0Assigned ID: 455
----- Attempting Submission 1 (Fri Aug 17 22:43:18 GMT 2018) -----
HST Phase I Proposal 455 (HST_Cycle26_46P_v0.4.apt) successfully submitted.
Receipt: # 455-1
----- Attempting Submission 2 (Fri Aug 17 22:47:40 GMT 2018) -----
HST Phase I Proposal 455 (HST_Cycle26_46P_v0.4.apt) successfully submitted.
Receipt: # 455-2
----- Attempting Submission 3 (Fri Aug 17 23:24:01 GMT 2018) -----
HST Phase I Proposal 455 (HST_Cycle26_46P_v0.4.apt) successfully submitted.
Receipt: # 455-3
----- Attempting Submission 4 (Fri Aug 17 23:36:06 GMT 2018) -----For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.This is a preliminary version of Phase II that only includes two visits, one for STIS/MAMA and one for COS/MAMA. The purpose is to allow the CS to check the feasibility of tracking the fast moving target. Full Phase II will be developed with refined sequence later.
11/16/2018 update:
Full observing plan completed.
11/19/2018 update:
Break all multi-orbit visits to single-orbit visits.
single guide stars: 1-8, 17-20
single guide stars: 25-26, 28
12/07/2018 update:
Replace all FP-POS=1 and 2 to 3 and 4 for COS visits, per request by Will Fischer on 12/6/2018.
12/07/2018 update 2:
Change FP-POS for COS G130M CENWAVE=1096 visits to use all four points.
single guide stars 14-16
12/11/2018 update:
Update target orbital elements to JPL K181/10
12/13/2018 update:
Optimize FP-POS for COS G130M CENWAVE=1291 visits
Update target orbital elements to JPL K181/11
cut 40s from exp. 3, visit 2.
12/19/2018 update:
Update target orbital elements to JPL K181/151056239921----- Attempting Submission 1 (Wed Oct 31 19:19:01 GMT 2018) -----
HST Phase II Proposal 15625 (15625.apt) successfully submitted.
Receipt: # 15625-1
----- Attempting Submission 2 (Fri Nov 16 18:15:02 GMT 2018) -----
----- Attempting Submission 3 (Mon Nov 19 18:58:04 GMT 2018) -----
----- Attempting Submission 4 (Mon Nov 19 20:49:11 GMT 2018) -----
----- Attempting Submission 5 (Wed Dec 05 20:34:40 GMT 2018) -----
----- Attempting Submission 6 (Fri Dec 07 19:27:32 GMT 2018) -----
HST Phase II Proposal 15625 (15625_20181207.apt) successfully submitted.
Receipt: # 15625-6
----- Attempting Submission 7 (Sat Dec 08 02:38:57 GMT 2018) -----
----- Attempting Submission 8 (Mon Dec 10 13:45:09 GMT 2018) -----
----- Attempting Submission 9 (Wed Dec 12 03:32:44 GMT 2018) -----
----- Attempting Submission 11 (Thu Dec 13 15:56:19 GMT 2018) -----
----- Attempting Submission 12 (Thu Dec 13 17:56:29 GMT 2018) -----
----- Attempting Submission 13 (Wed Dec 19 19:15:20 GMT 2018) -----All warnings are about COS observations of extended objects. We are aware of the potential issues and don't consider them as problemetic.Composition and physical processes of the inner coma of Comet 46P/WirtanenComet 46P/Wirtanen passes Earth with an historic closest approach distance of 0.077 au (12 million km) on 16 Dec. 2018. Its apparition is widely anticipated by planetary scientists and is the target of an organized world-wide observing campaign. We request HST STIS and COS observations of comet 46P/Wirtanen to create a comprehensive picture of the comet. We will measure its chemical composition (including H2O, CO2, CO, O2, and S2), investigate its hyperactivity by mapping the gas distribution, and to use the comet as a natural laboratory to study plasma processes that affect the gas in its coma. The unique close proximity of 46P allows us to study the inner part of the coma (within 100 km of the nucleus), a region rarely accessible to remote observations. These observations will allow us to detect the emission of short-lived species (such as S2, O2), of molecules not accessible from the ground (CO2), and to investigate the transitions between regions where either electrons or photons drive most of the chemistry in the coma. Finally, studies of comet Wirtanen around the time of its close approach to Earth will have spatial resolutions high enough to permit valuable comparisons to the Rosetta observations of 67P/Churyumov-Gerasimenko and the Deep Impact/EPOXI fly-by results of 103P/Hartley 2.
HST's sensitivity and spectroscopic abilities in the Far Ultraviolet makes it uniquely capable to simultaneously measure the highly diagnostics FUV gas emission features in the coma. HST cycle 26 offers the rare opportunity to measure the spatial profiles of these emission features at very small distances from the nucleus due to the close approach of 46P at perihelion.1. Overall observational strategy
We plan to observe the comet in four instrument settings for three pointings each, making a total of 12 instrument-pointing combanation. The four instrument settings and their science goals are listed below:
- 4 orbits with the COS instrument and the G130M grating, center wavelength at 1096 A, to capture emission from the Lyman-beta hydrogen emission feature.
- 2 orbits with the COS instrument and the G130M grating, center wavelength at 1291 A, to capture dissociative electron impact emission from OI 1304 and 1356 A, as well as the CII 1335 A emission feature.
- 4 orbits with the STIS/FUVMAMA instrument/detector, the 52x0.5 aperture, and the G140L grating to measure CO Fourth Positive group emission features.
- 2 orbits with the STIS/FUVMAMA instrument/detector, the 52x0.5 aperture, and the G230L grating to measure OH emission features.
For each setting, we will repeat the observations for three pointings to study the 2D spatial distribution of various gas species:
P1 - the optocenter of the comet
P2 - 2.5" offset towards the Sun
P3 - 8" offset towards the Sun
We organize our observations in a total of 12 visits, with each visit for one instrument-pointing combanation listed above.
The science priority order for the instrument-pointing combination is:
1. COS G130M (1291) for P1 and P2
2. STIS G230L (2376) for P1 and P2
3. COS G130M (1096) for P1 and P2, and STIS G140L (1425) for P1 and P2
4. COS G130M (1096) and (1291), STIS G140L (1425) and STIS G230L (2376) for P3
The science priority grossly reflects the order of visits to be executed. There is no strong time link and/or restrictions between these orbits, as long as they are executed as close to each other as possible.
2. Comet position uncertainty and acquisition:
Assuming continuous collection of astrometric data of 46P with two nights of optical data every week at 1 arcsec uncertainty through December 23, we expect a worst case 3-sigma uncertainty range of 5" for the comet's sky position after January 7. This positional uncertainty puts the comet right into the acquisition box of STIS, and allow us to use 3x3 ACQ/SEARCH scheme for COS. The actual positional uncertainty could be smaller than the current prediction. We plan to update the comet's orbital elements two weeks before the observations, to confirm the ephemerides and adjust the search box of COS accordingly if needed.
3. Observing sequence
For STIS, each visit starts with an ACQ with CCD, then spectral observations with either G140L or G230L, and conclude by a CCD imaging in the end to confirm the observations and provide context.
For COS, each visit starts with an ACQ/SEARCH in the NUV with MIRROR A and search box 3x3, followed by an ACQ/IMAGE to confirm acquisition. The spectral observations will follow with the spectral element and central wavelength as selected. We will split each spectral observation to put in all four FP-POS.
The exposure time calculation is based on the corresponding ETC. All exposures have ETC IDs provided for reference.
4. Constraints
There is no specific time constraints to our observations, except to perform the observations as early as possible once the window opens on or about January 7, 2019. All visits do not have to be consecutive, although close in time would definitely benefit the interpretations of data.
We do not need to put constraints on the orientation of STIS slit, as the available slit orientation in our observing window will be near the center of the sun-comet line and the perpendicular direction. The three pointing offsets will allow us to map out the spatial distribution of species of interest serving our science goals.Solar System6falsefalsetruefalsefalsefalsefalseSUPPORTEDSOLAR SYSTEMYESCOMETComet 46P/WirtanenTYPE=COMET,Q=1.055378332381298,E=0.6587501255046055,I=11.74563830919623
,O=82.15500849791734,W=356.3583389334793,T=12-DEC-2018:22:38:18,TTimeScale=TDB,EQUINOX=J2000,EPOCH=14-JAN-2019:00:00:00,EpochTimeScale=TDB,A1=4.999982714653E-9,A2=-2.47746527195E-9,A3=1.160315871239E-9EARTHSOLAR SYSTEMYESCOMETComet 46P/WirtanenTYPE=COMET,Q=1.055378332381298,E=0.6587501255046055,I=11.74563830919623
,O=82.15500849791734,W=356.3583389334793,T=12-DEC-2018:22:38:18,TTimeScale=TDB,EQUINOX=J2000,EPOCH=14-JAN-2019:00:00:00,EpochTimeScale=TDB,A1=4.999982714653E-9,A2=-2.47746527195E-9,A3=1.160315871239E-9TYPE=POS_ANGLE,RAD=2.5,ANG=0,REF=SUNEARTHSOLAR SYSTEMYESCOMETComet 46P/WirtanenTYPE=COMET,Q=1.055378332381298,E=0.6587501255046055,I=11.74563830919623
,O=82.15500849791734,W=356.3583389334793,T=12-DEC-2018:22:38:18,TTimeScale=TDB,EQUINOX=J2000,EPOCH=14-JAN-2019:00:00:00,EpochTimeScale=TDB,A1=4.999982714653E-9,A2=-2.47746527195E-9,A3=1.160315871239E-9TYPE=POS_ANGLE,RAD=8,ANG=0,REF=SUNEARTHCOS/FUVSpectroscopicNoNoG130M1096COS/NUVImagingNoNoMIRRORACOS/FUVSpectroscopicNoNoG130M1291COS/NUVImagingNoNoMIRRORASTIS/FUV-MAMASpectroscopicNoNoG140L1425STIS/CCDImagingNoNoF28X50LPSTIS/NUV-MAMASpectroscopicNoNoG230L2376STIS/CCDImagingNoNoF28X50LPCOS/FUVSpectroscopicNoNoG130M1096COS/NUVImagingNoNoMIRRORACOS/FUVSpectroscopicNoNoG130M1291COS/NUVImagingNoNoMIRRORASTIS/FUV-MAMASpectroscopicNoNoG140L1425STIS/CCDImagingNoNoF28X50LPSTIS/NUV-MAMASpectroscopicNoNoG230L2376STIS/CCDImagingNoNoF28X50LPCOS/FUVSpectroscopicNoNoG130M1096COS/NUVImagingNoNoMIRRORACOS/FUVSpectroscopicNoNoG130M1291COS/NUVImagingNoNoMIRRORASTIS/FUV-MAMASpectroscopicNoNoG140L1425STIS/CCDImagingNoNoF28X50LPSTIS/NUV-MAMASpectroscopicNoNoG230L2376STIS/CCDImagingNoNoF28X50LPUsing ephemeris for target 15625-01-46P-WIRTANENephemeris data for target 15625-01-46P-WIRTANEN does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.OI 1304 & 1356, and CII 1335: COS, G130M, 1291 A, x2 orbits(Tic-Visit
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(Tic-Obset
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)false10Using ephemeris for target 15625-03-46P-WIRTANEN-OFFSET1ephemeris data for target 15625-03-46P-WIRTANEN-OFFSET1 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.OI 1304 & 1356, and CII 1335: COS, G130M, 1291 A, x2 orbits(Tic-Visit
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-09-46P-WIRTANENephemeris data for target 15625-09-46P-WIRTANEN does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.Lyman-beta emission: COS, G130M grating, 1096 A, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "09"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:40:54.0"
: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 43600
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "09"
:obset-id "09"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "09"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2800
:al-overhead-at-end 0
:internal-dur-at-end 350
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-10-46P-WIRTANENephemeris data for target 15625-10-46P-WIRTANEN does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.Lyman-beta emission: COS, G130M grating, 1096 A, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "10"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:40:55.0"
: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 43600
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "10"
:obset-id "10"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "10"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2800
:al-overhead-at-end 0
:internal-dur-at-end 350
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-11-46P-WIRTANENephemeris data for target 15625-11-46P-WIRTANEN does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.Lyman-beta emission: COS, G130M grating, 1096 A, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "11"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:40:55.0"
: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 43600
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "11"
:obset-id "11"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "11"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2800
:al-overhead-at-end 0
:internal-dur-at-end 350
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-12-46P-WIRTANENephemeris data for target 15625-12-46P-WIRTANEN does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.Lyman-beta emission: COS, G130M grating, 1096 A, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "12"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:40:56.0"
: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 43600
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "12"
:obset-id "12"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "12"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2800
:al-overhead-at-end 0
:internal-dur-at-end 350
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-13-46P-WIRTANEN-OFFSET1ephemeris data for target 15625-13-46P-WIRTANEN-OFFSET1 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.Lyman-beta emission: COS, G130M grating, 1096 A, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "13"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:40:57.0"
: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 43600
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "13"
:obset-id "13"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "13"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2800
:al-overhead-at-end 0
:internal-dur-at-end 350
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-14-46P-WIRTANEN-OFFSET1ephemeris data for target 15625-14-46P-WIRTANEN-OFFSET1 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.Lyman-beta emission: COS, G130M grating, 1096 A, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "14"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:40:57.0"
: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 43600
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "14"
:obset-id "14"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "14"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2800
:al-overhead-at-end 0
:internal-dur-at-end 350
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-15-46P-WIRTANEN-OFFSET1ephemeris data for target 15625-15-46P-WIRTANEN-OFFSET1 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.Lyman-beta emission: COS, G130M grating, 1096 A, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "15"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:40:58.0"
: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 43600
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "15"
:obset-id "15"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "15"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2800
:al-overhead-at-end 0
:internal-dur-at-end 350
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-16-46P-WIRTANEN-OFFSET1ephemeris data for target 15625-16-46P-WIRTANEN-OFFSET1 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.Lyman-beta emission: COS, G130M grating, 1096 A, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "16"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:40:58.0"
: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 43600
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "16"
:obset-id "16"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "16"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2800
:al-overhead-at-end 0
:internal-dur-at-end 350
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-17-46P-WIRTANENephemeris data for target 15625-17-46P-WIRTANEN does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.CO Forth Positive group emission: STIS/FUVMAMA, 52x0.5 slit, G140L grating, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "17"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:40:59.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 124208
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "17"
:obset-id "17"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "17"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2777
:al-overhead-at-end 0
:internal-dur-at-end 434
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-18-46P-WIRTANENephemeris data for target 15625-18-46P-WIRTANEN does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.CO Forth Positive group emission: STIS/FUVMAMA, 52x0.5 slit, G140L grating, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "18"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:41:00.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 124208
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "18"
:obset-id "18"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "18"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2777
:al-overhead-at-end 0
:internal-dur-at-end 434
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-19-46P-WIRTANENephemeris data for target 15625-19-46P-WIRTANEN does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.CO Forth Positive group emission: STIS/FUVMAMA, 52x0.5 slit, G140L grating, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "19"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:41:01.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 124208
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "19"
:obset-id "19"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "19"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2777
:al-overhead-at-end 0
:internal-dur-at-end 434
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-20-46P-WIRTANENephemeris data for target 15625-20-46P-WIRTANEN does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.CO Forth Positive group emission: STIS/FUVMAMA, 52x0.5 slit, G140L grating, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "20"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:41:02.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 124208
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "20"
:obset-id "20"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "20"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2777
:al-overhead-at-end 0
:internal-dur-at-end 434
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-21-46P-WIRTANEN-OFFSET1ephemeris data for target 15625-21-46P-WIRTANEN-OFFSET1 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.CO Forth Positive group emission: STIS/FUVMAMA, 52x0.5 slit, G140L grating, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "21"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:41:03.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 124208
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "21"
:obset-id "21"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "21"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2777
:al-overhead-at-end 0
:internal-dur-at-end 434
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-22-46P-WIRTANEN-OFFSET1ephemeris data for target 15625-22-46P-WIRTANEN-OFFSET1 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.CO Forth Positive group emission: STIS/FUVMAMA, 52x0.5 slit, G140L grating, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "22"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:41:03.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 124208
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "22"
:obset-id "22"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "22"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2777
:al-overhead-at-end 0
:internal-dur-at-end 434
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-23-46P-WIRTANEN-OFFSET1ephemeris data for target 15625-23-46P-WIRTANEN-OFFSET1 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.CO Forth Positive group emission: STIS/FUVMAMA, 52x0.5 slit, G140L grating, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "23"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:41:04.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 124208
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "23"
:obset-id "23"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "23"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2777
:al-overhead-at-end 0
:internal-dur-at-end 434
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-24-46P-WIRTANEN-OFFSET1ephemeris data for target 15625-24-46P-WIRTANEN-OFFSET1 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.CO Forth Positive group emission: STIS/FUVMAMA, 52x0.5 slit, G140L grating, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "24"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:41:05.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 124208
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "24"
:obset-id "24"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "24"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2777
:al-overhead-at-end 0
:internal-dur-at-end 434
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-25-46P-WIRTANEN-OFFSET2ephemeris data for target 15625-25-46P-WIRTANEN-OFFSET2 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.OI 1304 & 1356, and CII 1335: COS, G130M, 1291 A, x2 orbits(Tic-Visit
:proposal-id 15625
:visit-id "25"
:proposal-version -1
:trans-version "20181130"
:date "13-Dec-2018 10:53:39.0"
: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 52304
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "25"
:obset-id "25"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "25"
:orbit-number 1
:pcs-time 241
:si-vis-utilization 2880
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3142
:pcs-gap 0
)false10Using ephemeris for target 15625-26-46P-WIRTANEN-OFFSET2ephemeris data for target 15625-26-46P-WIRTANEN-OFFSET2 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.OI 1304 & 1356, and CII 1335: COS, G130M, 1291 A, x2 orbits(Tic-Visit
:proposal-id 15625
:visit-id "26"
:proposal-version -1
:trans-version "20181130"
:date "13-Dec-2018 10:53:36.0"
: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 52304
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "26"
:obset-id "26"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "26"
:orbit-number 1
:pcs-time 241
:si-vis-utilization 2880
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3142
:pcs-gap 0
)false10Using ephemeris for target 15625-27-46P-WIRTANEN-OFFSET2ephemeris data for target 15625-27-46P-WIRTANEN-OFFSET2 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.OH emission: STIS/FUVMAMA, 52x0.5 slit, G230L grating, x2 orbits(Tic-Visit
:proposal-id 15625
:visit-id "27"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:41:08.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 124208
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "27"
:obset-id "27"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "27"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2805
:al-overhead-at-end 0
:internal-dur-at-end 434
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-28-46P-WIRTANEN-OFFSET2ephemeris data for target 15625-28-46P-WIRTANEN-OFFSET2 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.OH emission: STIS/FUVMAMA, 52x0.5 slit, G230L grating, x2 orbits(Tic-Visit
:proposal-id 15625
:visit-id "28"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:41:09.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 124208
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "28"
:obset-id "28"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "28"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2805
:al-overhead-at-end 0
:internal-dur-at-end 434
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-29-46P-WIRTANEN-OFFSET2ephemeris data for target 15625-29-46P-WIRTANEN-OFFSET2 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.Lyman-beta emission: COS, G130M grating, 1096 A, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "29"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:41:10.0"
: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 43600
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "29"
:obset-id "29"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "29"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2800
:al-overhead-at-end 0
:internal-dur-at-end 350
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-30-46P-WIRTANEN-OFFSET2ephemeris data for target 15625-30-46P-WIRTANEN-OFFSET2 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.Lyman-beta emission: COS, G130M grating, 1096 A, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "30"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:41:11.0"
: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 43600
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "30"
:obset-id "30"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "30"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2800
:al-overhead-at-end 0
:internal-dur-at-end 350
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-31-46P-WIRTANEN-OFFSET2ephemeris data for target 15625-31-46P-WIRTANEN-OFFSET2 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.Lyman-beta emission: COS, G130M grating, 1096 A, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "31"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:41:12.0"
: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 43600
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "31"
:obset-id "31"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "31"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2800
:al-overhead-at-end 0
:internal-dur-at-end 350
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-32-46P-WIRTANEN-OFFSET2ephemeris data for target 15625-32-46P-WIRTANEN-OFFSET2 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.Lyman-beta emission: COS, G130M grating, 1096 A, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "32"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:41:12.0"
: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 43600
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "32"
:obset-id "32"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "32"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2800
:al-overhead-at-end 0
:internal-dur-at-end 350
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-33-46P-WIRTANEN-OFFSET2ephemeris data for target 15625-33-46P-WIRTANEN-OFFSET2 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.CO Forth Positive group emission: STIS/FUVMAMA, 52x0.5 slit, G140L grating, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "33"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:41:13.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 124208
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "33"
:obset-id "33"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "33"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2777
:al-overhead-at-end 0
:internal-dur-at-end 434
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-34-46P-WIRTANEN-OFFSET2ephemeris data for target 15625-34-46P-WIRTANEN-OFFSET2 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.CO Forth Positive group emission: STIS/FUVMAMA, 52x0.5 slit, G140L grating, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "34"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:41:14.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 124208
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "34"
:obset-id "34"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "34"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2777
:al-overhead-at-end 0
:internal-dur-at-end 434
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-35-46P-WIRTANEN-OFFSET2ephemeris data for target 15625-35-46P-WIRTANEN-OFFSET2 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.CO Forth Positive group emission: STIS/FUVMAMA, 52x0.5 slit, G140L grating, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "35"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:41:14.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 124208
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "35"
:obset-id "35"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "35"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2777
:al-overhead-at-end 0
:internal-dur-at-end 434
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10Using ephemeris for target 15625-36-46P-WIRTANEN-OFFSET2ephemeris data for target 15625-36-46P-WIRTANEN-OFFSET2 does not cover planning interval. Physical constraints are assumed to be unschedulable outside of the ephemeris data. Planning interval: 18.213 to 20.090. ephemeris interval: 18.304 to 20.306The scheduling data was generated by CASM 26.2.CASM was run in Phase II mode.CO Forth Positive group emission: STIS/FUVMAMA, 52x0.5 slit, G140L grating, x4 orbits(Tic-Visit
:proposal-id 15625
:visit-id "36"
:proposal-version -1
:trans-version "20180927"
:date "19-Nov-2018 13:41:15.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 124208
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15625
:visit-id "36"
:obset-id "36"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15625
:visit-id "36"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2777
:al-overhead-at-end 0
:internal-dur-at-end 434
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)false10