! File: 2935C.PROP ! Database: PEPDB ! Date: 17-FEB-1994:22:55:29 coverpage: title_1: UNSEEN AND PLANETARY COMPANIONS PART ONE sci_cat: STELLAR ASTROPHYSICS proposal_for: GTO/AST longterm: 3 cont_id: 1005 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: UNSEEN COMPANIONS, PLANETRAY COMPANIONS, BLACK DWARFS hours_pri: 48.00 num_pri: 156 fgs: Y pi_position: PROFESSOR ! end of coverpage abstract: line_1: With observations using the Hubble Space Telescope (HST) we line_2: intend to initiate a systematic search for variable proper line_3: motion objects in an attempt to discover very low mass objects in line_4: orbit around red dwarfs. Using well established astrometric line_5: methods we will secure accurate relative positional measurements line_6: for selected objects over very long intervals of time looking line_7: for systematic perturbations to rectilinear motion. Within the line_8: Astrometric Data Reduction System (SDAS), such perturbations will line_9: be extracted and reduced further to provide the relevant mass and line_10: orbital parameters of the composents. The HST is an instrument, line_11: the engineering specifications of which, open up the opportunity line_12: to extend this astrometric discipline far beyond the present line_13: bounds of ground-based and other observations. ! ! end of abstract general_form_proposers: lname: JEFFERYS fname: WILLIAM title: DR. mi: H. inst: UNIVERSITY OF TEXAS country: USA ! lname: BENEDICT fname: GEORGE title: DR. mi: F. inst: UNIVERSITY OF TEXAS country: USA ! lname: DUNCOMBE fname: RAYNOR title: DR. mi: L. inst: UNIVERSITY OF TEXAS country: USA ! lname: HEMENWAY fname: PAUL title: DR. mi: D. inst: UNIVERSITY OF TEXAS country: USA ! lname: SHELUS fname: PETER title: DR. mi: S. inst: UNIVERSITY OF TEXAS country: USA ! lname: FRANZ fname: OTTO title: DR. mi: G. inst: LOWELL OBSERVATORY country: USA ! lname: FREDRICK fname: LAURENCE title: DR. mi: W. inst: UNIVERSITY OF VIRGINIA country: USA ! lname: VAN ALTENA fname: WILLIAM title: DR. mi: F. inst: YALE UNIVERSITY country: USA ! ! end of general_form_proposers block general_form_text: question: 2 section: 1 line_1: Similar to Bessell's study of Sirius and Procyon, which led to the line_2: discovery of previously unseen stellar companions, observatories line_3: having access to long focus astrometric instruments have line_4: established very-long-term systematic searches for variable proper line_5: motion objects as a normal part of their standard parallax programs. line_6: These efforts have been rewarded by the discovery of objects of line_7: extreme astrophysical interest. The objects which have aroused line_8: the greatest excitement are those of very low mass in orbit around line_9: late spectral type stars. On an ordinary mass-luminosity diagram line_10: many of these objects lie below the lower mass limit presently line_11: hypothesized for actual stellar objects. If such objects are line_12: found in orbit about other stars and yet have masses so small line_13: that they cannot physically be stars, can they be planetary type line_14: objects? With the HST, an instrument having the engineering line_15: specifications that it does, there opens up a magnificent line_16: opportunity to continue a vital astrometric discipline in ways line_17: not previously possible. With the use of the Fine Guidance line_18: Sensors (FGS) we are planning a series of observations to line_19: establish a two-pronged effort for seeking deviations of motion line_20: from that which is rectilinear. ! question: 2 section: 2 line_1: The first of these concerns a line_2: carefully chosen subset of objects which are at or near the line_3: limits of ground-based techniques; with these we would wish to line_4: firmly confirm or reject the actual existence of perturbations and line_5: allow for a smooth transition between ground- and space-based line_6: observations of this type. The second would be an effort to line_7: search for objects which are now beyond ground-based technologies. ! question: 3 section: 1 line_1: It is required that all of these parallax-type observations be line_2: made within +/- 10 days of the listed dates of maximum parallax line_3: factor. Observations which are made outside of these ranges line_4: degrade the accuracy of such observations to the point where they line_5: become worthless. It is expected that each parallax object will line_6: have 10-15 reference stars associated with it to provide the line_7: coordinate frame for the observation set. These reference stars line_8: were to have been selected from Science Institute Guide Star line_9: Selection System (ST/ScI GSSS) generated inventories. Because of line_10: extreme scheduling problems being encountered by that system, line_11: these reference objects are actually being provided by a system line_12: designed and implemented by the Space Telescope Astrometry Team line_13: (STAT). ! question: 3 section: 2 line_1: The actual observational procedure will be to first measure the line_2: parallax object, any secondary object (if necessary), the full line_3: complement of reference objects, and then the parallax object and line_4: any secondary object (if necessary) again. During each observing line_5: "season" of +/- 10 days from the date of maximum parallax factor, line_6: either 4 or 6 observations of this sequence must be made, as is line_7: indicated on the Exposure Log Sheet. Each of these observational line_8: sequences must be made on separate HST orbits to minimize the line_9: possibility of any correlations occurring between the systematic line_10: errors which are characteristic to an individual orbit from one line_11: observation sequence to another in the same field. ! question: 3 section: 3 line_1: The neutral density filter is to be used for cases where the line_2: brightness of any object exceeds the brightness limit of the FGS. line_3: Five observing seasons will be assumed, such that each season is line_4: separated from the previous one by approximately six months (always line_5: remaining within the allowed limits from the dates of maximum line_6: parallax factors). As mentioned above, each observing season will line_7: result in either 4 or 6 observing sessions distributed as 4, 6, 4, line_8: 6, 4, which yield a total of 12 observing sessions on either side line_9: of the earth's orbit. ! question: 3 section: 4 line_1: It is expected that the first time that an object is observed, it line_2: will be in the "Transfer Function Mode" to check for duplicity line_3: before any positional observations are made. ! question: 4 section: 1 line_1: Ground-based parallaxes in the very best of circumstances are line_2: limited to 0.002 seconds of arc, which are some 4 times poorer than line_3: that projected for HST observations. Of much more importance is line_4: the fact that this four-fold increase from the best of the line_5: ground-based accuracies will enhance the chances fror detecting line_6: orbital perturbations undetectable from the ground. ! question: 5 section: 1 line_1: All observations must be made within +/- 10 days of maximum line_2: parallax factor. ! question: 6 section: 1 line_1: All of the FGS observations must be uninterrupted in order to line_2: minimize the effects of thermal drifts in the HST structure. ! question: 7 section: 1 line_1: Data reduction will be performed using the ADRS within the SDAS line_2: system at STScI with other reductions being performed in Austin. line_3: All data will be put into the ADRS format for analysis using the line_4: GAUSS module. All results, together with best-level estimates of line_5: their errors and their covariances will be made available, as line_6: needed. ! question: 8 section: 1 line_1: FGS numbers refer to BAY NUMBERS. ! question: 9 section: 1 line_1: N/A ! question: 10 section: 1 line_1: ADRS will be available in Austin. ! !end of general form text general_form_address: lname: JEFFERYS category: PI ! lname: JEFFERYS fname: WILLIAM mi: H. title: DR. category: PI inst: UNIVERSITY OF TEXAS addr_1: DEPARTMENT OF ASTRONOMY city: AUSTIN state: TX zip: 78712 country: USA phone: (512)471-1455 telex: TEXASTRO ! lname: SHELUS fname: PETER mi: J. title: DR. category: CON inst: UNIVERSITY OF TEXAS addr_1: DEPARTMENT OF ASTRONOMY city: AUSTIN state: TX zip: 78712 country: USA phone: (512)471-3339 ! ! end of general_form_address records fixed_targets: targnum: 13 name_1: GLIESE065 name_2: L-726-8-B descr_1: PARALLAX STAR pos_1: RA = 24.7094196D +/- 0.0003D, pos_2: DEC = -17.958141D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 12.6 +/- 0.6 ! targnum: 14 name_1: GLIESE065-1-REF descr_1: REF. STAR(8) pos_1: RA = 24.6878382D +/- 0.0003D, pos_2: DEC = -17.906448D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 15.3 +/- 0.6 ! targnum: 15 name_1: GLIESE065-2-REF descr_1: REF. STAR(9) pos_1: RA = 24.6874858D +/- 0.0003D, pos_2: DEC = -17.844069D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 16.9 +/- 0.6 ! targnum: 16 name_1: GLIESE065-3-REF descr_1: REF. STAR(10) pos_1: RA = 24.6324312D +/- 0.0003D, pos_2: DEC = -17.868349D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 16.8 +/- 0.6 ! targnum: 17 name_1: GLIESE065-4-REF descr_1: REF. STAR(13) pos_1: RA = 24.7054651D +/- 0.0003D, pos_2: DEC = -17.987361D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 16.6 +/- 0.6 ! targnum: 18 name_1: GLIESE065-5-REF descr_1: REF. STAR(17) pos_1: RA = 24.7450292D +/- 0.0003D, pos_2: DEC = -18.031823D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 15.1 +/- 0.6 ! targnum: 19 name_1: GLIESE065-6-REF descr_1: REF. STAR(18) pos_1: RA = 24.7713088D +/- 0.0003D, pos_2: DEC = -18.005393D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 17.0 +/- 0.6 ! targnum: 20 name_1: GLIESE065-7-REF descr_1: REF. STAR(30) pos_1: RA = 24.6643394D +/- 0.0003D, pos_2: DEC = -17.831184D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 10.5 +/- 0.6 ! targnum: 21 name_1: GLIESE065-8-REF descr_1: REF. STAR(41) pos_1: RA = 24.6861074D +/- 0.0003D, pos_2: DEC = -17.898516D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 16.8 +/- 0.6 ! targnum: 34 name_1: GLIESE406 name_2: WOLF359 descr_1: PARALLAX STAR pos_1: RA = 164.167995D +/- 0.0003D, pos_2: DEC = 7.04463865D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 14.5 +/- 0.6 ! targnum: 35 name_1: GLIESE406-1-REF descr_1: REF. STAR(3) pos_1: RA = 164.190253D +/- 0.0003D, pos_2: DEC = 7.023959D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 14.6 +/- 0.6 ! targnum: 36 name_1: GLIESE406-2-REF descr_1: REF. STAR(7) pos_1: RA = 164.220637D +/- 0.0003D, pos_2: DEC = 7.118430D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 15.1 +/- 0.6 ! targnum: 37 name_1: GLIESE406-3-REF descr_1: REF. STAR(8) pos_1: RA = 164.205196D +/- 0.0003D, pos_2: DEC = 6.926406D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 14.4 +/- 0.6 ! targnum: 38 name_1: GLIESE406-4-REF descr_1: REF. STAR(10) pos_1: RA = 164.171231D +/- 0.0003D, pos_2: DEC = 7.049409D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 12.7 +/- 0.6 ! targnum: 39 name_1: GLIESE406-5-REF descr_1: REF. STAR(11) pos_1: RA = 164.179843D +/- 0.0003D, pos_2: DEC = 7.035945D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 14.6 +/- 0.6 ! targnum: 40 name_1: GLIESE406-6-REF descr_1: REF. STAR(12) pos_1: RA = 164.153761D +/- 0.0003D, pos_2: DEC = 7.034021D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 15.8+/- 0.6 ! targnum: 41 name_1: GLIESE406-7-REF descr_1: REF. STAR(13) pos_1: RA = 164.185997D +/- 0.0003D, pos_2: DEC = 7.014371D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 15.6 +/- 0.6 ! targnum: 42 name_1: GLIESE406-8-REF descr_1: REF. STAR(14) pos_1: RA = 164.203283D +/- 0.0003D, pos_2: DEC = 7.007548D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 16.6 +/- 0.6 ! targnum: 43 name_1: GLIESE406-9-REF descr_1: REF. STAR(15) pos_1: RA = 164.189893D +/- 0.0003D, pos_2: DEC = 7.002383D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 15.6 +/- 0.6 ! targnum: 44 name_1: GLIESE406-10-REF descr_1: REF. STAR(36) pos_1: RA = 164.221942D +/- 0.0003D, pos_2: DEC = 7.062799D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 15.7 +/- 0.6 ! targnum: 52 name_1: GLIESE551 name_2: PROX-CENTAURI descr_1: PARALLAX STAR pos_1: RA = 217.464821D +/- 0.0003D, pos_2: DEC = -62.683039D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 13.5 +/- 0.6 ! targnum: 53 name_1: GLIESE551-1-REF descr_1: REF. STAR(3) pos_1: RA = 217.416933D +/- 0.0003D, pos_2: DEC = -62.609589D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 16 +/- 0.6 ! targnum: 54 name_1: GLIESE551-2-REF descr_1: REF. STAR(4) pos_1: RA = 217.492894D +/- 0.0003D, pos_2: DEC = -62.605077D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 16.6 +/- 0.6 ! targnum: 55 name_1: GLIESE551-3-REF descr_1: REF. STAR(5) pos_1: RA = 217.590608D +/- 0.0003D, pos_2: DEC = -62.617525D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 15.7 +/- 0.6 ! targnum: 56 name_1: GLIESE551-4-REF descr_1: REF. STAR(10) pos_1: RA = 217.422620D +/- 0.0003D, pos_2: DEC = -62.754940D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 14.9 +/- 0.6 ! targnum: 57 name_1: GLIESE551-5-REF descr_1: REF. STAR(11) pos_1: RA = 217.287052D +/- 0.0003D, pos_2: DEC = -62.774459D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 13.5 +/- 0.6 ! targnum: 58 name_1: GLIESE551-6-REF descr_1: REF.STAR(14) pos_1: RA = 217.497813D +/- 0.0003D, pos_2: DEC = -62.712510D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 15.3 +/- 0.6 ! targnum: 59 name_1: GLIESE551-7-REF descr_1: REF. STAR(32) pos_1: RA = 217.522699D +/- 0.0003D, pos_2: DEC = -62.683843D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 16.9 +/- 0.6 ! targnum: 60 name_1: GLIESE551-8-REF descr_1: REF. STAR(37) pos_1: RA = 217.520477D +/- 0.0003D, pos_2: DEC = -62.698549D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 16.8 +/- 0.6 ! targnum: 72 name_1: GLIESE699 name_2: BARNARDS-STAR descr_1: PARALLAX STAR pos_1: RA = 269.455136D +/- 0.0003D, pos_2: DEC = 4.668080D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 9.5 +/- 0.6 ! targnum: 73 name_1: GLIESE699-1-REF descr_1: REF. STAR(1) pos_1: RA = 269.466587D +/- 0.0003D, pos_2: DEC = 4.616667D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 14.4 +/- 0.6 ! targnum: 74 name_1: GLIESE699-2-REF descr_1: REF. STAR(3) pos_1: RA = 269.510963D +/- 0.0003D, pos_2: DEC = 4.698725D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 15.8 +/- 0.6 ! targnum: 75 name_1: GLIESE699-3-REF descr_1: REF. STAR(4) pos_1: RA = 269.477019D +/- 0.0003D, pos_2: DEC = 4.680456D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 14.5 +/- 0.6 ! targnum: 76 name_1: GLIESE699-4-REF descr_1: REF. STAR(12) pos_1: RA = 269.401705D +/- 0.0003D, pos_2: DEC = 4.667849D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 15.2 +/- 0.6 ! targnum: 77 name_1: GLIESE699-5-REF descr_1: REF. STAR(76) pos_1: RA = 269.479581D +/- 0.0003D, pos_2: DEC = 4.681556D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 16.2+/- 0.6 ! targnum: 78 name_1: GLIESE699-6-REF descr_1: REF. STAR(90) pos_1: RA = 269.429240D+/- 0.0003D, pos_2: DEC = 4.666314D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 16.3 +/- 0.6 ! targnum: 79 name_1: GLIESE699-7-REF descr_1: REF. STAR(92) pos_1: RA = 269.460093D +/- 0.0003D, pos_2: DEC = 4.676119D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 16.4 +/- 0.6 ! targnum: 80 name_1: GLIESE699-8-REF descr_1: REF. STAR(109) pos_1: RA = 269.484039D +/- 0.0003D, pos_2: DEC = 4.663985D +/- 0.0003D equinox: 2000.0 fluxnum_1: 1 fluxval_1: V = 16.2 +/- 0.6 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 21.000 targname: GLIESE065 config: FGS opmode: TRANS aperture: PRIME sp_element: F583W num_exp: 1 time_per_exp: 100S s_to_n: 10 fluxnum_1: 1 priority: 3 req_1: EARLY ACQ FOR 24.1; req_2: CYCLE 9 / 21-27.2; req_3: NON-INT ! linenum: 22.000 sequence_1: DEFINE sequence_2: GLI-065A targname: GLIESE065 config: FGS opmode: POS aperture: PRIME sp_element: F550W num_exp: 1 time_per_exp: 52S s_to_n: 10 fluxnum_1: 1 priority: 3 param_1: DATA-RATE = 32 req_1: SEQ 22-24; req_2: NON-INT / 22-24 ! linenum: 22.300 sequence_1: ^ targname: GLIESE065-1-REF config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ param_1: ^ req_1: DO FOR TARG 14-21 ! linenum: 22.600 sequence_1: ^ targname: GLIESE065 config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 22.800 sequence_1: ^ targname: GLIESE065-1-REF config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ param_1: ^ req_1: DO FOR TARG 14-21 ! linenum: 23.000 sequence_1: ^ targname: GLIESE065 config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 23.300 sequence_1: ^ targname: GLIESE065-1-REF config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ param_1: ^ req_1: DO FOR TARG 14-21 ! linenum: 23.600 sequence_1: ^ targname: GLIESE065 config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 23.800 sequence_1: ^ targname: GLIESE065-1-REF config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ param_1: ^ req_1: DO FOR TARG 14-21 ! linenum: 24.000 sequence_1: DEFINE sequence_2: GLI-065A targname: GLIESE065 config: FGS opmode: POS aperture: PRIME sp_element: F550W num_exp: 1 time_per_exp: 52S s_to_n: 10 fluxnum_1: 1 priority: 3 param_1: DATA-RATE = 32 ! linenum: 24.100 sequence_1: USE sequence_2: GLI-065A req_2: AT 16-JAN-91 +/- 10D; req_3: COND ON 21 IF NOT DOUBLE ! linenum: 24.200 sequence_1: USE sequence_2: GLI-065A req_2: AFTER 24.1 BY 365D +/- 10D; req_3: COND ON 21 IF NOT DOUBLE ! linenum: 24.300 sequence_1: USE sequence_2: GLI-065A req_2: AFTER 24.2 BY 365D +/- 10D; req_3: COND ON 21 IF NOT DOUBLE ! linenum: 25.000 sequence_1: DEFINE sequence_2: GLI-065B targname: GLIESE065 config: FGS opmode: POS aperture: PRIME sp_element: F550W num_exp: 1 time_per_exp: 52S s_to_n: 10 fluxnum_1: 1 priority: 3 param_1: DATA-RATE = 32 req_1: SEQ 25-27; req_2: NON-INT / 25-27 ! linenum: 25.200 sequence_1: ^ targname: GLIESE065-1-REF config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ param_1: ^ req_1: DO FOR TARG 14-21 ! linenum: 25.400 sequence_1: ^ targname: GLIESE065 config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 25.600 sequence_1: ^ targname: GLIESE065-1-REF config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ param_1: ^ req_1: DO FOR TARG 14-21 ! linenum: 25.800 sequence_1: ^ targname: GLIESE065 config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 26.000 sequence_1: ^ targname: GLIESE065-1-REF config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ param_1: ^ req_1: DO FOR TARG 14-21 ! linenum: 26.200 sequence_1: DEFINE sequence_2: GLI-065B targname: GLIESE065 config: FGS opmode: POS aperture: PRIME sp_element: F550W num_exp: 1 time_per_exp: 52S s_to_n: 10 fluxnum_1: 1 priority: 3 param_1: DATA-RATE = 32 ! linenum: 26.400 sequence_1: ^ targname: GLIESE065-1-REF config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ param_1: ^ req_1: DO FOR TARG 14-21 ! linenum: 26.600 sequence_1: ^ targname: GLIESE065 config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 26.700 sequence_1: ^ targname: GLIESE065-1-REF config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ param_1: ^ req_1: DO FOR TARG 14-21 ! linenum: 26.800 sequence_1: ^ targname: GLIESE065 config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 26.900 sequence_1: ^ targname: GLIESE065-1-REF config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ param_1: ^ req_1: DO FOR TARG 14-21 ! linenum: 27.000 sequence_1: ^ targname: GLIESE065 config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 27.100 sequence_1: USE sequence_2: GLI-065B req_2: AT 18-JUL-91 +/- 10D; req_3: COND ON 21 IF NOT DOUBLE ! linenum: 27.200 sequence_1: USE sequence_2: GLI-065B req_2: AFTER 27.1 BY 365D +/- 10D; req_3: COND ON 21 IF NOT DOUBLE ! ! end of exposure logsheet ! No scan data records found