0 Assigned ID: 759 ----- Attempting Submission 1 (Fri Apr 08 20:04:08 GMT 2016) ----- HST Phase I Proposal 759 (M83.apt) successfully submitted. Receipt: # 759-1 Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. Defaults for SEGMENT have changed in APT25.2 for use of LP4 with G130M. See full description for details. I have completed BOP checking for pending visits 8, 10, 12, 13, and 16. Document with information will be sent separately. Only change is for Visit 16 where TA configuration has been chamged from PSA/MIRRORA to PSA/MIRRORB. Ale 1677283603 ----- Attempting Submission 1 (Thu Jul 21 20:04:14 GMT 2016) ----- ----- Attempting Submission 2 (Thu Mar 23 22:13:22 GMT 2017) ----- ----- Attempting Submission 3 (Fri Jul 07 23:28:28 GMT 2017) ----- The proposal has 21 warnings. This must be due to the new APT version (25.2.1) used for this version. I have not changed anything compared to previous submission except for visit 16, which has now PSA/MIRRORB dor TA. Tracing Galactic Outflows to the Source: Spatially Resolved Feedback in M83 with COS Star-formation (SF) feedback plays a vital role in shaping galaxy properties, but there are many open questions about how this feedback is created, propagated, and felt by galaxies. SF-driven feedback can be observationally constrained with rest-frame UV absorption-line spectroscopy that accesses a range of powerful gas density and kinematic diagnostics. Studies at both high and low redshift show clear evidence for large-scale outflows in star-forming galaxies that scale with galaxy SF rate. However, by sampling one sightline or the galaxy as a whole, these studies are not tailored to reveal how the large-scale outflows develop from their ultimate sources at the scale of individual SF regions. We propose the first spatially-resolved COS G130M/G160M (1130-1800 A) study of the ISM in the nearby (4.6 Mpc) face-on spiral starburst M83 using individual young star clusters as background sources. This is the first "down-the-barrel" study where blueshifted absorptions can be identified directly with outflowing gas in a spatially resolved fashion. The kpc-scale flows sampled by the COS pointings will be anchored to the properties of the large-scale (10-100 kpc) flows thanks to the wealth of multi-wavelength observations of M83 from X-ray to radio. A comparison of COS data with mock spectra from constrained simulations of spiral galaxies with FIRE (Feedback In Realistic Environments; a code with unprecedented 1-100 pc spatial resolution and self-consistent treatments of stellar feedback) will provide an important validation of these simulations and will supply the community with a powerful and well-tested tool for galaxy formation predictions applicable to all redshifts. We propose COS FUV spectroscopy of a complete magnitude-limited (m_F336W < 17 mag) sample of 16 young star clusters in the famous nearby (D = 4.6 Mpc) face-on grand-spiral starburst galaxy M83 to improve our understanding of the relationship between local SF processes on sub-galactic scales and feedback on large (galactic) scales. We will infer the chemistry, physical conditions, and kinematics of the multi-phase ISM in the halo of M83 at ~ 1 kpc spatial resolution. We will compare the observed COS absorption-line spectra to mock spectra of a set of spiral galaxies obtained by performing cosmological simulations with FIRE in order to test the effects of different SF feedback mechanisms on small galactic scales. Abundances of the neutral ISM will be compared to abundances of the nebular gas along the same COS sightlines as inferred by our group with ground-based LBT optical spectra. The G130M grating at 1291 A and the G160 M grating at 1623 A will be used to cover the 1130-1800 A range at R ~ 20, 000. We prefer COS in the FUV over STIS due to the much higher (a factor > 10-100) sensitivity. The COS targets were selected from HST/WFC3 multi-band photometry of M83 (HST Cycles 17 and 19 GO programs 11359, PI: O'Connell, and 12513, PI: Blair). The data cover the whole bright optical disk of M83 in the following WFC3/UVIS and WFC3/IR filters spanning the whole NUV-IR wavelength range: F336W (U), F438W (B), F555W or F547M (V), F657N (Ha), F814W (I), F110W (J), and F160W (H). The WFC3 images have been crucial to guide our COS pointings compared, e.g., to the GALEX FUV and NUV images, since the COS aperture (2.5" in diameter) is much smaller that the GALEX spatial resolution of ~ 5". COS is optimized for point sources, thus extended sources suffer from degraded resolution. From our past experience with FUSE and COS (e.g., HST program 11579, PI: Aloisi), a spectral resolution up to ~ 60 km/s, corresponding to a spatial extent of ~ 1", is still well suited for the kind of ISM analysis here proposed (Aloisi et al. 2003; James et al. 2014). This type of resolution is similar to or higher than the ~ 100-400 km/s resolution of star-forming galaxies studies at z ~ 0.5-3 (e.g., Steidel et al. 2010; Martin et al. 2012; Kornei et al. 2012). Phase 1 exposure times were calculated as follows. WFC3 photometry of each cluster was used to infer their brightness in the U and the average spectral type from their (U-B) colors. A foreground reddening E(B-V)=0.07 towards M83 from NED was also considered, while no intrinsic extinction was assumed, consistently with what found and already published for the UV brightest (and most massive) clusters (Whitmore et al. 2011). Exposure times were calculated to reach a S/N ~ 8 around 1300 A for G130M and 1600 A for G160M. This is a minimum requirement to detect the weakest lines (e.g., SII 1250, 1253 A, or MgII 1239, 1240) and measure their kinematics. For the calculation of the total number of orbits, we considered an HST orbit lasting 54 minutes minus overheads: guide star (re-)acquisition (5-6 min), target acquisition (10 min), and exposure overheads (2-5 min). This amounts to a total of 40 orbits in COS/FUV G130M@1291 A and G160M@1623 A for the magnitude-limited sample of star clusters in M83. A sanity check on the exposure times was performed with GALEX. Except for a few clusters blended together at the GALEX resolution of ~5" in the center of M83, all clusters of the sample are associated to a GALEX source within a few arcsecs. GALEX FUV magnitudes of ~ 14.5-17.5 mag give exposure times of ~ 200-2,500 sec in G130M and ~ 1,000-5,000 sec in G160M, consistent with what we calculated from the WFC3 photometry. However, these GALEX estimates were not adopted in the end due to the poorer spatial resolution of GALEX and the lack of this information for some of the clusters. The ETC reported no warnings for violations of the local and/or global bright object limits, so we expect the targets to be safe to observe. The spectroscopic exposures in each pointing will be executed with FP-split to mitigate flat-fielding uncertainties and improve the S/N. Since the targets of each pointing will be faint point-like sources, we will perform a standard peak-up target acquisition (TA) in NUV imaging mode. Where possible, the spectroscopic data will be analyzed using a multi-component fitting technique which fits individual absorption lines with Voigt profiles taking into account constraints from atomic physics and the spectral resolution of the data. For an accurate analysis we will thus need to know the actually achieved resolution and line-spread function (LSF). We will calibrate this similarly to what already done for the COS spectra of Cycle 17 GO program 11579, where TA images were used to estimate the intrinsic UV extension of each source to convolve with the LSF of the COS/FUV spectroscopic observations (see James et al. 2014). This study has not been possible with any other previous space-based mission or instrument. The unique capabilities of COS on HST, coupled with the ground-based LBT capabilities that will constrain the optical properties of the COS targets and the nebular gas surrounding them, will now finally provide the opportunity to probe this subject with a completely new approach. If this study is not completed while COS is operational onboard HST, many of the key questions related to galactic-scale star formation feedback and its connection to the sub-galactic scale of the stellar processes will continue to remain unanswered for at least another decade. Galaxies Intergalactic Medium and Cosmology false true false false false 0.0 0.0 false SUPPORTED EXT-CLUSTER DISK EMISSION LINE NEBULA HALO STAR FORMING REGION WIND NO This object was selected based on WFC3 images from HST Cycle 17 and Cycle 19 GO programs 11360 and 12513. Better pointing accuracy (< 0.05 Arcsec) was achieved by cross-correlating the WFC3 coordinates with HSC (< 0.01 arcsec) and GAIA (< 0.05 arcsec). No ACQ/SEARCH is needed as the uncertainty of the target coordinates is << 0.4 arcsec. J2000 J2000 EXT-CLUSTER DISK EMISSION LINE NEBULA HALO STAR FORMING REGION WIND NO This object was selected based on WFC3 images from HST Cycle 17 and Cycle 19 GO programs 11360 and 12513. Better pointing accuracy (< 0.05 Arcsec) was achieved by cross-correlating the WFC3 coordinates with HSC (< 0.01 arcsec) and GAIA (< 0.05 arcsec). No ACQ/SEARCH is needed as the uncertainty of the target coordinates is << 0.4 arcsec. J2000 J2000 EXT-CLUSTER DISK EMISSION LINE NEBULA HALO STAR FORMING REGION WIND NO This object was selected based on WFC3 images from HST Cycle 17 and Cycle 19 GO programs 11360 and 12513. Better pointing accuracy (< 0.05 Arcsec) was achieved by cross-correlating the WFC3 coordinates with HSC (< 0.01 arcsec) and GAIA (< 0.05 arcsec). No ACQ/SEARCH is needed as the uncertainty of the target coordinates is << 0.4 arcsec. J2000 J2000 EXT-CLUSTER DISK EMISSION LINE NEBULA HALO STAR FORMING REGION WIND NO This object was selected based on WFC3 images from HST Cycle 17 and Cycle 19 GO programs 11360 and 12513. Better pointing accuracy (< 0.05 Arcsec) was achieved by cross-correlating the WFC3 coordinates with HSC (< 0.01 arcsec) and GAIA (< 0.05 arcsec). No ACQ/SEARCH is needed as the uncertainty of the target coordinates is << 0.4 arcsec. J2000 J2000 EXT-CLUSTER DISK EMISSION LINE NEBULA HALO STAR FORMING REGION WIND NO This object was selected based on WFC3 images from HST Cycle 17 and Cycle 19 GO programs 11360 and 12513. Better pointing accuracy (< 0.05 Arcsec) was achieved by cross-correlating the WFC3 coordinates with HSC (< 0.01 arcsec) and GAIA (< 0.05 arcsec). No ACQ/SEARCH is needed as the uncertainty of the target coordinates is << 0.4 arcsec. J2000 J2000 EXT-CLUSTER DISK EMISSION LINE NEBULA HALO STAR FORMING REGION WIND NO This object was selected based on WFC3 images from HST Cycle 17 and Cycle 19 GO programs 11360 and 12513. Better pointing accuracy (< 0.05 Arcsec) was achieved by cross-correlating the WFC3 coordinates with HSC (< 0.01 arcsec) and GAIA (< 0.05 arcsec). No ACQ/SEARCH is needed as the uncertainty of the target coordinates is << 0.4 arcsec. J2000 J2000 EXT-CLUSTER DISK EMISSION LINE NEBULA HALO STAR FORMING REGION WIND NO This object was selected based on WFC3 images from HST Cycle 17 and Cycle 19 GO programs 11360 and 12513. Better pointing accuracy (< 0.05 Arcsec) was achieved by cross-correlating the WFC3 coordinates with HSC (< 0.01 arcsec) and GAIA (< 0.05 arcsec). No ACQ/SEARCH is needed as the uncertainty of the target coordinates is << 0.4 arcsec. J2000 J2000 EXT-CLUSTER DISK EMISSION LINE NEBULA HALO STAR FORMING REGION WIND NO This object was selected based on WFC3 images from HST Cycle 17 and Cycle 19 GO programs 11360 and 12513. Better pointing accuracy (< 0.05 Arcsec) was achieved by cross-correlating the WFC3 coordinates with HSC (< 0.01 arcsec) and GAIA (< 0.05 arcsec). No ACQ/SEARCH is needed as the uncertainty of the target coordinates is << 0.4 arcsec. J2000 J2000 EXT-CLUSTER DISK EMISSION LINE NEBULA HALO STAR FORMING REGION WIND NO This object was selected based on WFC3 images from HST Cycle 17 and Cycle 19 GO programs 11360 and 12513. Better pointing accuracy (< 0.05 Arcsec) was achieved by cross-correlating the WFC3 coordinates with HSC (< 0.01 arcsec) and GAIA (< 0.05 arcsec). No ACQ/SEARCH is needed as the uncertainty of the target coordinates is << 0.4 arcsec. J2000 J2000 EXT-CLUSTER DISK EMISSION LINE NEBULA HALO STAR FORMING REGION WIND NO This object was selected based on WFC3 images from HST Cycle 17 and Cycle 19 GO programs 11360 and 12513. Better pointing accuracy (< 0.05 Arcsec) was achieved by cross-correlating the WFC3 coordinates with HSC (< 0.01 arcsec) and GAIA (< 0.05 arcsec). No ACQ/SEARCH is needed as the uncertainty of the target coordinates is << 0.4 arcsec. J2000 J2000 EXT-CLUSTER DISK EMISSION LINE NEBULA HALO STAR FORMING REGION WIND NO This object was selected based on WFC3 images from HST Cycle 17 and Cycle 19 GO programs 11360 and 12513. Better pointing accuracy (< 0.05 Arcsec) was achieved by cross-correlating the WFC3 coordinates with HSC (< 0.01 arcsec) and GAIA (< 0.05 arcsec). No ACQ/SEARCH is needed as the uncertainty of the target coordinates is << 0.4 arcsec. J2000 J2000 EXT-CLUSTER DISK EMISSION LINE NEBULA HALO STAR FORMING REGION WIND NO This object was selected based on WFC3 images from HST Cycle 17 and Cycle 19 GO programs 11360 and 12513. Better pointing accuracy (< 0.05 Arcsec) was achieved by cross-correlating the WFC3 coordinates with HSC (< 0.01 arcsec) and GAIA (< 0.05 arcsec). No ACQ/SEARCH is needed as the uncertainty of the target coordinates is << 0.4 arcsec. J2000 J2000 EXT-CLUSTER DISK EMISSION LINE NEBULA HALO STAR FORMING REGION WIND NO This object was selected based on WFC3 images from HST Cycle 17 and Cycle 19 GO programs 11360 and 12513. Better pointing accuracy (< 0.05 Arcsec) was achieved by cross-correlating the WFC3 coordinates with HSC (< 0.01 arcsec) and GAIA (< 0.05 arcsec). No ACQ/SEARCH is needed as the uncertainty of the target coordinates is << 0.4 arcsec. J2000 J2000 EXT-CLUSTER DISK EMISSION LINE NEBULA HALO STAR FORMING REGION WIND NO This object was selected based on WFC3 images from HST Cycle 17 and Cycle 19 GO programs 11360 and 12513. Better pointing accuracy (< 0.05 Arcsec) was achieved by cross-correlating the WFC3 coordinates with HSC (< 0.01 arcsec) and GAIA (< 0.05 arcsec). No ACQ/SEARCH is needed as the uncertainty of the target coordinates is << 0.4 arcsec. J2000 J2000 EXT-CLUSTER DISK EMISSION LINE NEBULA HALO STAR FORMING REGION WIND NO This object was selected based on WFC3 images from HST Cycle 17 and Cycle 19 GO programs 11360 and 12513. Better pointing accuracy (< 0.05 Arcsec) was achieved by cross-correlating the WFC3 coordinates with HSC (< 0.01 arcsec) and GAIA (< 0.05 arcsec). No ACQ/SEARCH is needed as the uncertainty of the target coordinates is << 0.4 arcsec. J2000 J2000 EXT-CLUSTER DISK EMISSION LINE NEBULA HALO STAR FORMING REGION WIND NO This object was selected based on WFC3 images from HST Cycle 17 and Cycle 19 GO programs 11360 and 12513. Better pointing accuracy (< 0.05 Arcsec) was achieved by cross-correlating the WFC3 coordinates with HSC (< 0.01 arcsec) and GAIA (< 0.05 arcsec). No ACQ/SEARCH is needed as the uncertainty of the target coordinates is << 0.4 arcsec. J2000 J2000 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1623 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1623 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1623 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1623 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1623 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1623 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1623 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1623 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1623 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1623 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1623 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1623 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1623 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1623 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1623 COS/FUV Spectroscopic No No G130M 1291 COS/FUV Spectroscopic No No G160M 1623 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1500777374000 111.39818081960061 (Tic-Visit :proposal-id 14681 :visit-id "01" :proposal-version -1 :trans-version "20170109" :date "21-Mar-2017 13:52:13.0" :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 156864 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14681 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14681 :visit-id "01" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2896 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "01" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3007 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "01" :orbit-number 3 :pcs-time 222 :si-vis-utilization 3007 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "01" :orbit-number 4 :pcs-time 222 :si-vis-utilization 3007 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) true 4 0 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1495965382000 86.86311399363728 (Tic-Visit :proposal-id 14681 :visit-id "02" :proposal-version -1 :trans-version "20170109" :date "23-Mar-2017 17:46:59.0" :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 156864 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14681 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14681 :visit-id "02" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2894 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "02" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3007 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "02" :orbit-number 3 :pcs-time 222 :si-vis-utilization 3005 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) true 3 0 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 14681 :visit-id "03" :proposal-version -1 :trans-version "20170109" :date "23-Mar-2017 17:37:48.0" :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 87360 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14681 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14681 :visit-id "03" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2896 :al-overhead-at-end 0 :internal-dur-at-end 331 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 14681 :visit-id "04" :proposal-version -1 :trans-version "20170109" :date "23-Mar-2017 14:16:08.0" :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 87360 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14681 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14681 :visit-id "04" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2896 :al-overhead-at-end 0 :internal-dur-at-end 331 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1495106795000 76.92303671271372 (Tic-Visit :proposal-id 14681 :visit-id "05" :proposal-version -1 :trans-version "20170109" :date "23-Mar-2017 17:31:39.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 148176 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14681 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14681 :visit-id "05" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2893 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "05" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3006 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) true 2 0 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1495950464000 86.7192088181107 (Tic-Visit :proposal-id 14681 :visit-id "06" :proposal-version -1 :trans-version "20170109" :date "23-Mar-2017 14:34:33.0" :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 87360 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14681 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14681 :visit-id "06" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2896 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "06" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3007 :al-overhead-at-end 0 :internal-dur-at-end 331 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) true 2 0 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1494983414000 75.1139722534067 (Tic-Visit :proposal-id 14681 :visit-id "07" :proposal-version -1 :trans-version "20170109" :date "23-Mar-2017 14:00:16.0" :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 122112 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14681 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14681 :visit-id "07" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2896 :al-overhead-at-end 0 :internal-dur-at-end 331 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 14681 :visit-id "08" :proposal-version -1 :trans-version "20170109" :date "23-Mar-2017 15:31:47.0" :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 148176 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14681 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14681 :visit-id "08" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2896 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "08" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3007 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "08" :orbit-number 3 :pcs-time 222 :si-vis-utilization 3007 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "08" :orbit-number 4 :pcs-time 222 :si-vis-utilization 3007 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) true 4 0 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1496234264000 89.30135395941852 (Tic-Visit :proposal-id 14681 :visit-id "09" :proposal-version -1 :trans-version "20170109" :date "23-Mar-2017 17:21:01.0" :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 156864 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14681 :visit-id "09" :obset-id "09" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14681 :visit-id "09" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2893 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "09" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3006 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) true 2 0 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 14681 :visit-id "10" :proposal-version -1 :trans-version "20170109" :date "23-Mar-2017 17:09:09.0" :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 139488 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14681 :visit-id "10" :obset-id "10" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14681 :visit-id "10" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2895 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "10" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3007 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "10" :orbit-number 3 :pcs-time 222 :si-vis-utilization 3007 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) true 3 0 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1496394504000 90.59939037771301 (Tic-Visit :proposal-id 14681 :visit-id "11" :proposal-version -1 :trans-version "20170109" :date "23-Mar-2017 14:53:51.0" :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 156864 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14681 :visit-id "11" :obset-id "11" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14681 :visit-id "11" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2896 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "11" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3007 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "11" :orbit-number 3 :pcs-time 222 :si-vis-utilization 3005 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) true 3 0 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 14681 :visit-id "12" :proposal-version -1 :trans-version "20170109" :date "23-Mar-2017 16:11:36.0" :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 148176 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14681 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14681 :visit-id "12" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2896 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "12" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3007 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "12" :orbit-number 3 :pcs-time 222 :si-vis-utilization 3007 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "12" :orbit-number 4 :pcs-time 222 :si-vis-utilization 3007 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) true 4 0 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. (Tic-Visit :proposal-id 14681 :visit-id "13" :proposal-version -1 :trans-version "20170109" :date "23-Mar-2017 14:48:53.0" :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 156864 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14681 :visit-id "13" :obset-id "13" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14681 :visit-id "13" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2896 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "13" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3007 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "13" :orbit-number 3 :pcs-time 222 :si-vis-utilization 3005 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) true 3 0 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1494610322000 68.7903953006064 (Tic-Visit :proposal-id 14681 :visit-id "14" :proposal-version -1 :trans-version "20170109" :date "23-Mar-2017 14:05:53.0" :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 87360 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14681 :visit-id "14" :obset-id "14" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14681 :visit-id "14" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2896 :al-overhead-at-end 0 :internal-dur-at-end 331 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 1496468953000 91.10829138641361 (Tic-Visit :proposal-id 14681 :visit-id "15" :proposal-version -1 :trans-version "20170109" :date "23-Mar-2017 17:37:16.0" :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 87360 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14681 :visit-id "15" :obset-id "15" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14681 :visit-id "15" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2894 :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 3229 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "15" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3007 :al-overhead-at-end 0 :internal-dur-at-end 331 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3229 :pcs-gap 0 ) true 2 0 The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. /private/var/folders/b3/04y7qyd56s7gjj2btk4fgyd0000597/T/OPVisit966714011728222279.xml (Tic-Visit :proposal-id 14681 :visit-id "16" :proposal-version -1 :trans-version "20170613" :date "07-Jul-2017 19:19:11.0" :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 148176 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 14681 :visit-id "16" :obset-id "16" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 14681 :visit-id "16" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2892 :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 3225 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "16" :orbit-number 2 :pcs-time 222 :si-vis-utilization 3003 :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 3225 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "16" :orbit-number 3 :pcs-time 222 :si-vis-utilization 3003 :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 3225 :pcs-gap 0 ) (Tic-Orbit :proposal-id 14681 :visit-id "16" :orbit-number 4 :pcs-time 222 :si-vis-utilization 3003 :al-overhead-at-end 0 :internal-dur-at-end 341 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3225 :pcs-gap 0 ) true 4 0