0Assigned ID: 2115
----- Attempting Submission 1 (Fri Apr 09 18:58:12 GMT 2021) -----For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more 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 generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more 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 generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more 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 generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Spectral_Element=G160M.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: G160M.
This attribute cannot have this value due to other choices: Aperture=PSA.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: PSA.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Optional_Parameter=FLASH=YES.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
YES is not a valid selection
YES is not a valid selection
This attribute cannot have this value due to other choices: Spectral_Element=G160M.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: G160M.
This attribute cannot have this value due to other choices: Aperture=PSA.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: PSA.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Optional_Parameter=FLASH=YES.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
YES is not a valid selection
YES is not a valid selection
This attribute cannot have this value due to other choices: Spectral_Element=G160M.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: G160M.
This attribute cannot have this value due to other choices: Aperture=PSA.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: PSA.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Optional_Parameter=FLASH=YES.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
YES is not a valid selection
YES is not a valid selection
This attribute cannot have this value due to other choices: Spectral_Element=G160M.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: G160M.
This attribute cannot have this value due to other choices: Aperture=PSA.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: PSA.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Optional_Parameter=FLASH=YES.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
YES is not a valid selection
YES is not a valid selection
For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M.
This attribute cannot have this value due to other choices: Spectral_Element=G160M.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: G160M.
This attribute cannot have this value due to other choices: Aperture=PSA.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: PSA.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Optional_Parameter=FLASH=YES.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
YES is not a valid selection
YES is not a valid selection
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more 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 generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M.
This attribute cannot have this value due to other choices: Spectral_Element=G160M.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: G160M.
This attribute cannot have this value due to other choices: Aperture=PSA.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: PSA.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Optional_Parameter=FLASH=YES.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
YES is not a valid selection
YES is not a valid selection
This attribute cannot have this value due to other choices: Spectral_Element=G160M.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: G160M.
This attribute cannot have this value due to other choices: Aperture=PSA.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: PSA.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Optional_Parameter=FLASH=YES.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
YES is not a valid selection
YES is not a valid selection
This attribute cannot have this value due to other choices: Spectral_Element=G160M.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: G160M.
This attribute cannot have this value due to other choices: Aperture=PSA.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: PSA.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Optional_Parameter=FLASH=YES.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
YES is not a valid selection
YES is not a valid selection
For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M.
This attribute cannot have this value due to other choices: Spectral_Element=G160M.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: G160M.
This attribute cannot have this value due to other choices: Aperture=PSA.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: PSA.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Optional_Parameter=FLASH=YES.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
YES is not a valid selection
YES is not a valid selection
This attribute cannot have this value due to other choices: Spectral_Element=G160M.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: G160M.
This attribute cannot have this value due to other choices: Aperture=PSA.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: PSA.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Optional_Parameter=FLASH=YES.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
YES is not a valid selection
YES is not a valid selection
This attribute cannot have this value due to other choices: Spectral_Element=G160M.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: G160M.
This attribute cannot have this value due to other choices: Aperture=PSA.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: PSA.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Optional_Parameter=FLASH=YES.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
YES is not a valid selection
YES is not a valid selection
For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M.
This attribute cannot have this value due to other choices: Spectral_Element=G160M.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: G160M.
This attribute cannot have this value due to other choices: Aperture=PSA.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: PSA.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Optional_Parameter=FLASH=YES.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
YES is not a valid selection
YES is not a valid selection
This attribute cannot have this value due to other choices: Spectral_Element=G160M.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: G160M.
This attribute cannot have this value due to other choices: Aperture=PSA.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: PSA.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Optional_Parameter=FLASH=YES.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
YES is not a valid selection
YES is not a valid selection
This attribute cannot have this value due to other choices: Spectral_Element=G160M.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: G160M.
This attribute cannot have this value due to other choices: Aperture=PSA.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: PSA.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Optional_Parameter=FLASH=YES.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
YES is not a valid selection
YES is not a valid selection
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 generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more 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 generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
A target acquisition should probably be performed before doing
spectroscopy or coronography with STIS or COS.
For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M.
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 generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M.
This attribute cannot have this value due to other choices: Spectral_Element=G160M.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: G160M.
This attribute cannot have this value due to other choices: Aperture=PSA.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: PSA.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Optional_Parameter=FLASH=YES.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
YES is not a valid selection
YES is not a valid selection
For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M.
This attribute cannot have this value due to other choices: Spectral_Element=G160M.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: G160M.
This attribute cannot have this value due to other choices: Aperture=PSA.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: PSA.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Optional_Parameter=FLASH=YES.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
YES is not a valid selection
YES is not a valid selection
This attribute cannot have this value due to other choices: Spectral_Element=G160M.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: G160M.
This attribute cannot have this value due to other choices: Aperture=PSA.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: PSA.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Optional_Parameter=FLASH=YES.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
YES is not a valid selection
YES is not a valid selection
This attribute cannot have this value due to other choices: Spectral_Element=G160M.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: G160M.
This attribute cannot have this value due to other choices: Aperture=PSA.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: PSA.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Optional_Parameter=FLASH=YES.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
YES is not a valid selection
YES is not a valid selection
For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M.
This attribute cannot have this value due to other choices: Spectral_Element=G160M.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: G160M.
This attribute cannot have this value due to other choices: Aperture=PSA.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
Illegal selection: PSA.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
This attribute cannot have this value due to other choices: Optional_Parameter=FLASH=YES.
FLASH=NO is the only permitted value for G160M PSA exposures (implied LIFETIME-POS LP6).
YES is not a valid selection
YES is not a valid selection
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.
COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details.08/10/2022: Resubmission after corrections of errors due tu APT update-493743288----- Attempting Submission 1 (Thu Jul 29 11:49:51 GMT 2021) -----
----- Attempting Submission 2 (Wed Nov 24 19:55:22 GMT 2021) -----
----- Attempting Submission 3 (Wed Dec 08 22:33:14 GMT 2021) -----
----- Attempting Submission 4 (Wed Dec 29 17:35:59 GMT 2021) -----
----- Attempting Submission 5 (Fri May 06 15:17:48 GMT 2022) -----
----- Attempting Submission 6 (Wed Aug 10 22:23:39 GMT 2022) -----Errors are for visits already completed.
Warnings have been noted.Mapping the escape of ionizing photons across the full ionizing continuum using high-resolution Lyman alpha and C IV observations.Ly-alpha (LyA) is the strongest feature in the rest-frame far-UV emission-line spectra of galaxies and our most reliable indicator of leaking ionizing photons. However, the intergalactic medium is increasingly neutral at higher redshifts, attenuating both ionizing and LyA emission from galaxies within the epoch of reionization (EoR). Additionally, LyA provides a limited tracer of the escaping ionizing radiation as it probes the low-ionization gas properties (close to the H-ionizing edge at 912 A, 13.6 eV), while the ionizing continuum peaks at significantly higher energies (500 A or 24.6 eV). Higher-energy photons significantly contribute to reionizing the neutral hydrogen as they can each ionize 2 H atoms, nevertheless, their escape-fraction is dramatically underestimated by the standard measurement of the ionizing photon escape at 900 A.
To map the escape of ionizing photons across the full ionizing continuum for the first time, we propose to combine archival and new HST/COS G130M+G160M observations of the LyA and C IV emission profiles of 10 nearby extreme UV emission-line galaxies. LyA and C IV probe different ionization stages (low and high, respectively) of the gas, and thus different energies of ionizing photons. Therefore, these high-resolution observations will enable us to determine the column densities of the low and high ionization gas, estimate the fraction of both low- and high-energy photons escaping EoR systems, and provide reliable diagnostics from emission line features observable in the early universe, which is critical for interpreting FUV emission-line features in forthcoming spectra of high-z galaxies with JWST.Goal:
We will obtain NUV target aquisition images and high-resolution, high signal-to-noise (6-7) HST/COS spectral observations of the Lyman-alpha and C IV emission profiles of 5 nearby extreme UV emission-line galaxies. We will combine these observations to 5 galaxies having archival COS high-resolution observations of LyA and C IV emision profiles to have a sample of 10 reionization-era analogues. This sample wiill enable us to connect the properties of low- and high-ionization gas derived from resonant Ly-alpha and C IV in the same galaxies for the first time, and thus constrain the dominant properties that control the escape of high-ionization photons in local reionization-era analogs. The latter is critical for interpreting FUV emission-line features in forthcoming spectra of high-z galaxies with JWST.
Targets:
Our targets were selected from previous HST/COS and SDSS observations. We selected galaxies having high-ionization zones using an emission-line based diagnostic based on the [Ar IV] 4711,4740 and [Ar III] 7135 high-ionization lines which probe the intermediate to very high ionization zones, and the C III] equivalent width to select targets with similar properties as high-redshift ones. Our final proposed sample is composed of 10 metal-poor reionization-era analogs with extreme ionization fields. Additionally, our galaxies are low redshift, compact, and FUV bright such that we will capture the majority of the FUV light in the COS 2.5" aperture.
Target Acquisition:
All five targets in our sample already have HST/COS low-resolution observations, providing very accurate coordinates. The excellent input coordinates of our sample allow us to utilize the ACQ/IMAGE mode for target acquisition with the PSA aperture and MirrorA for the COS/NUV configuration. We used the reported GALEX FUV magnitudes, converted to surface brighteness, to compute the exposure time needed for each galaxy for the target acquisition image. We added "Visit Orientation Requirements" for all targets based either on previous G140L observations (J222821, J133126, J094718, J082555) or G130M observations (J150924)
Science Exposures:
We used the COS ETC to determine the time needed to achieve S/N>6-7 per 100 km/s element in G130M and G160M. The ETC reported no warnings for violations of the local and/or global bright object limits. ETCs were based upon the continuum flux at 1500 AA (as measured from archival G140L observations). Our observing strategy complies fully with the COS2025 restrictions: all G130M observations will be performed with cenwave 1291 and use only the FP-POS 3 and 4. We note that J082555 already has G160M observations from the proposal HST-GO-15881. Nevertheless, we are using a different cenwave in our proposal (1611 versus 1533 previously) to observe the O III line doublet at 1666AA.Our team has substantial expertise in leading and analyzing COS UV spectroscopic observations of star-forming galaxies (Berg+16, Berg+19, Chisholm+15, Chisholm+16a,b, Chisholm+18, and more). Further, our team is composed of leaders in the study of galaxies that serve as reionization-era analogs, including Dawn Erb, John Chisholm, and Simon Gazagnes who have worked on higher redshifts galaxies, stellar feedback, LyA emission, and UV absorption lines. Additionally, Danielle Berg is an expert in studies of high-ionization UV emission lines in dwarf galaxies.
Importantly, Simon Gazagnes is one of the few astronomers in the world with experience in resonant line radiation transfer modeling, which is critical for the science proposed here.Galaxies6falsefalsetruefalsefalsefalsefalseSUPPORTEDGALAXYDWARF COMPACTYESJ2000J2000GALEX FUV = 18.86, SDSS r-band = 18.91GALAXYDWARF COMPACTYESJ2000J2000GALEX FUV = 18.68, SDSS r-band = 18.09GALAXYDWARF COMPACTSTARBURSTYESJ2000J2000GALEX FUV = 18.04, SDSS r-band = 17.18GALAXYDWARF COMPACTYESJ2000J2000GALEX FUV = 19.37, SDSS r-band = 17.38GALAXYDWARF COMPACTSTAR FORMING REGIONYESJ2000J2000GALEX FUV = 18.80, SDSS r-band = 17.70COS/FUVSpectroscopicNoNoG130M1291COS/FUVSpectroscopicNoNoG160M1611COS/FUVSpectroscopicNoNoG160M1577COS/FUVSpectroscopicNoNoG130M1291COS/FUVSpectroscopicNoNoG160M1533COS/FUVSpectroscopicNoNoG130M1291COS/FUVSpectroscopicNoNoG160M1533COS/FUVSpectroscopicNoNoG130M1291COS/FUVSpectroscopicNoNoG160M1533Hst Same orient constraint links visits (01 02 03 04)The scheduling data was generated by CASM 30.3.CASM was run in Phase II mode.167048853400065.33000000000001(Tic-Visit
:proposal-id 16643
:visit-id "01"
:proposal-version -1
:trans-version "20220516"
:date "10-Aug-2022 17:17:12.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 139296
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16643
:visit-id "01"
:obset-id "01"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16643
:visit-id "01"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2756
:al-overhead-at-end 0
:internal-dur-at-end 67
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3149
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16643
:visit-id "01"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2757
:al-overhead-at-end 0
:internal-dur-at-end 76
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3149
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16643
:visit-id "01"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2757
:al-overhead-at-end 0
:internal-dur-at-end 372
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3149
:pcs-gap 0
)false30Hst Same orient constraint links visits (01 02 03 04)The scheduling data was generated by CASM 30.3.CASM was run in Phase II mode.167194525400065.33000000000001(Tic-Visit
:proposal-id 16643
:visit-id "02"
:proposal-version -1
:trans-version "20220516"
:date "10-Aug-2022 17:17:14.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 87136
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16643
:visit-id "02"
:obset-id "02"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16643
:visit-id "02"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2756
:al-overhead-at-end 0
:internal-dur-at-end 38
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)true30Hst Same orient constraint links visits (08 09 10 14 Z0 Z8)The scheduling data was generated by CASM 30.3.CASM was run in Phase II mode.This HOPR grants the repeat of the second orbit for failed visit 08. This visit should only total 1 orbit.(Tic-Visit
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(Tic-Orbit
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)true30The scheduling data was generated by CASM 30.1.CASM was run in Phase II mode.165279380700097.74000000000001(Tic-Visit
:proposal-id 16643
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:trans-version "20211222"
:date "06-May-2022 10:14:33.0"
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)
(Tic-Obset
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)
(Tic-Orbit
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)
(Tic-Orbit
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)
(Tic-Orbit
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)true30