! File: 2861C.PROP ! Database: PEPDB ! Date: 17-FEB-1994:18:59:18 coverpage: title_1: LINKING HIPPARCOS TO THE EXTRAGALACTIC REFERENCE FRAME title_2: PART 4 OF 6, NEWB, CYCLE 2,CONTINUATION OF 2565-HIGH 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. ! 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: 121 name_1: NEWEGOB-17NEWHIP-17 descr_1: E pos_1: RA = 14.3291667D +/- .0008D, pos_2: DEC = -22.379722D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.41 +/- 1 ! targnum: 122 name_1: NEWHIP-17-REF descr_1: A pos_1: RA = 14.359D +/- .0008D, pos_2: DEC = -22.419861D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: 0.004616 dec_pm_val: -0.0120 fluxnum_1: 1 fluxval_1: V=9.23 +/- 1 ! targnum: 123 name_1: 120-REF descr_1: J,701 pos_1: RA = 14.28546D +/- .0008D, pos_2: DEC = -22.30838D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15.52 +/- 1 ! targnum: 124 name_1: 121-REF descr_1: J,701 pos_1: RA = 14.30759D +/- .0008D, pos_2: DEC = -22.32706D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.64 +/- 1 ! targnum: 125 name_1: 122-REF descr_1: J,701 pos_1: RA = 14.38805D +/- .0008D, pos_2: DEC = -22.41675D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.03 +/- 1 ! targnum: 221 name_1: NEWEGOB-19NEWHIP-19 descr_1: E pos_1: RA = 89.9475D +/- .0008D, pos_2: DEC = -50.4475D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.97 +/- 1 ! targnum: 222 name_1: NEWHIP-19-REF descr_1: A pos_1: RA = 89.7451667D +/- .0008D, pos_2: DEC = -50.677306D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: 0.002525 dec_pm_val: 0.0620 fluxnum_1: 1 fluxval_1: V=9.74 +/- 1 ! targnum: 223 name_1: 220-REF descr_1: J,701 pos_1: RA = 89.91909D +/- .0008D, pos_2: DEC = -50.52208D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15.41 +/- 1 ! targnum: 224 name_1: 221-REF descr_1: J,701 pos_1: RA = 89.87907D +/- .0008D, pos_2: DEC = -50.61648D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.29 +/- 1 ! targnum: 225 name_1: 222-REF descr_1: J,701 pos_1: RA = 89.86592D +/- .0008D, pos_2: DEC = -50.63073D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15.01 +/- 1 ! targnum: 321 name_1: NEWEGOB-20NEWHIP-20 descr_1: E pos_1: RA = 89.9475D +/- .0008D, pos_2: DEC = -50.4475D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.97 +/- 1 ! targnum: 322 name_1: NEWHIP-20-REF descr_1: A pos_1: RA = 89.9100833D +/- .0008D, pos_2: DEC = -50.309194D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: 0.002714 dec_pm_val: -0.0050 fluxnum_1: 1 fluxval_1: V=8.35 +/- 1 ! targnum: 323 name_1: 320-REF descr_1: J,701 pos_1: RA = 89.90621D +/- .0008D, pos_2: DEC = -50.4551D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.88 +/- 1 ! targnum: 324 name_1: 321-REF descr_1: J,701 pos_1: RA = 89.93128D +/- .0008D, pos_2: DEC = -50.39632D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.44 +/- 1 ! targnum: 325 name_1: 322-REF descr_1: J,701 pos_1: RA = 89.91411D +/- .0008D, pos_2: DEC = -50.38295D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.16 +/- 1 ! targnum: 421 name_1: NEWEGOB-21NEWHIP-21 descr_1: E pos_1: RA = 106.805D +/- .0008D, pos_2: DEC = 64.5997222D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.61 +/- 1 ! targnum: 422 name_1: NEWHIP-21-REF descr_1: A pos_1: RA = 106.643583D +/- .0008D, pos_2: DEC = 64.4200833D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.002162 dec_pm_val: 0.0010 fluxnum_1: 1 fluxval_1: V=8.44 +/- 1 ! targnum: 423 name_1: 420-REF descr_1: J,701 pos_1: RA = 106.71772D +/- .0008D, pos_2: DEC = 64.44931D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=11.25 +/- 1 ! targnum: 424 name_1: 421-REF descr_1: J,701 pos_1: RA = 106.64837D +/- .0008D, pos_2: DEC = 64.4052D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=10.42 +/- 1 ! targnum: 425 name_1: 422-REF descr_1: J,701 pos_1: RA = 106.85377D +/- .0008D, pos_2: DEC = 64.60806D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=9.18 +/- 1 ! targnum: 521 name_1: NEWEGOB-22NEWHIP-22 descr_1: E pos_1: RA = 119.499583D +/- .0008D, pos_2: DEC = 39.3408333D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.36 +/- 1 ! targnum: 522 name_1: NEWHIP-22-REF descr_1: A pos_1: RA = 119.465917D +/- .0008D, pos_2: DEC = 39.35875D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.002156 dec_pm_val: -0.0260 fluxnum_1: 1 fluxval_1: V=10.65 +/- 1 ! targnum: 523 name_1: 520-REF descr_1: J,701 pos_1: RA = 119.54556D +/- .0008D, pos_2: DEC = 39.32857D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.53 +/- 1 ! targnum: 524 name_1: 521-REF descr_1: J,701 pos_1: RA = 119.37033D +/- .0008D, pos_2: DEC = 39.44331D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=11.94 +/- 1 ! targnum: 525 name_1: 522-REF descr_1: J,701 pos_1: RA = 119.43167D +/- .0008D, pos_2: DEC = 39.39284D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.13 +/- 1 ! targnum: 621 name_1: NEWEGOB-23NEWHIP-23 descr_1: E pos_1: RA = 119.499583D +/- .0008D, pos_2: DEC = 39.3408333D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.36 +/- 1 ! targnum: 622 name_1: NEWHIP-23-REF descr_1: A pos_1: RA = 119.71325D +/- .0008D, pos_2: DEC = 39.4471667D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: 0.001036 dec_pm_val: -0.0320 fluxnum_1: 1 fluxval_1: V=9.36 +/- 1 ! targnum: 623 name_1: 620-REF descr_1: J,701 pos_1: RA = 119.54815D +/- .0008D, pos_2: DEC = 39.361D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.43 +/- 1 ! targnum: 624 name_1: 621-REF descr_1: J,701 pos_1: RA = 119.73009D +/- .0008D, pos_2: DEC = 39.47081D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.58 +/- 1 ! targnum: 625 name_1: 622-REF descr_1: J,701 pos_1: RA = 119.59576D +/- .0008D, pos_2: DEC = 39.43394D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.45 +/- 1 ! targnum: 721 name_1: NEWEGOB-24NEWHIP-24 descr_1: E pos_1: RA = 131.927083D +/- .0008D, pos_2: DEC = 34.7513889D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14 +/- 1 ! targnum: 722 name_1: NEWHIP-24-REF descr_1: A pos_1: RA = 132.066667D +/- .0008D, pos_2: DEC = 34.6044167D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.000891 dec_pm_val: -0.0560 fluxnum_1: 1 fluxval_1: V=10.34 +/- 1 ! targnum: 723 name_1: 720-REF descr_1: J,701 pos_1: RA = 131.98514D +/- .0008D, pos_2: DEC = 34.67217D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.91 +/- 1 ! targnum: 724 name_1: 721-REF descr_1: J,701 pos_1: RA = 132.02629D +/- .0008D, pos_2: DEC = 34.59709D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.05 +/- 1 ! targnum: 725 name_1: 722-REF descr_1: J,701 pos_1: RA = 132.00562D +/- .0008D, pos_2: DEC = 34.64041D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=11.58 +/- 1 ! targnum: 821 name_1: NEWEGOB-25NEWHIP-25 descr_1: E pos_1: RA = 131.927083D +/- .0008D, pos_2: DEC = 34.7513889D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14 +/- 1 ! targnum: 822 name_1: NEWHIP-25-REF descr_1: A pos_1: RA = 132.0685D +/- .0008D, pos_2: DEC = 34.5990278D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.000891 dec_pm_val: -0.0560 fluxnum_1: 1 fluxval_1: V=8.07 +/- 1 ! targnum: 823 name_1: 820-REF descr_1: J,701 pos_1: RA = 131.94585D +/- .0008D, pos_2: DEC = 34.65505D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.71 +/- 1 ! targnum: 824 name_1: 821-REF descr_1: J,701 pos_1: RA = 131.98514D +/- .0008D, pos_2: DEC = 34.67217D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.91 +/- 1 ! targnum: 825 name_1: 822-REF descr_1: J,701 pos_1: RA = 132.00562D +/- .0008D, pos_2: DEC = 34.64041D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=11.58 +/- 1 ! targnum: 921 name_1: NEWEGOB-26NEWHIP-26 descr_1: E pos_1: RA = 139.039167D +/- .0008D, pos_2: DEC = -62.324722D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.55 +/- 1 ! targnum: 922 name_1: NEWHIP-26-REF descr_1: A pos_1: RA = 139.234042D +/- .0008D, pos_2: DEC = -62.439778D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.001441 dec_pm_val: 0.0010 fluxnum_1: 1 fluxval_1: V=8.85 +/- 1 ! targnum: 923 name_1: 920-REF descr_1: J,701 pos_1: RA = 139.03312D +/- .0008D, pos_2: DEC = -62.30087D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.39 +/- 1 ! targnum: 924 name_1: 921-REF descr_1: J,701 pos_1: RA = 139.11404D +/- .0008D, pos_2: DEC = -62.37008D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.53 +/- 1 ! targnum: 925 name_1: 922-REF descr_1: J,701 pos_1: RA = 139.28187D +/- .0008D, pos_2: DEC = -62.43984D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=9.82 +/- 1 ! targnum: 931 name_1: NEWEGOB-27NEWHIP-27 descr_1: E pos_1: RA = 149.21875D +/- .0008D, pos_2: DEC = 41.2611111D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.5 +/- 1 ! targnum: 932 name_1: NEWHIP-27-REF descr_1: A pos_1: RA = 149.375292D +/- .0008D, pos_2: DEC = 41.1940278D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.000177 dec_pm_val: -0.0290 fluxnum_1: 1 fluxval_1: V=8.56 +/- 1 ! targnum: 933 name_1: 1020-REF descr_1: J,701 pos_1: RA = 149.31945D +/- .0008D, pos_2: DEC = 41.18792D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.21 +/- 1 ! targnum: 934 name_1: 1021-REF descr_1: J,701 pos_1: RA = 149.41865D +/- .0008D, pos_2: DEC = 41.20632D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.01 +/- 1 ! targnum: 935 name_1: 1022-REF descr_1: J,701 pos_1: RA = 149.24299D +/- .0008D, pos_2: DEC = 41.21783D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.09 +/- 1 ! targnum: 937 name_1: NEWEGOB-28NEWHIP-28 descr_1: E pos_1: RA = 149.21875D +/- .0008D, pos_2: DEC = 41.2611111D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.5 +/- 1 ! targnum: 938 name_1: NEWHIP-28-REF descr_1: A pos_1: RA = 149.421458D +/- .0008D, pos_2: DEC = 41.0556944D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.010344 dec_pm_val: -0.0240 fluxnum_1: 1 fluxval_1: V=5.16 +/- 1 ! targnum: 939 name_1: 1120-REF descr_1: J,701 pos_1: RA = 149.27049D +/- .0008D, pos_2: DEC = 41.18491D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.62 +/- 1 ! targnum: 940 name_1: 1121-REF descr_1: J,701 pos_1: RA = 149.24299D +/- .0008D, pos_2: DEC = 41.21783D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.09 +/- 1 ! targnum: 941 name_1: 1122-REF descr_1: J,701 pos_1: RA = 149.30694D +/- .0008D, pos_2: DEC = 41.10469D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15.18 +/- 1 ! targnum: 943 name_1: NEWEGOB-32NEWHIP-32 descr_1: E pos_1: RA = 184.78625D +/- .0008D, pos_2: DEC = -1.8247222D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15 +/- 1 ! targnum: 944 name_1: NEWHIP-32-REF descr_1: A pos_1: RA = 184.781208D +/- .0008D, pos_2: DEC = -2.04025D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.001801 dec_pm_val: 0.0100 fluxnum_1: 1 fluxval_1: V=9.32 +/- 1 ! targnum: 945 name_1: 1220-REF descr_1: J,701 pos_1: RA = 184.78792D +/- .0008D, pos_2: DEC = -1.97349D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.02 +/- 1 ! targnum: 946 name_1: 1221-REF descr_1: J,701 pos_1: RA = 184.7578D +/- .0008D, pos_2: DEC = -1.91865D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.66 +/- 1 ! targnum: 947 name_1: 1222-REF descr_1: J,701 pos_1: RA = 184.80722D +/- .0008D, pos_2: DEC = -1.81734D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.46 +/- 1 ! targnum: 949 name_1: NEWEGOB-33NEWHIP-33 descr_1: E pos_1: RA = 208.315417D +/- .0008D, pos_2: DEC = 63.7611111D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.84 +/- 1 ! targnum: 950 name_1: NEWHIP-33-REF descr_1: A pos_1: RA = 208.523792D +/- .0008D, pos_2: DEC = 63.8749722D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: 0.002120 dec_pm_val: 0.0180 fluxnum_1: 1 fluxval_1: V=10.37 +/- 1 ! targnum: 951 name_1: 1320-REF descr_1: J,701 pos_1: RA = 208.42321D +/- .0008D, pos_2: DEC = 63.7948D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.4 +/- 1 ! targnum: 952 name_1: 1321-REF descr_1: J,701 pos_1: RA = 208.44867D +/- .0008D, pos_2: DEC = 63.82775D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.98 +/- 1 ! targnum: 953 name_1: 1322-REF descr_1: J,701 pos_1: RA = 208.31469D +/- .0008D, pos_2: DEC = 63.70319D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.13 +/- 1 ! targnum: 955 name_1: NEWEGOB-34NEWHIP-34 descr_1: E pos_1: RA = 216.752083D +/- .0008D, pos_2: DEC = 23.8D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.95 +/- 1 ! targnum: 956 name_1: NEWHIP-34-REF descr_1: A pos_1: RA = 216.939083D +/- .0008D, pos_2: DEC = 23.8406389D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.036151 dec_pm_val: 0.0810 fluxnum_1: 1 fluxval_1: V=11.06 +/- 1 ! targnum: 957 name_1: 1420-REF descr_1: J,701 pos_1: RA = 216.88695D +/- .0008D, pos_2: DEC = 23.81001D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.3 +/- 1 ! targnum: 958 name_1: 1421-REF descr_1: J,701 pos_1: RA = 216.939083D +/- .0008D, pos_2: DEC = 23.8406389D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.039526 dec_pm_val: 0.0810 fluxnum_1: 1 fluxval_1: V=11.06 +/- 1 ! targnum: 959 name_1: 1422-REF descr_1: J,701 pos_1: RA = 216.82779D +/- .0008D, pos_2: DEC = 23.80675D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.07 +/- 1 ! targnum: 961 name_1: NEWEGOB-35NEWHIP-35 descr_1: E pos_1: RA = 220.53125D +/- .0008D, pos_2: DEC = 35.4397222D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.58 +/- 1 ! targnum: 962 name_1: NEWHIP-35-REF descr_1: A pos_1: RA = 220.4349583D +/- .0008D, pos_2: DEC = 35.2404444D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.001388 dec_pm_val: -0.0570 fluxnum_1: 1 fluxval_1: V=8.47 +/- 1 ! targnum: 963 name_1: 1520-REF descr_1: J,701 pos_1: RA = 220.5013583D +/- .0008D, pos_2: DEC = 35.40741D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.64 +/- 1 ! targnum: 964 name_1: 1521-REF descr_1: J,701 pos_1: RA = 220.4349583D +/- .0008D, pos_2: DEC = 35.2404444D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: -0.001698 dec_pm_val: -0.0570 fluxnum_1: 1 fluxval_1: V=8.47 +/- 1 ! targnum: 965 name_1: 1522-REF descr_1: J,701 pos_1: RA = 220.4622D +/- .0008D, pos_2: DEC = 35.35951D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.9 +/- 1 ! targnum: 967 name_1: NEWEGOB-36NEWHIP-36 descr_1: E pos_1: RA = 238.93D +/- .0008D, pos_2: DEC = 11.1891667D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15 +/- 1 ! targnum: 968 name_1: NEWHIP-36-REF descr_1: A pos_1: RA = 238.987708D +/- .0008D, pos_2: DEC = 10.9871389D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: 0.005501 dec_pm_val: -0.0161 fluxnum_1: 1 fluxval_1: V=10.87 +/- 1 ! targnum: 969 name_1: 1620-REF descr_1: J,701 pos_1: RA = 238.9198D +/- .0008D, pos_2: DEC = 11.07903D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.42 +/- 1 ! targnum: 970 name_1: 1621-REF descr_1: J,701 pos_1: RA = 238.97657D +/- .0008D, pos_2: DEC = 11.02725D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.05 +/- 1 ! targnum: 971 name_1: 1622-REF descr_1: J,701 pos_1: RA = 238.94194D +/- .0008D, pos_2: DEC = 11.18869D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.64 +/- 1 ! targnum: 973 name_1: NEWEGOB-37NEWHIP-37 descr_1: E pos_1: RA = 311.040417D +/- .0008D, pos_2: DEC = -10.723056D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.12 +/- 1 ! targnum: 974 name_1: NEWHIP-37-REF descr_1: A pos_1: RA = 310.817792D +/- .0008D, pos_2: DEC = -10.742139D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: 0.001425 dec_pm_val: 0.0160 fluxnum_1: 1 fluxval_1: V=7.82 +/- 1 ! targnum: 975 name_1: 1720-REF descr_1: J,701 pos_1: RA = 310.97917D +/- .0008D, pos_2: DEC = -10.75868D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.95 +/- 1 ! targnum: 976 name_1: 1721-REF descr_1: J,701 pos_1: RA = 310.88755D +/- .0008D, pos_2: DEC = -10.74283D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.7 +/- 1 ! targnum: 977 name_1: 1722-REF descr_1: J,701 pos_1: RA = 310.93433D +/- .0008D, pos_2: DEC = -10.76947D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.51 +/- 1 ! targnum: 979 name_1: NEWEGOB-38NEWHIP-38 descr_1: E pos_1: RA = 311.040417D +/- .0008D, pos_2: DEC = -10.723056D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.12 +/- 1 ! targnum: 980 name_1: NEWHIP-38-REF descr_1: A pos_1: RA = 311.154125D +/- .0008D, pos_2: DEC = -10.494417D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: 0.008068 dec_pm_val: -0.1220 fluxnum_1: 1 fluxval_1: V=8.28 +/- 1 ! targnum: 981 name_1: 1820-REF descr_1: J,701 pos_1: RA = 311.0972D +/- .0008D, pos_2: DEC = -10.55899D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.53 +/- 1 ! targnum: 982 name_1: 1821-REF descr_1: J,701 pos_1: RA = 311.04456D +/- .0008D, pos_2: DEC = -10.65618D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.92 +/- 1 ! targnum: 983 name_1: 1822-REF descr_1: J,701 pos_1: RA = 311.04675D +/- .0008D, pos_2: DEC = -10.69789D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.76 +/- 1 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 12.001 targname: NEWEGOB-17NEWHIP-17 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 12.001-12.011 NO GAP; req_3: SAME POS FOR 12.002-12.011 AS 12.001; req_4: CYCLE 2 / 12.001-12.011; req_5: COND IF POS MODE ASTROMETRY OPERATIONAL req_6: / 12.001-182.011; req_7: ORIENT 338.35D +/- .3D; req_8: POS TARG +159.758,-57.6; comment_1: NEAR JD2448893.49 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: 12.002 targname: 120-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 12.003 targname: 121-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 12.004 targname: 122-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 12.005 targname: NEWHIP-17-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 12.006 targname: NEWEGOB-17NEWHIP-17 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 12.007 targname: NEWHIP-17-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 12.008 targname: 122-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 12.009 targname: 121-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: 12.010 targname: 120-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: 12.011 targname: NEWEGOB-17NEWHIP-17 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 22.001 targname: NEWEGOB-19NEWHIP-19 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: ORIENT 28.56D +/- .3D; req_6: POS TARG +486.904,-126.798; comment_1: NEAR JD2449004.79V1 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: NEWHIP-19-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 22.006 targname: NEWEGOB-19NEWHIP-19 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 22.007 targname: NEWHIP-19-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: 22.008 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: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 22.011 targname: NEWEGOB-19NEWHIP-19 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 32.001 targname: NEWEGOB-20NEWHIP-20 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 32.001-32.011 NO GAP; req_3: SAME POS FOR 32.002-32.011 AS 32.001; req_4: CYCLE 2 / 32.001-32.011; req_5: ORIENT 7.99D +/- .3D; req_6: POS TARG -167.793,+40.07; comment_1: NEAR JD2448985.22 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: 32.002 targname: 320-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 32.003 targname: 321-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 32.004 targname: 322-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 32.005 targname: NEWHIP-20-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: 32.006 targname: NEWEGOB-20NEWHIP-20 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 32.007 targname: NEWHIP-20-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 32.008 targname: 322-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: 32.009 targname: 321-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 32.010 targname: 320-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 32.011 targname: NEWEGOB-20NEWHIP-20 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 42.001 targname: NEWEGOB-21NEWHIP-21 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 196.24D +/- .3D; req_6: POS TARG -335.011,-105.444; comment_1: NEAR JD2448982.88 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: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 42.003 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: 42.004 targname: 422-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 42.005 targname: NEWHIP-21-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 42.006 targname: NEWEGOB-21NEWHIP-21 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 42.007 targname: NEWHIP-21-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: 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: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 42.010 targname: 420-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 42.011 targname: NEWEGOB-21NEWHIP-21 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 52.001 targname: NEWEGOB-22NEWHIP-22 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 52.001-52.011 NO GAP; req_3: SAME POS FOR 52.002-52.011 AS 52.001; req_4: CYCLE 2 / 52.001-52.011; req_5: ORIENT 126.14D +/- .3D; req_6: POS TARG +8.771,+13.642; comment_1: NEAR JD2449036.03 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: 52.002 targname: 520-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 52.003 targname: 521-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 52.004 targname: 522-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 52.005 targname: NEWHIP-22-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 52.006 targname: NEWEGOB-22NEWHIP-22 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: 52.007 targname: NEWHIP-22-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 52.008 targname: 522-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 52.009 targname: 521-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 52.010 targname: 520-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 52.011 targname: NEWEGOB-22NEWHIP-22 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: 62.001 targname: NEWEGOB-23NEWHIP-23 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 228.7D +/- .3D; req_6: POS TARG +338.435,-46.398; comment_1: NEAR JD2448988.54 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: 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: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 62.004 targname: 622-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 62.005 targname: NEWHIP-23-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: 62.006 targname: NEWEGOB-23NEWHIP-23 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 62.007 targname: NEWHIP-23-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: 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: 62.010 targname: 620-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 62.011 targname: NEWEGOB-23NEWHIP-23 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 72.001 targname: NEWEGOB-24NEWHIP-24 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 72.001-72.011 NO GAP; req_3: SAME POS FOR 72.002-72.011 AS 72.001; req_4: CYCLE 2 / 72.001-72.011; req_5: ORIENT 136.74D +/- .3D; req_6: POS TARG -362.542,-127.097; comment_1: NEAR JD2449037.57 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: 72.002 targname: 720-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 72.003 targname: 721-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 72.004 targname: 722-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: 72.005 targname: NEWHIP-24-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 72.006 targname: NEWEGOB-24NEWHIP-24 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 72.007 targname: NEWHIP-24-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: 72.008 targname: 722-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 72.009 targname: 721-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 72.010 targname: 720-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 72.011 targname: NEWEGOB-24NEWHIP-24 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 82.001 targname: NEWEGOB-25NEWHIP-25 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 135.78D +/- .3D; req_6: POS TARG -359.672,-146.332; comment_1: NEAR JD2449038.43 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: NEWHIP-25-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: 82.006 targname: NEWEGOB-25NEWHIP-25 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 82.007 targname: NEWHIP-25-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND 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: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 82.010 targname: 820-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 82.011 targname: NEWEGOB-25NEWHIP-25 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 92.001 targname: NEWEGOB-26NEWHIP-26 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 137.15D +/- .3D; req_6: POS TARG -345.29,-52.201; comment_1: NEAR JD2449161.47 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: 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: 92.003 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: 92.004 targname: 922-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 92.005 targname: NEWHIP-26-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 92.006 targname: NEWEGOB-26NEWHIP-26 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 92.007 targname: NEWHIP-26-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 92.008 targname: 922-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 92.009 targname: 921-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! 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: NEWEGOB-26NEWHIP-26 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 102.001 targname: NEWEGOB-27NEWHIP-27 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 115.75D +/- .3D; req_6: POS TARG -291.442,-57.939; comment_1: NEAR JD2449107.32 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: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! 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: NEWHIP-27-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 102.006 targname: NEWEGOB-27NEWHIP-27 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 102.007 targname: NEWHIP-27-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! 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: NEWEGOB-27NEWHIP-27 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: 112.001 targname: NEWEGOB-28NEWHIP-28 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 112.001-112.011 NO GAP; req_3: SAME POS FOR 112.002-112.011 AS 112.001; req_4: CYCLE 2 / 112.001-112.011; req_5: ORIENT 145.89D +/- .3D; req_6: POS TARG -504.047,-112.004; comment_1: NEAR JD2449057.77 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: 112.002 targname: 1120-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 112.003 targname: 1121-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 112.004 targname: 1122-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 112.005 targname: NEWHIP-28-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 112.006 targname: NEWEGOB-28NEWHIP-28 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 112.007 targname: NEWHIP-28-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 112.008 targname: 1122-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 112.009 targname: 1121-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: 112.010 targname: 1120-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: 112.011 targname: NEWEGOB-28NEWHIP-28 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 122.001 targname: NEWEGOB-32NEWHIP-32 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 122.001-122.011 NO GAP; req_3: SAME POS FOR 122.002-122.011 AS 122.001; req_4: CYCLE 2 / 122.001-122.011; req_5: ORIENT 182.19D +/- .3D; req_6: POS TARG -402.324,-71.025; comment_1: NEAR JD2449072.46 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: 122.002 targname: 1220-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 122.003 targname: 1221-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 122.004 targname: 1222-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 122.005 targname: NEWHIP-32-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 122.006 targname: NEWEGOB-32NEWHIP-32 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 122.007 targname: NEWHIP-32-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: 122.008 targname: 1222-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 122.009 targname: 1221-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: 122.010 targname: 1220-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 122.011 targname: NEWEGOB-32NEWHIP-32 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 132.001 targname: NEWEGOB-33NEWHIP-33 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 132.001-132.011 NO GAP; req_3: SAME POS FOR 132.002-132.011 AS 132.001; req_4: CYCLE 2 / 132.001-132.011; req_5: ORIENT 202.85D +/- .3D; req_6: POS TARG +142.494,+22.438; comment_1: NEAR JD2449075.27 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: 132.002 targname: 1320-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 132.003 targname: 1321-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 132.004 targname: 1322-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 132.005 targname: NEWHIP-33-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: 132.006 targname: NEWEGOB-33NEWHIP-33 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 132.007 targname: NEWHIP-33-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 132.008 targname: 1322-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: 132.009 targname: 1321-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 132.010 targname: 1320-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 132.011 targname: NEWEGOB-33NEWHIP-33 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 142.001 targname: NEWEGOB-34NEWHIP-34 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 142.001-142.011 NO GAP; req_3: SAME POS FOR 142.002-142.011 AS 142.001; req_4: CYCLE 2 / 142.001-142.011; req_5: ORIENT 264.29D +/- .3D; req_6: POS TARG +402.249,-73.574; comment_1: NEAR JD2449045.43 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: 142.002 targname: 1420-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 142.003 targname: 1421-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: 142.004 targname: 1422-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 142.005 targname: NEWHIP-34-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 142.006 targname: NEWEGOB-34NEWHIP-34 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 142.007 targname: NEWHIP-34-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: 142.008 targname: 1422-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 142.009 targname: 1421-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 142.010 targname: 1420-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 142.011 targname: NEWEGOB-34NEWHIP-34 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 152.001 targname: NEWEGOB-35NEWHIP-35 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 152.001-152.011 NO GAP; req_3: SAME POS FOR 152.002-152.011 AS 152.001; req_4: CYCLE 2 / 152.001-152.011; req_5: ORIENT 203.16D +/- .3D; req_6: POS TARG -449.094,-84.194; comment_1: NEAR JD2449092.66 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: 152.002 targname: 1520-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 152.003 targname: 1521-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 152.004 targname: 1522-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 152.005 targname: NEWHIP-35-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 152.006 targname: NEWEGOB-35NEWHIP-35 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: 152.007 targname: NEWHIP-35-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 152.008 targname: 1522-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 152.009 targname: 1521-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 152.010 targname: 1520-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 152.011 targname: NEWEGOB-35NEWHIP-35 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: 162.001 targname: NEWEGOB-36NEWHIP-36 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 162.001-162.011 NO GAP; req_3: SAME POS FOR 162.002-162.011 AS 162.001; req_4: CYCLE 2 / 162.001-162.011; req_5: ORIENT 163.15D +/- .3D; req_6: POS TARG -389.559,-109.203; comment_1: NEAR JD2449139.84 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: 162.002 targname: 1620-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 162.003 targname: 1621-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 162.004 targname: 1622-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 162.005 targname: NEWHIP-36-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: 162.006 targname: NEWEGOB-36NEWHIP-36 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 162.007 targname: NEWHIP-36-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 162.008 targname: 1622-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 162.009 targname: 1621-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: 162.010 targname: 1620-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 162.011 targname: NEWEGOB-36NEWHIP-36 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 172.001 targname: NEWEGOB-37NEWHIP-37 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 172.001-172.011 NO GAP; req_3: SAME POS FOR 172.002-172.011 AS 172.001; req_4: CYCLE 2 / 172.001-172.011; req_5: ORIENT 87.31D +/- .3D; req_6: POS TARG +377.642,-129.178; comment_1: NEAR JD2448867.9 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: 172.002 targname: 1720-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 172.003 targname: 1721-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 172.004 targname: 1722-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: 172.005 targname: NEWHIP-37-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 172.006 targname: NEWEGOB-37NEWHIP-37 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 172.007 targname: NEWHIP-37-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: 172.008 targname: 1722-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 172.009 targname: 1721-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 172.010 targname: 1720-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 172.011 targname: NEWEGOB-37NEWHIP-37 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 182.001 targname: NEWEGOB-38NEWHIP-38 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 182.001-182.011 NO GAP; req_3: SAME POS FOR 182.002-182.011 AS 182.001; req_4: CYCLE 2 / 182.001-182.011; req_5: ORIENT 204.02D +/- .3D; req_6: POS TARG +451.351,-92.81; comment_1: NEAR JD2448831.2 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: 182.002 targname: 1820-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 182.003 targname: 1821-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: 182.004 targname: 1822-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 182.005 targname: NEWHIP-38-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: 182.006 targname: NEWEGOB-38NEWHIP-38 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 182.007 targname: NEWHIP-38-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 182.008 targname: 1822-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 182.009 targname: 1821-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 182.010 targname: 1820-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 182.011 targname: NEWEGOB-38NEWHIP-38 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! ! end of exposure logsheet ! 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