0Assigned ID: 7045
----- Attempting Submission 1 (Tue Apr 14 01:30:18 GMT 2026) -----
HST Phase I Proposal 7045 successfully submitted.
Receipt: # 7045-1Full taget list complete. Changed to MIRROR A for ACQ IMAGE. Included quasar SED shape and redshift in the calculation.
Two targets have low redshift galaxies at z~0.11 and in the proposal had the G130M/1096 selected. I've changed those to the 1222. This does not change the science since little
to no throughput would be obtained below ~1100A. Having a 1222 actually increases the science that can be done. If you have any questions please let me know.-44986808----- Attempting Submission 1 (Wed Aug 12 04:58:09 GMT 2026) -----
HST Phase II Proposal 18431 successfully submitted.
Receipt: # 18431-1
----- Attempting Submission 2 (Mon Aug 17 05:58:19 GMT 2026) -----
HST Phase II Proposal 18431 successfully submitted.
Receipt: # 18431-2
----- Attempting Submission 3 (Thu Aug 27 16:01:44 GMT 2026) -----Minor Axis, Major Insight: A COS Survey of Multi-Phase Galactic OutflowsGalactic outflows are a key regulator of galaxy evolution, yet their physical structure, metal content, and radial evolution remain poorly constrained observationally. We propose to use HST/COS far-ultraviolet spectroscopy to characterize multi-phase outflowing gas in the circumgalactic medium of star-forming galaxies.
Our program targets nine inclined, isolated, star-forming disk galaxies at z~0.2, probed by background quasars along their minor axes at projected distances of 12-49 kpc. Each sightline already exhibits MgII absorption at the galaxy redshift, enabling a focused study of systems in which cool circumgalactic gas is known to be present. The COS data will measure the kinematics, metallicity, and ionization structure of the gas, from HI and low ions to OVI, thereby constraining the multi-phase nature of galactic winds across the inner and outer circumgalactic medium.
These observations will test the kinematic coupling of the cool and warm-hot phases with radius, provide empirical benchmarks for distinguishing among competing wind-driving scenarios, and constrain how mass and metals are transported from galaxies into their halos by combining the COS spectroscopy with existing ground-based galaxy and quasar data. This program will provide a well-characterized minor-axis dataset for clarifying how galactic outflows shape the physical and chemical structure of the circumgalactic medium.QSO Spectroscopy with COS: Our science analysis is focused on measuring (a) the kinematics of low, intermediate, and high-ionization CGM gas using both the pixel-velocity two-point correlation function (TPCF) and Voigt profile (VP) fitting and (b) measuring the metallicities from VP column densities and ionization modeling. From these measurements, we will then quantitatively characterize the differences and/or similarities major axis and minor axis CGM, with 9 minor axis (those proposed for here) and 9 major axis galaxies (from PID 17541).
We use the G130M grating with a single optimized central wavelength per target to cover a diverse range of low-ionization metal lines (OI, CII, NII, FeII, SiII), intermediate-ionization lines (NIII and CIII) and the OVI high-ionization lines. For 5 galaxies, we cover the entire Lyman series from Lybeta to the break and for
four galaxies from Lybeta to Lytau . Since all absorbers are expected to have logN(HI) > 17, we would gain little-to-no constraints from the highly-saturated Ly-alpha lines. We used the COS ETC to estimate exposure times required to achieve signal-to-noise ratios (S/N) of 12 per resolution element after binning by three in the dispersion direction, yielding 2.7 pixels per resolution element. For our binning at S/N = 12, COS delivers a 3-sigma detection threshold of 25 mA.
The coordinates of our point-source targets are much better then 0.5". We thus adopt the minimal approach to target acquisition. We use the NUV imager with MIRRORA in ACQ IMAGE mode through the PSA aperture. Exposure times were determined using the COS ETC to ensure we achieve the recommended SNR of 20 for target acquisitions. The NUV magnitudes were obtain from GALEX.
Our targets are observed using both A and B stripes of the G130 M. Five of our targets use the 1222 grating center. Two of our targets are optimal with the 1096 centering (G4O, G6O) and two are optimal for the 1291 center (G2O, G9O). For all gratings, we obtain exposures at all FP-POS setting. We move these in the forward direction in order to minimize overhead. For the 1291 center, we use only FP-POS=3,4 in order to avoid segment reconfiguration overhead. For all exposures, we adopt the recommended TIME-TAG photon counting with FLASH=yes, and adopt a standard BUFFER-TIME=6000 seconds based on the count rates of our targets. All targets are exposed through the PSA aperture and guidance is set to FINE. For Phase I, exposure time estimates were obtained using the COS ETC for a point source with published GALEX FUV fluxes, and employed average Galactic extinction, standard zodiacal light normalizations, standard earth-shine light normalizations, and average air glow.
Six of the targets have greater than 4 orbits and may need to be split.Prof. Glenn Kacprzak is a leader in morphological modeling and is one of the leaders in demonstrating the orientation dependence of the CGM. He is an expert in obtaining galaxy kinematics and rotation curves and comparing them to absorption-line kinematics. He is also experienced in fitting absorption-line systems using COS and HIRES/UVES data. In addition, Prof. Kacprzak has direct access to Keck through Swinburne's partnership with the observatory. He has published over 30 papers in the last three years, all of which include some component of HST data and involve galaxy evolution and CGM studies. Dr. Benjamin Oppenheimer is an expert in computational hydrodynamic simulations of galaxies and their gaseous environments. He specializes in understanding how the physical and evolutionary properties of the IGM and CGM can be constrained through observational campaigns. He is particularly experienced in interpreting COS ultraviolet data. He has served as principal investigator on five HST theory grants and as co-investigator on more than a dozen HST General Observer programs. Associate Prof. Nikole Nielsen is an expert in creating absorption-line catalogs and examining the kinematics of absorption systems. She has developed her own methods to quantify the internal velocity dispersions of the CGM using COS and HIRES/UVES data. She is also experienced in fitting absorption-line systems and modeling their metallicities. Kaustubh Rajesh Gupta is a second-year PhD student studying the CGM using gravitational lenses and has experience interpreting gas-flow signatures in low-ionization gas. Sarbeswar Das is a first-year PhD student who will be working on galaxy outflows, which relates directly to this proposal, and these data would form the basis of his thesis. He also has expertise in understanding the connection between galaxies and their low-ionization CGM.Intergalactic Medium and the Circumgalactic Medium6falsetruefalsefalsefalsefalsefalseSUPPORTEDGALAXYQUASARNOThis object was generated by the targetselector and retrieved from the SIMBAD database.SDSSJ224013.41-083628.7VV2006-J224013.4-083628J2000J2000FUV(GALEX AB) = 19.27, NUV(GALEX AB) =18.30234GALAXYQUASARNOThis object was generated by the targetselector and retrieved from the SIMBAD database.QSO-B1429+1008SDSSJ143216.78+095519.2J2000J2000FUV(GALEX AB) = 18.44, NUV(GALEX AB) =17.84695GALAXYQUASARNOThis object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.VV98-J154956.9+070045SDSSJ154956.87+070044.9J2000J2000FUV(GALEX AB) = 18.62 NUV(GALEX AB) =17.70879GALAXYQUASARNOThis object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.2MASS-J09560622+1238016SDSSJ095606.26+123802.5J2000J2000FUV(GALEX AB) = 19.47 NUV(GALEX AB) =18.658GALAXYQUASARNOThis object was generated by the targetselector and retrieved from the SIMBAD database.VV2006-J122934.7+100710SDSSJ122934.66+100709.9J2000J2000FUV(GALEX AB) = 19.49 NUV(GALEX AB) =18.79101GALAXYQUASARNOThis object was generated by the targetselector and retrieved from the SIMBAD database.LBQS-2231-0048SDSSJ223359.93-003315.8J2000J2000FUV(GALEX AB) = 19.34 NUV(GALEX AB) =18.21192GALAXYQUASARNOThis object was generated by the targetselector and retrieved from the SIMBAD database.2MASS-J15311298+0911389SDSSJ153112.97+091138.6J2000J2000FUV(GALEX AB) = 19.59 NUV(GALEX AB) =18.39993GALAXYQUASARNOThis object was generated by the targetselector and retrieved from the SIMBAD database.2MASS-J14040216+1028005SDSSJ140402.16+102800.6J2000J2000FUV(GALEX AB) = 19.39 NUV(GALEX AB) =17.78797GALAXYQUASARNOThis object was generated by the targetselector and retrieved from the SIMBAD database.VV2006-J093537.0+112408SDSSJ093536.98+112408.0J2000J2000FUV(GALEX AB) = 19.96 NUV(GALEX AB) =18.89013COS/FUVSpectroscopicNoNoG130M1222COS/FUVSpectroscopicNoNoG130M1291COS/FUVSpectroscopicNoNoG130M1222COS/FUVSpectroscopicNoNoG130M1096COS/FUVSpectroscopicNoNoG130M1222COS/FUVSpectroscopicNoNoG130M1096COS/FUVSpectroscopicNoNoG130M1222COS/FUVSpectroscopicNoNoG130M1222COS/FUVSpectroscopicNoNoG130M1291/Users/gkacprzak/Desktop/HST/Cycle34/OP-cache/COS-outflows-v01.xmlThe scheduling data was generated by CASM 34.2.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 18431
:visit-id "01"
:proposal-version -1
:trans-version "20260618"
:date "17-Aug-2026 15:48:46.0"
:trans-errors '(:WARNINGS 0 :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 278640
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18431
:visit-id "01"
:obset-id "01"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18431
:visit-id "01"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "01"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "01"
:orbit-number 3
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 547
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)true30BFT=20,174 BT=2/3*BFT=13449
expected SNR in this exposure is SNR = 2.5779 (per resolution element) at wavelength 1310.00 ABFT=20,174 BT=2/3*BFT=13449
expected SNR in this exposure is SNR = 2.8635 (per resolution element) at wavelength 1310.00 ABFT=20,174 BT=2/3*BFT=13449
expected SNR in this exposure is SNR = 2.8635 (per resolution element) at wavelength 1310.00 A/Users/gkacprzak/Desktop/HST/Cycle34/OP-cache/COS-outflows-v02.xmlThe scheduling data was generated by CASM 34.2.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 18431
:visit-id "02"
:proposal-version -1
:trans-version "20260618"
:date "17-Aug-2026 12:25:07.0"
: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 130736
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18431
:visit-id "02"
:obset-id "02"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18431
:visit-id "02"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "02"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 506
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)true20BFT=7,745 BT=2/3*BFT=5163
expected SNR in this exposure is SNR = 4.0607 (per resolution element) at wavelength 1310.00 ABFT=7,745 BT=2/3*BFT=5163
expected SNR in this exposure is SNR = 4.5478 (per resolution element) at wavelength 1310.00 A/Users/gkacprzak/Desktop/HST/Cycle34/OP-cache/COS-outflows-v03.xmlThe scheduling data was generated by CASM 34.2.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 18431
:visit-id "03"
:proposal-version -1
:trans-version "20260618"
:date "17-Aug-2026 15:48:51.0"
:trans-errors '(:WARNINGS 0 :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 278640
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18431
:visit-id "03"
:obset-id "03"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18431
:visit-id "03"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "03"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "03"
:orbit-number 3
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 547
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)true30BFT=17,838 BT=2/3*BFT=5288
expected SNR in this exposure is SNR = 3.5823 (per resolution element) at wavelength 1310.00 ABFT=17,838 BT=2/3*BFT=11892
expected SNR in this exposure is SNR =3.9792 (per resolution element) at wavelength 1310.00 ABFT=17,838 BT=2/3*BFT=11892
expected SNR in this exposure is SNR = 3.9792 (per resolution element) at wavelength 1310.00 A/private/var/folders/5j/9ttn910d3t98rj4zly83nv2r0000gs/T/OPVisit11546464898235461621.xmlThe scheduling data was generated by CASM 34.2.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 18431
:visit-id "04"
:proposal-version -1
:trans-version "20260618"
:date "28-Aug-2026 01:46:29.0"
: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 365696
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18431
:visit-id "04"
:obset-id "04"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18431
:visit-id "04"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "04"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "04"
:orbit-number 3
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "04"
:orbit-number 4
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 547
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)true40BFT=20,523 BT=2/3*BFT=13682
expected SNR in this exposure is SNR = 2.3915 (per resolution element) at wavelength 1310.00 A
Changed from 1096 to 1222 since the absorbing galaxy redshift is at z=0.126 and absorption below 1100A will be not detected. Science unchanged and now even more optimised.BFT=20,523 BT=2/3*BFT=13682
expected SNR in this exposure is SNR = 2.6728 (per resolution element) at wavelength 1310.00 A
Changed from 1096 to 1222 since the absorbing galaxy redshift is at z=0.126 and absorption below 1100A will be not detected. Science unchanged and now even more optimised.BFT=20,523 BT=2/3*BFT=13682
expected SNR in this exposure is SNR = 2.6728 (per resolution element) at wavelength 1310.00 A
Changed from 1096 to 1222 since the absorbing galaxy redshift is at z=0.126 and absorption below 1100A will be not detected. Science unchanged and now even more optimised.BFT=20,523 BT=2/3*BFT=13682
expected SNR in this exposure is SNR = 2.6728 (per resolution element) at wavelength 1310.00 A
Changed from 1096 to 1222 since the absorbing galaxy redshift is at z=0.126 and absorption below 1100A will be not detected. Science unchanged and now even more optimised./private/var/folders/5j/9ttn910d3t98rj4zly83nv2r0000gs/T/OPVisit1499375151995271012.xmlThe scheduling data was generated by CASM 34.2.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 18431
:visit-id "10"
:proposal-version -1
:trans-version "20260618"
:date "28-Aug-2026 01:46:19.0"
:trans-errors '(:WARNINGS 0 :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 278640
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18431
:visit-id "10"
:obset-id "10"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18431
:visit-id "10"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "10"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "10"
:orbit-number 3
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 547
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)true30BFT=20,523 BT=2/3*BFT=13682
expected SNR in this exposure is SNR = 2.3915 (per resolution element) at wavelength 1310.00 A
Changed from 1096 to 1222 since the absorbing galaxy redshift is at z=0.126 and absorption below 1100A will be not detected. Science unchanged and now even more optimised.BFT=20,523 BT=2/3*BFT=13682
expected SNR in this exposure is SNR = 2.6728 (per resolution element) at wavelength 1310.00 A
Changed from 1096 to 1222 since the absorbing galaxy redshift is at z=0.126 and absorption below 1100A will be not detected. Science unchanged and now even more optimised.BFT=20,523 BT=2/3*BFT=13682
expected SNR in this exposure is SNR = 2.6728 (per resolution element) at wavelength 1310.00 A
Changed from 1096 to 1222 since the absorbing galaxy redshift is at z=0.126 and absorption below 1100A will be not detected. Science unchanged and now even more optimised./private/var/folders/5j/9ttn910d3t98rj4zly83nv2r0000gs/T/OPVisit8992817522428557885.xmlThe scheduling data was generated by CASM 34.2.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 18431
:visit-id "05"
:proposal-version -1
:trans-version "20260618"
:date "28-Aug-2026 01:51:07.0"
: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 365696
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18431
:visit-id "05"
:obset-id "05"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18431
:visit-id "05"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "05"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "05"
:orbit-number 3
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "05"
:orbit-number 4
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 547
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)true40BFT=20,512 BT=2/3*BFT=13675
expected SNR in this exposure is SNR = 2.2650 (per resolution element) at wavelength 1310.00 ABFT=20,512 BT=2/3*BFT=13675
expected SNR in this exposure is SNR = 2.5185 (per resolution element) at wavelength 1310.00 ABFT=20,512 BT=2/3*BFT=13675
expected SNR in this exposure is SNR = 2.5185 (per resolution element) at wavelength 1310.00 ABFT=20,512 BT=2/3*BFT=13675
expected SNR in this exposure is SNR = 2.5185 (per resolution element) at wavelength 1310.00 A/private/var/folders/5j/9ttn910d3t98rj4zly83nv2r0000gs/T/OPVisit6106543681436705197.xmlThe scheduling data was generated by CASM 34.2.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 18431
:visit-id "11"
:proposal-version -1
:trans-version "20260618"
:date "28-Aug-2026 01:51:14.0"
:trans-errors '(:WARNINGS 0 :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 278640
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18431
:visit-id "11"
:obset-id "11"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18431
:visit-id "11"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "11"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "11"
:orbit-number 3
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 547
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)true30BFT=20,512 BT=2/3*BFT=13675
expected SNR in this exposure is SNR = 2.2650 (per resolution element) at wavelength 1310.00 ABFT=20,512 BT=2/3*BFT=13675
expected SNR in this exposure is SNR = 2.5185 (per resolution element) at wavelength 1310.00 ABFT=20,512 BT=2/3*BFT=13675
expected SNR in this exposure is SNR = 2.5185 (per resolution element) at wavelength 1310.00 A/private/var/folders/5j/9ttn910d3t98rj4zly83nv2r0000gs/T/OPVisit3403438765153672044.xmlThe scheduling data was generated by CASM 34.2.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 18431
:visit-id "06"
:proposal-version -1
:trans-version "20260618"
:date "28-Aug-2026 01:57:39.0"
:trans-errors '(:WARNINGS 0 :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 278640
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18431
:visit-id "06"
:obset-id "06"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18431
:visit-id "06"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "06"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "06"
:orbit-number 3
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 547
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)true30BFT=20,235 BT=2/3*BFT=13490
expected SNR in this exposure is SNR = 2.5807 (per resolution element) at wavelength 1310.00 A
Changed from 1096 to 1222 since the absorbing galaxy redshift is at z=0.1162 and absorption below 1100A will be not detected. Science unchanged and now even more optimised.BFT=20,235 BT=2/3*BFT=13490
expected SNR in this exposure is SNR = 2.8666 (per resolution element) at wavelength 1310.00 A
Changed from 1096 to 1222 since the absorbing galaxy redshift is at z=0.1162 and absorption below 1100A will be not detected. Science unchanged and now even more optimised.BFT=20,235 BT=2/3*BFT=13490
expected SNR in this exposure is SNR = 2.8666 (per resolution element) at wavelength 1310.00 A
Changed from 1096 to 1222 since the absorbing galaxy redshift is at z=0.1162 and absorption below 1100A will be not detected. Science unchanged and now even more optimised./private/var/folders/5j/9ttn910d3t98rj4zly83nv2r0000gs/T/OPVisit322961007399282554.xmlThe scheduling data was generated by CASM 34.2.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 18431
:visit-id "13"
:proposal-version -1
:trans-version "20260618"
:date "28-Aug-2026 01:58:06.0"
:trans-errors '(:WARNINGS 0 :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 278640
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18431
:visit-id "13"
:obset-id "13"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18431
:visit-id "13"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "13"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "13"
:orbit-number 3
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 547
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)true30BFT=20,235 BT=2/3*BFT=13490
expected SNR in this exposure is SNR = 2.5807 (per resolution element) at wavelength 1310.00 A
Changed from 1096 to 1222 since the absorbing galaxy redshift is at z=0.1162 and absorption below 1100A will be not detected. Science unchanged and now even more optimised.BFT=20,235 BT=2/3*BFT=13490
expected SNR in this exposure is SNR = 2.8666 (per resolution element) at wavelength 1310.00 A
Changed from 1096 to 1222 since the absorbing galaxy redshift is at z=0.1162 and absorption below 1100A will be not detected. Science unchanged and now even more optimised.BFT=20,235 BT=2/3*BFT=13490
expected SNR in this exposure is SNR = 2.8666 (per resolution element) at wavelength 1310.00 A
Changed from 1096 to 1222 since the absorbing galaxy redshift is at z=0.1162 and absorption below 1100A will be not detected. Science unchanged and now even more optimised./Users/gkacprzak/Desktop/HST/Cycle34/OP-cache/COS-outflows-v07.xmlThe scheduling data was generated by CASM 34.2.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 18431
:visit-id "07"
:proposal-version -1
:trans-version "20260618"
:date "17-Aug-2026 14:12:25.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 5
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 452752
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18431
:visit-id "07"
:obset-id "07"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18431
:visit-id "07"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "07"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "07"
:orbit-number 3
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "07"
:orbit-number 4
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "07"
:orbit-number 5
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 547
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)true50BFT=20,831 BT=2/3*BFT=13887
expected SNR in this exposure is SNR = 2.1743 (per resolution element) at wavelength 1310.00 ABFT=20,831 BT=2/3*BFT=13887
expected SNR in this exposure is SNR = 2.4164 (per resolution element) at wavelength 1310.00 ABFT=20,831 BT=2/3*BFT=13887
expected SNR in this exposure is SNR = 2.4164 (per resolution element) at wavelength 1310.00 ABFT=20,831 BT=2/3*BFT=13887
expected SNR in this exposure is SNR = 2.4164 (per resolution element) at wavelength 1310.00 ABFT=20,831 BT=2/3*BFT=13887
expected SNR in this exposure is SNR = 2.4164 (per resolution element) at wavelength 1310.00 A/Users/gkacprzak/Desktop/HST/Cycle34/OP-cache/COS-outflows-v08.xmlThe scheduling data was generated by CASM 34.2.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 18431
:visit-id "08"
:proposal-version -1
:trans-version "20260618"
:date "17-Aug-2026 14:22:52.0"
: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 365696
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18431
:visit-id "08"
:obset-id "08"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18431
:visit-id "08"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "08"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "08"
:orbit-number 3
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "08"
:orbit-number 4
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 547
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)true40BFT=20,379 BT=2/3*BFT=13586
expected SNR in this exposure is SNR = 2.5686 (per resolution element) at wavelength 1310.00 ABFT=20,379 BT=2/3*BFT=13586
expected SNR in this exposure is SNR = 2.8532 (per resolution element) at wavelength 1310.00 ABFT=20,379 BT=2/3*BFT=13586
expected SNR in this exposure is SNR = 2.8532 (per resolution element) at wavelength 1310.00 ABFT=20,379 BT=2/3*BFT=13586
expected SNR in this exposure is SNR = 2.8532 (per resolution element) at wavelength 1310.00 A/private/var/folders/5j/9ttn910d3t98rj4zly83nv2r0000gs/T/OPVisit16669870385347392863.xmlThe scheduling data was generated by CASM 34.2.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 18431
:visit-id "09"
:proposal-version -1
:trans-version "20260618"
:date "28-Aug-2026 01:55:18.0"
: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 226624
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18431
:visit-id "09"
:obset-id "09"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18431
:visit-id "09"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "09"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "09"
:orbit-number 3
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "09"
:orbit-number 4
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 497
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)true40BFT=8,742 BT=2/3*BFT=5828
expected SNR in this exposure is SNR = 1.9117 (per resolution element) at wavelength 1310.00 ABFT=8,742 BT=2/3*BFT=5828
expected SNR in this exposure is SNR = 2.0806 (per resolution element) at wavelength 1310.00 ABFT=8,742 BT=2/3*BFT=5828
expected SNR in this exposure is SNR = 2.0806 (per resolution element) at wavelength 1310.00 ABFT=8,742 BT=2/3*BFT=5828
expected SNR in this exposure is SNR = 2.0806 (per resolution element) at wavelength 1310.00 A/private/var/folders/5j/9ttn910d3t98rj4zly83nv2r0000gs/T/OPVisit361036507301864637.xmlThe scheduling data was generated by CASM 34.2.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 18431
:visit-id "12"
:proposal-version -1
:trans-version "20260618"
:date "28-Aug-2026 01:54:47.0"
:trans-errors '(:WARNINGS 0 :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 174336
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 18431
:visit-id "12"
:obset-id "12"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 18431
:visit-id "12"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "12"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 2402
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 18431
:visit-id "12"
:orbit-number 3
:pcs-time 380
:si-vis-utilization 2487
:al-overhead-at-end 0
:internal-dur-at-end 497
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2867
:pcs-gap 0
)true30BFT=8,742 BT=2/3*BFT=5828
expected SNR in this exposure is SNR = 1.9117 (per resolution element) at wavelength 1310.00 ABFT=8,742 BT=2/3*BFT=5828
expected SNR in this exposure is SNR = 2.0806 (per resolution element) at wavelength 1310.00 ABFT=8,742 BT=2/3*BFT=5828
expected SNR in this exposure is SNR = 2.0806 (per resolution element) at wavelength 1310.00 A