Deciphering Quasar Outflows and Measuring their Contribution to AGN Feedback

0 Assigned ID: 1060 ----- Attempting Submission 1 (Fri Apr 08 23:48:29 GMT 2016) ----- For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting. For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting. For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting. For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting. For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting. For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting. 0 ----- Attempting Submission 1 (Thu Jul 21 20:16:50 GMT 2016) ----- As stated in our proposal description, due to the placement of crucial spectral features in several of our spectra, we can not use all four FP-POS positions. Otherwise, our desired features fall out of the active area of the detector. We note that we use a wide diversity of grating settings in this proposal. Given the faintness of our objects, we do not feel that this will have a deleterious effect on the COS detector lifetime. At our target S/N=10 in these spectra, it also will not affect the noise quality of our final spectra. Deciphering Quasar Outflows and Measuring their Contribution to AGN Feedback We propose to observe, for the first time, a sample of quasar outflows covering the diagnostic-rich 500-1050 Angstrom rest-frame (XUV). This program will advance the science of quasar outflows and measure their contribution to AGN feedback more than the combined HST observations of quasar outflows to date. Using similar COS archival data of two such objects, we have published a robust case of two-ionization-phase outflow, which is the missing link between UV AGN outflows and X-ray warm absorbers. More importantly, the superb spectral diagnostics allowed us to determine the distances of these outflows from the central source, and thus their energetics. These findings demonstrate that outflows in luminous quasars have sufficient energy to fulfill the theoretical predictions of AGN feedback processes. However, to date, not a single dedicated COS observation of outflows in the XUV has been performed. An exhaustive survey of all HST and SDSS quasar spectra and a significant improvement in analysis techniques allow us now to target a sample of 10 such objects using a reasonable amount of exposure time, hence the extraordinary scientific promise of this program. Sample Selection We searched through all of the MAST UV quasar spectra with a resolution > 800 and a S/N > 6. This search encompassed all of the HST quasar programs (COS, STIS, FOS) and all of the FUSE AGN data with z>0.4. We also searched the SDSS and BOSS quasar spectra database. The search criteria we used were: a) 0.4 > z > 1.5 to cover the spectral rich 500--1050 A rest frame region (XUV) with COS FUV gratings, b) continuum flux across the observed waveband > 2e-15 ergs cm^-2 s^-1 A^-1) c) absorption troughs indicative of outflows, that is, satisfying at least two of the following: troughs from excited states, doublet optical depth ratio smaller than 2:1, trough width > 300 km s^-1, appearance suggestive of solar or super solar metalicity. We identified the best 10 targets fulfilling these requirements. All of them are high ionization outflows similar to 90% of all quasar outflows. Choice of instruments and SNR requirements Since absorption troughs show significant changes in physical characteristics over 200 km s^-1 scales (e.g. Arav et al., 2007, 2008) we require a resolution R > 5000 in order to obtain a few resolution elements across that width. The medium resolution of the COS FUV settings combined with their high throughput make them the only suitable instrumental setup to reach the S/N and resolution needed for our program. Our experience in analyzing similar data from LBQS 1206+1052 (Chamberlain & Arav 2015) show that we can achieve our scientific goals with S/N of 10 per R = 5000 resolution element. 9 of our targets have FUV fluxes above 2e-15 ergs cm^-2 s^-1 A^-1, based on their observed UV spectra or their Galax FUV fluxes. Using the COS ETC on the lower flux (2.0e-15 ergs cm^-2 s^-1 A^-1) such a S/N can be obtained in 3 ks and 6 ks for the G130M and G160M gratings, respectively. Taking into account the overheads, this translates to a total of 4 orbits per object. The higher throughput G130M covers shorter wavelength diagnostics, which tends to yield higher scientific return. Therefore, we opt to obtain 2 orbits each with G130M and G160M to slightly increase the S/N in the shorter wavelength covered. Instrument Configuration and Bright Object Checking In selecting our grating settings, we have chosen central wavelengths to avoid placing the gap between the COS detectors on any of the crucial spectral features we will use in our analysis. We note that in several cases, the proximity of crucial spectral features to the edge of a central wavelength's wavelength range precludes using all four FP-POS positions. For ETC calculations for our moderate redshift quasars, we use the FOS-based QSO composite spectrum at the redshift of the object with a foreground E(B-V) as given by NED. Bright object checking is simple--our brightest quasar, PKS0350-0711, has a continuum flux of 4e-15 at 1516 A. To be conservative, we have used an ETC calculation for a flux 3x brighter, the maximum range typically observed for AGN variability (if not a BL Lac) (Dunn et al. 2006). This flux is safe for all gratings, and for an imaging target acquisition using Mirror B. Since all other objects are fainter, they too are safe. (Emission lines in the wavelength ranges visible here do not have sufficient contrast relative to the continuum to cause any local count rate issues.) (We note also that the screening limits for variable objects include an additional factor of two safety in count rate above the limits we are using.) To plan our observations, we use ETC calculations that are conservative (both fainter and brighter) to ensure success--we plan target acquisition exposure times for minimum fluxes that are 3x lower than the mean observed historically, and set BUFFER-TIME for fluxes 3x brighter than the mean flux, and use the factor of 2/3 recommended by the ETC. In practice, all BUFFER times from the ETC are >2000, so, to optimize buffer useage and minimize overheads, we generally choose BUFFER-TIME such that BUFFER-TIME=ExposureTime - 110 s. Our results for all objects are summarized here for convenience. - ACQUISITION - Object F(1516) E(B-V) z COS-ETC-ID PKS0350-07 1.2e-14 0.070 0.966246 COS.ta.827061 (High flux: for BO checking) PKS0350-07 1.3e-15 0.070 0.966246 COS.ta.827060 (Low flux: for target acq) UM425 0.7e-15 0.032 1.472 COS.ta.827063 VV2006-J075514.6+230607 2.5e-16 0.047 0.85437 COS.ta.827066 VV2006-J132957.2+540506 3.3e-16 0.013 0.949595 COS.ta.827067 SDSS-J104244.23+164656.1 4.3e-16 0.023 0.978063 COS.ta.827068 SDSS-J093602.10+200542.9 6.3e-16 0.027 1.183234 COS.ta.827069 2MASS-J10512569+1247462 3.3e-16 0.021 1.282753 COS.ta.827070 7C-163119.39+393037.00 4.6e-16 0.007 1.024575 COS.ta.827072 LBQS-1206+1052 5.3e-16 0.021 0.395549 COS.ta.827074 2MASS-J143621.29+072720.8 5.0e-16 0.026 0.894367 COS.ta.827075 - EXPOSURES - Object F(1516) E(B-V) z G130M:COS-ETC-ID BUFF G160M:COS-ETC BUFF PKS0350-07 1.2e-14 0.070 0.966246 COS.sp.827078 2660 COS.sp.827081 7745 For all 10 visits in this program, we have set Schedulability to 100 to maximize flexibility in planning each observation and increase the opportunities for scheduling. Massive Black Holes and their Hosts 6 false true false false false false AVAILABLE GALAXY NUCLEUS QUASAR WIND NO This object was generated by the targetselector and retrieved from the SIMBAD database.This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 2.0e-15 at 2300 A GALAXY NUCLEUS QSO WIND NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 2.2e-15 at 1516 A GALAXY NUCLEUS QSO WIND NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 7.4e-16 at 1516 A GALAXY NUCLEUS QSO WIND NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 2.95e-15 at 1516 A GALAXY NUCLEUS QSO WIND NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 1.3e-15 at 1516 A GALAXY NUCLEUS QSO WIND NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 2.5e-15 at 1516 A GALAXY NUCLEUS QSO WIND NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 1.0e-15 at 1516 A GALAXY NUCLEUS QUASAR WIND NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 1.4e-15 at 1516 A GALAXY NUCLEUS QSO WIND NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 1.6e-15 at 1516 A GALAXY NUCLEUS QSO WIND NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 1.3e-15 at 1516 A COS/FUV Spectroscopic No No G130M 1309 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1309 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1318 COS/FUV Spectroscopic No No G160M 1623 COS/FUV Spectroscopic No No G130M 1300 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1300 COS/FUV Spectroscopic No No G160M 1600 COS/FUV Spectroscopic No No G130M 1318 COS/FUV Spectroscopic No No G160M 1577 COS/FUV Spectroscopic No No G130M 1309 COS/FUV Spectroscopic No No G160M 1600 COS/FUV Spectroscopic No No G160M 1611 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1623 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1623 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G160M 1623 1469042685041 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. 1501931127000 247.06130277147895 (Tic-Visit :proposal-id 14777 :visit-id "01" :proposal-version -1 :trans-version "20160601" :date "20-Jul-2016 15:24:44.0" :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 1339776 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14777 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14777 :visit-id "01" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2641 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "01" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2768 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "01" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2770 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "01" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2768 :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 2992 :pcs-gap 0 ) false 4 0 1469039643157 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 14777 :visit-id "02" :proposal-version -1 :trans-version "20160601" :date "20-Jul-2016 14:34:02.0" :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 1722432 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14777 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14777 :visit-id "02" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2655 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "02" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2768 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "02" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2770 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "02" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2768 :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 2992 :pcs-gap 0 ) false 4 0 1469039692171 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. 1505771763000 282.4232699178083 (Tic-Visit :proposal-id 14777 :visit-id "03" :proposal-version -1 :trans-version "20160601" :date "20-Jul-2016 14:34:51.0" :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 1357088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14777 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14777 :visit-id "03" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2657 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "03" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2768 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "03" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2770 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "03" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2768 :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 2993 :pcs-gap 0 ) false 4 0 First exposure in G130M/1291 must be in FP-POS-4 since lines of interest are in the 1130-1140 A range. 1469037928987 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 14777 :visit-id "04" :proposal-version -1 :trans-version "20160601" :date "20-Jul-2016 14:05:28.0" :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 1357088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14777 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14777 :visit-id "04" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2669 :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 3003 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "04" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2776 :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 3003 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "04" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2778 :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 3003 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "04" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2776 :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 3003 :pcs-gap 0 ) false 4 0 First exposure in G130M/1291 must be in FP-POS-4 since lines of interest are in the 1130-1140 A range. 1469131836134 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 14777 :visit-id "05" :proposal-version -1 :trans-version "20160601" :date "21-Jul-2016 16:10:35.0" :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 1513728 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14777 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14777 :visit-id "05" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2657 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "05" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2753 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "05" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2758 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "05" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2769 :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 2992 :pcs-gap 0 ) false 4 0 Can only use FP-POS=1 & 2 for this cenwave to retain coverage of the O II 833 absorption trough. Can only use FP-POS=1 & 2 for this cenwave to retain coverage of the O II 833 absorption trough. 1469130666239 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 14777 :visit-id "06" :proposal-version -1 :trans-version "20160601" :date "21-Jul-2016 15:51:05.0" :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 1217952 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14777 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14777 :visit-id "06" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2653 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "06" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2769 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "06" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2770 :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 2993 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "06" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2768 :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 2993 :pcs-gap 0 ) false 4 0 Can only use FP-POS=4 with cenwave 1327 to retain coverage of the Mg X 624 absorption trough. Can only use FP-POS=4 with cenwave 1327 to retain coverage of the Mg X 624 absorption trough. 1469039827374 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 14777 :visit-id "07" :proposal-version -1 :trans-version "20160601" :date "20-Jul-2016 14:37:07.0" :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 1339776 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14777 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14777 :visit-id "07" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2652 :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 2988 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "07" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2756 :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 2988 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "07" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2758 :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 2988 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "07" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2756 :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 2988 :pcs-gap 0 ) false 4 0 1469131338313 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. 1494690333000 199.5115115729355 (Tic-Visit :proposal-id 14777 :visit-id "08" :proposal-version -1 :trans-version "20160601" :date "21-Jul-2016 16:02:18.0" :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 730912 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14777 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14777 :visit-id "08" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2658 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "08" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2769 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "08" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2766 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "08" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2769 :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 2992 :pcs-gap 0 ) false 4 0 1469131535949 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. 1500353912000 107.69857844118718 (Tic-Visit :proposal-id 14777 :visit-id "09" :proposal-version -1 :trans-version "20160601" :date "21-Jul-2016 16:05:35.0" :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 1009136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14777 :visit-id "09" :obset-id "09" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14777 :visit-id "09" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2655 :al-overhead-at-end 0 :internal-dur-at-end 105 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2988 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "09" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2764 :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 2988 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "09" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2758 :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 2988 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "09" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2756 :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 2988 :pcs-gap 0 ) false 4 0 1469039393807 The scheduling data was generated by CASM 24.2. CASM was run in Phase II mode. 1500274324000 112.37528066039158 (Tic-Visit :proposal-id 14777 :visit-id "10" :proposal-version -1 :trans-version "20160601" :date "20-Jul-2016 14:29:53.0" :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 1722336 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14777 :visit-id "10" :obset-id "10" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14777 :visit-id "10" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2657 :al-overhead-at-end 0 :internal-dur-at-end 95 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "10" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2768 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "10" :orbit-number 3 :pcs-time 222 :si-vis-utilization 2770 :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 2992 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14777 :visit-id "10" :orbit-number 4 :pcs-time 222 :si-vis-utilization 2768 :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 2992 :pcs-gap 0 ) false 4 0 First exposure in G130M/1291 must be in FP-POS-4 since lines of interest are in the 1130-1140 A range.