Visit
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(Tic-Orbit
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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"
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:pcs-gap 0
)
true
1
0
Lock PA to maximise separation
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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(Tic-Orbit
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3213
:pcs-gap 0
)
true
1
0
Lock PA to avoid overlap with bright G star
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
(Tic-Visit
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:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3267
:pcs-gap 0
)
true
1
0
MR: PA increase to 195-220 to increase visibility
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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(Tic-Visit
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(Tic-Obset
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(Tic-Orbit
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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 3229
:pcs-gap 0
)
true
1
0
MR: PA change from 222-232 to 222-250 to increase visibility.
MF: Stop at 244 to avoid galaxies in NE.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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(Tic-Orbit
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:pcs-time 241
:si-vis-utilization 2988
: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 3229
:pcs-gap 0
)
true
1
0
Tilt to avoid nearby red object
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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270.0
(Tic-Visit
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:number-of-orbits 1
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:data-volume 1154976
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(Tic-Obset
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)
(Tic-Orbit
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:pcs-time 333
:si-vis-utilization 2934
: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 3267
: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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(Tic-Obset
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(Tic-Orbit
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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
Tilt angle for better scheduling and minimise overlap
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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(Tic-Visit
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(Tic-Obset
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(Tic-Orbit
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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 3229
:pcs-gap 0
)
true
1
0
Tweaked angle from PA position to avoid overlap with nearby K star
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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140.0
(Tic-Visit
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(Tic-Obset
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(Tic-Orbit
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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 3229
:pcs-gap 0
)
true
1
0
MR: PA change to avoid star (u=24.7, g=23.20) from 174-184 and 354-4 to 135-145 and 315-325. Significant increase in visibility too.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
1450318577000
65.0
(Tic-Visit
:proposal-id 14127
:visit-id "25"
:proposal-version -1
:trans-version "20150609"
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:number-of-orbits 1
:saa-model "29"
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:data-volume 1154976
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)
(Tic-Obset
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:obset-id "25"
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)
(Tic-Orbit
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:orbit-number 1
:pcs-time 333
: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
Bright star is G5V - no saturation (WFC3UVIS.im.718810)
Object potentially aligned is K0V star, with low flux below 4000A (WFC3UVIS.sp.718811), but best observed at titled angle (65 deg)
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
(Tic-Visit
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:data-volume 1154976
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)
(Tic-Obset
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:obset-id "26"
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(Tic-Orbit
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:orbit-number 1
:pcs-time 333
:si-vis-utilization 3122
: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 3456
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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:data-volume 1154976
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(Tic-Obset
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)
(Tic-Orbit
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:pcs-time 333
: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
Two bright stars in the field, but not overlapping in X or Y
MR: y offset to -83 from -50 to avoid bright star.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
(Tic-Visit
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)
(Tic-Orbit
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:pcs-time 333
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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 3218
:pcs-gap 0
)
true
1
0
Lock PA to void overlap - nearby source is red
MR: PA change from 292 to 280-282 to avoid a red star, slight decreasing qso separation
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
Removed from "on hold" on Aug 17 2015.
(Tic-Visit
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(Tic-Obset
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)
(Tic-Orbit
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3267
:pcs-gap 0
)
true
1
0
Overlapping object u = 26 mag. Tilted PA to minimise that.
MR: PA change from 105-115, 285-295 to 88-92 and 268-272
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
1461250522000
200.0
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Tilt/lock angle to avoid red sources in the south. Nearby red galaxy.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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The scheduling data was generated by CASM 23.2.
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MR: Added PA range from 230-240 to 230-250 to increase visibility. Even with this change, still can't pack the orbits. I think this increase is ok.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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Do not pack orbit for visibility
MR: Increased PA range from 172-182 to 165-182, increasing visibility from 6 to 9 days.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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MR: Increased PA range from 191-201 to 191-211. Increased visibility from 3 days to 11 days. Nothing we can do about faint star nearby. u-band of 23.42, so it should be ok.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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Observe at angle for scheduling
MR: Increased PA range from 150-160 to 140-160, to increase visibility from 4 days to 14 days. New PA range does not overlap other targets.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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Observe at angle for overlap with bright source and scheduling
Do not pack orbit
MR: Increased PA range from 210-220 to 210-223 to increase visibility from 4 days to 18 days. New PA does not cause overlap with bright object which is constraining.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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Overlapping object is very red (u > 24 mag)
The scheduling data was generated by CASM 24.2.
CASM was run in Phase II mode.
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Lock PA to avoid bright star and red galaxy
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Y-offset to -35 from -50 to avoid bright stars.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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Roll angle offset from PA to avoid overlap with F star
MR: PA change from 148-158 to 140-150 to avoid another star and increase visibility (second one less important).
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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Alinged target G5V star V = 20.3 with low flux below 4000A (WFC3UVIS.sp.718840)
MR: PA change from 144-154 and 324-334 to 153-163 and 333-343 to avoid u=23.47 and g=21.82 mag star nearby.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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Tilt angle to avoid overlap with two (red) nearby sources
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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Specific PA needed for overlap
MR: y-offset to -38 from -50 to avoid bright star
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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MR: PA change to avoid nearby galaxy u=24.37 g=21.52. OK that stars ruin the -1 trace. From 63 to 42-45. Would do smaller PA, but no visibility.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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Overlapping objects are very red (u > 25)
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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MR: PA change to avoid u=22.52 g=22.37 galaxy and u=22.78 g=22.32. galaxy. First galaxy between two QSOs otherwise can't avoid other galaxy (Would prefer 148-158, but no visibility). From 138-148 and 318-328 to 130-134 and 310-314.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
(Tic-Visit
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(Tic-Orbit
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:al-overhead-at-end 116
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3218
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true
1
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Do not pack orbit for visibility
MR: PA change to avoid u=22.4, g=21.86 galaxy. From PA of 163-175 to PA 143-153
MR: Changed pack a little with decent visibility.
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
(Tic-Visit
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(Tic-Orbit
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:orbit-number 1
:pcs-time 333
:si-vis-utilization 3144
: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 3478
:pcs-gap 0
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true
1
0
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
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117.0
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:orbit-number 1
:pcs-time 333
:si-vis-utilization 2912
: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 3245
:pcs-gap 0
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true
1
0
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
1456632817000
188.99999999999994
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:low-sky "N"
:pcs-visibility 3556
:pcs-gap 0
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true
1
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MR: y-offset to avoid bright star, from -50 to -70
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
Removed from "on hold" on Aug 17 2015.
(Tic-Visit
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:orbit-number 1
:pcs-time 333
: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
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Fix angle (off PA) to avoid overlap
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
(Tic-Visit
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(Tic-Orbit
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:orbit-number 1
:pcs-time 333
:si-vis-utilization 2896
: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 3229
:pcs-gap 0
)
true
1
0
Observed off of PA to avoid bright F star
The scheduling data was generated by CASM 23.2.
CASM was run in Phase II mode.
1460281640000
128.0
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:internal-dur-at-end 668
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:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3307
:pcs-gap 0
)
true
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