0Assigned ID: 296
----- Attempting Submission 1 (Fri Aug 17 16:20:53 GMT 2018) -----
HST Phase I Proposal 296 (lahrs_mh5.apt) successfully submitted.
Receipt: # 296-1
----- Attempting Submission 2 (Fri Aug 17 17:28:18 GMT 2018) -----
HST Phase I Proposal 296 (lahrs_mh5.apt) successfully submitted.
Receipt: # 296-2
----- Attempting Submission 3 (Fri Aug 17 21:28:38 GMT 2018) -----POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.Resubmitting with some CENWAVE settings modified to avoid gain-sag regions, and FP-POS set to all and exposure times adjusted.170494646----- Attempting Submission 1 (Wed Dec 05 19:16:50 GMT 2018) -----
----- Attempting Submission 2 (Mon Aug 05 12:08:17 GMT 2019) -----
----- Attempting Submission 3 (Tue Aug 20 15:29:27 GMT 2019) -----All warnings occur for one of the following two reasons:
- there is POS-TARG issued for an ACS ramp filter. However the POS-TARGs are all small, and the shift in bandpass will not affect the observations.
- the targets are entered as 'extended' (because they are galaxies, and COS has calibration issues for extneded tartets. However the targets all lie at distances of ~1000 Mpc, and the targes will be extremely compact in the ultraviolet, and possibly completely unresolved even by HST.The Cosmic Evolution of Circumgalactic Gas and Lyman alpha HalosThe Lyman alpha emission line (Lya) has recently fulfilled its decades-old promise to map the distribution of atomic gas around high-z galaxies: large, extended Lya halos are routinely discovered, and statistical samples are emerging. Unfortunately, at z>2-3 where this is systematically possible, galaxies are too faint, and poorly resolved to be studied in much detail, and the origin of these halos remains elusive. In the low-z universe, where galaxies' properties can be determined with high precision, the UV capabilities of HST have also made a huge impact. Lya halos are also common here and shown to result from resonance scattering, but the reported sizes are very different: halos become 3-10 times smaller, which hints at the cosmic evolution of circumgalactic gas. Absorption studies, however, show that the low-z CGM is still thick with HI, so why do the Lya halos disappear?
Another possibility is that almost every low-z galaxy imaged in Lya to date is too nearby to properly measure the CGM. Taking advantage of the UV initiative, we therefore propose to obtain deep Lya images and spectra of a new low-z sample that is nearby enough for high resolution, high SNR studies, but distant enough to capture CGM scales and halo sizes comparable to high-z. We will quantify the Lya scattering scales, search for low-z gas inflows, and detailed radiation transfer modeling will constrain density and clumping of the circumgalactic gas. This optimized sample will provide the anchor point for cosmic evolution studies that is ~10 Gyr later than high-z surveys, and will shed light on the formation process of cold gas in galaxy halos that is theoretically still not well understood.This program will obtain imaging and spectroscopy of a sample of 7 galaxies.
Imaging will be taken in six filters:
- 2 in the ultraviolet with ACS/SBC in F150LP and F165LP. This totals 5 orbits per target, that are divided into 3 visits.
- 4 in the optical with WCS/WFC in F435W, F555W, F814W, and a narrowband ramp filter, either FR853N or FR782N. This totals 2 orbits, to be executed in one visit.
ACS/SBC ultraviolet imaging
=============
A relatively large dither pattern is designed, sampling a 7x7 arcsec approximate square with 9 grid points, to average over residual low-frequency phenomena in the flat-field. Each pointing also has an additional step to guarantee that the broken anode is adequately shifted. From these baseline positions in the dither pattern, an additional sub-pixel term is added, based upon the standard 3-point dither pattern, that should properly sample the narrow core of the PSF.
Important: each SBC visits should only be executed when the SBC has not been used in the last 24 hours, and the MAMA detector has been allowed to cool. This minimizes the dark current in the SBC image, and was mentioned as a Special Requirement of the Phase I proposal.
One target (#1 in our listing) has a single orbit of archival F150LP imaging (GO 11107) and is only imaged over 4 orbits. A different dithering strategy is used for this target, but adheres to the same philosophy.
ACS/WFC optical imaging
=============
The observations in 4 filters are packed into two orbits, using two exposures per filter.
This ramp filter (FR853N or FR782N) is selected depending on the redshift of the galaxy, and determines the WFC aperture (WFC1-IRAMP or WFC2-ORAMP). In turn, this selects the aperture used for the broadband optical imaging in order to minimize overheads.
Each galaxy is imaged using a small subpixel dither to better sample the PSF, which is implemented with POS-TARGs. This gives a warning for the ramp filters, but the POS-TARGs are small and should have negligible impact upon the bandpass centering.
COS/G160M ultraviolet spectroscopy
=============
Each galaxy is observed with COS/G160M for one orbit. This observation is designed to detect the redshifted Ly-alpha emission line, not the UV continuum.
Target acquisition is done with ACQ/IMAGE in the NUV, aiming for SNR=20 based upon GALEX NUV photometry and the (conservative) assumption that NUV emission follows the u-band morphology. The galaxies are all selected to be compact in SDSS u-band imaging, which also gives very precise astrometry (verified with 2MASS). Experience from other programs shows that ACQ/IMAGE will be successful.
FUV/G160M spectroscopy is performed in different CENWAVE settings in order to well center the Ly-alpha line on one of the detectors, depending upon the redshift of the target. CENWAVE=1611 or 1623 are used. Two FP-POS settings are selected for each observation to perform the required spectral dither.Galaxies and the IGM6falsefalsetruefalsefalsefalsefalseSUPPORTEDGALAXYSTARBURSTYESoriginal coordinats: 23 18 13.0008 -00 41 26.15CG1449J2000J2000log(L_FUV/Lsun) = 10.934410GALAXYSTARBURSTYESoriginal coordinates : 01 39 13.2106 +01 08 55.95CG4164J2000J2000log(L_FUV/Lsun) = 10.139153GALAXYSTARBURSTYESCG3033J2000J2000log(L_FUV/Lsun) = 9.850926GALAXYSTARBURSTYESold coordinates: 00 04 30.3319 -10 11 29.61CG3711J2000J2000log(L_FUV/Lsun) = 10.236029GALAXYSTARBURSTYESCG4873J2000J2000log(L_FUV/Lsun) = 10.617557GALAXYSTARBURSTYESoriginal coordinates: 01 56 55.7664 -01 01 16.64CG3782J2000J2000log(L_FUV/Lsun) = 10.725078GALAXYSTARBURSTYESoriginal coordinates : 23 53 35.5440 +02 31 50.22CG2399J2000J2000log(L_FUV/Lsun) = 10.068764ACS/SBCImagingNoNoF150LPACS/SBCImagingNoNoF165LPACS/WFCImagingNoNoF435WACS/WFCImagingNoNoF555WACS/WFCImagingNoNoF814WACS/WFCRampFilterNoNoFR853NCOS/FUVSpectroscopicNoNoG160M1611ACS/SBCImagingNoNoF150LPACS/SBCImagingNoNoF165LPACS/WFCImagingNoNoF435WACS/WFCImagingNoNoF555WACS/WFCImagingNoNoF814WACS/WFCRampFilterNoNoFR853NCOS/FUVSpectroscopicNoNoG160M1611ACS/SBCImagingNoNoF150LPACS/SBCImagingNoNoF165LPACS/WFCImagingNoNoF435WACS/WFCImagingNoNoF555WACS/WFCImagingNoNoF814WACS/WFCRampFilterNoNoFR853NCOS/FUVSpectroscopicNoNoG160M1611ACS/SBCImagingNoNoF150LPACS/SBCImagingNoNoF165LPACS/WFCImagingNoNoF435WACS/WFCImagingNoNoF555WACS/WFCImagingNoNoF814WACS/WFCRampFilterNoNoFR853NCOS/FUVSpectroscopicNoNoG160M1611ACS/SBCImagingNoNoF150LPACS/SBCImagingNoNoF165LPACS/WFCImagingNoNoF435WACS/WFCImagingNoNoF555WACS/WFCImagingNoNoF814WACS/WFCRampFilterNoNoFR853NCOS/FUVSpectroscopicNoNoG160M1611ACS/SBCImagingNoNoF150LPACS/SBCImagingNoNoF165LPACS/WFCImagingNoNoF435WACS/WFCImagingNoNoF555WACS/WFCImagingNoNoF814WACS/WFCRampFilterNoNoFR853NCOS/FUVSpectroscopicNoNoG160M1611ACS/SBCImagingNoNoF150LPACS/SBCImagingNoNoF165LPACS/WFCImagingNoNoF435WACS/WFCImagingNoNoF555WACS/WFCImagingNoNoF814WACS/WFCRampFilterNoNoFR853NCOS/FUVSpectroscopicNoNoG160M1611The scheduling data was generated by CASM 27.2.CASM was run in Phase II mode./Users/matthew/Dropbox/Proposals/HST26/LyaHalo/PII/OP-cache/resub_20190820-v11.xmlTarget 1
SBC visit 1 (2 orbits)
orbit 1 to collect F165LP data matching F150LP observations under GO 11107
orbit 2 to collect the remaining orbit of F150LP in a 4-corner dither
This visit should only be executed when the SBC has not been used in the last 24 hours, and the MAMA detector has been allowed to cool. This minimizes the dark current in the SBC image, and was mentioned as a Special Requirement at Phase I.(Tic-Visit
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SBC visit 2 (2 orbits)
collect 2 orbits of F165LP imaging, on a 4-corner dither
2 images per position, separated by gap clearance and subpix
This visit should only be executed when the SBC has not been used in the last 24 hours, and the MAMA detector has been allowed to cool. This minimizes the dark current in the SBC image, and was mentioned as a Special Requirement at Phase I.(Tic-Visit
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SBC visit 1 (1 orbit)
1 pointing in the center
This visit should only be executed when the SBC has not been used in the last 24 hours, and the MAMA detector has been allowed to cool. This minimizes the dark current in the SBC image, and was mentioned as a Special Requirement at Phase I.(Tic-Visit
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SBC visit 2 (2 orbits)
L-shape 4 pointings
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SBC visit 3 (2 orbits)
L-shape 4 pointings
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SBC visit 1 (1 orbit)
1 pointing in the center
This visit should only be executed when the SBC has not been used in the last 24 hours, and the MAMA detector has been allowed to cool. This minimizes the dark current in the SBC image, and was mentioned as a Special Requirement at Phase I.(Tic-Visit
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)true10The scheduling data was generated by CASM 27.2.CASM was run in Phase II mode./Users/matthew/Dropbox/Proposals/HST26/LyaHalo/PII/OP-cache/resub_20190820-v32.xmlTarget 3
SBC visit 2 (2 orbits)
L-shape 4 pointings
This visit should only be executed when the SBC has not been used in the last 24 hours, and the MAMA detector has been allowed to cool. This minimizes the dark current in the SBC image, and was mentioned as a Special Requirement at Phase I.(Tic-Visit
:proposal-id 15643
:visit-id "32"
:proposal-version -1
:trans-version "20190514"
:date "20-Aug-2019 16:12:53.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "28"
:si-bright-earth-limb-angle 20.0
:data-volume 148112
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15643
:visit-id "32"
:obset-id "32"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15643
:visit-id "32"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2809
: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 3142
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15643
:visit-id "32"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2839
:al-overhead-at-end 0
:internal-dur-at-end 198
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3142
:pcs-gap 0
)true20The scheduling data was generated by CASM 27.2.CASM was run in Phase II mode./Users/matthew/Dropbox/Proposals/HST26/LyaHalo/PII/OP-cache/resub_20190820-v33.xmlTarget 3
SBC visit 3 (2 orbits)
L-shape 4 pointings
This visit should only be executed when the SBC has not been used in the last 24 hours, and the MAMA detector has been allowed to cool. This minimizes the dark current in the SBC image, and was mentioned as a Special Requirement at Phase I.(Tic-Visit
:proposal-id 15643
:visit-id "33"
:proposal-version -1
:trans-version "20190514"
:date "20-Aug-2019 16:12:55.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "28"
:si-bright-earth-limb-angle 20.0
:data-volume 148112
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15643
:visit-id "33"
:obset-id "33"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15643
:visit-id "33"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2809
: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 3142
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15643
:visit-id "33"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2839
:al-overhead-at-end 0
:internal-dur-at-end 198
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3142
:pcs-gap 0
)true20The scheduling data was generated by CASM 27.2.CASM was run in Phase II mode./Users/matthew/Dropbox/Proposals/HST26/LyaHalo/PII/OP-cache/resub_20190820-v36.xml(Tic-Visit
:proposal-id 15643
:visit-id "36"
:proposal-version -1
:trans-version "20190514"
:date "20-Aug-2019 16:12:56.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "27"
:si-bright-earth-limb-angle 20.0
:data-volume 2273792
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15643
:visit-id "36"
:obset-id "36"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15643
:visit-id "36"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2809
: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 3142
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15643
:visit-id "36"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2840
:al-overhead-at-end 0
:internal-dur-at-end 347
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3142
:pcs-gap 0
)true20The scheduling data was generated by CASM 27.2.CASM was run in Phase II mode./Users/matthew/Dropbox/Proposals/HST26/LyaHalo/PII/OP-cache/resub_20190820-v39.xml(Tic-Visit
:proposal-id 15643
:visit-id "39"
:proposal-version -1
:trans-version "20190514"
:date "20-Aug-2019 16:12:26.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 52416
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15643
:visit-id "39"
:obset-id "39"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15643
:visit-id "39"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2748
:al-overhead-at-end 0
:internal-dur-at-end 331
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3142
:pcs-gap 0
)true10The scheduling data was generated by CASM 27.2.CASM was run in Phase II mode./Users/matthew/Dropbox/Proposals/HST26/LyaHalo/PII/OP-cache/resub_20190820-v41.xmlTarget 4
SBC visit 1 (1 orbit)
1 pointing in the center
This visit should only be executed when the SBC has not been used in the last 24 hours, and the MAMA detector has been allowed to cool. This minimizes the dark current in the SBC image, and was mentioned as a Special Requirement at Phase I.1565988383000268.5200240303502(Tic-Visit
:proposal-id 15643
:visit-id "41"
:proposal-version -1
:trans-version "20190514"
:date "20-Aug-2019 16:12:57.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "28"
:si-bright-earth-limb-angle 20.0
:data-volume 74064
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15643
:visit-id "41"
:obset-id "41"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15643
:visit-id "41"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2815
:al-overhead-at-end 0
:internal-dur-at-end 117
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3149
:pcs-gap 0
)true10The scheduling data was generated by CASM 27.2.CASM was run in Phase II mode./Users/matthew/Dropbox/Proposals/HST26/LyaHalo/PII/OP-cache/resub_20190820-v42.xmlTarget 4
SBC visit 2 (2 orbits)
L-shape 4 pointings
This visit should only be executed when the SBC has not been used in the last 24 hours, and the MAMA detector has been allowed to cool. This minimizes the dark current in the SBC image, and was mentioned as a Special Requirement at Phase I.(Tic-Visit
:proposal-id 15643
:visit-id "42"
:proposal-version -1
:trans-version "20190514"
:date "20-Aug-2019 16:12:59.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "28"
:si-bright-earth-limb-angle 20.0
:data-volume 148112
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15643
:visit-id "42"
:obset-id "42"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15643
:visit-id "42"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2815
: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 3149
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15643
:visit-id "42"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2847
:al-overhead-at-end 0
:internal-dur-at-end 198
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3149
:pcs-gap 0
)true20The scheduling data was generated by CASM 27.2.CASM was run in Phase II mode./Users/matthew/Dropbox/Proposals/HST26/LyaHalo/PII/OP-cache/resub_20190820-v43.xmlTarget 4
SBC visit 3 (2 orbits)
L-shape 4 pointings
This visit should only be executed when the SBC has not been used in the last 24 hours, and the MAMA detector has been allowed to cool. This minimizes the dark current in the SBC image, and was mentioned as a Special Requirement at Phase I.(Tic-Visit
:proposal-id 15643
:visit-id "43"
:proposal-version -1
:trans-version "20190514"
:date "20-Aug-2019 16:13:00.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "28"
:si-bright-earth-limb-angle 20.0
:data-volume 148112
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15643
:visit-id "43"
:obset-id "43"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15643
:visit-id "43"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2815
: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 3149
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15643
:visit-id "43"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2847
:al-overhead-at-end 0
:internal-dur-at-end 198
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3149
:pcs-gap 0
)true20The scheduling data was generated by CASM 27.2.CASM was run in Phase II mode./Users/matthew/Dropbox/Proposals/HST26/LyaHalo/PII/OP-cache/resub_20190820-v46.xml(Tic-Visit
:proposal-id 15643
:visit-id "46"
:proposal-version -1
:trans-version "20190514"
:date "20-Aug-2019 16:13:02.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "27"
:si-bright-earth-limb-angle 20.0
:data-volume 2273792
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15643
:visit-id "46"
:obset-id "46"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15643
:visit-id "46"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2815
: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 3149
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15643
:visit-id "46"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2847
:al-overhead-at-end 0
:internal-dur-at-end 347
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3149
:pcs-gap 0
)true20The scheduling data was generated by CASM 27.2.CASM was run in Phase II mode./Users/matthew/Dropbox/Proposals/HST26/LyaHalo/PII/OP-cache/resub_20190820-v49.xml(Tic-Visit
:proposal-id 15643
:visit-id "49"
:proposal-version -1
:trans-version "20190514"
:date "20-Aug-2019 16:13:03.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 52416
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15643
:visit-id "49"
:obset-id "49"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15643
:visit-id "49"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2754
:al-overhead-at-end 0
:internal-dur-at-end 331
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3149
:pcs-gap 0
)true10The scheduling data was generated by CASM 27.2.CASM was run in Phase II mode./Users/matthew/Dropbox/Proposals/HST26/LyaHalo/PII/OP-cache/resub_20190820-v51.xmlTarget 5
SBC visit 1 (1 orbit)
1 pointing in the center
This visit should only be executed when the SBC has not been used in the last 24 hours, and the MAMA detector has been allowed to cool. This minimizes the dark current in the SBC image, and was mentioned as a Special Requirement at Phase I.(Tic-Visit
:proposal-id 15643
:visit-id "51"
:proposal-version -1
:trans-version "20190514"
:date "20-Aug-2019 16:13:03.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "28"
:si-bright-earth-limb-angle 20.0
:data-volume 74064
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15643
:visit-id "51"
:obset-id "51"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15643
:visit-id "51"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2809
:al-overhead-at-end 0
:internal-dur-at-end 117
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3142
:pcs-gap 0
)true10The scheduling data was generated by CASM 27.2.CASM was run in Phase II mode./Users/matthew/Dropbox/Proposals/HST26/LyaHalo/PII/OP-cache/resub_20190820-v52.xmlTarget 5
SBC visit 2 (2 orbits)
L-shape 4 pointings
This visit should only be executed when the SBC has not been used in the last 24 hours, and the MAMA detector has been allowed to cool. This minimizes the dark current in the SBC image, and was mentioned as a Special Requirement at Phase I.(Tic-Visit
:proposal-id 15643
:visit-id "52"
:proposal-version -1
:trans-version "20190514"
:date "20-Aug-2019 16:13:05.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "28"
:si-bright-earth-limb-angle 20.0
:data-volume 148112
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15643
:visit-id "52"
:obset-id "52"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15643
:visit-id "52"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2809
: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 3142
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15643
:visit-id "52"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2839
:al-overhead-at-end 0
:internal-dur-at-end 198
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3142
:pcs-gap 0
)true20The scheduling data was generated by CASM 27.2.CASM was run in Phase II mode./Users/matthew/Dropbox/Proposals/HST26/LyaHalo/PII/OP-cache/resub_20190820-v53.xmlTarget 5
SBC visit 3 (2 orbits)
L-shape 4 pointings
This visit should only be executed when the SBC has not been used in the last 24 hours, and the MAMA detector has been allowed to cool. This minimizes the dark current in the SBC image, and was mentioned as a Special Requirement at Phase I.(Tic-Visit
:proposal-id 15643
:visit-id "53"
:proposal-version -1
:trans-version "20190514"
:date "20-Aug-2019 16:13:06.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "28"
:si-bright-earth-limb-angle 20.0
:data-volume 148112
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15643
:visit-id "53"
:obset-id "53"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15643
:visit-id "53"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2809
: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 3142
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15643
:visit-id "53"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2839
:al-overhead-at-end 0
:internal-dur-at-end 198
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3142
:pcs-gap 0
)true20The scheduling data was generated by CASM 27.2.CASM was run in Phase II mode./Users/matthew/Dropbox/Proposals/HST26/LyaHalo/PII/OP-cache/resub_20190820-v56.xml(Tic-Visit
:proposal-id 15643
:visit-id "56"
:proposal-version -1
:trans-version "20190514"
:date "20-Aug-2019 16:13:07.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "27"
:si-bright-earth-limb-angle 20.0
:data-volume 2273792
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15643
:visit-id "56"
:obset-id "56"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15643
:visit-id "56"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2809
: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 3142
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15643
:visit-id "56"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2840
:al-overhead-at-end 0
:internal-dur-at-end 347
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3142
:pcs-gap 0
)true20The scheduling data was generated by CASM 27.2.CASM was run in Phase II mode./Users/matthew/Dropbox/Proposals/HST26/LyaHalo/PII/OP-cache/resub_20190820-v59.xml(Tic-Visit
:proposal-id 15643
:visit-id "59"
:proposal-version -1
:trans-version "20190514"
:date "20-Aug-2019 16:13:08.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 52416
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15643
:visit-id "59"
:obset-id "59"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15643
:visit-id "59"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2748
:al-overhead-at-end 0
:internal-dur-at-end 331
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3142
:pcs-gap 0
)true10The scheduling data was generated by CASM 27.2.CASM was run in Phase II mode./Users/matthew/Dropbox/Proposals/HST26/LyaHalo/PII/OP-cache/resub_20190820-v61.xmlTarget 6
SBC visit 1 (1 orbit)
1 pointing in the center
This visit should only be executed when the SBC has not been used in the last 24 hours, and the MAMA detector has been allowed to cool. This minimizes the dark current in the SBC image, and was mentioned as a Special Requirement at Phase I.(Tic-Visit
:proposal-id 15643
:visit-id "61"
:proposal-version -1
:trans-version "20190514"
:date "20-Aug-2019 16:13:09.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "28"
:si-bright-earth-limb-angle 20.0
:data-volume 74064
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15643
:visit-id "61"
:obset-id "61"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15643
:visit-id "61"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2809
:al-overhead-at-end 0
:internal-dur-at-end 117
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3142
:pcs-gap 0
)true10The scheduling data was generated by CASM 27.2.CASM was run in Phase II mode./Users/matthew/Dropbox/Proposals/HST26/LyaHalo/PII/OP-cache/resub_20190820-v62.xmlTarget 6
SBC visit 2 (2 orbits)
L-shape 4 pointings
This visit should only be executed when the SBC has not been used in the last 24 hours, and the MAMA detector has been allowed to cool. This minimizes the dark current in the SBC image, and was mentioned as a Special Requirement at Phase I.(Tic-Visit
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(Tic-Orbit
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SBC visit 3 (2 orbits)
L-shape 4 pointings
This visit should only be executed when the SBC has not been used in the last 24 hours, and the MAMA detector has been allowed to cool. This minimizes the dark current in the SBC image, and was mentioned as a Special Requirement at Phase I.(Tic-Visit
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(Tic-Obset
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(Tic-Orbit
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(Tic-Obset
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(Tic-Orbit
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(Tic-Obset
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(Tic-Orbit
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SBC visit 1 (1 orbit)
1 pointing in the center
This visit should only be executed when the SBC has not been used in the last 24 hours, and the MAMA detector has been allowed to cool. This minimizes the dark current in the SBC image, and was mentioned as a Special Requirement at Phase I.1565822385000242.68011499910972(Tic-Visit
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(Tic-Obset
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(Tic-Orbit
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SBC visit 2 (2 orbits)
L-shape 4 pointings
This visit should only be executed when the SBC has not been used in the last 24 hours, and the MAMA detector has been allowed to cool. This minimizes the dark current in the SBC image, and was mentioned as a Special Requirement at Phase I.(Tic-Visit
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(Tic-Orbit
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SBC visit 3 (2 orbits)
L-shape 4 pointings
This visit should only be executed when the SBC has not been used in the last 24 hours, and the MAMA detector has been allowed to cool. This minimizes the dark current in the SBC image, and was mentioned as a Special Requirement at Phase I.(Tic-Visit
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(Tic-Obset
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(Tic-Orbit
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(Tic-Obset
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(Tic-Orbit
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