! File: 5058C.PROP ! Database: PEPDB ! Date: 23-FEB-1994:18:12:59 coverpage: title_1: EXTRAGALACTIC ASTROMETRY AND ASTROPHYSICS title_2: FT12-23,PART 2 OF 2 - CONTINUATION OF 1013, CYCLE 2-FIXED sci_cat: QUASARS & AGN sci_subcat: ASTROMETRY proposal_for: GTO/AST longterm: 9 cont_id: 1013 pi_title: DR. pi_fname: WILLIAM pi_mi: H. pi_lname: JEFFERYS pi_inst: UNIVERSITY OF TEXAS AT AUSTIN pi_country: USA pi_phone: (512)471-1455 keywords_1: QUASARS, BL LACS, AGNS, HIPPARCOS, REFERENCE FRAMES keywords_2: FUNDAMENTAL ASTROMETRY, QUASAR INTERNAL MOTION hours_pri: 15.00 hours_par: 15.00 num_pri: 72 fgs: Y pi_position: PROFESSOR ! end of coverpage abstract: line_1: The goal of this project is the determination of the rotation of line_2: the HIPPARCOS Reference Frame with respect to an Extragalactic line_3: Frame. The program will derive the internal optical motions of line_4: extragalactic objects (QSOs, BL Lacs, AGNs) at the +/- 0.002 line_5: arcsecond per year level of accuracy. line_7: 160 SAO stars within the FGSFOV of all selected QSOs, BL Lacs, line_8: and AGNs are included in the HIPPARCOS catalog. Ground based line_9: speckle observations have been used to pre-detect doubles which line_10: would cause problems for the FGS. The FGSs will measure the line_11: relative positions of SAO stars with respect to objects brighter line_12: than 17 mag. Fainter objects will be observed with the WFPC and line_13: FGS together. The objects have been selected in conjunction with line_14: the recommendations of the IAU working group in Radio/Optical line_15: Identifications, and have been selected for compactness and line_16: intensity. Most of the objects are recommended as ultimate line_17: position calibrators. ! ! end of abstract general_form_proposers: lname: JEFFERYS fname: WILLIAM title: DR. mi: H. inst: UNIVERSITY OF TEXAS AT AUSTIN country: USA ! ! end of general_form_proposers block general_form_text: question: 2 section: 1 line_1: The HIPPARCOS satellite will produce positions, proper motions, line_2: and parallaxes for 100,000 stars with an accuracy of 0.002 line_3: arcseconds in the positions and parallaxes. However, the nature line_4: of the observations means that the HIPPARCOS Instrumental line_5: Coordinate system will have an unknown overall rotation with line_6: respect to an inertial reference frame. The extragalactic line_7: objects define a frame which is very close to being inertial, line_8: differing only by cosmological effects. The goal of these line_9: observations is twofold: first to determine the relative line_10: positions and motions of selected Extragalactic Objects (EGOs) line_11: with respect to the HIPPARCOS reference frrame, and, by line_12: inverting the observations, infer the rotation of the HIPPARCOS line_13: frame, as part of the Astrometry Team GTO time, and second, by line_14: using the Planetary Camera and guiding FGSs in the "Transit line_15: Circle" mode, obtain structural information about the EGOs as line_16: part of the WF/PC GTO time. ! question: 2 section: 2 line_1: Several methods have been proposed to "stop" the HIPPARCOS frame line_2: rotation. The Space Telescope observations have the possibility line_3: to provide the most accurate of these determinations, possibly line_4: to the level of 0.0002 arcsec/year accuracy. Such a line_5: determination would make a significant impact on our knowledge line_6: of the motions of groups of stars (which now must have line_7: precession removed) and would provide a more stable reference line_8: frame against which to measure the motions of solar system line_9: objects, for orbital and relativity studies. line_11: Because the observations will be made over the lifetime of ST, line_12: internal apparent motions within the EGO cores will be observed line_13: or not observed at a level which can only be obtained at radio line_14: wavelengths using VLBI at the present time. The study of time line_15: variable optical positions will bring a new aspect to bear on line_16: the study of these objects. line_18: Speckle observations of candidate HIPPARCOS stars were used to line_19: determine which ones are multiple and hence unsuitable for line_20: these studies. Franz and McAlister used the KPNO 4-meter and line_21: the Perkins telescope in the northern hemisphere, and Argue line_22: and Morgan used the AAT in the southern hemisphere to obtain line_23: observations. ! question: 3 section: 1 line_1: Observations will be made with the "Transit Circle" mode line_2: using PC-8 and the astrometric data from the guiding FGSs line_3: simultaneously. The spacecraft must be oriented so that line_4: the EGO and HIP stars are aligned for appropriate use of line_5: the guide stars. ! question: 4 section: 1 line_1: Because of astrometric limitations of the atmosphere, ground- line_2: based observations are capable of only about 0.01 arcsecond line_3: accuracy in measuring the relative positions between two line_4: objects separated by more than an isoplanatic patch. These line_5: observations require the longest focus telescopes and detailed line_6: analysis of the optical distortions. This accuracy has only line_7: been achieved in a handful of fields. ST will provide single line_8: observations at the 0.002 arcsecond level, and should allow line_9: an order of magnitude increase over the ground-based line_10: observations. The standard method of ground-based observation line_11: is still the transit circle, so relative optical positions of line_12: the HIPPARCOS stars with respect to EGOs will not be measured line_13: from the ground. Radio positions using VLBI and VLA line_14: observations of RS CVn stars will be made to relate the line_15: HIPPARCOS frame to EGOs indirectly. However, ST has the line_16: capability to measure this rotation directly, without the line_17: problem of relating the optical and radio emission regions. line_18: The possible transfer of the radio reference frame to the line_19: optical will of necessity require such assumptions about line_20: the EGOs, but the use of at least 50 objects will allow line_21: statistical statements to be made which will be of great line_22: astrophysical interest. ! question: 5 section: 1 line_1: In order to minimize the impact of power constraints, the dates line_2: of observations were picked so that the nominal FGS orientation line_3: is aligned with the EGO-HIP star position angle, and off-nominal line_4: rolls are not required. However, this constraint makes the line_5: observations time-critical. Because the goal is to measure line_6: motions, the repeat observations must be made within multiples line_7: of one year within two days, in order not to contaminate the line_8: motions with the parallaxes of other HIPPARCOS stars. line_9: DELETED LINES 84.001-84.011 FROM 1571 TO CREATE THIS PROPOSAL. ! question: 6 section: 1 line_1: The astrometric data will be reduced at STScI or the University line_2: of Texas using the SDAS/ADRS Software. The reduction of WF/PC line_3: data will use the SDAF/WF-PC Software. Analysis will be line_4: performed as appropriate. In particular, the reduced poitional line_5: data will be transmitted to the HIPPARCOS project, and the line_6: analysis will be performed in conjunction with that project. line_8: The PC observations using the F606W and F658N filters require line_9: the calibrations derived from the first 3 exposure log sheet line_10: lines of GTO proposal 1013. ! question: 8 section: 1 line_1: 160 HIPPARCOS stars have been identified within 10 arcminutes of line_2: 90 EGOs. During the GTO time, we expect to make three line_3: observations of 40 HIP star-EGO pairs, two observations of 40 line_4: more, and one observation of 40 more, for a total of 120 object line_5: pairs. We have included all the candidate objects, but expect line_6: scheduling constraints to limit which objects will be observed. line_8: The success of the program depends on obtaining essentially all line_9: of the priority one observations. Priority 2 solutions will line_10: strengthen the solution. Priority 3 observations are non- line_11: critical and should be treated as "fillers." ! question: 13 section: 1 line_1: Relative positions and motions of HIPPARCOS stars will be made line_2: with respect to Extragalactic Objects (EGOs), using the Fine line_3: Guidance Sensors and the Planetary Camera in the "transit line_4: circle" mode. The data will provide information line_5: on structure changes in the cores of these objects. The line_6: position measurements will be used to derive the overall line_7: rotation of the HIPPARCOS reference frame with respect to line_8: the extragalactic reference frame. ! !end of general form text general_form_address: lname: HEMENWAY fname: PAUL mi: D title: DR. category: CON 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 ! lname: JEFFERYS fname: WILLIAM mi: H. 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)471-1455 ! ! end of general_form_address records fixed_targets: targnum: 621 name_1: 1418+546INCA221-97 descr_1: E pos_1: RA = 214.9441563D +/- .0008D, pos_2: DEC = 54.38744094D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15.6 +/- 1 ! targnum: 622 name_1: INCA221-97-REF descr_1: A pos_1: RA = 215.0765792D +/- .0008D, pos_2: DEC = 54.50546111D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: 0.000900 dec_pm_val: -0.0810 fluxnum_1: 1 fluxval_1: V=9.27 +/- 1 ! targnum: 623 name_1: 620-REF descr_1: J,701 pos_1: RA = 214.9323585D +/- .0008D, pos_2: DEC = 54.3136763D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.92 +/- 1 ! targnum: 624 name_1: 621-REF descr_1: J,701 pos_1: RA = 214.9736685D +/- .0008D, pos_2: DEC = 54.3221962D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=10.5 +/- 1 ! targnum: 625 name_1: 622-REF descr_1: J,701 pos_1: RA = 215.1003186D +/- .0008D, pos_2: DEC = 54.4856762D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=12.61 +/- 1 ! targnum: 845 name_1: 2251+158INCA221-153 descr_1: E pos_1: RA = 343.4906179D +/- .0008D, pos_2: DEC = 16.14821196D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=16.1 +/- 1 ! targnum: 846 name_1: INCA221-153-REF descr_1: A pos_1: RA = 343.4455542D +/- .0008D, pos_2: DEC = 16.29190833D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=10.3 +/- 1 ! targnum: 848 name_1: 1921-REF descr_1: J,701 pos_1: RA = 343.4511631D +/- .0008D, pos_2: DEC = 16.2368027D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.37 +/- 1 ! targnum: 849 name_1: 1922-REF descr_1: J,701 pos_1: RA = 343.4923131D +/- .0008D, pos_2: DEC = 16.1518127D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.11 +/- 1 ! targnum: 851 name_1: 2251+158INCA221-154 descr_1: E pos_1: RA = 343.4906179D +/- .0008D, pos_2: DEC = 16.14821196D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=16.1 +/- 1 ! targnum: 852 name_1: INCA221-154-REF descr_1: A pos_1: RA = 343.5985375D +/- .0008D, pos_2: DEC = 15.99728611D +/- .0008D, equinox: 2000 pm_or_par: Y ra_pm_val: 0.001100 dec_pm_val: -0.0170 fluxnum_1: 1 fluxval_1: V=9.4 +/- 1 ! targnum: 854 name_1: 1941-REF descr_1: J,701 pos_1: RA = 343.6211231D +/- .0008D, pos_2: DEC = 15.9801427D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.14 +/- 1 ! targnum: 855 name_1: 1942-REF descr_1: J,701 pos_1: RA = 343.4923131D +/- .0008D, pos_2: DEC = 16.1518127D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.11 +/- 1 ! targnum: 875 name_1: 2300-683INCA221-159 descr_1: E pos_1: RA = 345.9335658D +/- .0008D, pos_2: DEC = -68.1268918D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=16.4 +/- 1 ! targnum: 876 name_1: INCA221-159-REF descr_1: A pos_1: RA = 346.0170488D +/- .0008D, pos_2: DEC = -68.3476246D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=8.7 +/- 1 ! targnum: 877 name_1: 2220-REF descr_1: J,701 pos_1: RA = 346.0694878D +/- .0008D, pos_2: DEC = -68.2589174D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15.17 +/- 1 ! targnum: 878 name_1: 2221-REF descr_1: J,701 pos_1: RA = 346.0170488D +/- .0008D, pos_2: DEC = -68.3476246D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=8.7 +/- 1 ! targnum: 879 name_1: 2222-REF descr_1: J,701 pos_1: RA = 346.0346878D +/- .0008D, pos_2: DEC = -68.3651574D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=15.29 +/- 1 ! targnum: 881 name_1: 2300-683INCA221-160 descr_1: E pos_1: RA = 345.9335658D +/- .0008D, pos_2: DEC = -68.1268918D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=16.4 +/- 1 ! targnum: 882 name_1: INCA221-160-REF descr_1: A pos_1: RA = 345.6452577D +/- .0008D, pos_2: DEC = -67.9431699D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=9.4 +/- 1 ! targnum: 883 name_1: 2240-REF descr_1: J,701 pos_1: RA = 346.273688D +/- .0008D, pos_2: DEC = -67.8917274D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.16 +/- 1 ! targnum: 884 name_1: 2241-REF descr_1: J,701 pos_1: RA = 346.1828179D +/- .0008D, pos_2: DEC = -67.9185474D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.22 +/- 1 ! targnum: 885 name_1: 2242-REF descr_1: J,701 pos_1: RA = 346.0462879D +/- .0008D, pos_2: DEC = -68.1005774D +/- .0008D, equinox: 2000 fluxnum_1: 1 fluxval_1: V=13.8 +/- 1 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 62.001 targname: 1418+546INCA221-97 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 198.56D +/- .3D; req_6: POS TARG +112.909,+35.643; comment_1: NEAR comment_2: JD2449087.3435764 V1 AXIS AND comment_3: ORIENTATION SPECIFIED TO PUT comment_4: REFERENCE STARS IN PICKLE. JDTOBS IS comment_5: THE JULIAN DATE THAT THIS ORIENTATION comment_6: 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: INCA221-97-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: 1418+546INCA221-97 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 62.007 targname: INCA221-97-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: 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: 62.011 targname: 1418+546INCA221-97 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 192.001 targname: 2251+158INCA221-153 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: ^ param_1: DATA-RATE = 32 req_2: SEQ 192.001-192.011 NO GAP; req_3: SAME POS FOR 192.003-192.011 AS 192.001; req_4: CYCLE 2 / 192.001-192.011; req_5: ORIENT 151.08D +/- .3D; req_6: POS TARG +138.912,-21.191; comment_1: NEAR JD2448881.3275642 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: 192.003 targname: 1921-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 192.004 targname: 1922-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 192.005 targname: INCA221-153-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: 192.006 targname: 2251+158INCA221-153 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 192.007 targname: INCA221-153-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 192.008 targname: 1922-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: 192.009 targname: 1921-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: 192.011 targname: 2251+158INCA221-153 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: 194.001 targname: 2251+158INCA221-154 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: ^ param_1: DATA-RATE = 32 req_2: SEQ 194.001-194.011 NO GAP; req_3: SAME POS FOR 194.003-194.011 AS 194.001; req_4: CYCLE 2 / 194.001-194.011; req_5: ORIENT 148.1D +/- .3D; req_6: POS TARG -337.275,-70.07; comment_1: NEAR JD2448882.4422188 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: 194.003 targname: 1941-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: 194.004 targname: 1942-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 194.005 targname: INCA221-154-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 194.006 targname: 2251+158INCA221-154 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 194.007 targname: INCA221-154-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: 194.008 targname: 1942-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: 194.009 targname: 1941-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 194.011 targname: 2251+158INCA221-154 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 222.001 targname: 2300-683INCA221-159 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 222.001-222.011 NO GAP; req_3: SAME POS FOR 222.002-222.011 AS 222.001; req_4: CYCLE 2 / 222.001-222.011; req_5: ORIENT 351.37D +/- .3D; req_6: POS TARG +371.924,-92.878; comment_1: NEAR JD2448863.7645833 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: 222.002 targname: 2220-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 222.003 targname: 2221-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 222.004 targname: 2222-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 222.005 targname: INCA221-159-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: 222.006 targname: 2300-683INCA221-159 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: 222.007 targname: INCA221-159-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: 222.008 targname: 2222-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 222.009 targname: 2221-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 222.010 targname: 2220-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 222.011 targname: 2300-683INCA221-159 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: 224.001 targname: 2300-683INCA221-160 config: FGS opmode: POS aperture: 3 sp_element: F583W num_exp: 1 time_per_exp: 51.2S fluxnum_1: 1 priority: ^ param_1: DATA-RATE = 32 req_2: SEQ 224.001-224.011 NO GAP; req_3: SAME POS FOR 224.002-224.011 AS 224.001; req_4: CYCLE 2 / 224.001-224.011; req_5: ORIENT 26.76D +/- .3D; req_6: POS TARG -440.771,-89.841; comment_1: NEAR JD2448902.0179282 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: 224.002 targname: 2240-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 224.003 targname: 2241-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: 224.004 targname: 2242-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 224.005 targname: INCA221-160-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: 224.006 targname: 2300-683INCA221-160 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: 224.007 targname: INCA221-160-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 224.008 targname: 2242-REF config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 224.009 targname: 2241-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: 224.010 targname: 2240-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: 224.011 targname: 2300-683INCA221-160 config: ^ opmode: ^ aperture: ^ sp_element: F583W num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! ! end of exposure logsheet ! 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