! $Id: 5337,v 4.1 1994/07/27 16:48:34 pepsa Exp $ coverpage: title_1: LINKING HIPPARCOS TO THE EXTRAGALACTIC REFERENCE FRAME title_2: NEWHIP-C, PART 5 OF 8 - CONTINUATION OF 2565, CYCLE 4 HIGH sci_cat: COOL STARS sci_subcat: ASTROMETRY proposal_for: GO large_proj: Y longterm: 3 cont_id: 5331 pi_fname: PAUL pi_lname: HEMENWAY pi_inst: 3550 pi_country: USA pi_phone: 512 4713431 hours_pri: 13.58 num_pri: 90 fgs: Y time_crit: Y funds_amount: 165000 funds_length: 12 ! 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 inst: UNIVERSITY OF TEXAS AT AUSTIN country: USA ! lname: ARGUE fname: NOEL inst: 8014 country: UK esa: Y ! lname: DUNCOMBE fname: RAYNOR inst: 3550 country: USA ! lname: JAUNCEY fname: DAVID inst: 4130 country: AUSTRALIA ! lname: JOHNSTON fname: KENNETH inst: 3640 country: USA ! lname: KOVALEVSKY fname: JEAN inst: 5410 country: FRANCE esa: Y ! lname: KRISTIAN fname: JEROME inst: 3030 country: USA ! lname: LATTANZI fname: MARIO inst: 3470 country: USA esa: Y ! lname: LESTRADE fname: JEAN inst: 5468 country: FRANCE esa: Y ! lname: PERRYMAN fname: MICHAEL inst: 6820 country: THE NETHERLANDS esa: Y ! lname: PRESTON fname: ROBERT inst: 2370 country: USA ! lname: TAPLEY fname: BYRON inst: 3550 country: USA ! lname: TURON fname: CATHERINE inst: 5468 country: FRANCE esa: Y ! lname: DEVEGT fname: CHRISTIAN inst: 5580 country: GERMANY esa: Y ! lname: WALTER fname: HANS inst: 5515 country: GERMANY esa: Y ! lname: WHITE fname: GRAEME inst: 4130 country: AUSTRALIA ! ! end of general_form_proposers block general_form_text: ! ! ! ! ! ! ! ! ! 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, optical, and line_5: mechanical instabilities during "exposures", 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. Since a single observation set of a single pair is line_9: expected to average about 30 minutes, overall slewing time is line_10: expected to be a major factor in actual time consumption. line_11: Based on OV/SV/GTO observations, this strategy will optimize line_12: the use of HST for the objectives of this program. line_13: The observations consist of line_14: obtaining FGS readings on: 1) the EGO, 2) the HIPPARCOS star, line_15: and 3-5) 3 background stars (when available) in the pickle. line_16: The following sequence is observed: 1,3-5,2,1,2,5-3,1. line_17: When a star is brighter than V=9.5, the neutral density filter line_18: is inserted. When possible, another HIPPARCOS star line_19: is included as one of the "background" stars. The objects in the fields in line_20: the three FGS field of views for 1435+638 and HIPPARCOS star 221-98 are ! question: 3 section: 2 line_1: shown in the last figure. The Extragalactic Object is marked with a line_2: triangle, the HIPPARCOS star with a cross, and the "reference stars" are line_3: indicted by circles in FGS3. The other two "Pickles" show potential guide line_4: stars. The numbers are Guide Star Catalogue magnitudes. FGS3 is the line_5: astrometer FGS. ! question: 3 section: 4 line_1: Cycle 2: Primary Hours: 20 Exposures: 40 line_2: Cycle 3: Primary Hours: 10 Exposures: 20 line_3: Cycle 4: Primary Hours: 40 Exposures: 80 line_4: Cycle 5: Primary Hours: 40 Exposures: 80 line_5: These times and exposures are estimates because the first cycle 2 line_6: observations of this program have just been taken at this writing (7 line_7: May 1993). ! 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 0.002-3 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. line_13: The second method is the one proposed here. The FGS measurements line_14: have an accuracy commensurate with both HIPPARCOS and line_15: radio measurements, again 0.002 arcsec. Other proposed line_16: methods rely on photographic astrometry of thousands of stars, line_17: galaxies, and QSOs, with measuring accuracies in the 0.1 to line_18: 0.01 arcsec range. These methods suffer from large systematic line_19: effects. No information about the optical structure of the line_20: EGOs or the stars can be obtained at the 0.04 to 0.002 arcsec ! question: 4 section: 2 line_1: level. Such information is obtained as a matter of course line_2: during HST observations. line_3: The proposed HST observations are the ONLY OPTICAL MEANS which line_4: can approach the expected accuracy of the individual HIPPARCOS line_5: star measurements, and these observations are REQUIRED, to line_6: achieve a reduction to a non-rotating coordinate frame at the line_7: level of the internal systematic accuracy of HIPPARCOS. ! question: 4 section: 3 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". 12 minutes are line_7: required for guide star acquisition. Each observation set line_8: is performed on a single orbit. Thus we have line_9: allotted 30 minutes for a single "average" observation with the line_10: FGSs. line_11: At an average of 2 single epoch observations/hour of HST time, line_12: with 40 hours allotted of GTO time and 40 hours GO time/year line_13: for 3 years, one arrives at 320 single-epoch observations to line_14: cover the 90 pairs. We expect to obtain observations at 3 line_15: epochs at 1 year intervals. Operational experience in the first line_16: year should substantially increase the efficiency of the line_17: observational procedures, so we should increase the number of line_18: observations we can obtain during the program, for the same line_19: number of requested hours. The program proposed here is the line_20: minimum acceptable program to reach an acceptable accuracy ! question: 4 section: 4 line_1: in the Extragalactic Link. The ideal goal is to obtain 10 line_2: year positions and proper motions for all pairs, yielding line_3: a system solution in the submilliarcsecond range. The 40 line_4: hours for the first GO year will provide single epochs for each pair. line_5: See the discussion of estimated Spacecraft time under section 8: line_6: Additional Comments, below. ! question: 5 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 conform to the position angle of the EGO-HIPPARCOS star pair line_6: for the nominal roll on that date. In order to remove the line_7: effect of the HIPPARCOS star parallax in the determination of line_8: the proper motion, the observations of a given HIPPARCOS star line_9: EGO pair must be made at intervals of one year exactly, within line_10: a few days. line_11: Each observation consists of separate settings of the FGSs. line_12: The thermal/mechanical/optical stability line_13: of the OTA/FGS holds only over about 10 minutes. line_14: We have included check star measurements in the observation line_15: plan. However, each entire observation sequence must be line_16: performed contiguously to allow accurate determination of the line_17: target relative positions. ! ! ! question: 8 section: 1 line_1: AT THE TIME OF THIS SUBMISSION, THE RESOURCE ESTIMATOR IS line_2: OVERESTIMATING THE GUIDE STAR LOCK-UP TIME. ONLY ONE GUIDE line_3: STAR LOCK-UP IS REQUIRED FOR EACH OBSERVATION SET, BUT WE line_4: ARE BEING CHARGED ONE LOCK-UP FOR EACH REFERENCE STAR AND line_5: HIPPARCOS STAR SETTING. THEREFORE, THE TOTAL SPACECRAFT line_6: TIME CHARGED IS TOO LARGE BY A FACTOR OF ABOUT 4. line_7: THE ACTUAL SPACECRAFT EFFICIENCY AND REQUIRED TIME WILL BE line_8: CLOSER TO 30% AND 40 HOURS. line_9: (7 MAY 1993--PDH). line_11: At the time of this writing, the field distortions in FGS3 have been line_12: mapped to the 1 milliarcsecond level using 20 orbits of overlapping line_13: plate data on M35. The Astrometry Science Team and the STScI are line_14: performing observations to monitor the field distortions and provide line_15: for their correction over time. The first observations have been line_16: made for this program with the expected stability necessary to line_17: achieve the desired accuracies stated above. The HIPPARCOS line_18: catalogue reductions are expected to be completed in 1995. In order line_19: for these observations of motions to be of direct value to the line_20: HIPPARCOS Project, both second epoch observations of targets ! question: 8 section: 2 line_1: observed in Cycles 2 and 3 and first epoch observations of those line_2: missed in Cycles 2 and 3 MUST BE PERFORMED in CYCLE 4. line_4: This proposal is intended to extend observations of the GTO line_5: sources over a longer time base to improve the accuracy of line_6: the proper motions and obtain more temporal structure data. line_7: The proposal also extends the GTO list by a factor of 3. ! question: 9 section: 1 line_1: This program has been granted observing time many times in the past line_2: under proposal number 2565. Because of prolonged analysis before the line_3: HST Project would let Astrometric Science Observations commence, the line_4: first three observations for this program have been taken only in the last line_5: month (as of 5/7/93) and due to a bottleneck in the Post Observation Data line_6: Processing System, none of the data have been delivered to the PI as yet. line_7: But we are ever hopeful. The rms scatter in the individual data points line_8: are available, and show 3-6 milliarcseconds jitter in the individual line_9: pointings. The averaged individual positions should be good to a line_10: milliarcsecond internally. ! question: 9 section: 2 line_1: This proposal is a continuation and extension of 2565. The status is that line_2: FGS3 is calibrated to 0.002 arcseconds in field distortion over most of its line_3: field of view. Observations are under way to calibrate the plate scale to line_4: that level of accuracy over 15 arcminutes. FGS observations are being line_5: made of these pairs which will allow the system rotation to be determined. line_6: We only need to obtain the observations. The main result so far is that we line_7: need the system to let us make the observations in a timely fashion. ! question: 9 section: 3 line_1: "The Current Status of HST Astrometry for Linking the HIPPARCOS line_2: Frame to the Extragalactic Frame." Hemenway, P. D., and Duncombe, line_3: R. L., Presented at the "Sub-Arcsecond Radio Astronomy line_4: Conference", University of Manchester, 20-24 July 1992. line_7: RAstrometric performance characteristics of the Hubble Space line_8: Telescope fine guidance sensors,SG.F. Benedict, Jefferys, W.H., E. line_9: Nelan, D. Story, B. McArthur, A.L. Whipple, R.L. Duncombe, P.D. line_10: Hemenway, P.J. Shelus, W. van Altena, T. Girard, O.G. Franz and L.W. line_11: Fredrick, Publications of the Astronomical Society of the Pacific 104, line_12: 958-975 (1992). line_14: REarly commissioning astrometry performance of the line_15: fine guidance sensors,S, G.F. Benedict, Jefferys, W.H., Q. Wang, A. Whipple, line_16: E. Nelan, D. Story, R.L. Duncombe, P. Hemenway, P.J. Shelus, B. McArthur, line_17: J. McCartney, O.G. Franz, L. Wasserman, T. Kreidl, W.F. van Altena, line_18: T. Girard, and L.W. Fredrick, in The First Year of HST Observations, line_19: A.L. Kinney and J.C. Blades, Editors. Baltimore: Space Telescope Science line_20: Institute. (1991) ! question: 9 section: 4 line_1: line_2: "Current Status of the Astrometric Capabilities of the Hubble Space Telescope line_3: Fine Guidance Sensors", Jefferys, W.H., Benedict, G.F., Duncombe, R.L., Franz, line_4: O.G., Fredrick, L.W., Gerard, T, Hemenway, P.D., McArthur, B., McCartney, J., line_5: Nelan, E., Shelus, P.J., Story, D., van Altena, W, Wasserman, L., Whipple A., line_6: Whitney, J., in "REFERENCE FRAMES", line_7: Proc 127th Col. IAU, eds: J.A. Hughes, C.A. Smith, and Kaplan, G line_8: H., USNO, Washington, DC., pp68-76, 1991 line_10: And papers on the current calibration submitted to the Astronomical line_11: Journal. ! question: 10 section: 1 line_1: The Astrometry Science Team of the HST is based in Austin. The PI and line_2: one of the Co-Is are members of the Astrometry Team and have access to line_3: the Astrometry Team reduction software, including the Team pipeline line_4: calibration software. For this project we also have access to the line_5: Astrometry Team complex of Macintosh and Sun , which will be used for line_6: the initial processing of the data. Separately, housed at the Aerospace line_7: Engineering Department's Center for Space Research, we have a VAXStation line_8: 3200, specifically allocated for the analysis of data for this project. We line_9: have a software system designed and programmed by Mr. Frank Shattuck line_10: which analyzes VLBI, HST, and HIPPARCOS data to yield the system line_11: rotation. (Frank Shattuch, Master's Thesis, UT-Austin, 1992). We have line_12: the resources of the Astrometry Team, the Astronomy Department, the line_13: Center for Space Research, and McDonald Observatory of the University of line_14: Texas at our disposal. Currently we have 3 undergraduate students, one line_15: graduate student, and we are negotiating for a post-doctoral fellow to work line_16: on this project in Austin. ! !end of general form text general_form_address: lname: Hemenway fname: Paul category: PI inst: 3550 addr_1: Astronomy Department addr_2: University of Texas city: Austin state: TX zip: 78712 country: USA phone: (512) 471 3431 telex: paul@astro.as.utexas.edu ! ! end of general_form_address records fixed_targets: targnum: 221 name_1: NEWEGOC-45NEWHIP-45 descr_1: E,316 pos_1: RA = 166.11375D +/- .0008D, pos_2: DEC = 38.2086111D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.5 +/- 1 ! targnum: 222 name_1: NEWHIP-45-REF descr_1: J,701 pos_1: RA = 166.130375D +/- .0008D, pos_2: DEC = 38.2413611D +/- .0008D, equinox: 2000 pm_or_par: Y pos_epoch_bj: J pos_epoch_yr: 2000.00 ra_pm_val: -0.005432 dec_pm_val: -0.0030 fluxnum_1: 1 fluxval_1: V=6.04 +/- 1 ! targnum: 223 name_1: 220-REF descr_1: J,701 pos_1: RA = 166.21337D +/- .0008D, pos_2: DEC = 38.28591D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.54 +/- 1 ! targnum: 224 name_1: 221-REF descr_1: J,701 pos_1: RA = 166.15892D +/- .0008D, pos_2: DEC = 38.26493D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15.26 +/- 1 ! targnum: 225 name_1: 222-REF descr_1: J,701 pos_1: RA = 166.18343D +/- .0008D, pos_2: DEC = 38.24675D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=7.1 +/- 1 ! targnum: 421 name_1: NEWEGOC-47NEWHIP-47 descr_1: E,316 pos_1: RA = 166.11375D +/- .0008D, pos_2: DEC = 38.2086111D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.5 +/- 1 ! targnum: 422 name_1: NEWHIP-47-REF descr_1: J,701 pos_1: RA = 166.384083D +/- .0008D, pos_2: DEC = 38.2758333D +/- .0008D, equinox: 2000 pm_or_par: Y pos_epoch_bj: J pos_epoch_yr: 2000.00 ra_pm_val: -0.027005 dec_pm_val: 0.0520 fluxnum_1: 1 fluxval_1: V=8.79 +/- 1 ! targnum: 423 name_1: 420-REF descr_1: J,701 pos_1: RA = 166.38806D +/- .0008D, pos_2: DEC = 38.29825D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.89 +/- 1 ! targnum: 424 name_1: 421-REF descr_1: J,701 pos_1: RA = 166.21337D +/- .0008D, pos_2: DEC = 38.28591D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.54 +/- 1 ! targnum: 425 name_1: 422-REF descr_1: J,701 pos_1: RA = 166.18343D +/- .0008D, pos_2: DEC = 38.24675D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=7.1 +/- 1 ! targnum: 521 name_1: NEWEGOC-48NEWHIP-48 descr_1: E,316 pos_1: RA = 166.11375D +/- .0008D, pos_2: DEC = 38.2086111D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.5 +/- 1 ! targnum: 522 name_1: NEWHIP-48-REF descr_1: J,701 pos_1: RA = 166.183083D +/- .0008D, pos_2: DEC = 38.2466389D +/- .0008D, equinox: 2000 pm_or_par: Y pos_epoch_bj: J pos_epoch_yr: 2000.00 ra_pm_val: -0.007351 dec_pm_val: -0.0120 fluxnum_1: 1 fluxval_1: V=7.55 +/- 1 ! targnum: 523 name_1: 520-REF descr_1: J,701 pos_1: RA = 166.17921D +/- .0008D, pos_2: DEC = 38.22103D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15.31 +/- 1 ! targnum: 524 name_1: 521-REF descr_1: J,701 pos_1: RA = 166.21337D +/- .0008D, pos_2: DEC = 38.28591D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.54 +/- 1 ! targnum: 525 name_1: 522-REF descr_1: J,701 pos_1: RA = 166.15892D +/- .0008D, pos_2: DEC = 38.26493D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15.26 +/- 1 ! targnum: 621 name_1: NEWEGOC-50NEWHIP-50 descr_1: E,316 pos_1: RA = 229.4242236D +/- .0008D, pos_2: DEC = -24.37207592D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15 +/- 1 ! targnum: 622 name_1: NEWHIP-50-REF descr_1: J,701 pos_1: RA = 229.438125D +/- .0008D, pos_2: DEC = -24.428639D +/- .0008D, equinox: 2000 pm_or_par: Y pos_epoch_bj: J pos_epoch_yr: 2000.00 ra_pm_val: -0.003588 dec_pm_val: -0.0580 fluxnum_1: 1 fluxval_1: V=9.08 +/- 1 ! targnum: 623 name_1: 620-REF descr_1: J,701 pos_1: RA = 229.49139D +/- .0008D, pos_2: DEC = -24.45816D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.92 +/- 1 ! targnum: 624 name_1: 621-REF descr_1: J,701 pos_1: RA = 229.45978D +/- .0008D, pos_2: DEC = -24.38389D +/- .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 = 229.46983D +/- .0008D, pos_2: DEC = -24.42986D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.53 +/- 1 ! targnum: 721 name_1: NEWEGOC-52NEWHIP-52 descr_1: E,316 pos_1: RA = 253.4675693D +/- .0008D, pos_2: DEC = 39.76016882D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.8 +/- 1 ! targnum: 722 name_1: NEWHIP-52-REF descr_1: J,701 pos_1: RA = 253.247458D +/- .0008D, pos_2: DEC = 39.6055278D +/- .0008D, equinox: 2000 pm_or_par: Y pos_epoch_bj: J pos_epoch_yr: 2000.00 ra_pm_val: -0.007441 dec_pm_val: -0.0220 fluxnum_1: 1 fluxval_1: V=9.89 +/- 1 ! targnum: 723 name_1: 720-REF descr_1: J,701 pos_1: RA = 253.32033D +/- .0008D, pos_2: DEC = 39.70772D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.53 +/- 1 ! targnum: 724 name_1: 721-REF descr_1: J,701 pos_1: RA = 253.44106D +/- .0008D, pos_2: DEC = 39.7359D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.43 +/- 1 ! targnum: 725 name_1: 722-REF descr_1: J,701 pos_1: RA = 253.28449D +/- .0008D, pos_2: DEC = 39.63098D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.08 +/- 1 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 22.001 targname: NEWEGOC-45NEWHIP-45 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 4 / 22.001-22.011; req_7: ORIENT 233.49D +/- .3D; req_8: POS TARG +127.1,-67.074; comment_1: NEAR JD2449754.98 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: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 22.005 targname: NEWHIP-45-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 22.006 targname: NEWEGOC-45NEWHIP-45 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 22.007 targname: NEWHIP-45-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: 22.008 targname: 222-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 22.009 targname: 221-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! 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: NEWEGOC-45NEWHIP-45 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 42.001 targname: NEWEGOC-47NEWHIP-47 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 4 / 42.001-42.011; req_5: ORIENT 253.73D +/- .3D; req_6: POS TARG +425.641,-132.683; comment_1: NEAR JD2449741.24 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: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 42.005 targname: NEWHIP-47-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 42.006 targname: NEWEGOC-47NEWHIP-47 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 42.007 targname: NEWHIP-47-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: F5ND 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: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 42.011 targname: NEWEGOC-47NEWHIP-47 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 52.001 targname: NEWEGOC-48NEWHIP-48 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 4 / 52.001-52.011; req_5: ORIENT 223.16D +/- .3D; req_6: POS TARG +3.406,-10.551; comment_1: NEAR JD2449760.63 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-48-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 52.006 targname: NEWEGOC-48NEWHIP-48 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 52.007 targname: NEWHIP-48-REF config: ^ opmode: ^ aperture: ^ sp_element: F5ND num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 52.008 targname: 522-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: 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: NEWEGOC-48NEWHIP-48 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: NEWEGOC-50NEWHIP-50 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 4 / 62.001-62.011; req_5: ORIENT 349.33D +/- .3D; req_6: POS TARG +223.825,-88.169; comment_1: NEAR JD2449483.69 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-50-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 62.006 targname: NEWEGOC-50NEWHIP-50 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 62.007 targname: NEWHIP-50-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: 62.008 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: NEWEGOC-50NEWHIP-50 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 72.001 targname: NEWEGOC-52NEWHIP-52 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 4 / 72.001-72.011; req_5: ORIENT 226.6D +/- .3D; req_6: POS TARG -427.591,-128.818; comment_1: NEAR JD2449465.89 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: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 72.005 targname: NEWHIP-52-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 72.006 targname: NEWEGOC-52NEWHIP-52 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: 72.007 targname: NEWHIP-52-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: NEWEGOC-52NEWHIP-52 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! ! end of exposure logsheet ! No scan data records found