0Assigned ID: 2125
----- Attempting Submission 1 (Fri Apr 09 19:10:00 GMT 2021) -----A target acquisition should probably be performed before doing
spectroscopy or coronography with STIS or COS.
A target acquisition should probably be performed before doing
spectroscopy or coronography with STIS or COS.
POS TARG OUTSIDE OF APERTURE
POS TARG OUTSIDE OF APERTURE
POS TARG OUTSIDE OF APERTURE
STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS
STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS
STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS
POS TARG OUTSIDE OF APERTURE
POS TARG OUTSIDE OF APERTURE
POS TARG OUTSIDE OF APERTURE
POS TARG OUTSIDE OF APERTURE
POS TARG OUTSIDE OF APERTURE
POS TARG OUTSIDE OF APERTURE
POS TARG OUTSIDE OF APERTURE
POS TARG OUTSIDE OF APERTURE
STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS
STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS
STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS
A target acquisition should probably be performed before doing
spectroscopy or coronography with STIS or COS.
A target acquisition should probably be performed before doing
spectroscopy or coronography with STIS or COS.
A target acquisition should probably be performed before doing
spectroscopy or coronography with STIS or COS.11.22.2023 - Visit 31 and 32 to replace failures on visits 25, 26, and 27 (HOPR 92698, 4 orbits)
Visit 29 to replace failed visit 06 (HOPR 92588, 3 orbits)
Update to minimize readnoise penalty for Horsehead CCD observation per program review.
Delta update to turn off MSOFF(sets) for G230L as well to maintain correct pointing between G140 and G230
Resubmitting with updates to G140L visits to assure correct spatial overlap with G230L visits. Warning and restricted explanantions in "Proposal Description"
Warnings addressed in "Proposal Description"
Resubmiting with new NGC7023 background target to avoid potential overlap with a stellar source. Updated background durations to fill orbit.
Resubmiting with new ORIENT range for visits 3-7
Resubmitting with NGC 7023 background observations updated to allow program scheudling.
Explanation of warnings:
1) Missing fring cal (01, 02): manual fringe cals specified in the mode of calspec
2) Target acquistion should be performed: (09,11) these are background observations and exact pointing is not important. No acquisition necessary
3) Target outside of aperture: (nearly all!) artifact of the mapping stratege - slits are offset from nominal pointing position to map the correct area but the nominal target (map center) is outside of the aperture.-386724268----- Attempting Submission 1 (Thu Jul 29 23:36:51 GMT 2021) -----
----- Attempting Submission 3 (Wed Sep 01 14:58:02 GMT 2021) -----
HST Phase II Proposal 16747 successfully submitted.
Receipt: # 16747-3
----- Attempting Submission 4 (Wed Sep 15 14:57:39 GMT 2021) -----
----- Attempting Submission 5 (Wed Nov 24 17:53:35 GMT 2021) -----
----- Attempting Submission 6 (Tue Aug 02 20:46:32 GMT 2022) -----
----- Attempting Submission 7 (Wed Aug 10 16:48:58 GMT 2022) -----
----- Attempting Submission 8 (Wed Oct 12 14:28:42 GMT 2022) -----
HST Phase II Proposal 16747 successfully submitted.
Receipt: # 16747-8
----- Attempting Submission 9 (Wed Oct 12 21:53:49 GMT 2022) -----
HST Phase II Proposal 16747 successfully submitted.
Receipt: # 16747-9
----- Attempting Submission 10 (Thu Oct 13 22:25:14 GMT 2022) -----
----- Attempting Submission 11 (Mon Aug 07 20:01:36 GMT 2023) -----
----- Attempting Submission 12 (Wed Nov 22 17:21:52 GMT 2023) -----Warnings and "Restricted" mode are addressed in "Proposal Description". Over orbit allocation as this is HOPR/repeat observation submissionFUV-Optical Spectroscopic Mapping of the PDRs in NGC7023 and The HorseheadPhotodissociation regions (PDRs) are predominantly neutral regions of the ISM in which the heating and chemistry are mainly regulated by far ultraviolet photons. They are extended regions at the interface between bright stars and molecular clouds, and contain dense structures and clumps immersed in a more diffuse medium which are subjected to photo-evaporation, which brings fresh matter into the diffuse hotter zone. The interaction of stellar radiation with in situ material includes: 1) the disruption of grain mantles/clusters and coagulated grains formed in shielded dense regions, 2) ionization and dissociation of the gas and 3) gas and dust heating. Studies of nearby PDRs have shown that these processes are strongly stratified and active on angular scales that can be as small as ~1" (0.002 pc/400 au at a distance of 400 pc), indicating that the physical conditions vary over orders of magnitude on small spatial-scales in PDRs. Nearby PDRs are therefore unique targets to study rapid variations in the dust and gas components as a function of the excitation and physical conditions. In light of the importance of PDRs in understanding ISM physics and chemistry, we propose to use STIS on HST to study two emblamematic PDRs, the Horsehead and NGC7023, at wavelengths covering the dominant energy input into the PDR, the optical and UV. These data will provide data that complements an accepted JWST GTO program combining imaging and spectroscopy of both PDRs. We will observe regions matched to the apertures defined in the JWST program from ~100-1000 nm using four STIS gratings, two paired with the STIS MAMA detectors and two with the STIS CCD detectors, all four in low resolution.08/07/2023 - Added Visit 29 to replace failed visit 06 under HOPR 92588.
10/13/2022 - Modified Horsehead CCD visits to minimize read noise penalty per review: Reduced total integration count, split out Optical backgrounds and restructured observations to accomodate longer integrations.
10/12/2002.a - updated all UV visits (i.e. including the G230L) to use MSOFF ZERO/RESTORE to maintain alignment of G140 and G230 internally.
10/12/2022 - Updated Horsehead visits: Split out UV backgrounds. Added POS TARG of 3.5" in Y to G140L observations to accound to spatial offset due to repeller wire avoidance. Added MSOFF=zero to all G140L visits to disable monthly 'random' updates to offsets to assure that G140L spatial position matches the G230L (and optical ). The later requires "Allow Restricted" and "Supported" to be selected. Modified the NGC7023 G140L visits in the same fasion. Approval for MSOFF changes given by Svea Hernandez.
All remaining warnings are due to mapping the PDR front using offsets from a single target position - "POS TARG OUTSIDE OF APERTURE". Expected. "Target acquisition should be performed..." warning is on background exposures where exact pointing is not necessary so no target acquisition is required.
08/10/2022 - Updated position of NGC7023 backgrounds to avoid any bright stars for all possible orients. Updated background integration for NGC7023 to fill the available time in orbit.
08/02/2022 - revision to separate out background observations for NGC 7023 from on-source orbits. Necessary to allow tools to properly ingest/schedule the program.
Observations are in the STIS low dispersion modes G140L, G230L, G230LB, G430L, and G750L with the 52x2 slit.
Exposure times on exciting stars and target acqs were computed using synthetic stellar spectra and the ETC. On the nebular sources, using a synthetic Orion SED scaled to the relevnat surface brightness as estimated in Phase I proposal. S/N on nebular sources reported as 'averages' in ETC; line SN will be higher, continuum will be binned spectrally to reach a S/N of 10.
Differences from Phase I proposal:
1) On exciting star visits (HD200775 and Sigma Orionis), request CCD fringe flats with 4 repetitions to attempt to match high SN on exciting start targets; exciting star may be included in calspec database.
2) Added background exposures for both nebular sources. Backgrounds were NOT requested in Phase I proposal. The inclusion of backgrounds is driven by data obtained in GO 12556 (cycle 19) and discussion with STIS experts during the data analysisin that program. Briefly, variable detector backgrounds, especially in the UV, resulted in poor background correction and a reduction in the science return of the data. Additionally, since the nebular observations will largely fill the slit in both spatial dimensions, dedicated backgrounds in all gratings will facilitate an estimation of the contribution of unassociated astronomical signal present in the target data.
EXPLANATION OF WARNINGS:
--------------------------------------------
1) Sigma Ori + HD200775: "MISSING FRINGE FLAT CALIBRATION". Fringe flats are specified manually to allow high SN flats (4 repeats).
2) All visists with "STIS SCIENCE TOO FAR FROM WAVECAL" have wave cals in occulations and at least 1 per orbit which should be sufficient.
3) Some visits (Those with POS TARG +/-1.5 in X) have "POS TARG OUTSIDE OF APERTURE" warnings due to the fact that we are using POSTARG to map a region that overlaps with the JWST IFU maps on these targets rather than absolute pointings. So the 'target' is not the actual target in those cases so the warning is not relevant.
Depth at each POS TARG is the same on each object/grating with the excpetion of HH G750L where opitmal orbit usage required slightly less depth at the 1.5 and -1.5 POS TARG positions. Since, to reach the required depth, all poitings perpendicular to the PDR front will be combined in a representative SED of the entire map, slightly different coverages at the different POS TARG positions should be of negligible impact.
Notes on individual targets/vists:
---------------------------------------------------
HD200775
-----------------
High SN spectra of the exciting star fpr NGC7023 used to seperate out scattered light contribution at the PDR. Gain=4 selected to avoid A/D saturation, exposure times selected to achieve 1/2 full well per exposure. HD200775 is also used as acquisition target for NGC7023 nebular observations as it is close enough to the front.
Request 4 fringe flat repititions to match high target S/N and match approach used in CALSPEC targets.
sigma Orionis
---------------------
High SN spectra of the exciting star for the Horsehead used to seperate out scattered light contribution at the PDR. Gain=4 selected to avoid A/D saturation, exposure times selected to avoid A/D saturation. Not used as acquisition target for Horsehead PDR given separation.
Request 4 fringe flat repititions to match high target S/N and match approach used in CALSPEC targets.
MSJ2009-L1630MIR14
---------------------------------
2MASS source very near Horsehead PDR, used for target acquisition on the PDR front for the Horsehead. No specrtral type for L1630MIR-14. Assume M2V, use J=9.703 (2mass) to normalize. Assume E(B-V)=0.1 Go for longer than you might expect! 10 seconds predicts SN of 50 with ND3, go for 25 seconds. (~80 SN)
NGC7023
--------------
Observations are constructed using XPOSTARG with 4 values (-1.5, -0.5, 0.5, 1.5). With the 2" slit, this should provide a mapping roughly 5" wide perpendicular to the PDR front. Slit orientation is restricted to a PA of 188 degrees (OR 8 degrees) to maintain perpendicular alignment to the PDR along the line of sight to the exciting star and roughly match the IFU maps obtained with JWST. With the G104L, the PA at scheduling will result in somewhat different penetrations spatially in to the molecular cloud with no appreciable impact on science return. For SN reasons, in the continuum, the map will be summed in the 5" direction, parallel to the PDR front.
All MAMA visits were defined to keep individual exposures below 300 seconds. For the CCDS, <~450 seconds. Iterations of each pattern were set to reach the final desired exposure time given the constraints on the indivdual exposure lengths. Total exposure times were matched to those requested in Phase 1 proposal, with slight changes to optimize orbital usage/filling and best estimates of SN in each grating .
G140L - 2 separate visits (to keep each visit at or below 3 orbits). For each visit, exposures set to 280 seconds, 11 iterations of the 4 pattern pointings for a total 6160 seconds per visit and 12320 seconds total on the PDR. 8 orbits total
G230L - 3 separate visits (to keep each visit at or below 3 orbits). For each visit, exposures set to 285 seconds, 14 iterations of the 4 pattern pointings of 15568 seconds total on the PDR. 6 orbits total
G430L - 1 visit, 2 orbits. 760 seconds with CR split=2 with 4 pattern pointings for a total of 3040 seconds on source
G750L - 1 visit, 2 orbits. 756 seconds with CR split=2 with 4 pattern pointings for a total of 3024 seconds on source
Horsehead
-----------------
Observations are constructed using XPOSTARG with 4 values (-1.5, -0.5, 0.5, 1.5). With the 2" slit, this should provide a mapping roughly 5" wide perpendicular to the PDR front. Slit orientation is restricted to a PA of 301 degrees (OR 121 degrees) to maintain perpendicular alignment to the PDR along the line of sight to the exciting star and roughly match the IFU maps obtained with JWST. With the G104L, the PA at scheduling will result in somewhat different penetrations spatially in to the molecular cloud with no appreciable impact on science return. For SN reasons, in the continuum, the map will be summed in the 5" direction, parallel to the PDR front.
All MAMA visits were defined to keep individual exposures below 310 seconds - where optimal orbit usage was served by slighly longer exposures, individual exposures were allowed to exceed 300 seconds by up to 10 seconds. For the CCDS, <~450 seconds. Iterations of each pattern were set to reach the final desired exposure time given the constraints on the indivdual exposure lengths and opitmal use of orbital visibility. Total exposure times were matched to those requested in Phase 1 proposal, with slight changes to optimize orbital usage/filling and best estimates of SN in each grating.
G140L - 2 separate visits (to keep each visit at or below 3 orbits). For each visit, exposures set to 310 seconds, 7 iterations of at 0.5 and -0.5, 6 at 1.5 and -1.5 pattern pointings for 8060 seconds total on the PDR. 5 orbits total
G230L - 3 separate visits (to keep each visit at or below 3 orbits). For each visit, exposures set to 306 seconds, 10 iterations of the 4 pattern pointings for a total of 12240 seconds total on the PDR. 8 orbits total
G430L - 2 visits. Individual exposure length was set to 313 seconds/exposure and CR split set to optimize orbit filling while maintaining constant exposure length and equivalent depth on all 4 pattern pointings, total of 7512 seconds on source, 5 orbits total.
G750L - 3 visits. Individual exposure length was set to 257 seconds/exposure and CR split set to optimize orbit filling while maintaining constant exposure length; depth is approximately the same at all 4 pointings, though 257 seconds shorter and 514 seconds shorted at 1.5 and -1.5 positions. Total on source is 14649 seconds. 9 orbits total.
Backgrounds
--------------------
Both targets have dedicated backgrounds. The backgrounds are matched to on source exposures (slit + single exposure duration) to track instrumental backgrounds/effects.Prof. Alain Abergel has extensive experience in the observation and modeling of PDRs and will contribute to the scientific analysis of the data.
Dr. Ralph C. Bohlin is an expert in planning and data reduction for STIS and will lead planning and data reduction, especially for the exciting stars.
Dr. Karl D. Gordon is an expert in radiative transfer and data analysis and will help with data extraction and the RT modeling of the PDR emission.
Dr. Pamela Klaassen has extensive experience in the analysis of gas dynamics and will aid in the interpretation of gas signatures.
Dr. Karl Misselt has extensive experience with data analysis and the physics of dust and will lead preparation of the data for publication.
Dr. Alberto Noriega-Crespo has worked previously on the analysis and interpretation of HST STIS optical observations of stellar outflows and will help with the data reduction and analysis of the STIS UV observations.
Dr. Adolf N. Witt an expert on dust from an observational and theoretical perspective, especially on the nature of the ERE, and has extensive experience with the extraction of relevant data from these sorts of data sets.
Dr. Nathalie Ysard is an expert in the evolution of dust and contributor to the development of the THEMIS dust model and will help with the modeling of the dust evolution across the PDR.Stellar Populations and the Interstellar Medium6falsefalsetruefalsefalsefalsefalsefalseAVAILABLEISMHII REGIONIONIZATION FRONTMOLECULAR CLOUDPDRYESThis object was generated by the targetselector and retrieved from the SIMBAD database.J2000J2000ISMHII REGIONIONIZATION FRONTMOLECULAR CLOUDPDRYESJ2000J2000EXT-STARB0-B2 V-IVNOThis object was generated by the targetselector and retrieved from the SIMBAD database.
Will be used for Target aquisition on NGC7023.J2000J2000EXT-STARB0-B2 V-IVNOThis object was generated by the targetselector and retrieved from the SIMBAD database.J2000J2000EXT-STARA0-A3 III-INOThis object was generated by the targetselector and retrieved from the SIMBAD database.J2000CALIBRATIONUNDESIGNATEDNOBackground region selected from Gallex image to monitor instrumental background/stability.J2000CALIBRATIONUNDESIGNATEDNOBackground region to monitor instrumental background/stability.J2000STIS/FUV-MAMASpectroscopicNoNoG140L1425STIS/NUV-MAMASpectroscopicNoNoG230L2376STIS/CCDSpectroscopicNoNoG430L4300STIS/CCDSpectroscopicNoNoG750L7751STIS/CCDSpectroscopicNoNoG750L7751STIS/CCDSpectroscopicNoNoG430L4300STIS/NUV-MAMASpectroscopicNoNoG230L2376STIS/FUV-MAMASpectroscopicNoNoG140L1425STIS/CCDSpectroscopicNoNoG230LB2375STIS/CCDSpectroscopicNoNoG430L4300STIS/CCDSpectroscopicNoNoG750L7751STIS/CCDSpectroscopicNoNoG230LB2375STIS/CCDSpectroscopicNoNoG430L4300STIS/CCDSpectroscopicNoNoG750L7751The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v01.xmlRe: Warning on missing fring flat - The fringe flat is manually specified to allow higher SN than default 2 exposure sequence.1660631370000170.19164253656982(Tic-Visit
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:internal-dur-at-end 132
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3151
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "06"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2767
:al-overhead-at-end 133
:internal-dur-at-end 132
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3151
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "06"
:orbit-number 3
:pcs-time 380
:si-vis-utilization 2770
:al-overhead-at-end 153
:internal-dur-at-end 394
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3151
:pcs-gap 0
)false30SN 350WIth total exposure time of 15568 seconds, SN in contiuum is 2-4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 15568 seconds, SN in contiuum is 2-4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 15568 seconds, SN in contiuum is 2-4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 15568 seconds, SN in contiuum is 2-4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 15568 seconds, SN in contiuum is 2-4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v29.xml(Tic-Visit
:proposal-id 16747
:visit-id "29"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:28:54.0"
:trans-errors '(:WARNINGS 5 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 1948848
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "29"
:obset-id "29"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "29"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2769
:al-overhead-at-end 133
:internal-dur-at-end 132
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3151
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "29"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2767
:al-overhead-at-end 133
:internal-dur-at-end 132
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3151
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "29"
:orbit-number 3
:pcs-time 380
:si-vis-utilization 2770
:al-overhead-at-end 153
:internal-dur-at-end 394
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3151
:pcs-gap 0
)true30SN 350WIth total exposure time of 15568 seconds, SN in contiuum is 2-4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 15568 seconds, SN in contiuum is 2-4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 15568 seconds, SN in contiuum is 2-4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 15568 seconds, SN in contiuum is 2-4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 15568 seconds, SN in contiuum is 2-4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v07.xml(Tic-Visit
:proposal-id 16747
:visit-id "07"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:28:58.0"
:trans-errors '(:WARNINGS 17 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 1235600
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "07"
:obset-id "07"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "07"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2769
:al-overhead-at-end 133
:internal-dur-at-end 132
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3151
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "07"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2771
:al-overhead-at-end 153
:internal-dur-at-end 394
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3151
:pcs-gap 0
)false20SN 350WIth total exposure time of 15568 seconds, SN in contiuum is 2-4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 15568 seconds, SN in contiuum is 2-4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 15568 seconds, SN in contiuum is 2-4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v08.xml(Tic-Visit
:proposal-id 16747
:visit-id "08"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:29:00.0"
:trans-errors '(:WARNINGS 5 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 1218176
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "08"
:obset-id "08"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "08"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2771
:al-overhead-at-end 133
:internal-dur-at-end 132
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3151
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "08"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2767
:al-overhead-at-end 153
:internal-dur-at-end 394
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3151
:pcs-gap 0
)false20SN 350WIth total exposure time of 15568 seconds, SN in contiuum is 2-4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 15568 seconds, SN in contiuum is 2-4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 15568 seconds, SN in contiuum is 2-4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 15568 seconds, SN in contiuum is 2-4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 15568 seconds, SN in contiuum is 2-4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v09.xml1690392471000206.5146670939451(Tic-Visit
:proposal-id 16747
:visit-id "09"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:29:02.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 661088
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "09"
:obset-id "09"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "09"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2766
:al-overhead-at-end 133
:internal-dur-at-end 394
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3151
:pcs-gap 0
)false10No ETC run performed. These are mainly targeted at instrumental background so are specified at the maximum exposure length on targets, not a specific SN target. ETC number is made up to reduce the number of yellow exclamation points I have to look at.No ETC run performed. These are mainly targeted at instrumental background so are specified at the maximum exposure length on targets, not a specific SN target. ETC number is made up to reduce the number of yellow exclamation points I have to look at.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v10.xml1690398188000187.99999999999994(Tic-Visit
:proposal-id 16747
:visit-id "10"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:29:05.0"
:trans-errors '(:WARNINGS 8 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 478896
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "10"
:obset-id "10"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "10"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2769
:al-overhead-at-end 120
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3151
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "10"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2767
:al-overhead-at-end 120
:internal-dur-at-end 227
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3151
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "10"
:orbit-number 3
:pcs-time 380
:si-vis-utilization 2769
:al-overhead-at-end 120
:internal-dur-at-end 666
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3151
:pcs-gap 0
)false30SN 350Total exposure time of 3040 seconds yields a S/N in the continuum is ~7. Line SN of 10-40. Spectral binning will be used in the continuum to increase SN.Total exposure time of 3040 seconds yields a S/N in the continuum is ~7. Line SN of 10-40. Spectral binning will be used in the continuum to increase SN.Total exposure time of 3040 seconds yields a S/N in the continuum is ~7. Line SN of 10-40. Spectral binning will be used in the continuum to increase SN.Total exposure time of 3040 seconds yields a S/N in the continuum is ~7. Line SN of 10-40. Spectral binning will be used in the continuum to increase SN.Total exposure time of 3040 seconds yields a S/N in the continuum is ~7. Line SN of 10-40. Spectral binning will be used in the continuum to increase SN.Total exposure time of 3024 seconds yields a S/N in the continuum is ~8-9. Line SN of ~15-50.Total exposure time of 3024 seconds yields a S/N in the continuum is ~8-9. Line SN of ~15-50.Total exposure time of 3024 seconds yields a S/N in the continuum is ~8-9. Line SN of ~15-50.Total exposure time of 3024 seconds yields a S/N in the continuum is ~8-9. Line SN of ~15-50.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v11.xml1664192232000129.83961470554732(Tic-Visit
:proposal-id 16747
:visit-id "11"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:29:06.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 184032
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "11"
:obset-id "11"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "11"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2767
:al-overhead-at-end 120
:internal-dur-at-end 606
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3151
:pcs-gap 0
)false10The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v12.xml1669124748000301.0(Tic-Visit
:proposal-id 16747
:visit-id "12"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:29:08.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 1009424
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "12"
:obset-id "12"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "12"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2625
:al-overhead-at-end 133
:internal-dur-at-end 132
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "12"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2624
:al-overhead-at-end 153
:internal-dur-at-end 394
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)false20No specrtral type for L1630MIR-14. Assume M2V, use J=9.703 (2mass) to normalize. Assume E(B-V)=0.1 Go for longer than you might expect!
10 seconds predicts SN of 50 with ND3, go for 25 seconds. (~80 SN)WIth total exposure time of 7880 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 7880 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 7880 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v13.xml1669290421000301.0(Tic-Visit
:proposal-id 16747
:visit-id "13"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:29:11.0"
:trans-errors '(:WARNINGS 6 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 1009424
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "13"
:obset-id "13"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "13"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2625
:al-overhead-at-end 133
:internal-dur-at-end 132
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "13"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2618
:al-overhead-at-end 153
:internal-dur-at-end 394
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)false20No specrtral type for L1630MIR-14. Assume M2V, use J=9.703 (2mass) to normalize. Assume E(B-V)=0.1 Go for longer than you might expect!
10 seconds predicts SN of 50 with ND3, go for 25 seconds. (~80 SN)WIth total exposure time of 7880 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 7880 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 7880 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v23.xml1699858937000301.0(Tic-Visit
:proposal-id 16747
:visit-id "23"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:29:13.0"
:trans-errors '(:WARNINGS 14 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 1009424
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "23"
:obset-id "23"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "23"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2625
:al-overhead-at-end 133
:internal-dur-at-end 132
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "23"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2622
:al-overhead-at-end 153
:internal-dur-at-end 394
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)false20No specrtral type for L1630MIR-14. Assume M2V, use J=9.703 (2mass) to normalize. Assume E(B-V)=0.1 Go for longer than you might expect!
10 seconds predicts SN of 50 with ND3, go for 25 seconds. (~80 SN)WIth total exposure time of 7880 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 7880 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 7880 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v14.xml1669558938000301.0(Tic-Visit
:proposal-id 16747
:visit-id "14"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:29:17.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 1583504
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "14"
:obset-id "14"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "14"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2624
:al-overhead-at-end 133
:internal-dur-at-end 132
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "14"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2624
:al-overhead-at-end 133
:internal-dur-at-end 132
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "14"
:orbit-number 3
:pcs-time 380
:si-vis-utilization 2622
:al-overhead-at-end 153
:internal-dur-at-end 394
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)false30No specrtral type for L1630MIR-14. Assume M2V, use J=9.703 (2mass) to normalize. Assume E(B-V)=0.1 Go for longer than you might expect!
10 seconds predicts SN of 50 with ND3, go for 25 seconds. (~80 SN)WIth total exposure time of 12240 seconds, SN in contiuum is 2-3 We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 12240 seconds, SN in contiuum is 2-3 We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 12240 seconds, SN in contiuum is 2-3 We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 12240 seconds, SN in contiuum is 2-3 We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v15.xml(Tic-Visit
:proposal-id 16747
:visit-id "15"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:29:21.0"
:trans-errors '(:WARNINGS 22 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 1583504
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "15"
:obset-id "15"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "15"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2624
:al-overhead-at-end 133
:internal-dur-at-end 132
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "15"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2620
:al-overhead-at-end 133
:internal-dur-at-end 132
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "15"
:orbit-number 3
:pcs-time 380
:si-vis-utilization 2622
:al-overhead-at-end 153
:internal-dur-at-end 394
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)false30No specrtral type for L1630MIR-14. Assume M2V, use J=9.703 (2mass) to normalize. Assume E(B-V)=0.1 Go for longer than you might expect!
10 seconds predicts SN of 50 with ND3, go for 25 seconds. (~80 SN)WIth total exposure time of 12240 seconds, SN in contiuum is 2-3 We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 12240 seconds, SN in contiuum is 2-3 We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 12240 seconds, SN in contiuum is 2-3 We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 12240 seconds, SN in contiuum is 2-3 We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v17.xml1667239570000301.0(Tic-Visit
:proposal-id 16747
:visit-id "17"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:30:47.0"
:trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 184448
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "17"
:obset-id "17"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "17"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2624
:al-overhead-at-end 120
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "17"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2623
:al-overhead-at-end 123
:internal-dur-at-end 379
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)false20No specrtral type for L1630MIR-14. Assume M2V, use J=9.703 (2mass) to normalize. Assume E(B-V)=0.1 Go for longer than you might expect!
10 seconds predicts SN of 50 with ND3, go for 25 seconds. (~80 SN)WIth total exposure time of 7512 seconds, SN in contiuum is 3-5. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 7512 seconds, SN in contiuum is 3-5. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 7512 seconds, SN in contiuum is 3-5. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v18.xml1667485281000301.0(Tic-Visit
:proposal-id 16747
:visit-id "18"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:30:48.0"
:trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 184448
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "18"
:obset-id "18"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "18"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2624
:al-overhead-at-end 120
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "18"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2623
:al-overhead-at-end 123
:internal-dur-at-end 379
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)false20No specrtral type for L1630MIR-14. Assume M2V, use J=9.703 (2mass) to normalize. Assume E(B-V)=0.1 Go for longer than you might expect!
10 seconds predicts SN of 50 with ND3, go for 25 seconds. (~80 SN)WIth total exposure time of 7512 seconds, SN in contiuum is 3-5. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 7512 seconds, SN in contiuum is 3-5. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.WIth total exposure time of 7512 seconds, SN in contiuum is 3-5. We will bin spectrally (and spatially if necessary to read a SN ~< 10. SN in any lines will be higher will not be binned.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v19.xml1667228142000301.0(Tic-Visit
:proposal-id 16747
:visit-id "19"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:30:49.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 258064
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "19"
:obset-id "19"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "19"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2623
:al-overhead-at-end 120
:internal-dur-at-end 227
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "19"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2623
:al-overhead-at-end 0
:internal-dur-at-end 598
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)false20No specrtral type for L1630MIR-14. Assume M2V, use J=9.703 (2mass) to normalize. Assume E(B-V)=0.1 Go for longer than you might expect!
10 seconds predicts SN of 50 with ND3, go for 25 seconds. (~80 SN)WIth total exposure time of 14649 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary) to reach a SN 10. Line SN is 5-40.WIth total exposure time of 14649 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary) to reach a SN 10. Line SN is 5-40.WIth total exposure time of 14649 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary) to reach a SN 10. Line SN is 5-40.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v25.xml1699630922000301.0(Tic-Visit
:proposal-id 16747
:visit-id "25"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:30:50.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 258064
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "25"
:obset-id "25"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "25"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2623
:al-overhead-at-end 120
:internal-dur-at-end 227
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "25"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2623
:al-overhead-at-end 0
:internal-dur-at-end 598
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)true20No specrtral type for L1630MIR-14. Assume M2V, use J=9.703 (2mass) to normalize. Assume E(B-V)=0.1 Go for longer than you might expect!
10 seconds predicts SN of 50 with ND3, go for 25 seconds. (~80 SN)WIth total exposure time of 14649 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary) to reach a SN 10. Line SN is 5-40.WIth total exposure time of 14649 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary) to reach a SN 10. Line SN is 5-40.WIth total exposure time of 14649 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary) to reach a SN 10. Line SN is 5-40.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v31.xmlcomplete -0.5" offset (2 of 3 failed in visit 25), partial at -1.5" offset (3 of 3 failed in visit 26)(Tic-Visit
:proposal-id 16747
:visit-id "31"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:30:52.0"
:trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 258064
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "31"
:obset-id "31"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "31"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2623
:al-overhead-at-end 120
:internal-dur-at-end 227
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "31"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2622
:al-overhead-at-end 0
:internal-dur-at-end 598
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)true20No specrtral type for L1630MIR-14. Assume M2V, use J=9.703 (2mass) to normalize. Assume E(B-V)=0.1 Go for longer than you might expect!
10 seconds predicts SN of 50 with ND3, go for 25 seconds. (~80 SN)WIth total exposure time of 14649 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary) to reach a SN 10. Line SN is 5-40.WIth total exposure time of 14649 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary) to reach a SN 10. Line SN is 5-40.WIth total exposure time of 14649 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary) to reach a SN 10. Line SN is 5-40.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v26.xml1699716427000301.0(Tic-Visit
:proposal-id 16747
:visit-id "26"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:30:53.0"
:trans-errors '(:WARNINGS 8 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 258064
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "26"
:obset-id "26"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "26"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2623
:al-overhead-at-end 120
:internal-dur-at-end 227
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "26"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2623
:al-overhead-at-end 0
:internal-dur-at-end 598
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)true20No specrtral type for L1630MIR-14. Assume M2V, use J=9.703 (2mass) to normalize. Assume E(B-V)=0.1 Go for longer than you might expect!
10 seconds predicts SN of 50 with ND3, go for 25 seconds. (~80 SN)WIth total exposure time of 14649 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary) to reach a SN 10. Line SN is 5-40.WIth total exposure time of 14649 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary) to reach a SN 10. Line SN is 5-40.WIth total exposure time of 14649 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary) to reach a SN 10. Line SN is 5-40.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v32.xmlcomplete -1.5" offset (3 of 3 failed in visit 26) complete (partial) +1.5" offset (2 of 3 failed in visit 27)(Tic-Visit
:proposal-id 16747
:visit-id "32"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:30:56.0"
:trans-errors '(:WARNINGS 8 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 258064
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "32"
:obset-id "32"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "32"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2623
:al-overhead-at-end 120
:internal-dur-at-end 227
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "32"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2621
:al-overhead-at-end 0
:internal-dur-at-end 598
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)true20No specrtral type for L1630MIR-14. Assume M2V, use J=9.703 (2mass) to normalize. Assume E(B-V)=0.1 Go for longer than you might expect!
10 seconds predicts SN of 50 with ND3, go for 25 seconds. (~80 SN)WIth total exposure time of 14649 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary) to reach a SN 10. Line SN is 5-40.WIth total exposure time of 14649 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary) to reach a SN 10. Line SN is 5-40.WIth total exposure time of 14649 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary) to reach a SN 10. Line SN is 5-40.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v27.xml1699796234000301.0(Tic-Visit
:proposal-id 16747
:visit-id "27"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:30:57.0"
:trans-errors '(:WARNINGS 8 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 258064
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "27"
:obset-id "27"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "27"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2623
:al-overhead-at-end 120
:internal-dur-at-end 227
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16747
:visit-id "27"
:orbit-number 2
:pcs-time 380
:si-vis-utilization 2623
:al-overhead-at-end 0
:internal-dur-at-end 598
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)true20No specrtral type for L1630MIR-14. Assume M2V, use J=9.703 (2mass) to normalize. Assume E(B-V)=0.1 Go for longer than you might expect!
10 seconds predicts SN of 50 with ND3, go for 25 seconds. (~80 SN)WIth total exposure time of 14649 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary) to reach a SN 10. Line SN is 5-40.WIth total exposure time of 14649 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary) to reach a SN 10. Line SN is 5-40.WIth total exposure time of 14649 seconds, SN in contiuum is ~4. We will bin spectrally (and spatially if necessary) to reach a SN 10. Line SN is 5-40.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v22.xml1695030413000271.0407567761351(Tic-Visit
:proposal-id 16747
:visit-id "22"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:30:58.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 521920
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "22"
:obset-id "22"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16747
:visit-id "22"
:orbit-number 1
:pcs-time 380
:si-vis-utilization 2620
:al-overhead-at-end 133
:internal-dur-at-end 394
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3005
:pcs-gap 0
)false10No ETC run performed. These are mainly targeted at instrumental background so are specified at the maximum exposure length on targets, not a specific SN target. ETC number is made up to reduce the number of yellow exclamation points I have to look at.No ETC run performed. These are mainly targeted at instrumental background so are specified at the maximum exposure length on targets, not a specific SN target. ETC number is made up to reduce the number of yellow exclamation points I have to look at.The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v24.xml1693017468000257.71009094614175(Tic-Visit
:proposal-id 16747
:visit-id "24"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:30:58.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 128816
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
:visit-id "24"
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)
(Tic-Orbit
:proposal-id 16747
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)true10The scheduling data was generated by CASM 32.1.3.CASM was run in Phase II mode./System/Volumes/Data/solaris/user1/wskipper/OP-cache/16747-v28.xml1694973386000271.0407567761351(Tic-Visit
:proposal-id 16747
:visit-id "28"
:proposal-version -1
:trans-version "20240627"
:date "30-Jul-2024 16:30:59.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 165632
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16747
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)
(Tic-Orbit
:proposal-id 16747
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:al-overhead-at-end 120
:internal-dur-at-end 606
:dark-offset NIL
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:max-dark-utilization 1920
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)true10