0 Assigned ID: 7100 ----- Attempting Submission 1 (Tue Apr 14 22:39:36 GMT 2026) ----- HST Phase I Proposal 7100 successfully submitted. Receipt: # 7100-1 ----- Attempting Submission 2 (Wed Apr 15 18:36:57 GMT 2026) ----- HST Phase I Proposal 7100 successfully submitted. Receipt: # 7100-2 ----- Attempting Submission 3 (Wed Apr 15 23:19:00 GMT 2026) ----- HST Phase I Proposal 7100 successfully submitted. Receipt: # 7100-3 ----- Attempting Submission 4 (Thu Apr 16 00:57:22 GMT 2026) ----- HST Phase I Proposal 7100 successfully submitted. Receipt: # 7100-4 ----- Attempting Submission 5 (Thu Apr 16 15:46:45 GMT 2026) ----- HST Phase I Proposal 7100 successfully submitted. Receipt: # 7100-5 ----- Attempting Submission 6 (Thu Apr 16 23:27:27 GMT 2026) ----- COS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS 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 EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS 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. INEFFICIENT ORDERING OF FP-POS POSITIONS COS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS 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. INEFFICIENT ORDERING OF FP-POS POSITIONS COS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS 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 EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS INEFFICIENT ORDERING OF FP-POS POSITIONS 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 EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS 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 EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS 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 EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS INEFFICIENT ORDERING OF FP-POS POSITIONS 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. INEFFICIENT ORDERING OF FP-POS POSITIONS COS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS 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 EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS INEFFICIENT ORDERING OF FP-POS POSITIONS 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. INEFFICIENT ORDERING OF FP-POS POSITIONS COS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS 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. 0 ----- Attempting Submission 1 (Sat Aug 15 00:08:53 GMT 2026) ----- COS exposure rounded to the nearest 0.1s: could not find the source of this issues. Integration time were specified in the requested format. COS FUV PSA science exposures with extended targets: we are aware of this and will re-calibrate spectra by comparing with expectations from sythetic photometry of the apertures in filters overlapping with the spectra. INEFFICIENT ORDERING OF FP-POS POSITIONS: the inneficient switches (e.g. FP-POS 1--> 4) happen during occultation. The Lya line of hydrogen is a critical probe of galaxies from the nearby Universe to the Epoch of Reionization, making it key to observationally constraining galaxy evolution. However, the line is resonant and undergoes a complex radiative transfer process in the ISM of galaxies, limiting our understanding of Lya profiles and what properties can be recovered from them. Lya photons are the result of UV radiation from stars, resonantly scattered by hydrogen atoms and absorbed by dust, so that Lya profiles are expected to vary spatially in galaxies. However, the effect of neutral gas content and kinematics on the line profiles have never been directly evaluated. Furthermore, how Lya profiles vary in galaxies, an information critical to designing observation strategies with HWO, is still poorly known. We propose to map Lya spectra using a grid of 11 new COS apertures in the Lya-emitting galaxy LARS08. LARS08 has a unique multi-wavelength dataset tracing every component of the ISM relevant to Lya transfer at high angular resolution, including 21cm cubes tracing HI content and kinematics at 3.5" resolution, and Ha and Hb cubes needed to recover the intrinsic Lya profiles and dust. The proposed apertures are designed to capture a wide range of the ISM properties thought to impact Lya profiles. We will use these observations as a case study to measure spatially-varying Lya profiles, capturing the total Lya output and kinematics at every position. With the exquisite supporting data, we will determine how Lya profiles are built by different regions of the ISM within a galaxy, providing a consistency check for simulations and helping pave the way for future HWO observations. These observations aim to obtain Far-UV spectra with COS in 11 new, distinct apertures in the nearby (z=0.038) star-forming galaxy LARS 08 (SDSS J125013.55+073439.5). The main purpose of these observations is to obtain emission/absorption spectra of the Lyman-alpha line at 1216 AA, the exposure times have been calculated with this goal in mind. A secondary goal is to observe low ionization state metal lines from the neutral ISM, including SiII 1260 and OI 1302, when possible. The 29 orbits we have been awarded will be distributed between the different apertures to detect and resolve the Lyman-alpha line at different positions, based on predictions from previous Halpha flux and Ly-alpha imaging. We use the G130M grating with CENWAVE = 1222, that allows observations of the Ly-alpha line at z=0.038. The apertures have a grid layout, which is set respective to the aperture that was already observed in program 12583, that targetted the brightest UV cluster in the galaxy. The offset between the proposed apertures is set by ancillary observations with the worst angular resolution (VLA 21cm line maps, ~3.6"). Coordinates are based on the coordinates of the aperture previously observed with COS, extracted from the NUV acquisition image. Given the coordinates and flux distribution are well-known, we perform target acquisition on the same cluster in the NUV with ACQ/IMAGE, with exposure times based on the flux in the previous NUV acquisition images. After target acquisition, we obtain a COS NUV image of the target aperture to verify its position; our analysis will be modified in case of offset. Our apertures are centered on mostly extended Lyman-alpha regions which we assume fill the COS aperture. To alleviate flux calibration uncertainties that arise when observing extended targets with the COS FUV PSA, we will use images of the target galaxy previously obtained with ACS/SBC (specifically in F125LP and F140LP) and perform synthetic photometry at the position of the apertures to re-calibrate the spectra. COS ETC runs for each science exposure assume an exposure time of 1000s, close to our longest integration times. While we have flux values in a long-pass filter overlapping with the Lyman-alpha line and thus have an approximate constraint for the fluxes, the Lyman-alpha line profile shape is not known, thus the count rate could be under-estimated for some apertures. For this reason and because the buffer fill times are otherwise very large (on the order of 10,000s), we fix the buffer time to be the exposure time for each science exposure. To achieve the goals of the proposal, Lyman-alpha spectra with S/N<20 are sufficient, thus we only use two FP-POS for galaxies with a single orbit, otherwise we use all four FP-POS settings. The team is composed of researchers with extensive observational and theoretical experience in Lya and ISM science. MJH, CS, JM, TERT, GO, AC, ASL and BLJ are experts in Lya observations, and in particular have extensive experience with using HST ACS and WFC3 imaging, and HST COS and STIS spectroscopy to observe Lya emission from nearby galaxies. MJH, CS, TERT, and GO have conducted a number of successful HST campaigns using COS for Lya spectroscopy. TERT and ASL are experts in the analysis of UV spectra from galaxies. ALR and JMC are experts in radio astronomy, they respectively obtained and reduced the VLA 21cm observations of LARS08 and have experience in multi-wavelength comparisons between 3D 21cm interferometric observations and Lya imaging and spectroscopy. AS is an expert in Lyman-alpha radiative transfer modelling and simulations who developped the COLT radiative transfer code. AC and ALR are involved in HWO preparation through science case development. In particular, AC led the HWO science case to establish fesc,LyC calibrators in faint galaxies. All the tools to process the data in this proposal are in place. Galaxies Stellar Populations and the Interstellar Medium 3 false false false false false false true SUPPORTED EXT-MEDIUM EMISSION LINE NEBULA STAR FORMING REGION YES This aperture is set relative to the aperture in program 12583, which was centered on the brightest UV cluster in galaxy LARS08. Aperture L08A1 should be shifted by dRA=0 arcsec, dDEC=-10.8 arcsec from the brihtest UV cluster in the acquisition image. J2000 f_acs-sbc_f125lp(1426.5AA)= 3.43e-17 erg/s/cm2/AA EXT-MEDIUM EMISSION LINE NEBULA STAR FORMING REGION YES This aperture is set relative to the aperture in program 12583, which was centered on the brightest UV cluster in galaxy LARS08. Aperture L08A2 should be shifted by dRA=3.6 arcsec, dDEC=-10.8 arcsec fron the brightest UV cluster in the acquisition image. J2000 f_acs-sbc_f125lp(1426.5AA)= 6.22e-17 erg/s/cm2/AA EXT-MEDIUM EMISSION LINE NEBULA STAR FORMING REGION YES This aperture is set relative to the aperture in program 12583, which was centered on the brightest UV cluster in galaxy LARS08. Aperture L08A3 should be shifted by dRA=-3.6 arcsec, dDEC=-7.2 arcsec fron the brightest UV cluster in the acquisition image. J2000 f_acs-sbc_f125lp(1426.5AA)= 3.37e-17 erg/s/cm2/AA EXT-MEDIUM EMISSION LINE NEBULA STAR FORMING REGION YES This aperture is set relative to the aperture in program 12583, which was centered on the brightest UV cluster in galaxy LARS08. Aperture L08A4 should be shifted by dRA=0 arcsec, dDEC=-7.2 arcsec fron the brightest UV cluster in the acquisition image. J2000 f_acs-sbc_f125lp(1426.5AA)= 4.08e-16 erg/s/cm2/AA EXT-MEDIUM EMISSION LINE NEBULA STAR FORMING REGION YES This aperture is set relative to the aperture in program 12583, which was centered on the brightest UV cluster in galaxy LARS08. Aperture L08A5 should be shifted by dRA=+3.6 arcsec, dDEC=-7.2 arcsec fron the brightest UV cluster in the acquisition image. J2000 f_acs-sbc_f125lp(1426.5AA)= 1.48e-16 erg/s/cm2/AA EXT-MEDIUM EMISSION LINE NEBULA STAR FORMING REGION YES This aperture is set relative to the aperture in program 12583, which was centered on the brightest UV cluster in galaxy LARS08. Aperture L08A6 should be shifted by dRA=+7.2 arcsec, dDEC=-7.2 arcsec fron the brightest UV cluster in the acquisition image. J2000 f_acs-sbc_f125lp(1426.5AA)= 4.12e-17 erg/s/cm2/AA EXT-MEDIUM EMISSION LINE NEBULA STAR FORMING REGION YES This aperture is set relative to the aperture in program 12583, which was centered on the brightest UV cluster in galaxy LARS08. Aperture L08A7 should be shifted by dRA=-3.6 arcsec, dDEC=-3.6 arcsec fron the brightest UV cluster in the acquisition image. J2000 f_acs-sbc_f125lp(1426.5AA)= 9.60e-17 erg/s/cm2/AA EXT-MEDIUM EMISSION LINE NEBULA STAR FORMING REGION YES This aperture is set relative to the aperture in program 12583, which was centered on the brightest UV cluster in galaxy LARS08. Aperture L08A8 should be shifted by dRA=0 arcsec, dDEC=-3.6 arcsec fron the brightest UV cluster in the acquisition image. J2000 f_acs-sbc_f125lp(1426.5AA)= 2.78e-16 erg/s/cm2/AA EXT-MEDIUM EMISSION LINE NEBULA STAR FORMING REGION YES This aperture is set relative to the aperture in program 12583, which was centered on the brightest UV cluster in galaxy LARS08. Aperture L08A9 should be shifted by dRA=+3.6 arcsec, dDEC=-3.6 arcsec fron the brightest UV cluster in the acquisition image. J2000 f_acs-sbc_f125lp(1426.5AA)= 2.78e-16 erg/s/cm2/AA EXT-MEDIUM EMISSION LINE NEBULA STAR FORMING REGION YES This aperture is set relative to the aperture in program 12583, which was centered on the brightest UV cluster in galaxy LARS08. Aperture L08A10 should be shifted by dRA=+7.2 arcsec, dDEC=-3.6 arcsec fron the brightest UV cluster in the acquisition image. J2000 f_acs-sbc_f125lp(1426.5AA)= 2.09e-17 erg/s/cm2/AA EXT-MEDIUM EMISSION LINE NEBULA STAR FORMING REGION YES This aperture is set relative to the aperture in program 12583, which was centered on the brightest UV cluster in galaxy LARS08. Aperture L08A11 should be shifted by dRA=+3.0 arcsec, dDEC=0 arcsec fron the brightest UV cluster in the acquisition image. J2000 f_acs-sbc_f125lp(1426.5AA)= 4.41e-16 erg/s/cm2/AA EXT-MEDIUM EMISSION LINE NEBULA STAR FORMING REGION NO This target is used as a reference to the position of the other apertures. We will not acquire spectra for this target. J2000 f_nuv-acq= 5.20e-16 erg/s/cm2/AA COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G130M 1327 /private/var/folders/xf/gdnc5b2x6jjdr7g00v0lcx740000gn/T/OPVisit14629146605753508738.xml 1786752120870 The scheduling data was generated by CASM 34.2. 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CASM was run in Phase II mode. (Tic-Visit :proposal-id 18361 :visit-id "08" :proposal-version -1 :trans-version "20260618" :date "14-Aug-2026 17:03:09.0" :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 626496 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 18361 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 18361 :visit-id "08" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2597 :al-overhead-at-end 0 :internal-dur-at-end 2292 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2977 :pcs-gap 0 ) (Tic-Orbit :proposal-id 18361 :visit-id "08" :orbit-number 2 :pcs-time 380 :si-vis-utilization 2597 :al-overhead-at-end 0 :internal-dur-at-end 613 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2977 :pcs-gap 0 ) true 2 0 /private/var/folders/xf/gdnc5b2x6jjdr7g00v0lcx740000gn/T/OPVisit4363759774876108870.xml 1786752219777 The scheduling data was generated by CASM 34.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 18361 :visit-id "09" :proposal-version -1 :trans-version "20260618" :date "14-Aug-2026 17:03:39.0" :trans-errors '(:WARNINGS 2 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 3 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 939728 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 18361 :visit-id "09" :obset-id "09" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 18361 :visit-id "09" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2597 :al-overhead-at-end 0 :internal-dur-at-end 304 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2977 :pcs-gap 0 ) (Tic-Orbit :proposal-id 18361 :visit-id "09" :orbit-number 2 :pcs-time 380 :si-vis-utilization 2597 :al-overhead-at-end 0 :internal-dur-at-end 2292 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2977 :pcs-gap 0 ) (Tic-Orbit :proposal-id 18361 :visit-id "09" :orbit-number 3 :pcs-time 380 :si-vis-utilization 2597 :al-overhead-at-end 0 :internal-dur-at-end 613 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2977 :pcs-gap 0 ) true 3 0 /private/var/folders/xf/gdnc5b2x6jjdr7g00v0lcx740000gn/T/OPVisit7670162730657589207.xml 1786752232112 The scheduling data was generated by CASM 34.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 18361 :visit-id "10" :proposal-version -1 :trans-version "20260618" :date "14-Aug-2026 17:03:51.0" :trans-errors '(:WARNINGS 2 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 3 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 922304 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 18361 :visit-id "10" :obset-id "10" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 18361 :visit-id "10" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2597 :al-overhead-at-end 0 :internal-dur-at-end 2292 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2977 :pcs-gap 0 ) (Tic-Orbit :proposal-id 18361 :visit-id "10" :orbit-number 2 :pcs-time 380 :si-vis-utilization 2597 :al-overhead-at-end 0 :internal-dur-at-end 2292 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2977 :pcs-gap 0 ) (Tic-Orbit :proposal-id 18361 :visit-id "10" :orbit-number 3 :pcs-time 380 :si-vis-utilization 2597 :al-overhead-at-end 0 :internal-dur-at-end 613 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2977 :pcs-gap 0 ) true 3 0 /private/var/folders/xf/gdnc5b2x6jjdr7g00v0lcx740000gn/T/OPVisit16179887200816528462.xml 1786752276246 The scheduling data was generated by CASM 34.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 18361 :visit-id "11" :proposal-version -1 :trans-version "20260618" :date "14-Aug-2026 17:04:36.0" :trans-errors '(:WARNINGS 2 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 3 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 939728 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 18361 :visit-id "11" :obset-id "11" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 18361 :visit-id "11" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2597 :al-overhead-at-end 0 :internal-dur-at-end 304 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2977 :pcs-gap 0 ) (Tic-Orbit :proposal-id 18361 :visit-id "11" :orbit-number 2 :pcs-time 380 :si-vis-utilization 2597 :al-overhead-at-end 0 :internal-dur-at-end 2292 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2977 :pcs-gap 0 ) (Tic-Orbit :proposal-id 18361 :visit-id "11" :orbit-number 3 :pcs-time 380 :si-vis-utilization 2597 :al-overhead-at-end 0 :internal-dur-at-end 613 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2977 :pcs-gap 0 ) true 3 0 /private/var/folders/xf/gdnc5b2x6jjdr7g00v0lcx740000gn/T/OPVisit5838387167608045148.xml 1786752286120 The scheduling data was generated by CASM 34.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 18361 :visit-id "12" :proposal-version -1 :trans-version "20260618" :date "14-Aug-2026 17:04:45.0" :trans-errors '(:WARNINGS 2 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 3 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 922304 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 18361 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 18361 :visit-id "12" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2597 :al-overhead-at-end 0 :internal-dur-at-end 2292 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2977 :pcs-gap 0 ) (Tic-Orbit :proposal-id 18361 :visit-id "12" :orbit-number 2 :pcs-time 380 :si-vis-utilization 2597 :al-overhead-at-end 0 :internal-dur-at-end 2292 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2977 :pcs-gap 0 ) (Tic-Orbit :proposal-id 18361 :visit-id "12" :orbit-number 3 :pcs-time 380 :si-vis-utilization 2597 :al-overhead-at-end 0 :internal-dur-at-end 613 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2977 :pcs-gap 0 ) true 3 0