removed the useless ORIENT constraint in V9 ----- Attempting Submission 1 (Tue May 08 18:15:26 GMT 2012) ----- ----- Attempting Submission 2 (Fri Jun 01 01:35:13 GMT 2012) ----- ONly V6 was changed. Successive re-submissions with different versions of APT led to visibitiy overruns in the other visits in the latest version of APT, A Direct CO/H2 Abundance Measurement in Diffuse and Translucent LMC and SMC Molecular Clouds Theoretical and observational evidence suggests that molecular gas (H2) is not always correlated with CO because CO is photo-dissociated more easily than H2. The mass of CO-poor H2 present in the envelopes of giant molecular clouds (GMCs) is higher in low metallicity GMCs, which are more exposed to dissociating radiation due to their lower dust abundance. Since we cannot detect H2 directly, the mass of these CO-poor envelopes is effectively "hidden" from radio telescopes. This limitation of CO emission observations hinders our understanding of the correlation between star formation rate, H2, and CO since, in those low metallicity galaxies, neither the CO/H2 abundance, nor the H2 mass can be accurately derived from CO emission. The most sensitive and direct way to determine CO and H2 column densities is to derive them from UV absorption lines. Because of their proximity and low metallicity, the Magellanic Clouds are ideal laboratories to test the current theory of CO/H2 abundance, which can be applied in the high-redshift universe. We propose to observe the 4th positive absorption band of CO with COS toward 9 translucent (Av~1) Magellanic Cloud sightlines probing the edges of GMCs. Covering the Lyman-Werner bands of H2, readily available FUSE spectra can be used to derive H2 column densities toward our targets. These COS observations, which are the only direct test of theoretical predictions for the CO/H2 abundance, will detect CO column densities as low as 1e13 cm-2. They will constrain the structure of GMCs in low-metallicity galaxies, the CO-to-H2 ratio required to estimate the H2 mass from CO emission, and the correlation between star formation rate, H2, and CO. Goal: We will observe the fourth positive CO absorption band system toward 6 stars in the Large Magellanic Cloud, and 3 stars in the Small Magellanic Cloud. Probing translucent CO column densities requires a S/N of 100:1. The (1-0) … (5-0) ro-vibrational transitions of the CO fourth positive system cover the wavelength range 1392 Å – 1520 Å, with the brighter (1-0)-(3-0) lines covering the range 1447 Å – 1515 Å. This range will require use of the G160M grating on COS. To obtain the required S/N = 100 after FPPOS correction, we will need an exposure time providing a statistical (based on Poisson statistics) of 120, split equally on all 4 FP-POS and 3 central wavelengths (1577 Å, 1589 Å, and 1600 Å). In addition, we will need to center the CO absorption lines on the center of segment B, and avoid the 2000 pixels located at each edge of the segment. Target Acquisition: Since our coordinates are tied to 2MASS and accurate to a fraction of an arcsecond, we will perform a NUV/IMAGE acquisition with the Bright Object Aperture (BOA), and with S/N = 60. CVZ targets: Four of our targets have fluxes of 1.5◊10-13 ergs cm-2 s-1 Å-1, which would require 5 orbits to achieve a statistical S/N of 120. We propose to observe these targets more efficiently, by requesting Continuous Viewing Zone (CVZ) visibility. Additional G130M observations to measure gas excitation: For 7 of our targets (all targets except AV6 and HD269445), we will have additional observing time at the end of the last orbit of the visit to perform G130M observations at central wavelength 1327 Å of key interstellar lines (CI, CII, NI, OI, SiII, SI, SII, FeII). These lines, ubiquitous in the ISM, typically have equivalent widths > 20 mÅ, and will be detected at the > 4σ level with S/N=20. Coordinated Parallel Observations: We will also obtain parallel observations with both the WFC3 and ACS instruments to study the star formation history nearby our sightlines. At the distance of the Magellanic Clouds, the brightest O stars will saturate in just a few seconds and characterizing solar type stars with high S/N will require exposure times of a few hundred seconds in visible filters. Our exposure times will therefore be set to include both very short observations at the start of each orbit to mitigate saturation among the most massive stars, and longer exposures to probe low mass stars along the main-sequence. Our default set up will use the same filters as the Panchromatic Hubble Andromeda Treasury Project (PHAT) to complete the multi-wavelength imaging. This will include F275W, F336W, F475W, F814W (UVIS) and F110W, F160W (IR) for WFC3 and F475W and F814W for ACS. However, for our shortest integration times (2 orbits), we will need to make small adjustments in the number of filters observed or scale back to imaging one parallel field with one instrument to manage buffer dumps from multiple filter exposures (e.g., WFC3/UVIS in one orbit and WFC3/IR in the second orbit). All parallel observations will be constructed to not impact the primary COS exposures. ISM IN EXTERNAL GALAXIES 12 false 0.0 0.0 false false false false SUPPORTED EXT-STAR WOLF RAYET This object was generated by the targetselector and retrieved from the SIMBAD database. Coordinates are from the 2MASS archive, which an absolute astrometric precision of 0.1 arcsec: http://vizier.u-strasbg.fr/viz-bin/VizieR-S?2MASS%20J05365516-6911376 The BOP was cleared for science and target acquisition, and the exposure time estimated using IUE spectra over the same wavelength range as COS FUV and NUV: http://archive.stsci.edu/xcorr.php?target=hd38029&max_records=10&action=Search&resolver=SIMBAD&missions%5B%5D=FUSE&missions%5B%5D=IMAPS&missions%5B%5D=BEFS&missions%5B%5D=TUES&missions%5B%5D=IUE&missions%5B%5D=COPERNICUS&missions%5B%5D=HUT&missions%5B%5D=WUPPE&missions%5B%5D=GHRS&missions%5B%5D=STIS-SPECTRUM&missions%5B%5D=COS-SPECTRUM&missions%5B%5D=WFC3-SPECTRUM&missions%5B%5D=ACS-SPECTRUM&missions%5B%5D=FOS&missions%5B%5D=HPOL J2000 J2000 Flux at 1300-1700 A (IUE): 3e-13 ergs/cm2/s/A; Flux at 2500A = 2.5e-13 EXT-STAR BE This object was generated by the targetselector and retrieved from the SIMBAD database. Coordinates are from the 2MASS archive, which an absolute astrometric precision of 0.1 arcsec: http://vizier.u-strasbg.fr/viz-bin/VizieR-S?2MASS%20J05414467-6935150 The BOP was cleared for science and target acquisition, and the exposure time estimated using IUE spectra over the same wavelength range as COS FUV and NUV: http://archive.stsci.edu/xcorr.php?target=sk-69279&max_records=10&action=Search&resolver=SIMBAD&missions%5B%5D=FUSE&missions%5B%5D=IMAPS&missions%5B%5D=BEFS&missions%5B%5D=TUES&missions%5B%5D=IUE&missions%5B%5D=COPERNICUS&missions%5B%5D=HUT&missions%5B%5D=WUPPE&missions%5B%5D=GHRS&missions%5B%5D=STIS-SPECTRUM&missions%5B%5D=COS-SPECTRUM&missions%5B%5D=WFC3-SPECTRUM&missions%5B%5D=ACS-SPECTRUM&missions%5B%5D=FOS&missions%5B%5D=HPOL J2000 J2000 Flux at 1300-1700 A from IUE: 1.8e-13 ergs/cm2/s/A; Flux at 2500A = 1.3e-13 EXT-STAR MAIN SEQUENCE O This object was generated by the targetselector and retrieved from the SIMBAD database. Coordinates are from the 2MASS archive, which an absolute astrometric precision of 0.1 arcsec: http://vizier.u-strasbg.fr/viz-bin/VizieR-S?2MASS%20J05425492-6856544 The BOP was cleared for science and target acquisition, and the exposure time estimated using IUE spectra over the same wavelength range as COS FUV and NUV: http://archive.stsci.edu/xcorr.php?target=sk-68155&max_records=10&action=Search&resolver=SIMBAD&missions%5B%5D=FUSE&missions%5B%5D=IMAPS&missions%5B%5D=BEFS&missions%5B%5D=TUES&missions%5B%5D=IUE&missions%5B%5D=COPERNICUS&missions%5B%5D=HUT&missions%5B%5D=WUPPE&missions%5B%5D=GHRS&missions%5B%5D=STIS-SPECTRUM&missions%5B%5D=COS-SPECTRUM&missions%5B%5D=WFC3-SPECTRUM&missions%5B%5D=ACS-SPECTRUM&missions%5B%5D=FOS&missions%5B%5D=HPOL J2000 J2000 Flux at 1300-1700 A (IUE): 1.7.e-13 ergs/cm2/s/A; Flux at 2500A = 1.5e-13 EXT-STAR MAIN SEQUENCE O This object was generated by the targetselector and retrieved from the SIMBAD database. Coordinates are from the 2MASS archive, which an absolute astrometric precision of 0.1 arcsec: http://vizier.u-strasbg.fr/viz-bin/VizieR-S?2MASS%20J05362676-6857319 The BOP was cleared for science and target acquisition, and the exposure time estimated using IUE spectra over the same wavelength range as COS FUV and NUV: http://archive.stsci.edu/xcorr.php?target=sk-68129&max_records=10&action=Search&resolver=SIMBAD&missions%5B%5D=FUSE&missions%5B%5D=IMAPS&missions%5B%5D=BEFS&missions%5B%5D=TUES&missions%5B%5D=IUE&missions%5B%5D=COPERNICUS&missions%5B%5D=HUT&missions%5B%5D=WUPPE&missions%5B%5D=GHRS&missions%5B%5D=STIS-SPECTRUM&missions%5B%5D=COS-SPECTRUM&missions%5B%5D=WFC3-SPECTRUM&missions%5B%5D=ACS-SPECTRUM&missions%5B%5D=FOS&missions%5B%5D=HPOL J2000 J2000 Flux at 1300-1700A (IUE): 1.5e-13 ergs/cm2/s/A; Flux at 2500A = 1.1e-13 EXT-STAR BE This object was generated by the targetselector and retrieved from the SIMBAD database. Coordinates are from the 2MASS archive, which an absolute astrometric precision of 0.1 arcsec: http://vizier.u-strasbg.fr/viz-bin/VizieR-S?2MASS%20J05385718-6856530 The BOP was cleared for science and target acquisition, and the exposure time estimated using IUE spectra over the same wavelength range as COS FUV and NUV: http://archive.stsci.edu/xcorr.php?target=sk-68140&max_records=10&action=Search&resolver=SIMBAD&missions%5B%5D=FUSE&missions%5B%5D=IMAPS&missions%5B%5D=BEFS&missions%5B%5D=TUES&missions%5B%5D=IUE&missions%5B%5D=COPERNICUS&missions%5B%5D=HUT&missions%5B%5D=WUPPE&missions%5B%5D=GHRS&missions%5B%5D=STIS-SPECTRUM&missions%5B%5D=COS-SPECTRUM&missions%5B%5D=WFC3-SPECTRUM&missions%5B%5D=ACS-SPECTRUM&missions%5B%5D=FOS&missions%5B%5D=HPOL J2000 J2000 Flux at 1300-1700 A (IUE): 1.5e-13 ergs/cm2/s/A;Flux at 2500A = 1e-13 EXT-STAR BE This object was generated by the targetselector and retrieved from the SIMBAD database. Coordinates are from the 2MASS archive, which an absolute astrometric precision of 0.1 arcsec: http://vizier.u-strasbg.fr/viz-bin/VizieR-S?2MASS%20J05225978-6801466 The BOP was cleared for science and target acquisition, and the exposure time estimated using IUE spectra over the same wavelength range as COS FUV and NUV: http://archive.stsci.edu/xcorr.php?target=hd269445&max_records=10&action=Search&resolver=SIMBAD&missions%5B%5D=FUSE&missions%5B%5D=IMAPS&missions%5B%5D=BEFS&missions%5B%5D=TUES&missions%5B%5D=IUE&missions%5B%5D=COPERNICUS&missions%5B%5D=HUT&missions%5B%5D=WUPPE&missions%5B%5D=GHRS&missions%5B%5D=STIS-SPECTRUM&missions%5B%5D=COS-SPECTRUM&missions%5B%5D=WFC3-SPECTRUM&missions%5B%5D=ACS-SPECTRUM&missions%5B%5D=FOS&missions%5B%5D=HPOL J2000 J2000 Flux at 1300-1700A (IUE): 3.5e-13 ergs/cm2/s/A;Flux at 2500A = 2.5e-13 EXT-STAR MAIN SEQUENCE O This object was generated by the targetselector and retrieved from the SIMBAD database. Coordinates are from the 2MASS archive, which an absolute astrometric precision of 0.1 arcsec: http://vizier.u-strasbg.fr/viz-bin/VizieR-S?2MASS%20J01105576-7242563 The BOP was cleared for science and target acquisition, and the exposure time estimated using IUE spectra over the same wavelength range as COS FUV and NUV: http://archive.stsci.edu/xcorr.php?target=av456&max_records=10&action=Search&resolver=SIMBAD&missions%5B%5D=FUSE&missions%5B%5D=IMAPS&missions%5B%5D=BEFS&missions%5B%5D=TUES&missions%5B%5D=IUE&missions%5B%5D=COPERNICUS&missions%5B%5D=HUT&missions%5B%5D=WUPPE&missions%5B%5D=GHRS&missions%5B%5D=STIS-SPECTRUM&missions%5B%5D=COS-SPECTRUM&missions%5B%5D=WFC3-SPECTRUM&missions%5B%5D=ACS-SPECTRUM&missions%5B%5D=FOS&missions%5B%5D=HPOL J2000 J2000 Flux at 1300-1700A (IUE): 1.5e-13 ergs/cm2/s/A; Flux at 2500A = 1e-13 EXT-STAR MAIN SEQUENCE O This object was generated by the targetselector and retrieved from the SIMBAD database. Coordinates are from the 2MASS archive, which an absolute astrometric precision of 0.1 arcsec: The BOP was cleared for science and target acquisition, and the exposure time estimated using IUE spectra over the same wavelength range as COS FUV and NUV: http://archive.stsci.edu/xcorr.php?target=av6&max_records=10&action=Search&resolver=SIMBAD&missions%5B%5D=FUSE&missions%5B%5D=IMAPS&missions%5B%5D=BEFS&missions%5B%5D=TUES&missions%5B%5D=IUE&missions%5B%5D=COPERNICUS&missions%5B%5D=HUT&missions%5B%5D=WUPPE&missions%5B%5D=GHRS&missions%5B%5D=STIS-SPECTRUM&missions%5B%5D=COS-SPECTRUM&missions%5B%5D=WFC3-SPECTRUM&missions%5B%5D=ACS-SPECTRUM&missions%5B%5D=FOS&missions%5B%5D=HPOL J2000 J2000 Flux at 1300-1700A (IUE): 3.6e-13 ergs/cm2/s/A; Flux at 2500A = 1e-13 EXT-STAR B0-B2 III-I This object was generated by the targetselector and retrieved from the SIMBAD database. Coordinates are from the 2MASS archive, which an absolute astrometric precision of 0.1 arcsec: http://vizier.u-strasbg.fr/viz-bin/VizieR-S?2MASS%20J01134244-7317294 The BOP was cleared for science and target acquisition, and the exposure time estimated using IUE spectra over the same wavelength range as COS FUV and NUV: http://archive.stsci.edu/xcorr.php?target=av476&max_records=10&action=Search&resolver=SIMBAD&missions%5B%5D=FUSE&missions%5B%5D=IMAPS&missions%5B%5D=BEFS&missions%5B%5D=TUES&missions%5B%5D=IUE&missions%5B%5D=COPERNICUS&missions%5B%5D=HUT&missions%5B%5D=WUPPE&missions%5B%5D=GHRS&missions%5B%5D=STIS-SPECTRUM&missions%5B%5D=COS-SPECTRUM&missions%5B%5D=WFC3-SPECTRUM&missions%5B%5D=ACS-SPECTRUM&missions%5B%5D=FOS&missions%5B%5D=HPOL J2000 J2000 Flux at 1300-1700A (IUE): 1.5e-13 ergs/cm2/s/A; Flux at 2500A = 1e-13 COS/FUV Spectroscopic No No G160M 1577 COS/FUV Spectroscopic No No G160M 1589 COS/FUV Spectroscopic No No G160M 1600 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G160M 1577 COS/FUV Spectroscopic No No G160M 1589 COS/FUV Spectroscopic No No G160M 1600 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G160M 1577 COS/FUV Spectroscopic No No G160M 1589 COS/FUV Spectroscopic No No G160M 1600 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G160M 1577 COS/FUV Spectroscopic No No G160M 1589 COS/FUV Spectroscopic No No G160M 1600 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G160M 1577 COS/FUV Spectroscopic No No G160M 1589 COS/FUV Spectroscopic No No G160M 1600 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G160M 1577 COS/FUV Spectroscopic No No G160M 1589 COS/FUV Spectroscopic No No G160M 1600 COS/FUV Spectroscopic No No G160M 1577 COS/FUV Spectroscopic No No G160M 1589 COS/FUV Spectroscopic No No G160M 1600 COS/FUV Spectroscopic No No G130M 1327 COS/FUV Spectroscopic No No G160M 1577 COS/FUV Spectroscopic No No G160M 1589 COS/FUV Spectroscopic No No G160M 1600 COS/FUV Spectroscopic No No G160M 1577 COS/FUV Spectroscopic No No G160M 1589 COS/FUV Spectroscopic No No G160M 1600 COS/FUV Spectroscopic No No G130M 1327 WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F475W WFC3/UVIS Imaging No No F814W WFC3/IR Imaging No No F110W WFC3/IR Imaging No No F160W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F475W WFC3/UVIS Imaging No No F814W WFC3/IR Imaging No No F110W WFC3/IR Imaging No No F160W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F475W WFC3/UVIS Imaging No No F814W WFC3/IR Imaging No No F110W WFC3/IR Imaging No No F160W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F475W WFC3/UVIS Imaging No No F814W WFC3/IR Imaging No No F110W WFC3/IR Imaging No No F160W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F475W WFC3/UVIS Imaging No No F814W WFC3/IR Imaging No No F110W WFC3/IR Imaging No No F160W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F475W WFC3/UVIS Imaging No No F814W WFC3/IR Imaging No No F110W WFC3/IR Imaging No No F160W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F475W WFC3/UVIS Imaging No No F814W WFC3/IR Imaging No No F110W WFC3/IR Imaging No No F160W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F475W WFC3/UVIS Imaging No No F814W WFC3/IR Imaging No No F110W WFC3/IR Imaging No No F160W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F475W WFC3/UVIS Imaging No No F814W WFC3/IR Imaging No No F110W WFC3/IR Imaging No No F160W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W The scheduling data was generated by CASM 20.0. CASM was run in Phase II mode. /private/var/folders/vM/vMA8Vj5BEf8KnAIzPHl8Mk++2h2/-Tmp-/OPVisit2643233737665778421.xml (Tic-Visit :proposal-id 12581 :visit-id "01" :proposal-version -1 :trans-version "20120125" :date "31-May-2012 21:27:45.0" :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 2765984 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12581 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12581 :visit-id "01" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3249 :al-overhead-at-end 0 :internal-dur-at-end 67 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3599 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "01" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3369 :al-overhead-at-end 0 :internal-dur-at-end 152 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3599 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "01" :orbit-number 3 :pcs-time 222 :si-vis-utilization 3377 :al-overhead-at-end 0 :internal-dur-at-end 379 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3599 :pcs-gap 0 ) true 3 0 The scheduling data was generated by CASM 20.0. CASM was run in Phase II mode. /private/var/folders/vM/vMA8Vj5BEf8KnAIzPHl8Mk++2h2/-Tmp-/OPVisit3365277319505141951.xml (Tic-Visit :proposal-id 12581 :visit-id "02" :proposal-version -1 :trans-version "20120125" :date "31-May-2012 21:29:04.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 8596288 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12581 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12581 :visit-id "02" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3249 :al-overhead-at-end 0 :internal-dur-at-end 48 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3599 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "02" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3376 :al-overhead-at-end 0 :internal-dur-at-end 773 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3599 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "02" :orbit-number 3 :pcs-time 222 :si-vis-utilization 3375 :al-overhead-at-end 30 :internal-dur-at-end 114 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3599 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "02" :orbit-number 4 :pcs-time 222 :si-vis-utilization 3377 :al-overhead-at-end 0 :internal-dur-at-end 1330 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3599 :pcs-gap 0 ) true 4 0 The scheduling data was generated by CASM 20.0. CASM was run in Phase II mode. /private/var/folders/vM/vMA8Vj5BEf8KnAIzPHl8Mk++2h2/-Tmp-/OPVisit8732030131138060611.xml 95 1327459166000 38.307235008216 (Tic-Visit :proposal-id 12581 :visit-id "03" :proposal-version -1 :trans-version "20120125" :date "31-May-2012 21:31:58.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 7928752 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12581 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12581 :visit-id "03" :orbit-number 1 :pcs-time 333 :si-vis-utilization 5377 :al-overhead-at-end 9 :internal-dur-at-end 31 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 5700.0 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "03" :orbit-number 2 :pcs-time 222 :si-vis-utilization 5224 :al-overhead-at-end 12 :internal-dur-at-end 38 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 5700.0 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "03" :orbit-number 3 :pcs-time 222 :si-vis-utilization 4423 :al-overhead-at-end 0 :internal-dur-at-end 872 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 5700.0 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "03" :orbit-number 4 :pcs-time 0 :si-vis-utilization 0 :al-overhead-at-end 0 :internal-dur-at-end 281 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 5700.0 :pcs-gap 0 ) true 4 1 The scheduling data was generated by CASM 20.0. CASM was run in Phase II mode. /private/var/folders/vM/vMA8Vj5BEf8KnAIzPHl8Mk++2h2/-Tmp-/OPVisit7016628620663165230.xml (Tic-Visit :proposal-id 12581 :visit-id "04" :proposal-version -1 :trans-version "20120125" :date "31-May-2012 21:32:08.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 5 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 10431136 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12581 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12581 :visit-id "04" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3249 :al-overhead-at-end 0 :internal-dur-at-end 700 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3599 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "04" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3375 :al-overhead-at-end 20 :internal-dur-at-end 57 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3599 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "04" :orbit-number 3 :pcs-time 222 :si-vis-utilization 3357 :al-overhead-at-end 0 :internal-dur-at-end 744 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3599 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "04" :orbit-number 4 :pcs-time 222 :si-vis-utilization 3373 :al-overhead-at-end 0 :internal-dur-at-end 404 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3599 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "04" :orbit-number 5 :pcs-time 222 :si-vis-utilization 3356 :al-overhead-at-end 0 :internal-dur-at-end 1125 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3599 :pcs-gap 0 ) true 5 0 The scheduling data was generated by CASM 20.0. CASM was run in Phase II mode. /private/var/folders/vM/vMA8Vj5BEf8KnAIzPHl8Mk++2h2/-Tmp-/OPVisit2027885149674913716.xml 95 1322781007000 344.0729827501216 (Tic-Visit :proposal-id 12581 :visit-id "05" :proposal-version -1 :trans-version "20120125" :date "31-May-2012 21:32:42.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 7954848 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12581 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12581 :visit-id "05" :orbit-number 1 :pcs-time 333 :si-vis-utilization 5359 :al-overhead-at-end 0 :internal-dur-at-end 38 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 5700.0 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "05" :orbit-number 2 :pcs-time 222 :si-vis-utilization 5224 :al-overhead-at-end 12 :internal-dur-at-end 38 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 5700.0 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "05" :orbit-number 3 :pcs-time 222 :si-vis-utilization 4423 :al-overhead-at-end 0 :internal-dur-at-end 882 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 5700.0 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "05" :orbit-number 4 :pcs-time 0 :si-vis-utilization 0 :al-overhead-at-end 0 :internal-dur-at-end 271 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 5700.0 :pcs-gap 0 ) true 4 1 The scheduling data was generated by CASM 20.0. CASM was run in Phase II mode. 54.5 (Tic-Visit :proposal-id 12581 :visit-id "06" :proposal-version -1 :trans-version "20120125" :date "08-May-2012 13:37:39.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 3280592 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12581 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12581 :visit-id "06" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2920 :al-overhead-at-end 0 :internal-dur-at-end 95 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3270.0 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "06" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3038 :al-overhead-at-end 0 :internal-dur-at-end 1164 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3270.0 :pcs-gap 0 ) true 2 0 The scheduling data was generated by CASM 20.0. CASM was run in Phase II mode. /private/var/folders/vM/vMA8Vj5BEf8KnAIzPHl8Mk++2h2/-Tmp-/OPVisit6876428165272510055.xml 95 (Tic-Visit :proposal-id 12581 :visit-id "07" :proposal-version -1 :trans-version "20120125" :date "31-May-2012 21:32:52.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 3 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 7564064 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12581 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12581 :visit-id "07" :orbit-number 1 :pcs-time 333 :si-vis-utilization 5304 :al-overhead-at-end 0 :internal-dur-at-end 86 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 5700.0 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "07" :orbit-number 2 :pcs-time 222 :si-vis-utilization 5196 :al-overhead-at-end 0 :internal-dur-at-end 86 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 5700.0 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "07" :orbit-number 3 :pcs-time 222 :si-vis-utilization 4489 :al-overhead-at-end 0 :internal-dur-at-end 811 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 5700.0 :pcs-gap 0 ) true 3 0 The scheduling data was generated by CASM 20.0. CASM was run in Phase II mode. /private/var/folders/vM/vMA8Vj5BEf8KnAIzPHl8Mk++2h2/-Tmp-/OPVisit1664683479647178308.xml (Tic-Visit :proposal-id 12581 :visit-id "08" :proposal-version -1 :trans-version "20120125" :date "31-May-2012 21:33:15.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 3620064 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12581 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12581 :visit-id "08" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3295 :al-overhead-at-end 0 :internal-dur-at-end 76 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3645 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "08" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3422 :al-overhead-at-end 0 :internal-dur-at-end 983 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3645 :pcs-gap 0 ) true 2 0 The scheduling data was generated by CASM 20.0. CASM was run in Phase II mode. /private/var/folders/vM/vMA8Vj5BEf8KnAIzPHl8Mk++2h2/-Tmp-/OPVisit4528262893813933361.xml 95 (Tic-Visit :proposal-id 12581 :visit-id "09" :proposal-version -1 :trans-version "20120125" :date "31-May-2012 21:33:25.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 3 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 7564064 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12581 :visit-id "09" :obset-id "09" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12581 :visit-id "09" :orbit-number 1 :pcs-time 333 :si-vis-utilization 5264 :al-overhead-at-end 0 :internal-dur-at-end 86 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 5700.0 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "09" :orbit-number 2 :pcs-time 222 :si-vis-utilization 5196 :al-overhead-at-end 0 :internal-dur-at-end 86 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 5700.0 :pcs-gap 0 ) (Tic-Orbit :proposal-id 12581 :visit-id "09" :orbit-number 3 :pcs-time 222 :si-vis-utilization 4489 :al-overhead-at-end 0 :internal-dur-at-end 811 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 5700.0 :pcs-gap 0 ) true 3 0