0 Assigned ID: 543 ----- Attempting Submission 1 (Fri Apr 05 17:01:28 GMT 2019) ----- HST Phase I Proposal 543 (O.apt) successfully submitted. Receipt: # 543-1 1) To avoid target duplication with another prposal, four alternative targets were selected. 2) The observing strategy is updated compared to Phase I. Now, the brighter stars are observed with STIS, while the fainter one are observed with COS The duplications are removed. The changes were approved by the HOPR. We would be grateful for an expert opinion on our observing strategy, specifically the use of COS G130M cenwave 1291 with only 2 FP-POS 14 April 2020 - changed ACQ in Visit 5 15 APril 2020 - changed ACQ in Visit 7. 9. 12, 12, 13 22 April 2020 lables corrected for Visit 12 and 13 1402794726 ----- Attempting Submission 1 (Thu Jul 25 18:40:21 GMT 2019) ----- HST Phase II Proposal 15837 (phase2-stis.apt) successfully submitted. Receipt: # 15837-1 ----- Attempting Submission 2 (Mon Sep 02 15:23:33 GMT 2019) ----- ----- Attempting Submission 3 (Wed Nov 06 11:08:59 GMT 2019) ----- ----- Attempting Submission 4 (Tue Apr 14 21:32:13 GMT 2020) ----- HST Phase II Proposal 15837 successfully submitted. Receipt: # 15837-4 ----- Attempting Submission 5 (Wed Apr 15 21:18:49 GMT 2020) ----- HST Phase II Proposal 15837 successfully submitted. Receipt: # 15837-5 ----- Attempting Submission 6 (Wed Apr 22 14:00:24 GMT 2020) ----- The HST follows galactic influencers: a COS UV survey of the most massive O-stars in the SMC We propose to measure the stellar winds of a nearly complete sample of O stars in the SMC with evolutionary masses above 30 Msol. Recent works indicate that stars of such high masses remain largely chemically mixed, hot, and compact during their evolution. This strongly questions the accepted models for gravitational wave progenitors as well as for various types of core-collapse SNe. These models explicitly assume a scaling of stellar mass loss with metallicity, which is not yet verified empirically in the upper mass range. Stellar winds are best studied in the UV, but up to now UV spectra exist for only a handful among the most massive O stars in the SMC. Their analyses revealed serious problems with commonly adopted mass loss recipes, but the existing sample of UV spectra is highly insufficient. We will obtain excellent quality UV COS spectra of 18 O-type stars with evolutionary masses above 30 Msol, dramatically increasing (by a factor of 3) and largely completing the existing sample. The COS spectra will be analyzed using highly advanced non-LTE stellar atmosphere models. We will determine stellar wind mass loss rates, velocity fields, clumping properties, abundances, and rotation rates. On this basis, empirical recipes for the dependence of the stellar mass-loss rate on metallicity will be derived and compared to theoretical predictions. The analyses of spectral lines and spectral energy distribution will provide hints on binary status. As the result, each star will be well characterized. The comparison with single and binary star evolutionary models will disrupt the current understanding of massive star lives and deaths at low metallicities. For the majority of targets, the coordinates are from GAIA DR2 ctalog, unless commented otherwise. Proper motions of the SMC stars are negligible. Whenever possible, the positions and crowding were checked using the HST, XMM OM, and SWIFT UV and optical images. The target list is updated. Four targets, LIN-78, SK-32, MA93-1694, and SK-101, were substituted to avoid target duplication with proposal 15629. Instead, alternative targets with similar spectral types and lacking previous high-resolution UV spectrosocpy were selected. In addition, one target, LHA-115-N-9, was substituted after it was discovered that this object is significanly reddened (E(B-V)=0.9). One more target, MA93-1125, was substituted because a star with exactly the same spectral type but one magntide brighter was identified. All new targets are fully in the framework of the proposal - O stars with high initial masses. The new targets are commented in the apt. We adopted different observing strategies depending on the target brightness. For the targets with V<14 we use STIS E140M single exposure. The desired S/N will be achieved by binning 3-7 spectral resolution elements which is sufficient for O type stars. For the targets with V>14 we use COS. For stars with earlier spectral type, we use G130M with cenwave 1291 with two allowed FP-POS, and G160M cenwave 1611 with ALL FP-POS. For stars with later spectral types, we use G160M cenwave 1533 and cenwave 1611 using ALL FP-POS. The team consists of experts in all subjects relevant for the proposal. Drs. W.-R. Hamann, R. Prinja, D. Massa are leading experts in UV spectroscopy of O stars and stellar wind modeling. Drs. T. Shenar, A. Sander, L. Oskinova, R. Hainich have large experience with studies of massive stars in the SMC. Dr. Shenar has developed, applied, and published tools for spectral deconvolution of binary O star spectra. Dr. Sander is an expert in hydrodynamic modeling of stellar winds, including winds from metal poor stars. Dr. Hainich has recently published grids of spectral models for O-type stars in the SMC. Dr. Oskinova is the PI of large observing campaigns in optical to spectroscopically study OB stars in the SMC, and of the HST UV spectroscopic observations of the massive star cluster NGC 346 in the SMC. All co-Is have large experience in developing the models and theory of stellar wind clumping, and in mass loss diagnostics in clumped winds based on UV spectroscopy. Ms. Ramachandran is the last year PhD student, who has already published large spectroscopic studies of OB stars in the SMC and LMC; Mr. M. Rickard is the first year PhD student, the subject of his PhD is spectroscopic analysis of O stars in the SMC. The primary modeling tools for the analysis of the observations will be the PoWR non-LTE stellar atmosphere model which is actively used for the analysis of metal poor OB stars. Recent publications include: Ramachandran et al., 2019, A&A accepted, arXiv190301762 Spectroscopic analysis of OB stars in the SMC questions the standard picture of massive star evolution, star-formation history and feedback at low metallicity Massa et al., 2019, ApJ, 873, 81 Coordinated UV and X-Ray Spectroscopic Observations of the O-type Giant ksi Per Hainich et al., 2019, A&A 621, 85 PoWR grids of non-LTE model atmospheres for OB-type stars of various metallicities Gruner, D.; Hainich, R.; Sander, A. A. C.; Shenar, T., et al., 2019, A&A 621, 63 The extreme O-type spectroscopic binary HD 93129A. A quantitative, multiwavelength analysis Ramachandran, V.; Hamann, W.-R.; Hainich, R.; et al, 2018, A&A 615, 40 Stellar population of the superbubble N 206 in the LMC. II. Parameters of the OB and WR stars, and the total massive star feedback Sander et al., 2018, A&A 610, 60 Coupling hydrodynamics with comoving frame radiative transfer. Hainich, R.; Oskinova, L. M.; Shenar, T.; et al., 2018, A&A, 609, 94 Observational properties of massive black hole binary progenitors Ramachandran, Varsha; Hainich, R.; Hamann, W.-R.; et al., 2018, A&A 609, 7 Stellar population of the superbubble N 206 in the LMC. I. Analysis of the Of-type stars Stellar Physics Stellar Populations 0 false false false false false false false SUPPORTED STAR MAIN SEQUENCE O NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 STAR MAIN SEQUENCE O NO This object was generated by the targetselector and retrieved from the SIMBAD database. The object has large parallax in Gaia DR2 catalog, taking it as a face value this would imply a foreground star. Howevere, the astrometric error indicated for thisw object in DR2 catalog is very large, letting us to conclude that the GAIA parallax is an error. Simalrly, the GAIA's proper motion is discarded. Arbitray value, is included in the apt form. The coordinates, the error, and the V magnitude are from the UCAC4 catalog. J2000 J2000 STAR MAIN SEQUENCE O NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 STAR MAIN SEQUENCE O WOLF RAYET This target substitutes LIN-78. LIN-78 was approved as a target for the Cycle 26 propsal 15629. To avoid target duplication we now choose this O4+WO star, where the secondary has a similar type to LIN 78 (O4) and no previous high-resolution UV spectra exist. J2000 J2000 STAR GIANT O MAIN SEQUENCE O NO This target substitutes the target LIN-508 which has high reddening. The new target SSN-25 is less reddened, 1.5 magnitides brighter, has SpType O6V and no previous high-resolution UV spectroscopy J2000 J2000 STAR MAIN SEQUENCE O NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 STAR MAIN SEQUENCE O NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 STAR MAIN SEQUENCE O NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 STAR GIANT O This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 STAR MAIN SEQUENCE O This target substitutes SK-32. SK-32 was approved as a target for the Cycle 26 propsal 15629. To avoid target duplication we now use NGC 346 MPG 342 (V=13.1) which has a similar spectral type, O5, and no previous high-resolution UV spectra exist. J2000 J2000 STAR MAIN SEQUENCE O NO The target substitutes the proposed target MA93-1125. The new target has identical spectral type, O5.5V, but is one magnitude brighter. The target has no previous UV spectroscopic observations. J2000 J2000 STAR SUPERGIANT O NO This object was generated by the targetselector and retrieved from the SIMBAD database. AZV-26 J2000 J2000 STAR MAIN SEQUENCE O NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 STAR MAIN SEQUENCE O NO This object was generated by the targetselector and retrieved from the SIMBAD database. 2DFS-5066 J2000 J2000 STAR MAIN SEQUENCE O NO This target substitutes MA93-1694 which was approved as a target for the Cycle 26 propsal 15629. To avoid target duplication we now use NGC 346 MPG 396 (V=14.39) which has a similar spectral type, O7, and no previous high-resolution UV spectroscoy. The coordinates are from the UCAC4 catalogue. J2000 J2000 STAR SUPERGIANT O NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 STAR SUPERGIANT O NO This target substitutes Sk 101 which was approved as a target for the Cycle 26 propsal 15629. To avoid target duplication we now use Sk 35 which is a supergiant with a similar spectral type, O9, and no previous high-resolution UV spectra exist J2000 J2000 STAR SUPERGIANT O This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1611 /home/lida/SMC-O.DIR/OP-cache/apt-acq-v01.xml The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. 1587982350000 192.86332811936336 (Tic-Visit :proposal-id 15837 :visit-id "01" :proposal-version -1 :trans-version "20191203" :date "15-Apr-2020 23:16:12.0" :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 104848 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15837 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15837 :visit-id "01" :orbit-number 1 :pcs-time 393 :si-vis-utilization 3132 :al-overhead-at-end 194 :internal-dur-at-end 319 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3525 :pcs-gap 0 ) true 1 0 /home/lida/SMC-O.DIR/OP-cache/apt-acq-v02.xml The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15837 :visit-id "02" :proposal-version -1 :trans-version "20191203" :date "15-Apr-2020 23:16:13.0" :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 417600 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15837 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15837 :visit-id "02" :orbit-number 1 :pcs-time 393 :si-vis-utilization 3129 :al-overhead-at-end 0 :internal-dur-at-end 388 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3525 :pcs-gap 0 ) true 1 0 /home/lida/SMC-O.DIR/OP-cache/apt-acq-v03.xml The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. 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(Tic-Visit :proposal-id 15837 :visit-id "04" :proposal-version -1 :trans-version "20191203" :date "15-Apr-2020 23:16:14.0" :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 104848 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15837 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15837 :visit-id "04" :orbit-number 1 :pcs-time 393 :si-vis-utilization 3132 :al-overhead-at-end 194 :internal-dur-at-end 319 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3525 :pcs-gap 0 ) true 1 0 /home/lida/SMC-O.DIR/OP-cache/apt-acq-v05.xml The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15837 :visit-id "05" :proposal-version -1 :trans-version "20191203" :date "15-Apr-2020 23:16:15.0" :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 243696 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15837 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15837 :visit-id "05" :orbit-number 1 :pcs-time 393 :si-vis-utilization 3127 :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 3525 :pcs-gap 0 ) true 1 0 /home/lida/SMC-O.DIR/OP-cache/apt-acq-v06.xml The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15837 :visit-id "06" :proposal-version -1 :trans-version "20191203" :date "15-Apr-2020 23:16:17.0" :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 348032 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15837 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15837 :visit-id "06" :orbit-number 1 :pcs-time 393 :si-vis-utilization 3132 :al-overhead-at-end 0 :internal-dur-at-end 379 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3525 :pcs-gap 0 ) true 1 0 /home/lida/SMC-O.DIR/OP-cache/apt-acq-v07.xml The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15837 :visit-id "07" :proposal-version -1 :trans-version "20191203" :date "15-Apr-2020 23:16:18.0" :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 226320 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15837 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15837 :visit-id "07" :orbit-number 1 :pcs-time 393 :si-vis-utilization 3131 :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 3525 :pcs-gap 0 ) true 1 0 /home/lida/SMC-O.DIR/OP-cache/apt-acq-v08.xml The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15837 :visit-id "08" :proposal-version -1 :trans-version "20191203" :date "15-Apr-2020 23:16:18.0" :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 104848 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15837 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15837 :visit-id "08" :orbit-number 1 :pcs-time 393 :si-vis-utilization 3132 :al-overhead-at-end 194 :internal-dur-at-end 319 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3525 :pcs-gap 0 ) true 1 0 /home/lida/SMC-O.DIR/OP-cache/apt-acq-v09.xml The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15837 :visit-id "09" :proposal-version -1 :trans-version "20191203" :date "15-Apr-2020 23:16:20.0" :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 374144 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15837 :visit-id "09" :obset-id "09" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15837 :visit-id "09" :orbit-number 1 :pcs-time 393 :si-vis-utilization 3126 :al-overhead-at-end 0 :internal-dur-at-end 379 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3525 :pcs-gap 0 ) true 1 0 /home/lida/SMC-O.DIR/OP-cache/apt-acq-v10.xml The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15837 :visit-id "10" :proposal-version -1 :trans-version "20191203" :date "15-Apr-2020 23:16:20.0" :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 104848 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15837 :visit-id "10" :obset-id "10" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15837 :visit-id "10" :orbit-number 1 :pcs-time 393 :si-vis-utilization 3132 :al-overhead-at-end 194 :internal-dur-at-end 319 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3525 :pcs-gap 0 ) true 1 0 /home/lida/SMC-O.DIR/OP-cache/apt-acq-v11.xml The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. 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(Tic-Visit :proposal-id 15837 :visit-id "12" :proposal-version -1 :trans-version "20191203" :date "15-Apr-2020 23:16:23.0" :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 313264 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15837 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15837 :visit-id "12" :orbit-number 1 :pcs-time 393 :si-vis-utilization 3131 :al-overhead-at-end 0 :internal-dur-at-end 379 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3525 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. /home/lida/SMC-O.DIR/OP-cache/apt-acq-v13.xml (Tic-Visit :proposal-id 15837 :visit-id "13" :proposal-version -1 :trans-version "20191203" :date "15-Apr-2020 23:16:24.0" :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 226288 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15837 :visit-id "13" :obset-id "13" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15837 :visit-id "13" :orbit-number 1 :pcs-time 393 :si-vis-utilization 3131 :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 3525 :pcs-gap 0 ) true 1 0 /home/lida/SMC-O.DIR/OP-cache/apt-acq-v14.xml The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15837 :visit-id "14" :proposal-version -1 :trans-version "20191203" :date "15-Apr-2020 23:16:25.0" :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 104848 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15837 :visit-id "14" :obset-id "14" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15837 :visit-id "14" :orbit-number 1 :pcs-time 393 :si-vis-utilization 3132 :al-overhead-at-end 194 :internal-dur-at-end 319 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3525 :pcs-gap 0 ) true 1 0 /home/lida/SMC-O.DIR/OP-cache/apt-acq-v15.xml The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15837 :visit-id "15" :proposal-version -1 :trans-version "20191203" :date "15-Apr-2020 23:16:26.0" :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 104848 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15837 :visit-id "15" :obset-id "15" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15837 :visit-id "15" :orbit-number 1 :pcs-time 393 :si-vis-utilization 3132 :al-overhead-at-end 194 :internal-dur-at-end 319 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3525 :pcs-gap 0 ) true 1 0 /home/lida/SMC-O.DIR/OP-cache/apt-acq-v16.xml The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15837 :visit-id "16" :proposal-version -1 :trans-version "20191203" :date "15-Apr-2020 23:16:26.0" :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 104848 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15837 :visit-id "16" :obset-id "16" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15837 :visit-id "16" :orbit-number 1 :pcs-time 393 :si-vis-utilization 3132 :al-overhead-at-end 194 :internal-dur-at-end 319 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3525 :pcs-gap 0 ) true 1 0 /home/lida/SMC-O.DIR/OP-cache/apt-acq-v17.xml The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15837 :visit-id "17" :proposal-version -1 :trans-version "20191203" :date "15-Apr-2020 23:16:27.0" :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 104848 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15837 :visit-id "17" :obset-id "17" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15837 :visit-id "17" :orbit-number 1 :pcs-time 393 :si-vis-utilization 3132 :al-overhead-at-end 194 :internal-dur-at-end 319 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3525 :pcs-gap 0 ) true 1 0 /home/lida/SMC-O.DIR/OP-cache/apt-acq-v18.xml The scheduling data was generated by CASM 28.0. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15837 :visit-id "18" :proposal-version -1 :trans-version "20191203" :date "15-Apr-2020 23:16:28.0" :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 104848 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15837 :visit-id "18" :obset-id "18" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15837 :visit-id "18" :orbit-number 1 :pcs-time 393 :si-vis-utilization 3132 :al-overhead-at-end 194 :internal-dur-at-end 319 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3525 :pcs-gap 0 ) true 1 0