The number of orbits used exceeds the number allocated Visit 09 -- HOPR 92652 1880355073 ----- Attempting Submission 2 (Thu Jan 28 15:39:08 GMT 2021) ----- Your proposal could not be saved. Submission aborted. ----- Attempting Submission 3 (Mon Mar 15 20:25:39 GMT 2021) ----- ----- Attempting Submission 4 (Thu Aug 31 13:37:08 GMT 2023) ----- ----- Attempting Submission 6 (Tue Sep 05 11:33:59 GMT 2023) ----- HST Phase II Proposal 16489 successfully submitted. Receipt: # 16489-6 ----- Attempting Submission 7 (Tue Sep 05 12:02:51 GMT 2023) ----- HST Phase II Proposal 16489 successfully submitted. Receipt: # 16489-7 ----- Attempting Submission 8 (Tue Sep 05 13:09:38 GMT 2023) ----- HST Phase II Proposal 16489 successfully submitted. Receipt: # 16489-8 ----- Attempting Submission 9 (Tue Sep 05 18:01:58 GMT 2023) ----- ----- Attempting Submission 10 (Fri Sep 15 12:47:26 GMT 2023) ----- ----- Attempting Submission 12 (Fri Sep 22 12:13:08 GMT 2023) ----- HST Phase II Proposal 16489 successfully submitted. Receipt: # 16489-12 ----- Attempting Submission 13 (Fri Sep 22 12:56:49 GMT 2023) ----- Your proposal could not be saved. Submission aborted. ----- Attempting Submission 14 (Fri Sep 22 13:40:16 GMT 2023) ----- ----- Attempting Submission 15 (Fri Sep 29 12:01:22 GMT 2023) ----- ----- Attempting Submission 16 (Mon Oct 02 15:27:57 GMT 2023) ----- ----- Attempting Submission 17 (Tue Oct 03 12:06:08 GMT 2023) ----- I ran the planners, but not recorded by the app? Data warnings are known Outflow Legacy Accretion Survey: unveiling the wind driving mechanism in BHXRBs Transient black-hole X-ray binaries viewed at high inclinations display blue-shifted absorption lines in their X-ray spectra. These features are the signatures of powerful, hot and equatorial accretion disk winds being driven from these systems in their luminous soft states. Remarkably, blue-shifted absorption lines have recently also been discovered in optical and NIR recombination lines and ultraviolet resonance features. These features must also be produced in an outflow, but the physical conditions traced by these outflows are different. Despite this, the characteristic Doppler velocities of all three types of signatures are comparable, yet they have never been observed simultaneously. It is therefore completely unclear if they are associated with distinct outflows (e.g. driven by different mechanisms) or simply with different regions/phases within the same outflow. Here, we propose to answer this question by carrying out simultaneous time-resolved spectroscopy of a high-inclination system in the X-ray, ultraviolet and optical bands, in its two distinct physical configurations (hard- and soft-states). This will allow us to test if the three types of wind features are present simultaneously, and, if so, whether they display correlated variability and/or velocity structure. We will observe LMXRB in the hard and soft states coordinated with XMM-Newton. Ideally we will have 3 visits, at the begining and end of the XMM exposure, in order to swarch for simultaneous accretion disk winds in the X-ray and FUV. Given the unknown UV luminosity of the transient I am leaving different observing strategies in this mock phase II. Once we have a suitable target I will update all this carefully. For now the target is Swift J1858 which is a transient where we triggered similar programs during the past two cycles. n/a Stellar Physics and Stellar Types 6 false false false false false false false false SUPPORTED STAR LMXB X-RAY NOVAE X-RAY TRANSIENT NO J2000 COS/FUV Spectroscopic No No G140L 1105 COS/FUV Spectroscopic No No G140L 1105 COS/FUV Spectroscopic No No G140L 1105 1695198764000 92.65513330498561 (Tic-Visit :proposal-id 16489 :visit-id "03" :proposal-version -1 :trans-version "20230626" :date "22-Sep-2023 09:35:49.0" :trans-errors '(:WARNINGS 1 :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 2279232 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16489 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16489 :visit-id "03" :orbit-number 1 :pcs-time 443 :si-vis-utilization 2696 :al-overhead-at-end 0 :internal-dur-at-end 2241 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3139 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16489 :visit-id "03" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2747 :al-overhead-at-end 0 :internal-dur-at-end 440 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3139 :pcs-gap 0 ) true 2 0 For this we used a 25kK Blackbody with 0.34 extinction Quoted ETC is for a 25kK blackbody based on standard theory, using the line of sight extinction. radio observations of the current outburst confirm the extinction is at least the 0.34 observed by the dust maps. The NUV flux used it for the ETC simulation is 2E-12 (ergs/s/cm2/AA) at 2030 Angstroms. More than the highest flux ever observed by swift UVOT (1.7E-12) only in one observation. All the other observations have NUV fluxes are below 1.3. To be even more conservative we also estimated the count rate for extinction E(B-V) = 0.2: STIS.sp.1889430 Increasing the flux a factor of 2 of the above, 25kK and E(B-V)=0.2 will only lead a buffer warning: STIS.sp.1889442 An blackbody with infitinte temperature and 0.35 extinction and 2E-12 flux only lead to a buffer warning: STIS.sp.1889438 The target shows small modulation of 0.5 mag in the optical the optical V band from 12.5 to 13, less than a factor of two and consistent with the observed variability in the Swift UVOT observations. NUV with the higher flux and realistic 25kK blackbody emission with 2e-12 erg/s/cm2/A @ 2030 will give buffer warnings:STIS.sp.1889476 about 60% of the photons will be lost due to buffer overload. 400s should give a good signal to noise to estimate the extinction and tetect any weak emission line. Quoted ETC is for a 25kK blackbody based on standard theory, using the line of sight extinction. radio observations of the current outburst confirm the extinction is at least the 0.34 observed by the dust maps. The NUV flux used it for the ETC simulation is 2E-12 (ergs/s/cm2/AA) at 2030 Angstroms. More than the highest flux ever observed by swift UVOT (1.7E-12) only in one observation. All the other observations have NUV fluxes are below 1.3. To be even more conservative we also estimated the count rate for extinction E(B-V) = 0.2: STIS.sp.1889430 Increasing the flux a factor of 2 of the above, 25kK and E(B-V)=0.2 will only lead a buffer warning: STIS.sp.1889442 An blackbody with infitinte temperature and 0.35 extinction and 2E-12 flux only lead to a buffer warning: STIS.sp.1889438 The target shows small modulation of 0.5 mag in the optical the optical V band from 12.5 to 13, less than a factor of two and consistent with the observed variability in the Swift UVOT observations. 1695609292000 92.0742373983876 (Tic-Visit :proposal-id 16489 :visit-id "04" :proposal-version -1 :trans-version "20230626" :date "22-Sep-2023 09:35:50.0" :trans-errors '(:WARNINGS 1 :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 2401024 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16489 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16489 :visit-id "04" :orbit-number 1 :pcs-time 443 :si-vis-utilization 2696 :al-overhead-at-end 0 :internal-dur-at-end 178 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3139 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16489 :visit-id "04" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2747 :al-overhead-at-end 0 :internal-dur-at-end 578 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3139 :pcs-gap 0 ) true 2 0 For this we used a 25kK Blackbody with 0.34 extinction Quoted ETC is for a 25kK blackbody based on standard theory, using the line of sight extinction. radio observations of the current outburst confirm the extinction is at least the 0.34 observed by the dust maps. The NUV flux used it for the ETC simulation is 2E-12 (ergs/s/cm2/AA) at 2030 Angstroms. More than the highest flux ever observed by swift UVOT (1.7E-12) only in one observation. All the other observations have NUV fluxes are below 1.3. To be even more conservative we also estimated the count rate for extinction E(B-V) = 0.2: STIS.sp.1889430 Increasing the flux a factor of 2 of the above, 25kK and E(B-V)=0.2 will only lead a buffer warning: STIS.sp.1889442 An blackbody with infitinte temperature and 0.35 extinction and 2E-12 flux only lead to a buffer warning: STIS.sp.1889438 The target shows small modulation of 0.5 mag in the optical the optical V band from 12.5 to 13, less than a factor of two and consistent with the observed variability in the Swift UVOT observations. Quoted ETC is for a 25kK blackbody based on standard theory, using the line of sight extinction. radio observations of the current outburst confirm the extinction is at least the 0.34 observed by the dust maps. The NUV flux used it for the ETC simulation is 2E-12 (ergs/s/cm2/AA) at 2030 Angstroms. More than the highest flux ever observed by swift UVOT (1.7E-12) only in one observation. All the other observations have NUV fluxes are below 1.3. To be even more conservative we also estimated the count rate for extinction E(B-V) = 0.2: STIS.sp.1889430 Increasing the flux a factor of 2 of the above, 25kK and E(B-V)=0.2 will only lead a buffer warning: STIS.sp.1889442 An blackbody with infitinte temperature and 0.35 extinction and 2E-12 flux only lead to a buffer warning: STIS.sp.1889438 The target shows small modulation of 0.5 mag in the optical the optical V band from 12.5 to 13, less than a factor of two and consistent with the observed variability in the Swift UVOT observations. (Tic-Visit :proposal-id 16489 :visit-id "05" :proposal-version -1 :trans-version "20230626" :date "22-Sep-2023 09:35:52.0" :trans-errors '(:WARNINGS 1 :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 3583952 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16489 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16489 :visit-id "05" :orbit-number 1 :pcs-time 443 :si-vis-utilization 2696 :al-overhead-at-end 0 :internal-dur-at-end 178 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3139 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16489 :visit-id "05" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2747 :al-overhead-at-end 0 :internal-dur-at-end 578 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3139 :pcs-gap 0 ) true 2 0 For this we used a 25kK Blackbody with 0.34 extinction Quoted ETC is for a 25kK blackbody based on standard theory, using the line of sight extinction. radio observations of the current outburst confirm the extinction is at least the 0.34 observed by the dust maps. The NUV flux used it for the ETC simulation is 2E-12 (ergs/s/cm2/AA) at 2030 Angstroms. More than the highest flux ever observed by swift UVOT (1.7E-12) only in one observation. All the other observations have NUV fluxes are below 1.3. To be even more conservative we also estimated the count rate for extinction E(B-V) = 0.2: STIS.sp.1889430 Increasing the flux a factor of 2 of the above, 25kK and E(B-V)=0.2 will only lead a buffer warning: STIS.sp.1889442 An blackbody with infitinte temperature and 0.35 extinction and 2E-12 flux only lead to a buffer warning: STIS.sp.1889438 The target shows small modulation of 0.5 mag in the optical the optical V band from 12.5 to 13, less than a factor of two and consistent with the observed variability in the Swift UVOT observations. Quoted ETC is for a 25kK blackbody based on standard theory, using the line of sight extinction. radio observations of the current outburst confirm the extinction is at least the 0.34 observed by the dust maps. The NUV flux used it for the ETC simulation is 2E-12 (ergs/s/cm2/AA) at 2030 Angstroms. More than the highest flux ever observed by swift UVOT (1.7E-12) only in one observation. All the other observations have NUV fluxes are below 1.3. To be even more conservative we also estimated the count rate for extinction E(B-V) = 0.2: STIS.sp.1889430 Increasing the flux a factor of 2 of the above, 25kK and E(B-V)=0.2 will only lead a buffer warning: STIS.sp.1889442 An blackbody with infitinte temperature and 0.35 extinction and 2E-12 flux only lead to a buffer warning: STIS.sp.1889438 The target shows small modulation of 0.5 mag in the optical the optical V band from 12.5 to 13, less than a factor of two and consistent with the observed variability in the Swift UVOT observations. 1696709532000 93.0 (Tic-Visit :proposal-id 16489 :visit-id "06" :proposal-version -1 :trans-version "20230627" :date "29-Sep-2023 11:25:45.0" :trans-errors '(:WARNINGS 1 :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 3583952 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16489 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16489 :visit-id "06" :orbit-number 1 :pcs-time 443 :si-vis-utilization 2696 :al-overhead-at-end 0 :internal-dur-at-end 178 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3139 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16489 :visit-id "06" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2747 :al-overhead-at-end 0 :internal-dur-at-end 578 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3139 :pcs-gap 0 ) true 2 0 For this we used a 25kK Blackbody with 0.34 extinction Quoted ETC is for a 25kK blackbody based on standard theory, using the line of sight extinction. radio observations of the current outburst confirm the extinction is at least the 0.34 observed by the dust maps. The NUV flux used it for the ETC simulation is 2E-12 (ergs/s/cm2/AA) at 2030 Angstroms. More than the highest flux ever observed by swift UVOT (1.7E-12) only in one observation. All the other observations have NUV fluxes are below 1.3. To be even more conservative we also estimated the count rate for extinction E(B-V) = 0.2: STIS.sp.1889430 Increasing the flux a factor of 2 of the above, 25kK and E(B-V)=0.2 will only lead a buffer warning: STIS.sp.1889442 An blackbody with infitinte temperature and 0.35 extinction and 2E-12 flux only lead to a buffer warning: STIS.sp.1889438 The target shows small modulation of 0.5 mag in the optical the optical V band from 12.5 to 13, less than a factor of two and consistent with the observed variability in the Swift UVOT observations. Quoted ETC is for a 25kK blackbody based on standard theory, using the line of sight extinction. radio observations of the current outburst confirm the extinction is at least the 0.34 observed by the dust maps. The NUV flux used it for the ETC simulation is 2E-12 (ergs/s/cm2/AA) at 2030 Angstroms. More than the highest flux ever observed by swift UVOT (1.7E-12) only in one observation. All the other observations have NUV fluxes are below 1.3. To be even more conservative we also estimated the count rate for extinction E(B-V) = 0.2: STIS.sp.1889430 Increasing the flux a factor of 2 of the above, 25kK and E(B-V)=0.2 will only lead a buffer warning: STIS.sp.1889442 An blackbody with infitinte temperature and 0.35 extinction and 2E-12 flux only lead to a buffer warning: STIS.sp.1889438 The target shows small modulation of 0.5 mag in the optical the optical V band from 12.5 to 13, less than a factor of two and consistent with the observed variability in the Swift UVOT observations. (Tic-Visit :proposal-id 16489 :visit-id "07" :proposal-version -1 :trans-version "20230626" :date "22-Sep-2023 09:35:54.0" :trans-errors '(:WARNINGS 1 :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 3583952 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16489 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16489 :visit-id "07" :orbit-number 1 :pcs-time 443 :si-vis-utilization 2696 :al-overhead-at-end 0 :internal-dur-at-end 178 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3139 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16489 :visit-id "07" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2747 :al-overhead-at-end 0 :internal-dur-at-end 578 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3139 :pcs-gap 0 ) true 2 0 For this we used a 25kK Blackbody with 0.34 extinction Quoted ETC is for a 25kK blackbody based on standard theory, using the line of sight extinction. radio observations of the current outburst confirm the extinction is at least the 0.34 observed by the dust maps. The NUV flux used it for the ETC simulation is 2E-12 (ergs/s/cm2/AA) at 2030 Angstroms. More than the highest flux ever observed by swift UVOT (1.7E-12) only in one observation. All the other observations have NUV fluxes are below 1.3. To be even more conservative we also estimated the count rate for extinction E(B-V) = 0.2: STIS.sp.1889430 Increasing the flux a factor of 2 of the above, 25kK and E(B-V)=0.2 will only lead a buffer warning: STIS.sp.1889442 An blackbody with infitinte temperature and 0.35 extinction and 2E-12 flux only lead to a buffer warning: STIS.sp.1889438 The target shows small modulation of 0.5 mag in the optical the optical V band from 12.5 to 13, less than a factor of two and consistent with the observed variability in the Swift UVOT observations. Quoted ETC is for a 25kK blackbody based on standard theory, using the line of sight extinction. radio observations of the current outburst confirm the extinction is at least the 0.34 observed by the dust maps. The NUV flux used it for the ETC simulation is 2E-12 (ergs/s/cm2/AA) at 2030 Angstroms. More than the highest flux ever observed by swift UVOT (1.7E-12) only in one observation. All the other observations have NUV fluxes are below 1.3. To be even more conservative we also estimated the count rate for extinction E(B-V) = 0.2: STIS.sp.1889430 Increasing the flux a factor of 2 of the above, 25kK and E(B-V)=0.2 will only lead a buffer warning: STIS.sp.1889442 An blackbody with infitinte temperature and 0.35 extinction and 2E-12 flux only lead to a buffer warning: STIS.sp.1889438 The target shows small modulation of 0.5 mag in the optical the optical V band from 12.5 to 13, less than a factor of two and consistent with the observed variability in the Swift UVOT observations. 1696196492000 93.0 (Tic-Visit :proposal-id 16489 :visit-id "A5" :proposal-version -1 :trans-version "20230626" :date "22-Sep-2023 09:35:57.0" :trans-errors '(:WARNINGS 1 :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 3062032 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16489 :visit-id "A5" :obset-id "A5" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16489 :visit-id "A5" :orbit-number 1 :pcs-time 443 :si-vis-utilization 2696 :al-overhead-at-end 0 :internal-dur-at-end 2261 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3139 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16489 :visit-id "A5" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2747 :al-overhead-at-end 0 :internal-dur-at-end 440 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3139 :pcs-gap 0 ) true 2 0 For this we used a 25kK Blackbody with 0.34 extinction Quoted ETC is for a 25kK blackbody based on standard theory, using the line of sight extinction. radio observations of the current outburst confirm the extinction is at least the 0.34 observed by the dust maps. The NUV flux used it for the ETC simulation is 2E-12 (ergs/s/cm2/AA) at 2030 Angstroms. More than the highest flux ever observed by swift UVOT (1.7E-12) only in one observation. All the other observations have NUV fluxes are below 1.3. To be even more conservative we also estimated the count rate for extinction E(B-V) = 0.2: STIS.sp.1889430 Increasing the flux a factor of 2 of the above, 25kK and E(B-V)=0.2 will only lead a buffer warning: STIS.sp.1889442 An blackbody with infitinte temperature and 0.35 extinction and 2E-12 flux only lead to a buffer warning: STIS.sp.1889438 The target shows small modulation of 0.5 mag in the optical the optical V band from 12.5 to 13, less than a factor of two and consistent with the observed variability in the Swift UVOT observations. NUV with the higher flux and realistic 25kK blackbody emission with 2e-12 erg/s/cm2/A @ 2030 will give buffer warnings:STIS.sp.1889476 about 60% of the photons will be lost due to buffer overload. 400s should give a good signal to noise to estimate the extinction and tetect any weak emission line. NUV with the higher flux and realistic 25kK blackbody emission with 2e-12 erg/s/cm2/A @ 2030 will give buffer warnings:STIS.sp.1889476 about 60% of the photons will be lost due to buffer overload. 400s should give a good signal to noise to estimate the extinction and tetect any weak emission line. 0.5e-12 at 2600 -- STIS.sp.1892366 Quoted ETC is for a 25kK blackbody based on standard theory, using the line of sight extinction. radio observations of the current outburst confirm the extinction is at least the 0.34 observed by the dust maps. The NUV flux used it for the ETC simulation is 2E-12 (ergs/s/cm2/AA) at 2030 Angstroms. More than the highest flux ever observed by swift UVOT (1.7E-12) only in one observation. All the other observations have NUV fluxes are below 1.3. To be even more conservative we also estimated the count rate for extinction E(B-V) = 0.2: STIS.sp.1889430 Increasing the flux a factor of 2 of the above, 25kK and E(B-V)=0.2 will only lead a buffer warning: STIS.sp.1889442 An blackbody with infitinte temperature and 0.35 extinction and 2E-12 flux only lead to a buffer warning: STIS.sp.1889438 The target shows small modulation of 0.5 mag in the optical the optical V band from 12.5 to 13, less than a factor of two and consistent with the observed variability in the Swift UVOT observations. The scheduling data was generated by CASM 31.1. CASM was run in Phase II mode. 1697234041000 87.5 (Tic-Visit :proposal-id 16489 :visit-id "A7" :proposal-version -1 :trans-version "20230627" :date "29-Sep-2023 12:59:39.0" :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 434976 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16489 :visit-id "A7" :obset-id "A7" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16489 :visit-id "A7" :orbit-number 1 :pcs-time 443 :si-vis-utilization 2687 :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 3139 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16489 :visit-id "A7" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2747 :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 3139 :pcs-gap 0 ) true 2 0 FUV flux matched to the observed as of 25th Sep 2500K BB generously matching the observed FUV flux from HST obs taken on 25th Sep The scheduling data was generated by CASM 31.1. CASM was run in Phase II mode. (Tic-Visit :proposal-id 16489 :visit-id "08" :proposal-version -1 :trans-version "20230627" :date "02-Oct-2023 16:24:13.0" :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 417600 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16489 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16489 :visit-id "08" :orbit-number 1 :pcs-time 443 :si-vis-utilization 2687 :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 3139 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16489 :visit-id "08" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2738 :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 3139 :pcs-gap 0 ) true 2 0 FUV flux matched to the observed as of 25th Sep 2500K BB generously matching the observed FUV flux from HST obs taken on 25th Sep The scheduling data was generated by CASM 31.1. CASM was run in Phase II mode. /private/var/folders/qw/bm7knqg9493_9mh63wbjwdkh0000gp/T/OPVisit15535870487428376488.xml (Tic-Visit :proposal-id 16489 :visit-id "09" :proposal-version -1 :trans-version "20230627" :date "03-Oct-2023 13:04:24.0" :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 417600 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16489 :visit-id "09" :obset-id "09" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16489 :visit-id "09" :orbit-number 1 :pcs-time 443 :si-vis-utilization 2687 :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 3139 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16489 :visit-id "09" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2738 :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 3139 :pcs-gap 0 ) true 2 0 FUV flux matched to the observed as of 25th Sep 2500K BB generously matching the observed FUV flux from HST obs taken on 25th Sep