0
Assigned ID: 5172
----- Attempting Submission 1 (Mon Mar 25 13:25:04 GMT 2024) -----
Hi Amber & John,
here's the revised Phase II for this program. See the "Proposal Description" for the changes:
(1) the four four duplicated targets replaced,
(2) exposure times of nine visits shortened to fit within the 45min limit.
Best wishes,
Boris
1681034416
----- Attempting Submission 1 (Wed Aug 14 14:10:27 GMT 2024) -----
----- Attempting Submission 2 (Thu Jan 09 14:20:04 GMT 2025) -----
The target confirmation tool keeps crashing after downloading a few finding charts.
A legacy survey for evolved planetary systems within 100pc
In just 25 years, we went from not knowing if the solar system is a fluke of Nature to realising that it is totally normal for stars to have planets. More remarkably, it is now clear that planet formation is a robust process, as rich multi-planet systems are found around stars more massive and less massive than the Sun. More recently, planetary systems have been identified in increasingly complex architectures, including circumbinary planets, wide binaries with planets orbiting one or both stellar components, and planets in triple stellar systems.
We have also learned that many planetary systems will survive the evolution of their host stars into the white dwarf phase. Small bodies are scattered by unseen planets into the gravitational field of the white dwarfs, tidally disrupt, form dust discs, and eventually accrete onto the white dwarf, where they can be spectroscopically detected. HST/COS has played a critical role in the study these evolved planetary systems, demonstrating that overall the bulk composition of the debris is rocky and resembles in composition the inner the solar system, including evidence for water-rich planetesimals.
Past observations of planetary systems at white dwarfs were limited to biased and incomplete samples. Here we propose a legacy HST survey of all white dwarfs within 100pc identified with Gaia to answer the following questions:
* How efficient is planet formation around 2-10Msun stars?
* What are the metallicities of the progenitors of debris-accreting white dwarfs?
* What is the fate of circumbinary planets?
* Can star-planet interactions generate magnetic fields in the white dwarf host?
============================================================================
Original submission: 2024-Aug-16
============================================================================
This program is a continuation of our previous snapshot surveys of white dwarfs (12169, 12474, 13652, 14077, 15073, 16011, 16642, 17420). The overall goal of this project is to identify white dwarfs that exhibit metal contamination, indicating the accretion of debris from tidally disrupted asteroids.
In this Cycle 32 program, we focus on obtaining COS far-ultraviolet spectroscopy of white dwarfs with temperatures in the range 15000-30000K, i.e. exploiting the diagnostic potential of the strong resonance lines in the far-ultraviolet.
The observations will be carried out with the G130M grating, which gives the best coverage of all important lines (O I 1150A, C III 1175A, Si II 1260/65A, C II 1330/35A, Si IV 1393/1403). The 1291A central wavelength places the detector gap in a line-free region.
The targets for this program were chosen from the catalogue of Gentile Fusillo et al. https://ui.adsabs.harvard.edu/abs/2021MNRAS.508.3877G who identified white dwarfs based on their Gaia astrometry and photometry, and determined their effective temperatures (Teff) and surface gravities (log g) using the Gaia data. Specifically, we selected white dwarfs with
* d<=100pc
* 15000K < Teff < 30000K
We removed from that list all white dwarfs that have been previously observed with COS/G130M, either in our snapshot programs, or other programs.
Next, we computed white dwarf model spectra for all potential targets, using the Teff and log g from the Gaia white dwarf catalogue, which in turn also fixes the white dwarf radii - in other words, the model spectra are on an absolute flux scale. We then scaled these models to the Gaia parallax, and finally computed synthetic magnitudes in the GALEX FUV band. Finally, we carried out all ETC simulations for the target acquisition and G130M spectroscopy, using the model spectra "unscaled", as the above procedure results in an ETC input as expected for the actual targts [minus the effect of reddening, which is low towards all targets within 100pc, but any small amount of reddening will slightly *reduce* the actually observed flux w.r.t. the input model - i.e. the input models are conservative in terms of upper flux level].
To evaluate how good (and safe!) the synthetic magnitudes are, we cross-matched the with the GALEX data base and compared the synthetic vs observed GALEX FUV magnitudes. We find that the synthetic magnitudes are brighter than the observed ones, typically by ~0.2mag. Therefore, we conclude that the ETC simulations using the synthetic FUV magnitudes are on the conservative side. This procedure has been well-tested in Snapshot programs 16642 &17420.
The model spectra used for the ETC simulations are here: https://drive.google.com/drive/folders/1TIiBwLpgA2kny-NW5R3gMdorKtnvqQt4?usp=sharing
The targets 100 - 149 / Visits A0 - AJ are 50 new targets (reduced w.r.t. the orignal allocation as per Julia Roman-Duval's e-mail from 29-July-2024). We used DA white dwarf models for the appropriate temperature / surface gravity of each star to carry out the target acquisition and spectroscopic ETC calculations. To comply with the S/N restrictions, we implemented these 50 visits as follows:
(1) we enforced a maximum S/N=30 across all visits.
(2) we set a maximum exposure time of 2 x 900s (FP-POS 3,4), the vast majority of the visits with a total of 1800s exposure time reach 20 < S/N < 30. Exceptions are visits BA, bla bla which fall below S/N=20, but we include those as they are massive white dwarfs that remain under-represented in our sample.
All 50 new targets were screened for nearby cool stars within 8" using the Gaia DR3 catalogues. Details are given in the comments box of each target, and a spreadsheet with the matching Gaia sources within 8" is available here:
https://docs.google.com/spreadsheets/d/1W0x_zvomyjAfhfyChKvDwtSH19Ocg0ALIdE92AmD5sU/edit?usp=sharing
============================================================================
Updates: 2025-Jan-07
============================================================================
Target replacements:
Visit A9: Replaced the duplicate target WDJ052950.25+523953.39 with the new target WDJ183751.12-725311.73.
Visit B2: Replaced the duplicate target WDJ165948.42+440104.04 with the new target WDJ055915.83+255450.61.
Visit B3: Replaced the duplicate target WDJ170145.15-524609.22 with the new target WDJ205037.82+424619.20.
Visit AF: Replaced the duplicate target WDJ205442.80-203925.93 with the new target WDJ155452.92-125306.70.
The properties of the four replacement targets are listed at the bottom of the two spreadsheets in
https://docs.google.com/spreadsheets/d/1W0x_zvomyjAfhfyChKvDwtSH19Ocg0ALIdE92AmD5sU/edit?usp=sharing
Shortened exposure times
Visit B4: shortened exposure times to fit within the 45min (2700sec) limit for SNAPs.
Visit BB: shortened exposure times to fit within the 45min (2700sec) limit for SNAPs.
Visit AW: shortened exposure times to fit within the 45min (2700sec) limit for SNAPs.
Visit AX: shortened exposure times to fit within the 45min (2700sec) limit for SNAPs.
Visit AY: shortened exposure times to fit within the 45min (2700sec) limit for SNAPs.
Visit AO: shortened exposure times to fit within the 45min (2700sec) limit for SNAPs.
Visit AQ: shortened exposure times to fit within the 45min (2700sec) limit for SNAPs.
Visit AB: shortened exposure times to fit within the 45min (2700sec) limit for SNAPs.
Visit AC: shortened exposure times to fit within the 45min (2700sec) limit for SNAPs.
Hermes is an expert on white dwarf stars, especially those in wide binaries as well as those with photometric variability.
Gaensicke has been PI of 20 HST programs, carrying out far-ultraviolet spectroscopy of white dwarfs, including large, medium, small GO programs and several snapshot programs. He has in-depth experience in the analysis and interpretation of the observations of accreting white dwarfs, both in binary systems, and evolved planetary systems. He will implement the observations, and lead the analysis.
Gentile Fusillo has been using large astronomical surveys to (a) identify white dwarfs, most recently producing the first all-sky catalogue of white dwarfs using Gaia DR2, and (b) to then search for white dwarfs with signature of evolved planetary systems. He identified the targets of this proposal.
Hollands is an expert in the analysis of strongly magnetic white dwarfs.
Koester has developed the model atmosphere code that will be used for this project, and he will provide guidance on the use of the code.
Manser is an expert on gaseous debris disks at white dwarfs, and he will contribute to the discussion of the line morphology. He recently identified the first spectroscopic signature of a solid planetesimal.
Sahu is an expert on photometric modelling of white dwarfs, particularly in the ultraviolet.
Toloza is an expert in the analysis of COS time-tag observations. She will carry out the data reduction and the computation of white dwarf model atmospheres using the code of Detlev Koester.
Veras is a dynamicist with a long track record at simulating the late evolution of planetary systems.
Williams is a PhD candidate studying COS observations of white dwarfs accreting rocky debris.
Exoplanets and Exoplanet Formation
0
false
SUPPORTED
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.14
STAR
DA
NO
New Cycle 32 target.
Two faint distant background stars (separations 5", 2.7", G=20.3, G=19.3) - neither are nearby cool stars.
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.10
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.19
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=15.29 SYNTHETIC_FUV=15.03
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=15.19 SYNTHETIC_FUV=14.94
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.10
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=15.07 SYNTHETIC_FUV=14.93
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=14.98
STAR
DA
NO
New Cycle 32 target.
One faint distant background star (separation 5.4", G=19.8) - not a nearby cool star.
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.15
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.14
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=14.82 SYNTHETIC_FUV=15.08
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=15.27 SYNTHETIC_FUV=15.11
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=15.04 SYNTHETIC_FUV=14.99
STAR
DA
NO
New Cycle 32 target.
Two faint distant background stars (separations 2.7", 7.4", G=19.0, G=18.2) - neither are nearby cool stars.
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=14.97
STAR
DA
NO
New Cycle 32 target.
One faint distant background star (separation 7.4", G=19.4) - not a nearby cool star.
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=14.98
STAR
DA
NO
New Cycle 32 target.
Two faint distant background stars (separations 5", 5.2", G=19.6, G=17.7) - neither are nearby cool stars.
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=14.99
STAR
DA
NO
New Cycle 32 target.
One faint distant background star (separation 7.8", G=18.8) - not a nearby cool star.
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=15.63 SYNTHETIC_FUV=15.13
STAR
DA
NO
New Cycle 32 target.
One faint distant background star (separation 5.3", G=21.1) - not a nearby cool star.
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.11
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=15.77 SYNTHETIC_FUV=15.13
STAR
DA
NO
New Cycle 32 target.
One faint distant background star (separation 4.5", G=20.9) - not a nearby cool star.
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=16.02 SYNTHETIC_FUV=15.20
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.00
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=15.31 SYNTHETIC_FUV=15.13
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.13
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.03
STAR
DA
NO
New Cycle 32 target.
Common proper motion companion (separation 4.5", G=11.3, Bp=12.0, Rp=10.5, Gaia DR3 source_id = 3685072667134560896) The magnitude and colour implies Teff~4500K, not a cool active star.
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=15.32 SYNTHETIC_FUV=15.09
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=14.97
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=15.05 SYNTHETIC_FUV=14.95
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=15.02 SYNTHETIC_FUV=15.02
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.11
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=15.28 SYNTHETIC_FUV=15.06
STAR
DA
NO
New Cycle 32 target.
Faint (G=20) and distant (parallax=-1.35mas) object at 5.2" distance. Definitely not a low-mass star.
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.14
STAR
DA
NO
New Cycle 32 target.
Crowded field, eight distant faint (G=18.7-21.1) sources within 8", none of them are nearby, cool stars.
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.15
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.05
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=19.07 SYNTHETIC_FUV=15.35
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=15.17 SYNTHETIC_FUV=15.05
STAR
DA
NO
New Cycle 32 target.
Crowded field, 16 distant faint (G=15.1-20.2) sources within 8", none of them are nearby, cool stars. This target is in the Galactic plane (b=-2.7deg), some of the brighter sources are highly reddened distant background stars.
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.04
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=15.78 SYNTHETIC_FUV=15.01
STAR
DA
NO
New Cycle 32 target.
Two faint distant background stars (separations 6.3,6.7", G=20.6, 20.9) - neither are nearby cool stars.
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.54
STAR
DA
NO
New Cycle 32 target.
Crowded field, nine distant faint (G=17.6-20.7) sources within 8", none of them are nearby, cool stars. This target is in the Galactic plane (b=+1.5deg), some of the brighter sources are highly reddened distant background stars.
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC FUV=14.05
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.13
STAR
DA
NO
New Cycle 32 target.
Three faint distant background stars (separations 0.9", 4.4", 7.8", G=19.4, 19.1, 20.3) - neither are nearby cool stars.
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.10
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=15.29 SYNTHETIC_FUV=15.03
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=14.94
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=15.85 SYNTHETIC_FUV=15.71
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=14.99 SYNTHETIC_FUV=14.95
STAR
DA
NO
New Cycle 32 target.
Faint (G=18.3) and distant (parallax=0.28mas) object at 3.7" separation. Based on color and absolute magnitude, this is not a low-mass star.
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=15.35 SYNTHETIC_FUV=15.15
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=15.24 SYNTHETIC_FUV=15.10
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.01
STAR
DA
NO
New Cycle 32 target.
No Gaia sources within 8".
See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
SYNTHETIC_FUV=15.08
STAR
DA
NO
New Cycle 32 target.
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See https://docs.google.com/spreadsheets/d/1VJyGiZvhPd6IzTapTP4f3fmcNxTQ9ngohbc01tttWQw/edit?usp=sharing (17698 Companions tab).
J2000
GALEX_FUV=15.05 SYNTHETIC_FUV=15.05
COS/FUV
Spectroscopic
No
No
G130M
1291
COS/FUV
Spectroscopic
No
No
G130M
1291
COS/FUV
Spectroscopic
No
No
G130M
1291
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:pcs-visibility 3032
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vBA.xml
(Tic-Visit
:proposal-id 17698
:visit-id "BA"
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:trans-version "20240604"
:date "09-Jan-2025 13:44:01.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:number-of-orbits 1
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:data-volume 191440
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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)
(Tic-Orbit
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:pcs-time 380
:si-vis-utilization 2527
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3039
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vBB.xml
(Tic-Visit
:proposal-id 17698
:visit-id "BB"
:proposal-version -1
:trans-version "20240604"
:date "09-Jan-2025 13:44:02.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:number-of-orbits 1
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:data-volume 191440
:tdrss-contact-duration 0
:coron NIL
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(Tic-Obset
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)
(Tic-Orbit
:proposal-id 17698
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:pcs-time 380
:si-vis-utilization 2272
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3099
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vBC.xml
(Tic-Visit
:proposal-id 17698
:visit-id "BC"
:proposal-version -1
:trans-version "20240604"
:date "09-Jan-2025 13:44:02.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:number-of-orbits 1
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:data-volume 191440
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:coron NIL
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(Tic-Obset
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)
(Tic-Orbit
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:pcs-time 380
:si-vis-utilization 2319
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:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3032
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vBD.xml
(Tic-Visit
:proposal-id 17698
:visit-id "BD"
:proposal-version -1
:trans-version "20240604"
:date "09-Jan-2025 13:44:03.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:number-of-orbits 1
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:si-bright-earth-limb-angle 20.0
:data-volume 191440
:tdrss-contact-duration 0
:coron NIL
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(Tic-Obset
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)
(Tic-Orbit
:proposal-id 17698
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:pcs-time 380
:si-vis-utilization 2311
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3023
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAV.xml
(Tic-Visit
:proposal-id 17698
:visit-id "AV"
:proposal-version -1
:trans-version "20240604"
:date "09-Jan-2025 13:44:03.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:number-of-orbits 1
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 191440
:tdrss-contact-duration 0
:coron NIL
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(Tic-Obset
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)
(Tic-Orbit
:proposal-id 17698
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:orbit-number 1
:pcs-time 380
:si-vis-utilization 2319
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAW.xml
(Tic-Visit
:proposal-id 17698
:visit-id "AW"
:proposal-version -1
:trans-version "20240604"
:date "09-Jan-2025 13:44:04.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 191440
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 17698
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:orbit-number 1
:pcs-time 380
:si-vis-utilization 2272
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAX.xml
(Tic-Visit
:proposal-id 17698
:visit-id "AX"
:proposal-version -1
:trans-version "20240604"
:date "09-Jan-2025 13:44:05.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 191440
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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)
(Tic-Orbit
:proposal-id 17698
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:orbit-number 1
:pcs-time 380
:si-vis-utilization 2272
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3251
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAY.xml
(Tic-Visit
:proposal-id 17698
:visit-id "AY"
:proposal-version -1
:trans-version "20240604"
:date "09-Jan-2025 13:44:05.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:number-of-orbits 1
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 191440
:tdrss-contact-duration 0
:coron NIL
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(Tic-Obset
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)
(Tic-Orbit
:proposal-id 17698
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:orbit-number 1
:pcs-time 380
:si-vis-utilization 2272
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3032
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAZ.xml
(Tic-Visit
:proposal-id 17698
:visit-id "AZ"
:proposal-version -1
:trans-version "20240604"
:date "09-Jan-2025 13:44:07.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 191440
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 17698
:visit-id "AZ"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2319
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3032
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vB0.xml
(Tic-Visit
:proposal-id 17698
:visit-id "B0"
:proposal-version -1
:trans-version "20240604"
:date "09-Jan-2025 13:44:08.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 191440
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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:pcs-mode "FGS"
)
(Tic-Orbit
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:orbit-number 1
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:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3010
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vB1.xml
(Tic-Visit
:proposal-id 17698
:visit-id "B1"
:proposal-version -1
:trans-version "20240604"
:date "09-Jan-2025 13:44:08.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 191440
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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:pcs-mode "FGS"
)
(Tic-Orbit
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:orbit-number 1
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:si-vis-utilization 2319
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3023
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vB2.xml
(Tic-Visit
:proposal-id 17698
:visit-id "B2"
:proposal-version -1
:trans-version "20240604"
:date "09-Jan-2025 13:44:09.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
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:si-bright-earth-limb-angle 20.0
:data-volume 191440
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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:obset-id "B2"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 17698
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:orbit-number 1
:pcs-time 380
:si-vis-utilization 2272
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3032
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vB3.xml
(Tic-Visit
:proposal-id 17698
:visit-id "B3"
:proposal-version -1
:trans-version "20240604"
:date "09-Jan-2025 13:44:09.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
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:number-of-orbits 1
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:data-volume 191440
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 17698
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:orbit-number 1
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:si-vis-utilization 2272
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3049
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAL.xml
(Tic-Visit
:proposal-id 17698
:visit-id "AL"
:proposal-version -1
:trans-version "20240604"
:date "09-Jan-2025 13:44:10.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
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:si-bright-earth-limb-angle 20.0
:data-volume 191440
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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:obset-id "AL"
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)
(Tic-Orbit
:proposal-id 17698
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:orbit-number 1
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:si-vis-utilization 2311
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3039
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAM.xml
(Tic-Visit
:proposal-id 17698
:visit-id "AM"
:proposal-version -1
:trans-version "20240604"
:date "09-Jan-2025 13:44:11.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 191440
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 17698
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:obset-id "AM"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 17698
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:orbit-number 1
:pcs-time 380
:si-vis-utilization 2719
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3099
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAN.xml
(Tic-Visit
:proposal-id 17698
:visit-id "AN"
:proposal-version -1
:trans-version "20240604"
:date "09-Jan-2025 13:44:11.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 191440
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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:visit-id "AN"
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:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 17698
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:orbit-number 1
:pcs-time 380
:si-vis-utilization 2319
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3184
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAO.xml
(Tic-Visit
:proposal-id 17698
:visit-id "AO"
:proposal-version -1
:trans-version "20240604"
:date "09-Jan-2025 13:44:12.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 191440
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 17698
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:orbit-number 1
:pcs-time 380
:si-vis-utilization 2272
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3034
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAP.xml
(Tic-Visit
:proposal-id 17698
:visit-id "AP"
:proposal-version -1
:trans-version "20240604"
:date "09-Jan-2025 13:44:12.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 191440
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
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:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 17698
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:orbit-number 1
:pcs-time 380
:si-vis-utilization 2319
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3119
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAQ.xml
(Tic-Visit
:proposal-id 17698
:visit-id "AQ"
:proposal-version -1
:trans-version "20240604"
:date "09-Jan-2025 13:44:13.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 191440
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 17698
:visit-id "AQ"
:obset-id "AQ"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 17698
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:orbit-number 1
:pcs-time 380
:si-vis-utilization 2272
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3119
:pcs-gap 0
)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAR.xml
(Tic-Visit
:proposal-id 17698
:visit-id "AR"
:proposal-version -1
:trans-version "20240604"
:date "09-Jan-2025 13:44:14.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 208816
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 17698
:visit-id "AR"
:obset-id "AR"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 17698
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)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAS.xml
(Tic-Visit
:proposal-id 17698
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(Tic-Obset
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)
(Tic-Orbit
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:dark-utilization 0
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:low-sky "N"
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)
true
1
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The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAT.xml
(Tic-Visit
:proposal-id 17698
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(Tic-Obset
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)
(Tic-Orbit
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:low-sky "N"
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)
true
1
0
The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAB.xml
(Tic-Visit
:proposal-id 17698
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(Tic-Obset
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(Tic-Orbit
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:low-sky "N"
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)
true
1
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The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAC.xml
(Tic-Visit
:proposal-id 17698
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(Tic-Obset
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(Tic-Orbit
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)
true
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The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAD.xml
(Tic-Visit
:proposal-id 17698
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(Tic-Obset
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(Tic-Orbit
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:si-vis-utilization 2669
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)
true
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The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAE.xml
(Tic-Visit
:proposal-id 17698
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(Tic-Obset
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(Tic-Orbit
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)
true
1
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The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAF.xml
(Tic-Visit
:proposal-id 17698
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(Tic-Obset
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(Tic-Orbit
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)
true
1
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The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAG.xml
(Tic-Visit
:proposal-id 17698
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(Tic-Obset
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true
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The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAH.xml
(Tic-Visit
:proposal-id 17698
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(Tic-Obset
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(Tic-Orbit
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true
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The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAI.xml
(Tic-Visit
:proposal-id 17698
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(Tic-Obset
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(Tic-Orbit
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)
true
1
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The scheduling data was generated by CASM 32.1.3.
CASM was run in Phase II mode.
/home/astro/btg/OP-cache/17698-vAJ.xml
(Tic-Visit
:proposal-id 17698
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:tdrss-contact-duration 0
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(Tic-Obset
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(Tic-Orbit
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true
1
0