! File: 5060C.PROP ! Database: PEPDB ! Date: 23-FEB-1994:18:19:05 coverpage: title_1: LINKING HIPPARCOS TO THE EXTRAGALACTIC REFERENCE FRAME title_2: PART 2 OF 6, BR12-23, CYCLE 2,CONTINUATION OF 2565-HIGH-FIXED sci_cat: COOL STARS sci_subcat: ASTROMETRY proposal_for: GO cont_id: 2565 pi_title: DR pi_fname: PAUL pi_mi: D pi_lname: HEMENWAY pi_inst: UNIVERSITY OF TEXAS AT AUSTIN pi_country: USA pi_phone: (512)471-3431 keywords_1: REFERENCE FRAMES, HIPPARCOS, QUASARS hours_pri: 80.00 num_pri: 175 fgs: Y funds_amount: 292590 funds_length: 36 pi_position: RSSCI ! end of coverpage abstract: line_1: Determination of a non-rotating Reference Frame is crucial line_2: to progress in many areas, including: Galactic motions, line_3: local (Oort's A and B) and global (R0) parameters derived line_4: from them, solar system motion discrepancies (Planet X); line_5: and in conjunction with the VLBI radio reference frame, line_6: the registration of radio and optical images at an accuracy line_7: well below the resolution limit of HST images (0.06 arcsec). line_8: The goal of the Program is to tie the HIPPARCOS and Extra- line_9: galactic Reference Frames together at the 0.0005 arcsec and line_10: 0.0005 arcsec/year level. The HST data will allow a deter- line_11: mination of the brightness distribution in the stellar and line_12: extragalactic objects observed and time dependent changes line_13: therein at the 0.001 arcsec/year level. line_14: The Program requires targets distributed over the whole sky line_15: to define a rigid Reference Frame. GTO observations will line_16: provide initial first epoch data and preliminary proper motions. line_17: The observations will consist of relative positions of Extra- line_18: galactic objects (EGOs) and HIPPARCOS stars, measured with the line_19: FGSs. ! ! end of abstract general_form_proposers: lname: HEMENWAY fname: PAUL title: DR mi: D inst: UNIVERSITY OF TEXAS AT AUSTIN country: USA ! lname: ARGUE fname: NOEL title: DR inst: THE OBSERVATORIES country: ENGLAND ! lname: DUNCOMBE fname: RAYNOR title: DR mi: L inst: UNIVERSITY OF TEXAS AT AUSTIN country: USA ! lname: HUGHES fname: JAMES title: DR inst: U.S. NAVAL OBSERVATORY country: USA ! lname: JAUNCEY fname: DAVID title: DR inst: C.S.I.R.O. country: AUSTRALIA ! lname: JOHNSTON fname: KENNETH title: DR inst: U.S. NAVAL RESEARCH LAB country: USA ! lname: KOVALEVSKY fname: JEAN title: DR inst: C.E.R.G.A. country: FRANCE ! lname: LESTRADE fname: JEAN title: DR inst: BUREAU DE LONGITUDE country: FRANCE ! lname: PERRYMAN fname: MICHAEL title: DR inst: E.S.T.E.C. country: HOLLAND ! lname: PRESTON fname: ROBERT title: DR inst: JET PROPULSION LAB country: USA ! lname: TURON fname: CATHERINE title: DR inst: OBSERVATOIRE DE MEUDON country: FRANCE ! lname: DEVEGT fname: CHRISTIAN title: DR inst: HAMBURGER STERNWARTE country: FGR ! lname: WALTER fname: HANS title: DR inst: ANSTRONOMISCHE RECHENINSTITUT country: FGR ! lname: WHITE fname: GRAEME title: DR inst: C.S.I.R.O. country: AUSTRALIA ! lname: KRISTIAN fname: JEROME title: DR inst: CALTECH country: USA ! lname: TAPLEY fname: BYRON title: PROF. inst: UNIV OF TEXAS AT AUSTIN country: USA ! ! end of general_form_proposers block general_form_text: question: 2 section: 1 line_1: The astronomical uses of an accurate coordinate reference frame line_2: are manifest. The reference frame provides the kinematic basis line_3: for all dynamical studies of celestial objects. The HIPPARCOS line_4: satellite will determine positions, proper motions, and line_5: parallaxes for about 100000 stars evenly distributed over the line_6: sky (Kovalevsky, _Space Science Rev._, 39,41,1984). A residual line_7: time dependent rotation of the reference frame would introduce line_8: a systematic effect in the system of proper motions that biases line_9: all the astronomical uses that can be made of the system in line_10: kinematical and dynamical studies of the Galaxy. (Galactic line_11: differential rotation and its variation with distance, asymmetry line_12: of motions with respect to the galactic plane, kinematics of line_13: halo stars and other stellar populations, group motions, and line_14: determining the birth places of stars, are a few examples of line_15: galactic studies which are adversely affected by a residual line_16: rotation of the reference frame.) This proposal is to reduce line_17: this undesirable bias by determining the rotation of the line_18: HIPPARCOS frame with respect to extragalactic objects. The line_19: method is to measure the proper motion of some stars in the line_20: HIPPARCOS system with respect to extragalactic objects (EGOs) line_21: using the Hubble Space Telescope (HST). ! question: 2 section: 2 line_1: HST can provide the information needed to link the HIPPARCOS line_2: proper motion system to the fixed reference system defined by line_3: the EGOs. The object of the overall program is to obtain the line_4: observations necessary to determine this link to an accuracy line_5: of the order of the systematic regional errors that may exist line_6: in the final HIPPARCOS catalogue. line_8: The nominal HIPPARCOS accuracy for stars brighter than 10.5 is line_9: expected to be 0.002 arcsec in position and parallax, and 0.002 line_10: arcsec/year in proper motion. HIPPARCOS will observe objects line_11: between 10.5 and 12 magnitude with reduced accuracy. The basic line_12: HIPPARCOS data will be accurate large angle separations of stars line_13: (chords on the celestial sphere). The system solution will line_14: yield a "solid body" celestial coordinate system an order of line_15: magnitude more accurate systematically than the individual line_16: random errors of the individual stars. Caused by unknown line_17: systematic biases of instrumental origin, they have not been line_18: properly assessed, but they should not exceed 0.1 milliarcsec line_19: in position, or 0.1 milliarcsec/year in proper motion. ! question: 2 section: 3 line_1: However, the nature of the HIPPARCOS reference system is such line_2: that it has a double indeterminacy: an arbitrary "solid body" line_3: rotation proportional to time in its proper motion system, line_4: and an arbitrary solid body rotational offset from any line_5: "standard" (e.g. inertial or quasi-inertial) coordinate line_6: system, in position. line_8: R. L. Duncombe and P. D. Hemenway plan to use about 40 hours line_9: of GTO time to observe HIPPARCOS stars near extragalactic line_10: objects. The stars have been screened from about 300 stars line_11: by a large program of speckle interferometry specifically for line_12: this purpose. (C.f. Hemenway, et al., 1985 ESA special line_13: Publication SP-234, p.281; Argue, et al., _Mon. Not. RAS_, line_14: 206,669, and 216,447.) Drs. Franz and McAlister have done line_15: the northern hemisphere speckle observations (private line_16: communcation to PDH). ! question: 2 section: 4 line_1: Simulations by Froeschle and Kovalevsky (_Astron. Astrophys._, line_2: 116, 89, 1982) show that for observations evenly distribued line_3: over the sky, the elements of the rotation matrix would be line_4: obtained with an accuracy of 0.003 arcsec/year rms for 40 line_5: pairs and 0.0023 arcsec/year for 70 pairs. We have identified line_6: 175 stars around 91 EGOs that are observable astrometrically line_7: with HST. This distribution should allow the determination of line_8: the rotation matrix to an accuracy of the order of 0.0016 line_9: arcsec/year. However, these figures represent measurements line_10: over the lifetime of the HIPPARCOS mission, 2.5 years and the line_11: subsequent accuracy for the tie to EGOs at the end of the line_12: mission. A longer time base will reduce the error propor- line_13: tionally to the time base for the next several years after the line_14: HIPPARCOS mission is completed. The determination of the line_15: components of the rotation matrices depends critically on line_16: the distribution being uniform over the sphere. A loss of the line_17: sources south of -30 degrees declination increases the rms of line_18: the solution by a factor of 1.4, for example. Therefore, the line_19: first priority is to make sure that the EGOs that are observed line_20: are well distributed over the celestial sphere. ! question: 2 section: 5 line_1: Although this result is very accurate, it does not reach the line_2: expected accuracy of the HIPPARCOS system by a factor of 2 line_3: or 3. By reobserving all the HIPPARCOS star-EGO pairs over line_4: the course of the HST lifetime, the error of the individual line_5: motions is reduced proportionally to the time, and the overall line_6: solution should reach the 0.0008 arcsec/year level. If, in line_7: addition, about 15 radio stars are observed by VLBI giving a line_8: precision of proper motion of about 0.002 arcsec/year, then line_9: the expected global accuracy will become: line_10: a) 0.0025 arcsec/year if this proposal is not accepted, line_11: b) 0.0016 arcsec/yr if the GTO plus this proposal is accepted, line_12: c) 0.0012 arcsec/year if the full combined list is observed, and line_13: d) 0.0005 arcsec/yr if all observations of all types over the line_14: HST lifetime are observed. line_16: Some points which need stressing: line_17: a) Two HST time scales are important, one common to the line_18: HIPPARCOS epoch should start AS SOON AS POSSIBLE AFTER LAUNCH line_19: to reach the full potential of the tie between the VLBI frame line_20: and the HIPPARCOS frame, which requires observations of the line_21: same objects at the same epochs. The early epoch observations line_22: will also give the longest time base for the proper motion line_23: determinations, ! question: 2 section: 6 line_1: b) HIPPARCOS can only observe down to 12th magnitude with line_2: reduced accuracy. It cannot observe the Exragalactic objects line_3: directly, line_5: c) The program and object selection have been the subjects of line_6: intensive efforts by many people over the last few years, line_7: including the Working Group on Radio/Optical Identifications line_8: of IAU Commission 24, Subgroup 2130 of the HIPPARCOS Input line_9: Catalogue Consortium, a working group of one of the HIPPARCOS line_10: reduction consortia (F.A.S.T.), the speckle observers headed line_11: by Franz and McAlister in the north and Argue and Morgan in line_12: the south, and the southern hemisphere radio observers headed line_13: by Jauncey and White, who have identified the southern sources line_14: in this proposal through a major effort in the last two years, line_16: d) Jauncey, White, and Preston are working to make all the line_17: radio sources in this proposal part of the VLBI reference line_18: frame, including establishing the Australian VLBI capability, ! question: 2 section: 7 line_1: e) A set of 414 candidate stars near EGOs was included in the line_2: HIPPARCOS Input Catalogue in 1982 to make sure that the stars line_3: would be observed by HIPPARCOS. The speckle programs comprised line_4: these stars and the stars near the southern EGOs subsequently line_5: indentified by Jauncey and White. line_7: The objectives of this program are: line_8: 1) Provide an accurate tie of the HIPPARCOS Coordinate line_9: Reference System (positions and proper motions) to the best line_10: available extragalactic (e.g. VLBI) system, at the epoch of line_11: HIPPARCOS, line_13: 2) Tie the HIPPARCOS Reference System of proper motions to a line_14: (non-rotating) extragalactic system of optical objects, line_16: 3) Thereby establishing the connection between the Radio and line_17: Optical reference frames to the millarcsecond level (allowing line_18: the registration of HST images to radio images (VLA, VLBI, line_19: VLBA) to an accuracy well below the reolution limit of HST), line_20: anywhere in the sky, ! question: 2 section: 8 line_1: 4) Obtain single-epoch information on the brightness distri- line_2: bution of EGOs and stars, and line_4: 5) Obtain time dependent studies of the resolved and unresolved line_5: structure of (4) at the 0.001 arcsec/year level of accuracy. line_7: We have a brief statement from the HIPPARCOS Science Team line_8: supporting the importance of this work to the HIPPARCOS project, line_9: and its usefulness for both HIPPARCOS and HST astrometric data. line_10: The stement is included as an appendix to the proposal. ! question: 2 section: 9 line_1: APPENDIX: line_2: The following statement was communicated at the end of line_3: December, 1985: line_5: The eleven members of the HIPPARCOS Science Team, the scientific line_6: representatives who advise ESA directly on the scientific line_7: conduct, planning and organisation of the HIPPARCOS project, line_8: have expressed their full support for this collaborative line_9: programme. For the reasons set out in the proposal, the line_10: HIPPARCOS Science Team has confirmed the importance of the line_11: propsed observations for the interpretation and exploitation line_12: of both HIPPARCOS and Space Telescope astrometric data. line_14: Professor Adrian Blaauw, chairman of the ESA HIPPARCOS proposal line_15: selection committee; and Professor Walter Fricke*, chairman of line_16: the HIPPARCOS Input Catalogue Consortium steering committee, line_17: have also given their support to the present proposal. line_19: *Deceased 28 March 1988. ! question: 3 section: 1 line_1: The basic datum required is the relative separation line_2: angle of an EGO and a HIPPARCOS star. One would hope to rely on line_3: the knowledge of the FGS calibrations to simply measure one line_4: object and then the other. However, because of thermal and line_5: mechanical instabilities during "exposures", initially we will line_6: follow the GTO observing strategy of measuring two objects line_7: several times with some intermediate background stars as a line_8: stability check. Should the FGS measurements prove to be as line_9: stable as expected, then the number of check stars and the line_10: frequency of measurement may be reduced by a large factor (up line_11: to about 5). Since a single measurement of a single pair is line_12: expected to average about 20 minutes, overall slewing time is line_13: expected to be a major factor in actual time consumption. line_14: Based on OV/SV/GTO observations, we will learn how to optimize line_15: the use of HST for the objectives of this program. ! question: 3 section: 2 line_1: For EGOs brighter than 17.0, the observations will consist of line_2: obtaining FGS reading on: 1) the EGO, 2) the HIPPARCOS star, line_3: and 3-5) 3 background stars (when available) in the pickle. line_4: The following sequence will be observed: 1,3-5,2,1,2,5-3,1. line_5: When a star is brighter than V=9.0, the neutral density filter line_6: will be inserted. Whenever possible, another HIPPARCOS star line_7: will be included as one of the "background" stars. ! question: 4 section: 1 line_1: Simulations have shown that the expected regional systematic line_2: effects within the HIPPARCOS catalogue should be ~0.0001 arcsec. line_3: The expected individual HIPPARCOS position and motion errors line_4: are expected to be 0.002 arcsec and 0.002 arcsec/year. In line_5: tying the HIPPARCOS Reference Frame to EGOs, the error of the line_6: frame will depend on the errors of observations of the line_7: individual objects used. Two methods of high accuracy line_8: observations have been proposed. First is the VLBI observation line_9: of radio stars in HIPPARCOS directly with respect to EGOs. line_10: VLBI sensitivity limits the stars to a few RS CVn stars, with line_11: an accuracy of 0.002 arcsec. Some of these stars show radio- line_12: optical offsets at the 0.002 arcsec level. ! question: 4 section: 2 line_1: The second method is the one proposed here. The FGS measure- line_2: ments have an accuracy commensurate with both HIPPARCOS and line_3: radio measurements, again 0.002 arcsec. Other proposed line_4: methods rely on photographic astrometry of thousands of stars, line_5: galaxies, and QSOs, with measuring accuracies in the 0.1 to line_6: 0.01 arcsec range. These methods suffer from large systematic line_7: effects. No information about the optical structure of the line_8: EGOs or the stars can be obtained at teh 0.04 to 0.002 arcsec line_9: level. Such information is obtained as a matter of course line_10: during HST observations. line_12: The proposed HST observations are the only optical means which line_13: can approach the expected accuracy of the individual HIPPARCOS line_14: star measurements, and these observations are REQUIRED, to line_15: achieve a reduction to a non-rotating coordinate frame at the line_16: level of the internal systematic accuracy of HIPPARCOS. ! question: 5 section: 1 line_1: The FGS observations are expected to take 51.2 sec/setting= line_2: (1/40 sec/sample)*(32 samples/integration)*(2^6 integrations/ line_3: setting) seconds/setting for the 11 settings/"observation" line_4: described in (3) above, due to the need to average over the line_5: "thermal hunt" cycle of the FGSs. The overhead per observation line_6: is expected to be twice the "time on target". Thus we have line_7: allotted 20 minutes for a single "average" observation with the line_8: FGSs. line_9: DELETED LINES 52.001-52.011 FROM 2859 TO CREATE THIS PROPOSAL ! question: 5 section: 2 line_1: At an average of 3 single epoch observations/hour of HST time, line_2: with 40 hours allotted of GTO time and 8 hours GO time/year line_3: for 10 years, one arrives at 360 single-epoch observations to line_4: cover the 165 pairs. We expect to obtain 160 single epoch line_5: separations, 120 one-year proper motions, and a distribution line_6: of 2-5 year proper motions. Operational experience in the first line_7: year should substantially increase the efficiency of the line_8: observational procedures, so we should increase the number of line_9: observations we can obtain during the program, for the same line_10: number of requested hours. The program proposed here is the line_11: minimum acceptable program to reach an acceptable accuracy line_12: in the Extragalactic Link. The ideal goal is to obtain 10 line_13: year positions and proper motions for all 165 pairs, yielding line_14: a system solution in the submilliarcsecond range. The 20 line_15: hours for the first GO year will provide 30 single epochs. ! question: 6 section: 1 line_1: Because of power constraints, off-nominal roll will be available line_2: only under restricted conditions. Therefore, in order to line_3: maintain the maximum scheduling flexibility, the time of year line_4: has been selected to make the orientation of the astrometer line_5: FGS line_6: conform to the position angle of the EGO-HIPPARCOS star pair line_7: for the nominal roll on that date. In order to remove the line_8: effect of the HIPPARCOS star parallax in the determination of line_9: the proper motion, the observations of a given HIPPARCOS star line_10: EGO pair must be made at intervals of one year exactly, within line_11: a few days. line_14: Each observation consists of separate settings of the FGSs. line_15: The thermal/mechanical stability line_16: of the OTA/FGS is expected to hold only over about 10 minutes. line_17: We have included check star measurements in the observation line_18: plan. However, each entire observation sequence must be line_19: performed contiguously to allow accurate determination of the line_20: target relative positions. ! question: 8 section: 1 line_1: AT THE TIME OF THIS SUBMISSION, THE RESOURCE ESTIMATOR IS line_2: OVERESTIMATING THE FGS OVERHEAD. WE HAVE BEEN TOLD TO line_3: USE THE RESOURCE ESTIMATOR NUMBER, BUT THAT THE ACTUAL TIME line_4: CHARGED WILL BE REDUCED TO REFLECT A BETTER ESTIMATE OF THE line_5: TRUE OVERHEAD WHEN IT BECOMES AVAILABLE. The RESOURCE line_6: ESTIMATOR is currently giving 4.2 min between each FGS line_7: setting, while it takes less than a minute in reality. line_8: (1/26/93--PDH). ! question: 8 section: 2 line_1: This proposal is inteded to extend observations of the GTO line_2: sources over a longer time base to improve the accuracy of line_3: the proper motions and obtain more temporal structure data. line_4: The distribution of labor will be as follows: line_6: Cycle 1: Identification of Reference Stars - Hemenway line_7: Measurement of Positions of Targets, Reference Stars line_8: - Hemenway, UT Staff line_9: - Argue line_10: - Jauncey and White line_11: - deVegt line_13: Observations: Obtain HST data - All line_14: (Some at STScI, some at ECF) line_16: Reduction: Reduce HST data to positional differences and line_17: brightness distribution - All line_19: Incorporation of Stars in HIPPARCOS - Turon ! question: 8 section: 3 line_1: Reduction of HIPPARCOS Coordinates to Radio Frame line_2: - Kovalevsky line_3: - Preston line_4: - Lestrade line_5: - Johnston line_7: Reduction of HIPPARCOS Proper Motion System to EGO System line_8: - Johnston line_9: - Jauncey line_10: - deVegt line_11: - Preston line_12: - Hemenway line_13: - Perryman ! !end of general form text general_form_address: lname: HEMENWAY fname: PAUL mi: D title: DR. category: PI inst: UNIVERSITY OF TEXAS AT AUSTIN addr_1: DEPARTMENT OF ASTRONOMY addr_2: UNIVERSITY OF TEXAS AT AUSTIN city: AUSTIN state: TX zip: 78712 country: USA phone: (512)471-3431 ! ! end of general_form_address records fixed_targets: targnum: 221 name_1: 1226+023INCA221-83 descr_1: E pos_1: RA = 187.2779168D +/- .0008D, pos_2: DEC = 2.05238844D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.8 +/- 1 ! targnum: 222 name_1: INCA221-83-REF descr_1: A pos_1: RA = 187.3426375D +/- .0008D, pos_2: DEC = 1.977741667D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=10.2 +/- 1 ! targnum: 223 name_1: 220-REF descr_1: J,701 pos_1: RA = 187.2632525D +/- .0008D, pos_2: DEC = 2.0550676D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.9 +/- 1 ! targnum: 224 name_1: 221-REF descr_1: J,701 pos_1: RA = 187.4269925D +/- .0008D, pos_2: DEC = 1.9233676D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.35 +/- 1 ! targnum: 225 name_1: 222-REF descr_1: J,701 pos_1: RA = 187.3046925D +/- .0008D, pos_2: DEC = 2.0025076D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.49 +/- 1 ! targnum: 341 name_1: 1302-102INCA221-88 descr_1: E pos_1: RA = 196.3875619D +/- .0008D, pos_2: DEC = -10.55539617D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.9 +/- 1 ! targnum: 342 name_1: INCA221-88-REF descr_1: A pos_1: RA = 196.4238917D +/- .0008D, pos_2: DEC = -10.50187778D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.001424 dec_pm_val: -0.0040 fluxnum_1: 1 fluxval_1: V=9.33 +/- 1 ! targnum: 343 name_1: 340-REF descr_1: J,701 pos_1: RA = 196.410192D +/- .0008D, pos_2: DEC = -10.5667027D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.51 +/- 1 ! targnum: 344 name_1: 341-REF descr_1: J,701 pos_1: RA = 196.334062D +/- .0008D, pos_2: DEC = -10.6086927D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.71 +/- 1 ! targnum: 345 name_1: 342-REF descr_1: J,701 pos_1: RA = 196.389562D +/- .0008D, pos_2: DEC = -10.5285427D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.51 +/- 1 ! targnum: 361 name_1: 1302-102INCA221-89 descr_1: E pos_1: RA = 196.3875619D +/- .0008D, pos_2: DEC = -10.55539617D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.9 +/- 1 ! targnum: 363 name_1: 360-REF descr_1: J,701 pos_1: RA = 196.410192D +/- .0008D, pos_2: DEC = -10.5667027D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.51 +/- 1 ! targnum: 364 name_1: 361-REF descr_1: J,701 pos_1: RA = 196.6219D +/- .0008D, pos_2: DEC = -10.46196389D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.011050 dec_pm_val: 0.0020 fluxnum_1: 1 fluxval_1: V=9.53 +/- 1 ! targnum: 365 name_1: 362-REF descr_1: J,701 pos_1: RA = 196.557142D +/- .0008D, pos_2: DEC = -10.5340827D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.01 +/- 1 ! targnum: 381 name_1: INCA221-88INCA221-89 descr_1: E pos_1: RA = 196.4238917D +/- .0008D, pos_2: DEC = -10.50187778D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.001424 dec_pm_val: -0.0040 fluxnum_1: 1 fluxval_1: V=9.33 +/- 1 ! targnum: 382 name_1: INCA221-89-REF descr_1: A pos_1: RA = 196.6219D +/- .0008D, pos_2: DEC = -10.46196389D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.011050 dec_pm_val: 0.0020 fluxnum_1: 1 fluxval_1: V=9.53 +/- 1 ! targnum: 383 name_1: 380-REF descr_1: J,701 pos_1: RA = 196.5571439D +/- .0008D, pos_2: DEC = -10.5340828D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.01 +/- 1 ! targnum: 384 name_1: 381-REF descr_1: J,701 pos_1: RA = 196.4238917D +/- .0008D, pos_2: DEC = -10.50187778D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.001424 dec_pm_val: -0.0040 fluxnum_1: 1 fluxval_1: V=9.33 +/- 1 ! targnum: 385 name_1: 382-REF descr_1: J,701 pos_1: RA = 196.4283007D +/- .0008D, pos_2: DEC = -10.5314728D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15.09 +/- 1 ! targnum: 421 name_1: 1404+286INCA221-92 descr_1: E pos_1: RA = 211.7516444D +/- .0008D, pos_2: DEC = 28.4540805D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14 +/- 1 ! targnum: 422 name_1: INCA221-92-REF descr_1: A pos_1: RA = 211.6681167D +/- .0008D, pos_2: DEC = 28.48405556D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=10.7 +/- 1 ! targnum: 423 name_1: 420-REF descr_1: J,701 pos_1: RA = 211.7328958D +/- .0008D, pos_2: DEC = 28.43802778D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.005610 dec_pm_val: 0.0030 fluxnum_1: 1 fluxval_1: V=6.87 +/- 1 ! targnum: 424 name_1: 421-REF descr_1: J,701 pos_1: RA = 211.5370846D +/- .0008D, pos_2: DEC = 28.5498265D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.26 +/- 1 ! targnum: 425 name_1: 422-REF descr_1: J,701 pos_1: RA = 211.6156746D +/- .0008D, pos_2: DEC = 28.5051865D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=11.94 +/- 1 ! targnum: 441 name_1: 1404+286INCA221-93 descr_1: E pos_1: RA = 211.75164444D +/- .0008D, pos_2: DEC = 28.4540805D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14 +/- 1 ! targnum: 442 name_1: INCA221-93-REF descr_1: A pos_1: RA = 211.7328958D +/- .0008D, pos_2: DEC = 28.43802778D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.005610 dec_pm_val: 0.0030 fluxnum_1: 1 fluxval_1: V=6.96 +/- 1 ! targnum: 443 name_1: 440-REF descr_1: J,701 pos_1: RA = 211.8134146D +/- .0008D, pos_2: DEC = 28.4711465D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.93 +/- 1 ! targnum: 444 name_1: 441-REF descr_1: J,701 pos_1: RA = 211.7328958D +/- .0008D, pos_2: DEC = 28.43802778D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.005610 dec_pm_val: 0.0030 fluxnum_1: 1 fluxval_1: V=6.96 +/- 1 ! targnum: 445 name_1: 442-REF descr_1: J,701 pos_1: RA = 211.7212546D +/- .0008D, pos_2: DEC = 28.4544065D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.11 +/- 1 ! targnum: 621 name_1: 1514-241INCA221-104 descr_1: E pos_1: RA = 229.4242236D +/- .0008D, pos_2: DEC = -24.37207592D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15.2 +/- 1 ! targnum: 622 name_1: INCA221-104-REF descr_1: A pos_1: RA = 229.3956125D +/- .0008D, pos_2: DEC = -24.4771728D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.001099 dec_pm_val: 0.0150 fluxnum_1: 1 fluxval_1: V=10.3 +/- 1 ! targnum: 623 name_1: 620-REF descr_1: J,701 pos_1: RA = 229.3971298D +/- .0008D, pos_2: DEC = -24.451865D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.2 +/- 1 ! targnum: 624 name_1: 621-REF descr_1: J,701 pos_1: RA = 229.459759D +/- .0008D, pos_2: DEC = -24.383885D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.76 +/- 1 ! targnum: 625 name_1: 622-REF descr_1: J,701 pos_1: RA = 229.4388006D +/- .0008D, pos_2: DEC = -24.428315D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=10.46 +/- 1 ! targnum: 641 name_1: 1514-241INCA221-105 descr_1: E pos_1: RA = 229.4242236D +/- .0008D, pos_2: DEC = -24.37207592D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15.2 +/- 1 ! targnum: 642 name_1: INCA221-105-REF descr_1: A pos_1: RA = 229.6495083D +/- .0008D, pos_2: DEC = -24.24916667D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.001316 dec_pm_val: -0.0700 fluxnum_1: 1 fluxval_1: V=8.12 +/- 1 ! targnum: 643 name_1: 640-REF descr_1: J,701 pos_1: RA = 229.6495083D +/- .0008D, pos_2: DEC = -24.2491667D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=8.12 +/- 1 ! targnum: 644 name_1: 641-REF descr_1: J,701 pos_1: RA = 229.6331398D +/- .0008D, pos_2: DEC = -24.2182351D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.98 +/- 1 ! targnum: 645 name_1: 642-REF descr_1: J,701 pos_1: RA = 229.5622398D +/- .0008D, pos_2: DEC = -24.3241751D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.11 +/- 1 ! targnum: 741 name_1: 1758-651INCA221-117 descr_1: E pos_1: RA = 270.8473827D +/- .0008D, pos_2: DEC = -65.1269529D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15.4 +/- 1 ! targnum: 742 name_1: INCA221-117-REF descr_1: A pos_1: RA = 270.84880958D +/- .0008D, pos_2: DEC = -65.09446389D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.000792 dec_pm_val: -0.0190 fluxnum_1: 1 fluxval_1: V=8.349 +/- 1 ! targnum: 743 name_1: 740-REF descr_1: J,701 pos_1: RA = 270.8244952D +/- .0008D, pos_2: DEC = -65.0953701D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.61 +/- 1 ! targnum: 744 name_1: 741-REF descr_1: J,701 pos_1: RA = 270.8162744D +/- .0008D, pos_2: DEC = -65.0185201D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.25 +/- 1 ! targnum: 745 name_1: 742-REF descr_1: J,701 pos_1: RA = 270.8800077D +/- .0008D, pos_2: DEC = -65.0837601D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.98 +/- 1 ! targnum: 821 name_1: 2005-489INCA221-131 descr_1: E pos_1: RA = 302.3557951D +/- .0008D, pos_2: DEC = -48.83158905D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15.3 +/- 1 ! targnum: 822 name_1: INCA221-131-REF descr_1: A pos_1: RA = 302.24062D +/- .0008D, pos_2: DEC = -49.07865D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: 0.002036 dec_pm_val: -0.0270 fluxnum_1: 1 fluxval_1: V=9 +/- 1 ! targnum: 823 name_1: 820-REF descr_1: J,701 pos_1: RA = 302.34688D +/- .0008D, pos_2: DEC = -48.87523D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=10.13 +/- 1 ! targnum: 824 name_1: 821-REF descr_1: J,701 pos_1: RA = 302.25078D +/- .0008D, pos_2: DEC = -49.02343D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=11.67 +/- 1 ! targnum: 825 name_1: 822-REF descr_1: J,701 pos_1: RA = 302.35764D +/- .0008D, pos_2: DEC = -48.94211D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.63 +/- 1 ! targnum: 841 name_1: 2005-489INCA221-132 descr_1: E pos_1: RA = 302.3557951D +/- .0008D, pos_2: DEC = -48.83158905D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15.3 +/- 1 ! targnum: 842 name_1: INCA221-132-REF descr_1: A pos_1: RA = 302.27957D +/- .0008D, pos_2: DEC = -48.92646D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=10 +/- 1 ! targnum: 843 name_1: 840-REF descr_1: J,701 pos_1: RA = 302.41109D +/- .0008D, pos_2: DEC = -48.77169D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.12 +/- 1 ! targnum: 844 name_1: 841-REF descr_1: J,701 pos_1: RA = 302.34688D +/- .0008D, pos_2: DEC = -48.87523D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=10.13 +/- 1 ! targnum: 845 name_1: 842-REF descr_1: J,701 pos_1: RA = 302.24663D +/- .0008D, pos_2: DEC = -48.94986D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.43 +/- 1 ! targnum: 921 name_1: 2128-123INCA221-138 descr_1: E pos_1: RA = 322.8969252D +/- .0008D, pos_2: DEC = -12.11799794D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15.5 +/- 1 ! targnum: 922 name_1: INCA221-138-REF descr_1: A pos_1: RA = 322.8955875D +/- .0008D, pos_2: DEC = -11.93800278D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: 0.000681 dec_pm_val: -0.0300 fluxnum_1: 1 fluxval_1: V=8.57 +/- 1 ! targnum: 923 name_1: 920-REF descr_1: J,701 pos_1: RA = 322.8739708D +/- .0008D, pos_2: DEC = -12.0350361D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.35 +/- 1 ! targnum: 924 name_1: 921-REF descr_1: J,701 pos_1: RA = 322.90425D +/- .0008D, pos_2: DEC = -12.1236761D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.22 +/- 1 ! targnum: 925 name_1: 922-REF descr_1: J,701 pos_1: RA = 322.8902917D +/- .0008D, pos_2: DEC = -11.9345461D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.75 +/- 1 ! targnum: 941 name_1: 2128-123INCA221-139 descr_1: E pos_1: RA = 322.8969252D +/- .0008D, pos_2: DEC = -12.1179794D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15.5 +/- 1 ! targnum: 942 name_1: INCA221-139-REF descr_1: A pos_1: RA = 323.0774875D +/- .0008D, pos_2: DEC = -12.07151111D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=10.5 +/- 1 ! targnum: 943 name_1: 940-REF descr_1: J,701 pos_1: RA = 322.9042514D +/- .0008D, pos_2: DEC = -12.1236761D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.22 +/- 1 ! targnum: 944 name_1: 941-REF descr_1: J,701 pos_1: RA = 322.9944114D +/- .0008D, pos_2: DEC = -12.1441561D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.75 +/- 1 ! targnum: 945 name_1: 942-REF descr_1: J,701 pos_1: RA = 322.9991514D +/- .0008D, pos_2: DEC = -12.1520061D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.05 +/- 1 ! targnum: 967 name_1: 2200+420INCA221-143 descr_1: E pos_1: RA = 330.6803823D +/- .0008D, pos_2: DEC = 42.7777284D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.5 +/- 1 ! targnum: 968 name_1: INCA221-143-REF descr_1: A pos_1: RA = 330.605875D +/- .0008D, pos_2: DEC = 42.42541667D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: 0.001535 dec_pm_val: 0.0060 fluxnum_1: 1 fluxval_1: V=8.5 +/- 1 ! targnum: 969 name_1: 1020-REF descr_1: J,701 pos_1: RA = 330.6892658D +/- .0008D, pos_2: DEC = 42.2765133D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.81 +/- 1 ! targnum: 970 name_1: 1021-REF descr_1: J,701 pos_1: RA = 330.5786359D +/- .0008D, pos_2: DEC = 42.4255134D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.49 +/- 1 ! targnum: 971 name_1: 1022-REF descr_1: J,701 pos_1: RA = 330.6066758D +/- .0008D, pos_2: DEC =42.2963234D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.17 +/- 1 ! targnum: 973 name_1: 2200+420INCA221-172 descr_1: E pos_1: RA = 330.6803823D +/- .0008D, pos_2: DEC = 42.27777284D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.5 +/- 1 ! targnum: 974 name_1: INCA221-172-REF descr_1: A pos_1: RA = 330.5242959D +/- .0008D, pos_2: DEC = 42.3796434D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=8.5 +/- 1 ! targnum: 975 name_1: 1040-REF descr_1: J,701 pos_1: RA = 330.6892658D +/- .0008D, pos_2: DEC = 42.2765133D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.81 +/- 1 ! targnum: 976 name_1: 1041-REF descr_1: J,701 pos_1: RA = 330.5711559D +/- .0008D, pos_2: DEC = 42.3516534D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.41 +/- 1 ! targnum: 977 name_1: 1042-REF descr_1: J,701 pos_1: RA = 330.6066758D +/- .0008D, pos_2: DEC = 42.2963234D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.17 +/- 1 ! targnum: 979 name_1: INCA221-172 descr_1: E pos_1: RA = 330.5242959D +/- .0008D, pos_2: DEC = 42.3796434D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=8.5 +/- 1 ! targnum: 980 name_1: INCA221-143INCA221-172-REF descr_1: A pos_1: RA = 330.6059259D +/- .0008D, pos_2: DEC = 42.4254234D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: 0.001535 dec_pm_val: 0.0060 fluxnum_1: 1 fluxval_1: V=12 +/- 1 ! targnum: 981 name_1: 1060-REF descr_1: J,701 pos_1: RA = 330.5786359D +/- .0008D, pos_2: DEC = 42.4255134D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.49 +/- 1 ! targnum: 982 name_1: 1061-REF descr_1: J,701 pos_1: RA = 330.5711559D +/- .0008D, pos_2: DEC = 42.3516534D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.41 +/- 1 ! targnum: 983 name_1: 1062-REF descr_1: J,701 pos_1: RA = 330.4976759D +/- .0008D, pos_2: DEC = 42.3033234D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.19 +/- 1 ! targnum: 985 name_1: 2201+315INCA221-173 descr_1: E pos_1: RA = 330.8123988D +/- .0008D, pos_2: DEC = 31.76063005D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15.5 +/- 1 ! targnum: 986 name_1: INCA221-173-REF descr_1: A pos_1: RA = 330.7885083D +/- .0008D, pos_2: DEC = 31.86579167D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: 0.004082 dec_pm_val: 0.0290 fluxnum_1: 1 fluxval_1: V=9.4 +/- 1 ! targnum: 987 name_1: 8020-REF descr_1: J,701 pos_1: RA = 330.8075931D +/- .0008D, pos_2: DEC = 31.8431033D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.38 +/- 1 ! targnum: 988 name_1: 8021-REF descr_1: J,701 pos_1: RA = 330.7956931D +/- .0008D, pos_2: DEC = 31.7318433D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.11 +/- 1 ! targnum: 989 name_1: 8022-REF descr_1: J,701 pos_1: RA = 330.7822431D +/- .0008D, pos_2: DEC = 31.8192133D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.31 +/- 1 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 22.001 targname: 1226+023INCA221-83 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 req_2: SEQ 22.001-22.011 NO GAP; req_3: SAME POS FOR 22.002-22.011 AS 22.001; req_4: CYCLE 2 / 22.001-22.011; req_5: COND IF POS MODE ASTROMETRY OPERATIONAL req_6: / 22.001-802.011; req_7: ORIENT 130.14D +/- .3D; req_8: POS TARG -322.128,-41.621; comment_1: NEAR JD2449089.17 V1 AXIS AND comment_2: ORIENTATION SPECIFIED TO PUT comment_3: REFERENCE STARS IN PICKLE. JDTOBS IS comment_4: THE JULIAN DATE THAT THIS ORIENTATION comment_5: IS AT NOMINAL ROLL. 180D OPTION IS NOT ! linenum: 22.002 targname: 220-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 22.003 targname: 221-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 22.004 targname: 222-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 22.005 targname: INCA221-83-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 22.006 targname: 1226+023INCA221-83 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 22.007 targname: INCA221-83-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 22.008 targname: 222-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 22.009 targname: 221-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 22.010 targname: 220-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 22.011 targname: 1226+023INCA221-83 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 34.001 targname: 1302-102INCA221-88 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 req_2: SEQ 34.001-34.011 NO GAP; req_3: SAME POS FOR 34.002-34.011 AS 34.001; req_4: CYCLE 2 / 34.001-34.011; req_5: ORIENT 28.55D +/- .3D; req_6: POS TARG -71.738,-28.785; comment_1: NEAR JD2449086.54 V1 AXIS AND comment_2: ORIENTATION SPECIFIED TO PUT comment_3: REFERENCE STARS IN PICKLE. JDTOBS IS comment_4: THE JULIAN DATE THAT THIS ORIENTATION comment_5: IS AT NOMINAL ROLL. 180D OPTION IS NOT ! linenum: 34.002 targname: 340-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 34.003 targname: 341-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 34.004 targname: 342-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 34.005 targname: INCA221-88-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 34.006 targname: 1302-102INCA221-88 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 34.007 targname: INCA221-88-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 34.008 targname: 342-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 34.009 targname: 341-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 34.010 targname: 340-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 34.011 targname: 1302-102INCA221-88 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 36.001 targname: 1302-102INCA221-89 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 req_2: SEQ 36.001-36.011 NO GAP; req_3: SAME POS FOR 36.002-36.011 AS 36.001; req_4: CYCLE 2 / 36.001-36.011; req_5: ORIENT 61.8D +/- .3D; req_6: POS TARG -398.743,-202.752; comment_1: NEAR JD2449088.94 V1 AXIS AND comment_2: ORIENTATION SPECIFIED TO PUT comment_3: REFERENCE STARS IN PICKLE. JDTOBS IS comment_4: THE JULIAN DATE THAT THIS ORIENTATION comment_5: IS AT NOMINAL ROLL. 180D OPTION IS NOT ! linenum: 36.002 targname: 360-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 36.003 targname: 361-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 36.004 targname: 362-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 36.005 targname: INCA221-89-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 36.006 targname: 1302-102INCA221-89 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 36.007 targname: INCA221-89-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 36.008 targname: 362-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 36.009 targname: 361-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 36.010 targname: 360-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 36.011 targname: 1302-102INCA221-89 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 38.001 targname: INCA221-88INCA221-89 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 req_2: SEQ 38.001-38.011 NO GAP; req_3: SAME POS FOR 38.002-38.011 AS 38.001; req_4: CYCLE 2 / 38.001-38.011; req_5: ORIENT 78.96D +/- .3D; req_6: POS TARG -362.997,-134.744; comment_1: NEAR JD2449093.86 V1 AXIS AND comment_2: ORIENTATION SPECIFIED TO PUT comment_3: REFERENCE STARS IN PICKLE. JDTOBS IS comment_4: THE JULIAN DATE THAT THIS ORIENTATION comment_5: IS AT NOMINAL ROLL. 180D OPTION IS NOT ! linenum: 38.002 targname: 380-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 38.003 targname: 381-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 38.004 targname: 382-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 38.005 targname: INCA221-89-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 38.006 targname: INCA221-88INCA221-89 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 38.007 targname: INCA221-89-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 38.008 targname: 382-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 38.009 targname: 381-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 38.010 targname: 380-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 38.011 targname: INCA221-88INCA221-89 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 42.001 targname: 1404+286INCA221-92 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 req_2: SEQ 42.001-42.011 NO GAP; req_3: SAME POS FOR 42.002-42.011 AS 42.001; req_4: CYCLE 2 / 42.001-42.011; req_5: ORIENT 293.44D +/- .3D; req_6: POS TARG +27.788,-24.276; comment_1: NEAR JD2448998.37 V1 AXIS AND comment_2: ORIENTATION SPECIFIED TO PUT comment_3: REFERENCE STARS IN PICKLE. JDTOBS IS comment_4: THE JULIAN DATE THAT THIS ORIENTATION comment_5: IS AT NOMINAL ROLL. 180D OPTION IS NOT ! linenum: 42.002 targname: 420-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 42.003 targname: 421-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 42.004 targname: 422-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 42.005 targname: INCA221-92-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 42.006 targname: 1404+286INCA221-92 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 42.007 targname: INCA221-92-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 42.008 targname: 422-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 42.009 targname: 421-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 42.010 targname: 420-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 42.011 targname: 1404+286INCA221-92 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 44.001 targname: 1404+286INCA221-93 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 req_2: SEQ 44.001-44.011 NO GAP; req_3: SAME POS FOR 44.002-44.011 AS 44.001; req_4: CYCLE 2 / 44.001-44.011; req_5: ORIENT 293.44D +/- .3D; req_6: POS TARG +100.23,-0.454; comment_1: NEAR JD2449055.15 V1 AXIS AND comment_2: ORIENTATION SPECIFIED TO PUT comment_3: REFERENCE STARS IN PICKLE. JDTOBS IS comment_4: THE JULIAN DATE THAT THIS ORIENTATION comment_5: IS AT NOMINAL ROLL. 180D OPTION IS NOT ! linenum: 44.002 targname: 440-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 44.003 targname: 441-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 44.004 targname: 442-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 44.005 targname: INCA221-93-REF config: FGS opmode: POS aperture: 3 sp_element: F5ND num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 44.006 targname: 1404+286INCA221-93 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 44.007 targname: INCA221-93-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 44.008 targname: 442-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 44.009 targname: 441-REF config: FGS opmode: POS aperture: 3 sp_element: F5ND num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 44.010 targname: 440-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 44.011 targname: 1404+286INCA221-93 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 62.001 targname: 1514-241INCA221-104 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 req_2: SEQ 62.001-62.011 NO GAP; req_3: SAME POS FOR 62.002-62.011 AS 62.001; req_4: CYCLE 2 / 62.001-62.011; req_5: ORIENT 36.47D +/- .3D; req_6: POS TARG +265.6,-105.443; comment_1: NEAR JD2449123.81 V1 AXIS AND comment_2: ORIENTATION SPECIFIED TO PUT comment_3: REFERENCE STARS IN PICKLE. JDTOBS IS comment_4: THE JULIAN DATE THAT THIS ORIENTATION comment_5: IS AT NOMINAL ROLL. 180D OPTION IS NOT ! linenum: 62.002 targname: 620-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 62.003 targname: 621-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 62.004 targname: 622-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 62.005 targname: INCA221-104-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 62.006 targname: 1514-241INCA221-104 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 62.007 targname: INCA221-104-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 62.008 targname: 622-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 62.009 targname: 621-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 62.010 targname: 620-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 62.011 targname: 1514-241INCA221-104 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 64.001 targname: 1514-241INCA221-105 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 req_2: SEQ 64.001-64.011 NO GAP; req_3: SAME POS FOR 64.002-64.011 AS 64.001; req_4: CYCLE 2 / 64.001-64.011; req_5: ORIENT 54.83D +/- .3D; req_6: POS TARG -479.889,-101.869; comment_1: NEAR JD2449126.48 V1 AXIS AND comment_2: ORIENTATION SPECIFIED TO PUT comment_3: REFERENCE STARS IN PICKLE. JDTOBS IS comment_4: THE JULIAN DATE THAT THIS ORIENTATION comment_5: IS AT NOMINAL ROLL. 180D OPTION IS NOT ! linenum: 64.002 targname: 640-REF config: FGS opmode: POS aperture: 3 sp_element: F5ND num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 64.003 targname: 641-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 64.004 targname: 642-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 64.005 targname: INCA221-105-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 64.006 targname: 1514-241INCA221-105 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 64.007 targname: INCA221-105-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 64.008 targname: 642-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 64.009 targname: 641-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 64.010 targname: 640-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 64.011 targname: 1514-241INCA221-105 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 74.001 targname: 1758-651INCA221-117 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 req_2: SEQ 74.001-74.011 NO GAP; req_3: SAME POS FOR 74.002-74.011 AS 74.001; req_4: CYCLE 2 / 74.001-74.011; req_5: ORIENT 358.3D +/- .3D; req_6: POS TARG -114.747,+1.855; comment_1: NEAR JD2449158.68 V1 AXIS AND comment_2: ORIENTATION SPECIFIED TO PUT comment_3: REFERENCE STARS IN PICKLE. JDTOBS IS comment_4: THE JULIAN DATE THAT THIS ORIENTATION comment_5: IS AT NOMINAL ROLL. 180D OPTION IS NOT ! linenum: 74.002 targname: 740-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 74.003 targname: 741-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 74.004 targname: 742-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 74.005 targname: INCA221-117-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 74.006 targname: 1758-651INCA221-117 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 74.007 targname: INCA221-117-REF config: FGS opmode: POS aperture: 3 sp_element: F5ND num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 74.008 targname: 742-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 74.009 targname: 741-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 74.010 targname: 740-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 74.011 targname: 1758-651INCA221-117 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 82.001 targname: 2005-489INCA221-131 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 req_2: SEQ 82.001-82.011 NO GAP; req_3: SAME POS FOR 82.002-82.011 AS 82.001; req_4: CYCLE 2 / 82.001-82.011; req_5: ORIENT 19.43D +/- .3D; req_6: POS TARG +470.997,-89.003; comment_1: NEAR JD2448836.86 V1 AXIS AND comment_2: ORIENTATION SPECIFIED TO PUT comment_3: REFERENCE STARS IN PICKLE. JDTOBS IS comment_4: THE JULIAN DATE THAT THIS ORIENTATION comment_5: IS AT NOMINAL ROLL. 180D OPTION IS NOT ! linenum: 82.002 targname: 820-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 82.003 targname: 821-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 82.004 targname: 822-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 82.005 targname: INCA221-131-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 82.006 targname: 2005-489INCA221-131 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 82.007 targname: INCA221-131-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 82.008 targname: 822-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 82.009 targname: 821-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 82.010 targname: 820-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 82.011 targname: 2005-489INCA221-131 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 84.001 targname: 2005-489INCA221-132 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 req_2: SEQ 84.001-84.011 NO GAP; req_3: SAME POS FOR 84.002-84.011 AS 84.001; req_4: CYCLE 2 / 84.001-84.011; req_5: ORIENT 22.83D +/- .3D; req_6: POS TARG +132.04,-56.08; comment_1: NEAR JD2448839.11 V1 AXIS AND comment_2: ORIENTATION SPECIFIED TO PUT comment_3: REFERENCE STARS IN PICKLE. JDTOBS IS comment_4: THE JULIAN DATE THAT THIS ORIENTATION comment_5: IS AT NOMINAL ROLL. 180D OPTION IS NOT ! linenum: 84.002 targname: 840-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 84.003 targname: 841-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 84.004 targname: 842-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 84.005 targname: INCA221-132-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 84.006 targname: 2005-489INCA221-132 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 84.007 targname: INCA221-132-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 84.008 targname: 842-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 84.009 targname: 841-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 84.010 targname: 840-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 84.011 targname: 2005-489INCA221-132 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 92.001 targname: 2128-123INCA221-138 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 req_2: SEQ 92.001-92.011 NO GAP; req_3: SAME POS FOR 92.002-92.011 AS 92.001; req_4: CYCLE 2 / 92.001-92.011; req_5: ORIENT 168.57D +/- .3D; req_6: POS TARG +261.154,-88.061; comment_1: NEAR JD2448848.13 V1 AXIS AND comment_2: ORIENTATION SPECIFIED TO PUT comment_3: REFERENCE STARS IN PICKLE. JDTOBS IS comment_4: THE JULIAN DATE THAT THIS ORIENTATION comment_5: IS AT NOMINAL ROLL. 180D OPTION IS NOT ! linenum: 92.002 targname: 920-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 92.003 targname: 921-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 92.004 targname: 922-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 92.005 targname: INCA221-138-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 92.006 targname: 2128-123INCA221-138 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 92.007 targname: INCA221-138-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 92.008 targname: 922-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 92.009 targname: 921-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 92.010 targname: 920-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 92.011 targname: 2128-123INCA221-138 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 94.001 targname: 2128-123INCA221-139 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 req_2: SEQ 94.001-94.011 NO GAP; req_3: SAME POS FOR 94.002-94.011 AS 94.001; req_4: CYCLE 2 / 94.001-94.011; req_5: ORIENT 69.23D +/- .3D; req_6: POS TARG -388.133,-163.627; comment_1: NEAR JD2448877.65 V1 AXIS AND comment_2: ORIENTATION SPECIFIED TO PUT comment_3: REFERENCE STARS IN PICKLE. JDTOBS IS comment_4: THE JULIAN DATE THAT THIS ORIENTATION comment_5: IS AT NOMINAL ROLL. 180D OPTION IS NOT ! linenum: 94.002 targname: 940-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 94.003 targname: 941-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 94.004 targname: 942-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 94.005 targname: INCA221-139-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 94.006 targname: 2128-123INCA221-139 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 94.007 targname: INCA221-139-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 94.008 targname: 942-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 94.009 targname: 941-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 94.010 targname: 940-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 94.011 targname: 2128-123INCA221-139 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 102.001 targname: 2200+420INCA221-143 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 req_2: SEQ 102.001-102.011 NO GAP; req_3: SAME POS FOR 102.002-102.011 AS 102.001; req_4: CYCLE 2 / 102.001-102.011; req_5: ORIENT 123.42D +/- .3D; req_6: POS TARG +261.361,-93.065; comment_1: NEAR JD2448850.42 V1 AXIS AND comment_2: ORIENTATION SPECIFIED TO PUT comment_3: REFERENCE STARS IN PICKLE. JDTOBS IS comment_4: THE JULIAN DATE THAT THIS ORIENTATION comment_5: IS AT NOMINAL ROLL. 180D OPTION IS NOT ! linenum: 102.002 targname: 1020-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 102.003 targname: 1021-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 102.004 targname: 1022-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 102.005 targname: INCA221-143-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 102.006 targname: 2200+420INCA221-143 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 102.007 targname: INCA221-143-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 102.008 targname: 1022-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 102.009 targname: 1021-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 102.010 targname: 1020-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 102.011 targname: 2200+420INCA221-143 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 104.001 targname: 2200+420INCA221-172 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 req_2: SEQ 104.001-104.011 NO GAP; req_3: SAME POS FOR 104.002-104.011 AS 104.001; req_4: CYCLE 2 / 104.001-104.011; req_5: ORIENT 136.75D +/- .3D; req_6: POS TARG +272.019,-93.703; comment_1: NEAR JD2448891.02 V1 AXIS AND comment_2: ORIENTATION SPECIFIED TO PUT comment_3: REFERENCE STARS IN PICKLE. JDTOBS IS comment_4: THE JULIAN DATE THAT THIS ORIENTATION comment_5: IS AT NOMINAL ROLL. 180D OPTION IS NOT ! linenum: 104.002 targname: 1040-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 104.003 targname: 1041-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 104.004 targname: 1042-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 104.005 targname: INCA221-172-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 104.006 targname: 2200+420INCA221-172 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 104.007 targname: INCA221-172-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 104.008 targname: 1042-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 104.009 targname: 1041-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 104.010 targname: 1040-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 104.011 targname: 2200+420INCA221-172 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 106.001 targname: INCA221-172 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 req_2: SEQ 106.001-106.011 NO GAP; req_3: SAME POS FOR 106.002-106.011 AS 106.001; req_4: CYCLE 2 / 106.001-106.011; req_5: ORIENT 207.52D +/- .3D; req_6: POS TARG -222.971,-39.259; comment_1: NEAR JD2448827.79 V1 AXIS AND comment_2: ORIENTATION SPECIFIED TO PUT comment_3: REFERENCE STARS IN PICKLE. JDTOBS IS comment_4: THE JULIAN DATE THAT THIS ORIENTATION comment_5: IS AT NOMINAL ROLL. 180D OPTION IS NOT ! linenum: 106.002 targname: 1060-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 106.003 targname: 1061-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 106.004 targname: 1062-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 106.005 targname: INCA221-143INCA221-172-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 106.006 targname: INCA221-172 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 106.007 targname: INCA221-143INCA221-172-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 106.008 targname: 1062-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 106.009 targname: 1061-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 106.010 targname: 1060-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 106.011 targname: INCA221-172 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 802.001 targname: 2201+315INCA221-173 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 req_2: SEQ 802.001-802.011 NO GAP; req_3: SAME POS FOR 802.002-802.011 AS 802.001; req_4: CYCLE 2 / 802.001-802.011; req_5: ORIENT 174.37D +/- .3D; req_6: POS TARG +180.714,-31.474; comment_1: NEAR JD2448860.34 V1 AXIS AND comment_2: ORIENTATION SPECIFIED TO PUT comment_3: REFERENCE STARS IN PICKLE. JDTOBS IS comment_4: THE JULIAN DATE THAT THIS ORIENTATION comment_5: IS AT NOMINAL ROLL. 180D OPTION IS NOT ! linenum: 802.002 targname: 8020-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 802.003 targname: 8021-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 802.004 targname: 8022-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 802.005 targname: INCA221-173-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 802.006 targname: 2201+315INCA221-173 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 802.007 targname: INCA221-173-REF config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: 1 param_1: DATA-RATE = 32 ! linenum: 802.008 targname: 8022-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 802.009 targname: 8021-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 802.010 targname: 8020-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 802.011 targname: 2201+315INCA221-173 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! ! end of exposure logsheet ! 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