0Assigned ID: 720
----- Attempting Submission 1 (Fri Apr 07 18:38:44 GMT 2017) -----
HST Phase I Proposal 720 (filaments_c25.apt) successfully submitted.
Receipt: # 720-1For 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.
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.
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.
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.
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.
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.
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.
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.
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.
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.
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.Ignoring the "Inefficient ordering of FP-POS" warnings, following CS' advice.
Due to COS2025 policies, only FP-POS 3 and 4 are used for G130M/1291 grating.
BOT was performed using GALEX catalog.
10/19/17 Royle - Submitting on behalf of PI
07/26/18 - ROYLE
Added visit 65 as repeat of failed visit 15. No changes - exact duplicate-223628546----- Attempting Submission 1 (Thu Jul 20 02:23:30 GMT 2017) -----
----- Attempting Submission 2 (Thu Oct 19 19:55:59 GMT 2017) -----
----- Attempting Submission 3 (Thu Jul 26 13:02:33 GMT 2018) -----Ignoring the "Inefficient ordering of FP-POS" warnings, following CS' advice.
Due to COS2025 policies, only FP-POS 3 and 4 are used for G130M/1291 grating.Pinpointing the cosmic web between massive galaxy clustersWe propose to observe and characterize the intergalactic medium (IGM) in the densest filaments of the cosmic web at 0.1<z<0.5. We use massive galaxy cluster-pairs (M_cl > 1.3 10^14 M_sun) to identify zones where inter-cluster filaments should reside with high probabilities, and cross-matched them with bright UV QSOs for feasible FUV spectroscopy. Here we propose to observe the 9 best QSOs with HST/COS, in order to probe the HI and OVI transitions at the redshifts of 9 independent massive cluster-pairs within <3 Mpc from the inter-cluster axes. We require S/N>12 using the G130M (and G160M for those at z>0.16) to ensure a full characterization of low column density gas (N~10^13.0-13.5 cm^-2) in these intervening structures. This proposal builds upon our previous pilot programs from single targeted QSO sightlines intersecting multiple cluster-pairs (IDs 12958 and 13832, PI Tejos), which have led to promising results (Tejos et al. 2016). In particular, the present experiment will enable the detection of broad and shallow HI lines with OVI (if any), believed to be associated with portions of the warm-hot intergalactic medium (WHIM), as well as test alternative hypothesis regarding the origin of OVI lines. This proposal will double the current sample available in the HST archive, for a total of ~20 high-quality cluster-pairs probed. According to our estimations, this sample will provide a roboust statistical detection of the elusive WHIM signatures, at the 99% confidence level. Even more fundamentally, these data will provide a unique test of structure and galaxy formation by comparing them with state-of-the-art hydrodynamical simulations.We use galaxy cluster-pairs to identify and target the densest filaments in the "cosmic web". We cross-match these cluster-pairs with QSO positions, with the aim to probe the filamentary structures in absorption along the QSO sightlines (e.g. Tejos et al. 2016).
We used clusters from the redMaPPer catalog (Rykoff et al. 2014). Although the redMaPPer detection algorithm is mainly based on photometry, around 50% of these have spectroscopic redshifts from their Brightest Galaxy Cluster (BCG). We use the BCG spectroscopic redshift as the cluster redshift when available.
The QSOs were chosen from the combination of SDSS DR7 data (Schneider+2010), BOSS data (Paris+2012), and the UVQS survey (Monroe+2016) intersecting the SDSS volume, imposing a magnitude limit of FUV = 18.5 (AB). These comprise a large number of reliably identified QSOs with well known spectroscopic redshifts which are bright enough for FUV spectroscopy in relatively short exposure times each.
We constructed a sample of galaxy cluster-pairs satisfying the following criteria: (i) the redshift of the clusters must be 0.1 < z < 0.5; (ii) the minimum richness of the clusters must be 15 (which for redMaPPer roughly corresponds to ~ 1.3 x 10^{14} Msun); (iii) the maximum transverse separation between two clusters of a pair must be no larger than 15 Mpc; (iv) the redshift difference between the clusters of a pair has to be no larger than 1500 km/s; and (v) both clusters must have a spectroscopic redshift. These criteria are stricter than those used in Tejos+2016, in order to ensure a high fidelity in probing real filaments and thus minimize potential systematic uncertainties. Finally, for each cluster-pair we assign its redshift to be the average between the two cluster members.
We then cross-matched these cluster-pairs with our bright UV QSO list, imposing the following criteria: (i) the redshift of the QSOs must be larger than the redshift of the cluster-pair probed plus 3000 km/s from the QSOs systemic redshift (to avoid the proximity zone of the QSO); (ii) the QSO sightline must be within 3 Mpc from the inter-cluster axis; and (iii) the QSO sightline must be at a distance larger than 3 Mpc from the closest cluster of a pair, along the inter-cluster axis (to avoid zones close to individual galaxy clusters). For a given QSO, we counted the number of intervening cluster-pairs satisfying our criteria. When multiple cluster-pairs appeared in a given QSO, we grouped those lying within 1000 km/s from one another, and treated each of these final grouped structures as independent, n_ind, taking its redshift to be the average between its grouped cluster-pairs. Finally, for a given QSO with at least 1 independent cluster-pair, we calculated the
number of orbits, n_orb, needed to reach a signal-to-noise of S/N = 12 per resolution element, at the redshift of the known cluster-pairs for HI Lya and OVI, using the COS ETC (v25.1.1). We note that for cluster-pairs at 0.1 < z < 0.16, only G130M is needed to cover both species, and this fact was taken into account in our calculations. We then sorted the QSO list by n_ind/n_orb, and chose the required 9 most optimal QSOs for this project. We also made sure that none of our top priority QSOs showed strong intervening Mgii absorption that may compromise the quality of the FUV data due to the presence of a Lyman Limit System.
Note: the optimization strategy was done before the COS2025 policies were known to the community.Galaxies and the IGMCosmology6falsefalsetruefalsefalsefalsefalseSUPPORTEDGALAXYQSONOThis object was generated by the targetselector and retrieved from the SIMBAD database.J2000J2000FUV=17.41GALAXYQSONOThis object was generated by the targetselector and retrieved from the SIMBAD database.J2000J2000FUV=16.90GALAXYQSONOThis object was generated by the targetselector and retrieved from the SIMBAD database.J2000J2000FUV=17.60GALAXYQSONOThis object was generated by the targetselector and retrieved from the SIMBAD database.J2000J2000FUV=17.85GALAXYQSONOThis object was generated by the targetselector and retrieved from the SIMBAD database.J2000J2000FUV=18.07GALAXYQSONOThis object was generated by the targetselector and retrieved from the SIMBAD database.J2000J2000FUV=17.53GALAXYQSONOThis object was generated by the targetselector and retrieved from the SIMBAD database.J2000J2000FUV=17.51GALAXYQUASARNOThis object was generated by the targetselector and retrieved from the SIMBAD database.J2000J2000FUV=17.81GALAXYQSONOThis object was generated by the targetselector and retrieved from the SIMBAD database.J2000J2000FUV=17.96COS/FUVSpectroscopicNoNoG130M1291COS/FUVSpectroscopicNoNoG130M1327COS/FUVSpectroscopicNoNoG160M1577COS/FUVSpectroscopicNoNoG130M1318COS/FUVSpectroscopicNoNoG130M1291COS/FUVSpectroscopicNoNoG130M1327COS/FUVSpectroscopicNoNoG160M1577COS/FUVSpectroscopicNoNoG130M1318COS/FUVSpectroscopicNoNoG130M1318COS/FUVSpectroscopicNoNoG160M1577COS/FUVSpectroscopicNoNoG130M1327COS/FUVSpectroscopicNoNoG160M1600COS/FUVSpectroscopicNoNoG130M1291COS/FUVSpectroscopicNoNoG160M1623The scheduling data was generated by CASM 25.2.CASM was run in Phase II mode.This visit corresponds to the visit 1/1 of the J1456+2750 using G130M:
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:pcs-gap 0
)true40The scheduling data was generated by CASM 25.2.CASM was run in Phase II mode.This visit corresponds to the visit 2/2 of the J1216+1819 using G130M:
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- 2 segments A+B
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- Buffer times set to 2/3 of that given by the ETC(Tic-Visit
:proposal-id 15293
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:trans-version "20170613"
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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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)true40The scheduling data was generated by CASM 25.2.CASM was run in Phase II mode.This visit corresponds to the visit 1/1 of the J1358+0213 using G130M:
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- 1 central wavelengths 1291
- 2 segments A+B
- 2 FP-POS in total (COS2025 policy)
- Buffer times set to 2/3 of that given by the ETC1533355512000110.40780999999998(Tic-Visit
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:proposal-version -1
:trans-version "20170613"
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(Tic-Orbit
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(Tic-Orbit
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:dark-offset NIL
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:max-dark-utilization 1920
:low-sky "N"
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)true30The scheduling data was generated by CASM 25.2.CASM was run in Phase II mode.This visit corresponds to the visit 1/2 of the J1358+0213 using G160M:
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- 1 central wavelengths 1577
- 2 segments A+B
- 4 FP-POS in total
- Buffer times set to 2/3 of that given by the ETC(Tic-Visit
:proposal-id 15293
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:trans-version "20170613"
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:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:data-volume 95856
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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(Tic-Orbit
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(Tic-Orbit
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:dark-offset NIL
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:max-dark-utilization 1920
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)
(Tic-Orbit
:proposal-id 15293
:visit-id "10"
:orbit-number 3
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:si-vis-utilization 2979
:al-overhead-at-end 0
:internal-dur-at-end 341
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)true30The scheduling data was generated by CASM 25.2.CASM was run in Phase II mode.This visit corresponds to the visit 2/2 of the J1358+0213 using G160M:
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- 1 central wavelengths 1577
- 2 segments A+B
- 4 FP-POS in total
- Buffer times set to 2/3 of that given by the ETC1532995116000110.40780999999998(Tic-Visit
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:proposal-version -1
:trans-version "20170613"
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:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:number-of-orbits 2
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 69792
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15293
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:si-vis-utilization 2869
:al-overhead-at-end 0
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(Tic-Orbit
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)true20The scheduling data was generated by CASM 25.2.CASM was run in Phase II mode.This visit corresponds to the visit 1/1 of the J1210+0154 using G130M:
- 3 orbits in total
- 1 central wavelengths 1291
- 2 segments A+B
- 2 FP-POS in total (COS2025 policy)
- Buffer times set to 2/3 of that given by the ETC(Tic-Visit
:proposal-id 15293
:visit-id "11"
:proposal-version -1
:trans-version "20170613"
:date "18-Oct-2017 12:00:15.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:number-of-orbits 3
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 200192
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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:obset-id "11"
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)
(Tic-Orbit
:proposal-id 15293
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:si-vis-utilization 2869
:al-overhead-at-end 0
:internal-dur-at-end 86
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)
(Tic-Orbit
:proposal-id 15293
:visit-id "11"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2980
:al-overhead-at-end 0
:internal-dur-at-end 67
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:max-dark-utilization 1920
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)
(Tic-Orbit
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:si-vis-utilization 2980
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)true30The scheduling data was generated by CASM 25.2.CASM was run in Phase II mode.This visit corresponds to the visit 1/2 of the J1210+0154 using G160M:
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- 1 central wavelengths 1577
- 2 segments A+B
- 4 FP-POS in total
- Buffer times set to 2/3 of that given by the ETC(Tic-Visit
:proposal-id 15293
:visit-id "12"
:proposal-version -1
:trans-version "20170613"
:date "18-Oct-2017 12:00:19.0"
: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 104544
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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:obset-id "12"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15293
:visit-id "12"
:orbit-number 1
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:si-vis-utilization 2869
:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15293
:visit-id "12"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2980
:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15293
:visit-id "12"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 2979
:al-overhead-at-end 0
:internal-dur-at-end 341
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)true30The scheduling data was generated by CASM 25.2.CASM was run in Phase II mode.This visit corresponds to the visit 2/2 of the J1210+0154 using G160M:
- 3 orbits in total
- 1 central wavelengths 1577
- 2 segments A+B
- 4 FP-POS in total
- Buffer times set to 2/3 of that given by the ETC(Tic-Visit
:proposal-id 15293
:visit-id "13"
:proposal-version -1
:trans-version "20170613"
:date "18-Oct-2017 12:00:23.0"
: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 104544
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15293
:visit-id "13"
:obset-id "13"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15293
:visit-id "13"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2869
:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
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)
(Tic-Orbit
:proposal-id 15293
:visit-id "13"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2980
:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15293
:visit-id "13"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 2979
:al-overhead-at-end 0
:internal-dur-at-end 341
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3202
:pcs-gap 0
)true30The scheduling data was generated by CASM 25.2.CASM was run in Phase II mode.This visit corresponds to the visit 1/1 of the J1120+1104 using G130M:
- 4 orbits in total
- 1 central wavelengths 1222 (COS2025 policy; originally 1223, changed back to 1222 by STScI request)
- 2 segments A+B (COS2025 policy)
- 4 FP-POS in total
- Buffer times set to 2/3 of that given by the ETC1531209418000113.0(Tic-Visit
:proposal-id 15293
:visit-id "14"
:proposal-version -1
:trans-version "20170613"
:date "18-Oct-2017 11:58:50.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 4
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 121920
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15293
:visit-id "14"
:obset-id "14"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15293
:visit-id "14"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2876
:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
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:max-dark-utilization 1920
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:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15293
:visit-id "14"
:orbit-number 2
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:si-vis-utilization 2987
:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
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:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15293
:visit-id "14"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 2987
:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
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:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15293
:visit-id "14"
:orbit-number 4
:pcs-time 222
:si-vis-utilization 2987
: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 3209
:pcs-gap 0
)true40The scheduling data was generated by CASM 25.2.CASM was run in Phase II mode.This visit corresponds to the visit 1/2 of the J1120+1104 using G160M:
- 3 orbits in total
- 1 central wavelengths 1577
- 2 segments A+B
- 4 FP-POS in total
- Buffer times set to 2/3 of that given by the ETC1530065352000113.0(Tic-Visit
:proposal-id 15293
:visit-id "15"
:proposal-version -1
:trans-version "20170613"
:date "18-Oct-2017 12:00:28.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:number-of-orbits 3
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 95856
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15293
:visit-id "15"
:obset-id "15"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15293
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:orbit-number 1
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:si-vis-utilization 2876
:al-overhead-at-end 0
:internal-dur-at-end 48
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3209
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15293
:visit-id "15"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2987
:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3209
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15293
:visit-id "15"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 2987
:al-overhead-at-end 0
:internal-dur-at-end 341
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3209
:pcs-gap 0
)true30The scheduling data was generated by CASM 26.0.CASM was run in Phase II mode./private/var/folders/h2/_3b1kkv56nn2rfp1zrxtm0sc0006z1/T/OPVisit2491694688573169277.xmlThis visit corresponds to the visit 1/2 of the J1120+1104 using G160M:
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- 1 central wavelengths 1577
- 2 segments A+B
- 4 FP-POS in total
- Buffer times set to 2/3 of that given by the ETC(Tic-Visit
:proposal-id 15293
:visit-id "65"
:proposal-version -1
:trans-version "20180409"
:date "26-Jul-2018 08:58:23.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:number-of-orbits 3
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 95856
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15293
:visit-id "65"
:obset-id "65"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15293
:visit-id "65"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2870
:al-overhead-at-end 0
:internal-dur-at-end 48
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3209
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15293
:visit-id "65"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 2987
:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3209
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15293
:visit-id "65"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 2987
:al-overhead-at-end 0
:internal-dur-at-end 341
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3209
:pcs-gap 0
)true30The scheduling data was generated by CASM 25.2.CASM was run in Phase II mode.This visit corresponds to the visit 2/2 of the J1120+1104 using G160M:
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- 1 central wavelengths 1577
- 2 segments A+B
- 4 FP-POS in total
- Buffer times set to 2/3 of that given by the ETC1531558394000113.0(Tic-Visit
:proposal-id 15293
:visit-id "16"
:proposal-version -1
:trans-version "20170613"
:date "18-Oct-2017 12:00:32.0"
: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 95856
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 15293
:visit-id "16"
:obset-id "16"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 15293
:visit-id "16"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2876
:al-overhead-at-end 0
:internal-dur-at-end 48
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3209
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15293
:visit-id "16"
:orbit-number 2
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:si-vis-utilization 2987
:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3209
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 15293
:visit-id "16"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 2987
:al-overhead-at-end 0
:internal-dur-at-end 341
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3209
:pcs-gap 0
)true30The scheduling data was generated by CASM 25.2.CASM was run in Phase II mode.This visit corresponds to the visit 1/2 of the J1637+4254 using G130M:
- 2 orbits in total
- 1 central wavelengths 1291
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