0 Assigned ID: 1147 ----- Attempting Submission 1 (Fri Apr 07 23:43:57 GMT 2017) ----- HST Phase I Proposal 1147 (haro11cos.apt) failed submission. ----- Attempting Submission 2 (Fri Apr 07 23:45:46 GMT 2017) ----- HST Phase I Proposal 1147 (haro11cos.apt) failed submission. ----- Attempting Submission 3 (Sat Apr 08 00:03:59 GMT 2017) ----- HST Phase I Proposal 1147 (haro11cos.apt) failed submission. ----- Attempting Submission 4 (Sat Apr 08 00:15:04 GMT 2017) ----- HST Phase I Proposal 1147 (haro11cos.apt) failed submission. ----- Attempting Submission 5 (Sat Apr 08 00:17:36 GMT 2017) ----- HST Phase I Proposal 1147 (haro11cos.apt) failed submission. ----- Attempting Submission 6 (Sat Apr 08 00:18:26 GMT 2017) ----- HST Phase I Proposal 1147 (haro11cos.apt) successfully submitted. Receipt: # 1147-6 ----- Attempting Submission 7 (Sat Apr 08 01:16:29 GMT 2017) ----- HST Phase I Proposal 1147 (haro11cos.apt) successfully submitted. Receipt: # 1147-7 ----- Attempting Submission 8 (Sat Apr 08 01:21:00 GMT 2017) ----- HST Phase I Proposal 1147 (haro11cos.apt) successfully submitted. Receipt: # 1147-8 ----- Attempting Submission 9 (Sat Apr 08 01:22:16 GMT 2017) ----- HST Phase I Proposal 1147 (haro11cos.apt) successfully submitted. Receipt: # 1147-9 ----- Attempting Submission 10 (Sat Apr 08 05:22:02 GMT 2017) ----- HST Phase I Proposal 1147 (haro11cos.apt) successfully submitted. Receipt: # 1147-10 ----- Attempting Submission 11 (Sat Apr 08 05:23:49 GMT 2017) ----- HST Phase I Proposal 1147 (haro11cos.apt) successfully submitted. Receipt: # 1147-11 ----- Attempting Submission 12 (Mon Apr 10 14:57:18 GMT 2017) ----- HST Phase I Proposal 1147 (haro11cos.apt) successfully submitted. Receipt: # 1147-12 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. 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. 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. ORBITAL VISIBILITY OVERRUN 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. 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. 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. 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. 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. 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. 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. 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. 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. COS FUV PSA science exposures with extended targets have special calibration limitations. See "Errors and Warnings" for more details. resubmitting with visit 51 as HOPR repeat of second orbit of visit 50 that failed gs reacq -1392532110 ----- Attempting Submission 1 (Fri Jul 14 21:22:27 GMT 2017) ----- HST Phase II Proposal 15352 (haro11cos_mybackupwithnosplits.apt) successfully submitted. Receipt: # 15352-1 ----- Attempting Submission 2 (Sun Aug 06 21:35:48 GMT 2017) ----- ----- Attempting Submission 3 (Thu Nov 02 16:03:40 GMT 2017) ----- ----- Attempting Submission 4 (Mon Jul 30 21:45:29 GMT 2018) ----- ----- Attempting Submission 5 (Tue Jul 31 12:27:16 GMT 2018) ----- ----- Attempting Submission 6 (Wed Oct 03 20:07:18 GMT 2018) ----- ----- Attempting Submission 7 (Thu Dec 06 14:33:39 GMT 2018) ----- ----- Attempting Submission 8 (Wed Nov 06 22:47:50 GMT 2019) ----- BOT and ETC complains about COS/NUV acquisition on knot C. We have verified this is OK. Since only FP-POS=3&4 are available for G130M/1291 we combine with FP-POS=1&2 for G130M/1223. We do a similar split for G160M to allow all lines of interest to be included. All G130M spectra will be combined, as will the G160M hence the effective number of FP-POS is 4 per grating and pointing. Lyman alpha and ISM Tomography of Haro 11 The compact starburst Haro11 is one of the nearest Lyman break analogs and the closest galaxy with a confirmed leakage of Lyman continuum photons. It is also one of the nearest Lyman alpha emitting galaxies known. Haro11 has three bright emission knots (A,B and C). Knot C has previously been observed with COS. We have used absorption lines in these spectra to determine the covering fraction and velocity structure of the neutral and ionized gas along the line of sight, finding la wide range of outflow velocities and covering fractions, indicating the presence of an outflowing clumpy ISM. These are conditions that should be benign for the escape of Lyman continuum emission, but there are other observations suggesting that knot C may not be the cause of the Lyman continuum leakage: its ionization level is low, and there is no Lyman alpha at the systemic velocity which one would predict if Lyman continuum was escaping through a clumpy medium. We propose COS spectroscopy of the other two knots and two positions showing bright diffuse Lyman alpha emission. With multiple sightlines probing the ISM and Lyman alpha emission we can perform a spatially resolved tomographic study of the ISM and Lyman alpha emission in this key galaxy. By adding STIS spectroscopy, we propose to furthermore study these proceses at the finest scale offered by HST. This program consists of COS spectroscopy on knot A and B in Haro11 with G130M+G160M. Knot C has already this data in the archive. In addition, G130M spectroscopy will be obatined at one position north and one position south of knot C. For all COS visits, knot C is used for target acquisition, followed by offsets to the primary target. In addition, STIS spectroscopy will be obtained at two slit positions. One that runs through knot C in approximately N-S direction, and one approximately orthogonal that runs through knot C and also includes knot B. COS visits: knot-A: Acquisition on knot C, offset, followed by NUV image, followed by G130/1223 (FP-POS=1 & 2), 1291 (FP-POS 3 & 4) and G160/1577(FP-POS=2 & 3),1611 (FP-POS 3 & 4). knot-B: as for knot A Knot-C-offset positions: Acquisition on knot C, offset to N position, observations with G130M/1223 (1 & 2), 1291 (FP-POS 3 & 4); offset to S position, followed by G130M/1223 (1 & 2), 1291 (FP-POS 3 & 4) observations. The motivation for using two cenwaves with two FP-POS each is to maximise wavelength coverage (in order to capture all ISM absorption lines of interest). STIS visits: STIS-slit-1 and STIS-slit-2: acquisition on Knot-C followed by exposures in G430M (on 2 along-slit positions with 2 exposures each), G750M (on 2 along-slit positions with 2 exposures each), G130M (4 exposures at different along slit positions as defined by POS-TARGs in the Y-direction). All visits have individual orient constraints. For STIS the reason is obviously to achieve the correct slit position angle. For COS we have chosen the ORIENT in order to optimise the dispersion direction. To achive this, we have added 45 deg to the desired PA of the dispersion direction, as specified in the phase2 proposal instructions. Galaxies and the IGM 6 false false true false false false false SUPPORTED EXT-CLUSTER NUCLEUS STAR FORMING REGION YES V-band magnitude refers to total value in a 2.5 arcsec aperture (measured in HST/ACS/WFC/F550M image). FUV refers to flux at 1530 Angstrom in 2.5 arcsec COS aperture (measured in HST/ACS/SBC/F140LP image). This target is very compact, in an unconfused region of the galaxy, and hence ideal for target acquisition. This source is, however, not a true point source. Its peak pixel counts for COS/NUV/MIRRORB and ACS/SBC/F140LP are both about a factor 8 lower than the ETC expectations for a true point source. Hence, using this source as a reference target with COS/NUV/MIRROR-A is safe. J2000 FUV=1.93E-14 erg/s/cm2 EXT-CLUSTER EMISSION LINE NEBULA MULTIPLE NUCLEI NUCLEUS STAR FORMING REGION YES V-band magnitude refers to total value in a 2.5 arcsec aperture (measured in HST/ACS/WFC/F550M image). FUV refers to flux at 1530 Angstrom in 2.5 arcsec COS aperture (measured in HST/ACS/SBC/F140LP image). FUV=5.3E-15 erg/s/cm2 EXT-CLUSTER EMISSION LINE NEBULA MULTIPLE NUCLEI NUCLEUS STAR FORMING REGION YES V-band magnitude refers to total value in a 2.5 arcsec aperture (measured in HST/ACS/WFC/F550M image). FUV refers to flux at 1530 Angstrom in 2.5 arcsec COS aperture (measured in HST/ACS/SBC/F140LP image). FUV=1.1E-14 erg/s/cm2 EXT-MEDIUM EMISSION LINE NEBULA YES V-band magnitude refers to total value in a 2.5 arcsec aperture (measured in HST/ACS/WFC/F550M image). FUV refers to flux at 1530 Angstrom in 2.5 arcsec COS aperture (measured in HST/ACS/SBC/F140LP image). FUV=6E-16 erg/s/cm2 EXT-MEDIUM EMISSION LINE NEBULA YES V-band magnitude refers to total value in a 2.5 arcsec aperture (measured in HST/ACS/WFC/F550M image). FUV refers to flux at 1530 Angstrom in 2.5 arcsec COS aperture (measured in HST/ACS/SBC/F140LP image). FUV=1E-15 erg/s/cm2 COS/FUV Spectroscopic No No G160M 1623 COS/FUV Spectroscopic No No G130M 1300 COS/NUV Imaging No No MIRRORA STIS/FUV-MAMA Spectroscopic No No G140M 1218 STIS/CCD Spectroscopic No No G430M 4961 STIS/CCD Spectroscopic No No G750M 6768 POS-TARG DITHER 0.5070 LINE false false 2 90.0 STIS-ALONG-SLIT 1 false The scheduling data was generated by CASM 25.2. 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Based on existing COS/NUV imaging with MIRROR B and ACS/SBC/F140LP imaging we estimate the peak pixel intensity to be a factor of 8.4 fainter than the ETC prediction for a true point source. /Users/ostlin/Proposals/HST25/Phase2/OP-cache/haro11-15352-repeat-knotC-Nporth-v50.xml orient constraint chosen to optimise dispersion direction HOPR repeat of visit 10 1569781741000 353.6933732046092 (Tic-Visit :proposal-id 15352 :visit-id "50" :proposal-version -1 :trans-version "20190514" :date "06-Nov-2019 23:31:55.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 87360 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15352 :visit-id "50" :obset-id "50" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15352 :visit-id "50" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2844 :al-overhead-at-end 0 :internal-dur-at-end 38 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3180 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15352 :visit-id "50" :orbit-number 2 :pcs-time 302 :si-vis-utilization 2875 :al-overhead-at-end 0 :internal-dur-at-end 331 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3180 :pcs-gap 0 ) true 2 1 ETC run assuming quasi-point source with total intensity scaled down accordingly. Based on existing COS/NUV imaging with MIRROR B and ACS/SBC/F140LP imaging we estimate the peak pixel intensity to be a factor of 8.4 fainter than the ETC prediction for a true point source. /Users/ostlin/Proposals/HST25/Phase2/OP-cache/haro11-15352-repeat-knotC-Nporth-v51.xml orient constraint chosen to optimise dispersion direction HOPR repeat of second orbit of visit 50 due to guide star failure (Tic-Visit :proposal-id 15352 :visit-id "51" :proposal-version -1 :trans-version "20190514" :date "06-Nov-2019 23:38:21.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 52416 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15352 :visit-id "51" :obset-id "51" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15352 :visit-id "51" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2786 :al-overhead-at-end 0 :internal-dur-at-end 331 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3180 :pcs-gap 0 ) true 1 0 ETC run assuming quasi-point source with total intensity scaled down accordingly. Based on existing COS/NUV imaging with MIRROR B and ACS/SBC/F140LP imaging we estimate the peak pixel intensity to be a factor of 8.4 fainter than the ETC prediction for a true point source. The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. orient constraint chosen to optimise dispersion direction 1543112296000 45.0 (Tic-Visit :proposal-id 15352 :visit-id "07" :proposal-version -1 :trans-version "20180409" :date "30-Jul-2018 10:42:24.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 104768 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15352 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15352 :visit-id "07" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2902 :al-overhead-at-end 0 :internal-dur-at-end 38 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3240 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15352 :visit-id "07" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3018 :al-overhead-at-end 0 :internal-dur-at-end 331 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3240 :pcs-gap 0 ) false 2 0 ETC run assuming quasi-point source with total intensity scaled down accordingly. Based on existing COS/NUV imaging with MIRROR B and ACS/SBC/F140LP imaging we estimate the peak pixel intensity to be a factor of 8.4 fainter than the ETC prediction for a true point source. The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. orient constraint chosen to optimise dispersion direction 1527036586000 229.2016832995351 (Tic-Visit :proposal-id 15352 :visit-id "09" :proposal-version -1 :trans-version "20180409" :date "30-Jul-2018 10:42:25.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 104768 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15352 :visit-id "09" :obset-id "09" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15352 :visit-id "09" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2902 :al-overhead-at-end 0 :internal-dur-at-end 38 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3240 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15352 :visit-id "09" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3018 :al-overhead-at-end 0 :internal-dur-at-end 331 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3240 :pcs-gap 0 ) false 2 0 ETC run assuming quasi-point source with total intensity scaled down accordingly. Based on existing COS/NUV imaging with MIRROR B and ACS/SBC/F140LP imaging we estimate the peak pixel intensity to be a factor of 8.4 fainter than the ETC prediction for a true point source. Timing link suitability includes constraints ([11 After 04 by at most 0.1 days]) The scheduling data was generated by CASM 26.0. CASM was run in Phase II mode. 1536779191000 322.00039718014943 (Tic-Visit :proposal-id 15352 :visit-id "04" :proposal-version -1 :trans-version "20180409" :date "30-Jul-2018 23:18:46.0" :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 147680 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15352 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15352 :visit-id "04" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2907 :al-overhead-at-end 75 :internal-dur-at-end 340 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3240 :pcs-gap 0 ) false 1 0 Timing link suitability includes constraints ([11 After 04 by at most 0.1 days]) The scheduling data was generated by CASM 26.0. CASM was run in Phase II mode. Should preferably be scheduled imediately after visit 'STIS-slit-2-visit-1' 1536786003000 322.00039718014943 (Tic-Visit :proposal-id 15352 :visit-id "11" :proposal-version -1 :trans-version "20180409" :date "30-Jul-2018 23:05:21.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 368816 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15352 :visit-id "11" :obset-id "11" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15352 :visit-id "11" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2907 :al-overhead-at-end 125 :internal-dur-at-end 132 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3240 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15352 :visit-id "11" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3018 :al-overhead-at-end 125 :internal-dur-at-end 394 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3240 :pcs-gap 0 ) false 2 0 Timing link suitability includes constraints ([13 After 12 by at most 0.1 days]) The scheduling data was generated by CASM 26.0. CASM was run in Phase II mode. 1544513551000 59.29351402208701 (Tic-Visit :proposal-id 15352 :visit-id "12" :proposal-version -1 :trans-version "20180409" :date "30-Jul-2018 23:21:28.0" :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 147680 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15352 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15352 :visit-id "12" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2907 :al-overhead-at-end 75 :internal-dur-at-end 340 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3240 :pcs-gap 0 ) false 1 0 Timing link suitability includes constraints ([13 After 12 by at most 0.1 days]) The scheduling data was generated by CASM 26.0. CASM was run in Phase II mode. Should preferably be scheduled imediately after visit 'STIS-slit-1-visit-1' 1544519270000 59.33129923705579 (Tic-Visit :proposal-id 15352 :visit-id "13" :proposal-version -1 :trans-version "20180409" :date "30-Jul-2018 23:21:23.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 368816 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15352 :visit-id "13" :obset-id "13" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15352 :visit-id "13" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2907 :al-overhead-at-end 125 :internal-dur-at-end 132 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3240 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15352 :visit-id "13" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3018 :al-overhead-at-end 125 :internal-dur-at-end 394 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3240 :pcs-gap 0 ) false 2 0