! File: 4893C.PROP ! Database: PEPDB ! Date: 23-FEB-1994:08:28:40 coverpage: title_1: ORBITAL MOTIONS OF CLOSE BINARY STARS title_2: CYCLE 3 HIGH sci_cat: STELLAR ASTROPHYSICS sci_subcat: ASTROMETRY proposal_for: GTO/AST cont_id: 1001 pi_fname: WILLIAM pi_mi: H. pi_lname: JEFFERYS pi_inst: TEXAS, UNIVERSITY OF pi_country: USA pi_phone: 512-471-4461 keywords_1: BINARY STARS; ORBITAL ELEMENTS; STELLAR MASSES hours_pri: 16.34 num_pri: 29 time_crit: X pi_position: PROFESSOR OF ASTRONO ! end of coverpage abstract: line_1: Nearby binary-star systems with rapid orbital motion are and line_2: will continue to be the principal source of our knowledge line_3: on stellar masses. Owing to its expected high angular line_4: resolution and high-precision astrometric performance, HST line_6: will provide unusual opportunities for binary-star research. line_7: The purpose of this project is to measure with HST/FGS in line_8: the transfer-function mode selected binary stars, primarily line_9: visual pairs at critical phases in their orbits, in order to line_10: improve substantially our knowledge of their orbital line_11: elements. These results will not only yield improved mass line_12: values for the systems so investigated, but will also serve line_13: as important calibrators for a large body of existing data line_14: on binary-star orbits and stellar masses. ! ! end of abstract general_form_proposers: lname: JEFFERYS fname: WILLIAM mi: H. inst: TEXAS, UNIVERSITY OF country: USA ! lname: BENEDICT fname: GEORGE mi: F. inst: TEXAS, UNIVERSITY OF country: USA ! lname: DUNCOMBE fname: RAYNOR mi: L. inst: TEXAS, UNIVERSITY OF country: USA ! lname: FRANZ fname: OTTO mi: G. inst: LOWELL OBSERVATORY country: USA ! lname: FREDRICK fname: LAURENCE mi: W. inst: VIRGINIA, UNIVERSITY OF country: USA ! lname: HEMENWAY fname: PAUL mi: D. inst: TEXAS, UNIVERSITY OF country: USA ! lname: SHELUS fname: PETER mi: J. inst: TEXAS, UNIVERSITY OF country: USA ! lname: VAN ALTENA fname: WILLIAM mi: F. inst: YALE UNIVERSITY country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: Each observation will consis of two separate sets of ten line_2: individual scans carried out in the multiple scan mode, line_3: i.e., continuous scans with reversal of scan direction line_4: between any two subsequent scans. The two sets of scans line_5: constituting each observation will be separated by 45 +/- line_6: 15 days, i.e., by about 45 +/- deg. in scan-axes line_7: orientations. A scan rate of 0.04 arcsec/sec and scan line_8: length of 1.2 arcsec per interferometer axis will be used. line_9: The corresponding exposure time will be 300 sec. For line_10: purposes of S/N calculations, a sample time of 0.025 line_11: sec is adopted, corresponding to an effective step-size line_12: of 0.001 arcsec. One observation (as defined above) is line_13: desired per target during cycle 3. ! question: 4 section: 1 line_1: Most of the binary targets selected for HST observation line_2: are expected to have angular separations less than 30 mas line_3: (the current resolution limit for speckle interferometry line_4: with 4-m class telescopes). Several are also fainter than line_5: the current speckle limit. ! question: 5 section: 1 line_1: The requirement to obtain scan sets separated by 45 days line_2: +/- 15 days is justified in order to obtain relative line_3: positions of binary-star components with similar or line_4: equal accuracy in two (orthogonal) coordinates. The line_5: (preferable but less likely) alternative is to roll the line_6: spacecraft by 45 +/- 15 deg between sets of scans made line_7: in quicker succession. ! question: 7 section: 1 line_1: Data reduction and analysis will be carried out with the line_2: use of algorithms and software developed and already line_3: successfully used by STAT. The data reduction and anlysis line_4: will be carried out at Lowell Observatory. ! question: 10 section: 1 line_1: Computer facilities at STAT members' institutions. ! question: 13 section: 1 line_1: Close visual binaries as well as potentially resolvable line_2: spectroscopic and occultation binaries will be observed line_3: for the pupose of measuring relative positions and orbital line_4: motions of their components. Most of the visual binaries line_5: will be at orbital phases never before observed. ! !end of general form text general_form_address: lname: FRANZ fname: OTTO mi: G. category: CON inst: LOWELL OBSERVATORY addr_1: 1400 W. MARS HILL RD city: FLAGSTAFF state: AZ zip: 86001 country: USA phone: 602-774-3358 ! lname: JEFFERYS fname: WILLIAM mi: H. category: PI inst: TEXAS, UNIVERSITY OF addr_1: ASTRONOMY DEPARTMENT city: AUSTIN state: TX zip: 78712 country: USA phone: 512-471-4461 telex: TEXASTRO ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: HD16739 name_2: 12 PER descr_1: A pos_1: RA=02H 39M 05.0S +/- 0.1S, pos_2: DEC=+39D 59' 01" +/- 1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: -0.001331 dec_pm_val: -0.1800 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=4.91 ! targnum: 2 name_1: HD22262 name_2: B52 descr_1: A pos_1: RA=03H 31M 55.5S +/- 0.1S, pos_2: DEC=-31D 14' 52" +/- 1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: -0.001731 ra_pm_unct: 0.000936 dec_pm_val: 0.0650 dec_pm_unct: 0.0100 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=6.2 ! targnum: 3 name_1: BD+31D637 name_2: COU691 descr_1: A pos_1: RA=03H 39M 08.3S +/- 0.1S, pos_2: DEC=+31D 31' 04" +/- 1" equinox: 1950 pm_or_par: N plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=8.30 ! targnum: 4 name_1: HD32923 name_2: ADS3701 descr_1: A pos_1: RA=05H 04M 29.5S +/- 0.1S, pos_2: DEC=+18D 34' 47" +/- 1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: 0.035799 ra_pm_unct: 0.000134 dec_pm_val: 0.0190 dec_pm_unct: 0.0020 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=4.90 ! targnum: 5 name_1: HD41511 name_2: 17 LEP pos_1: RA=06H 04M 59.0S +/- 0.1S, pos_2: DEC=-16D 29' 04" +/- 1" equinox: 2000 pm_or_par: N plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=4.93 ! targnum: 6 name_1: BD+14D1690 name_2: ADS6154 descr_1: A pos_1: RA=07H 29M 25.3S +/- 0.1S, pos_2: DEC=+14D 10' 52" +/- 1" equinox: 1950 pm_or_par: N plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=9.5 ! targnum: 7 name_1: HD60414 name_2: BD-14D1971 pos_1: RA=07H 33M 47.8S +/- 0.1S, pos_2: DEC=-14D 31' 26" +/- 1" equinox: 2000 pm_or_par: N plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=4.97 ! targnum: 8 name_1: HD61994 name_2: BD+70D474 pos_1: RA=07H 47M 30.4S +/- 0.1S, pos_2: DEC=+70D 12' 24" +/- 1" equinox: 2000 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 2000.00 ra_pm_val: -0.006261 ra_pm_unct: 0.000591 dec_pm_val: -0.1440 dec_pm_unct: 0.0120 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=7.2 ! targnum: 9 name_1: HD64606 name_2: BD-1D1883 pos_1: RA=07H 52M 02.6S +/- 0.1S, pos_2: DEC=-01D 16' 47" +/- 1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: -0.017798 ra_pm_unct: 0.000667 dec_pm_val: -0.0600 dec_pm_unct: 0.0100 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=7.43 ! targnum: 10 name_1: HD73900 name_2: I314 descr_1: A pos_1: RA=08H 37M 27.2S +/- 0.1S, pos_2: DEC=-36D 25' 48" +/- 1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: -0.011799 ra_pm_unct: 0.000804 dec_pm_val: 0.0360 dec_pm_unct: 0.0090 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=6.13 ! targnum: 11 name_1: HD80671 name_2: FIN363 descr_1: A pos_1: RA=09H 16M 35.7S +/- 0.1S, pos_2: DEC=-68D 28' 42" +/- 1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: -0.006996 ra_pm_unct: 0.000672 dec_pm_val: -0.0250 dec_pm_unct: 0.0100 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=5.38 ! targnum: 12 name_1: HD88021 name_2: ADS7662 descr_1: A pos_1: RA=10H 06M 34.2S +/- 0.1S, pos_2: DEC=+20D 34' 41" +/- 1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: -0.001467 ra_pm_unct: 0.000598 dec_pm_val: -0.0270 dec_pm_unct: 0.0100 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=7.3 ! targnum: 13 name_1: HD115488 name_2: FIN350 descr_1: A pos_1: RA=13H 14M 56.1S +/- 0.1S, pos_2: DEC=-00D 24' 47" +/- 1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: -0.004067 ra_pm_unct: 0.000600 dec_pm_val: -0.0290 dec_pm_unct: 0.0090 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=6.37 ! targnum: 14 name_1: GLIESE568 name_2: ROSS52 descr_1: A pos_1: RA=14H 53M 51.500S +/- 0.1S, pos_2: DEC=+23D 33' 21.00" +/- 1" equinox: 2000 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: -0.046668 ra_pm_unct: 0.000670 dec_pm_val: 0.1900 dec_pm_unct: 0.0100 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=11.1 ! targnum: 15 name_1: GLIESE660 name_2: L989-20 descr_1: A pos_1: RA=17H 09M 18.0S +/- 0.1S, pos_2: DEC=-01D 47' 18" +/- 1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: -0.029334 ra_pm_unct: 0.000667 dec_pm_val: -0.3200 dec_pm_unct: 0.0100 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=11.32 ! targnum: 16 name_1: HD163840 name_2: BD+24D3283 descr_1: A pos_1: RA=17H 55M 10.3S +/- 0.1S, pos_2: DEC=+23D 59' 58" +/- 1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: -0.001664 ra_pm_unct: 0.000664 dec_pm_val: 0.0760 dec_pm_unct: 0.0100 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=6.30 ! targnum: 17 name_1: BD+4D3562 name_2: KUI84 descr_1: A pos_1: RA=17H 58M 24.567S +/- 0.1S, pos_2: DEC=+04D 27' 43.61" +/- 1" equinox: 2000 pm_or_par: N plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=10.6 ! targnum: 18 name_1: HD166988 name_2: ADS11149 descr_1: A pos_1: RA=18H 09M 55.3S +/- 0.1S, pos_2: DEC=+33D 26' 01" +/- 1" equinox: 1950 pm_or_par: N plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=5.85 ! targnum: 19 name_1: HD179950 name_2: ADS12214 descr_1: A pos_1: RA=19H 12M 28.5S +/- 0.1S, pos_2: DEC=-25D 20' 41" +/- 1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: 0.003069 ra_pm_unct: 0.000133 dec_pm_val: -0.0250 dec_pm_unct: 0.0020 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=4.85 ! targnum: 20 name_1: HD181391 name_2: 26 AQL descr_1: A pos_1: RA=19H 20M 32.8S +/- 0.1S, pos_2: DEC=-05D 24' 57" +/- 1" equinox: 2000 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 2000.00 ra_pm_val: 0.007467 ra_pm_unct: 0.000201 dec_pm_val: 0.0480 dec_pm_unct: 0.0030 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=5.01 ! targnum: 21 name_1: HD182369 name_2: FIN327 descr_1: A pos_1: RA=19H 22M 14.0S +/- 0.1S, pos_2: DEC=-24D 36' 27" +/- 1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: 0.004004 dec_pm_val: -0.0500 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=5.02 ! targnum: 22 name_1: HD193194 name_2: I1416 descr_1: A pos_1: RA=20H 17M 02.5S +/- 0.1S, pos_2: DEC=-34D 44' 34" +/- 1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: 0.002596 ra_pm_unct: 0.000730 dec_pm_val: -0.0400 dec_pm_unct: 0.0110 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=6.6 ! targnum: 23 name_1: HD195987 name_2: BD+41D3799 descr_1: A pos_1: RA=20H 31M 05.6S +/- 0.1S, pos_2: DEC=+41D 43' 15" +/- 1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: -0.011004 ra_pm_unct: 0.000402 dec_pm_val: 0.4500 dec_pm_unct: 0.0060 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=7.09 ! targnum: 24 name_1: HD201038 name_2: ADS14648 descr_1: A pos_1: RA=21H 04M 45.8S +/- 0.1S, pos_2: DEC=-08D 26' 13" +/- 1" equinox: 1950 pm_or_par: N plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=7.50 ! targnum: 25 name_1: HD207964 name_2: CPD-62D6277 descr_1: A pos_1: RA=21H 51M 31.4S +/- 0.1S, pos_2: DEC=-62D 07' 20" +/- 1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: 0.003735 ra_pm_unct: 0.000727 dec_pm_val: -0.0810 dec_pm_unct: 0.0070 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=5.90 ! targnum: 26 name_1: HD208816 name_2: VV CEP descr_1: A pos_1: RA=21H 56M 39.1S +/- 0.1S, pos_2: DEC=+63D 37' 33" +/- 1" equinox: 2000 pm_or_par: N plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=4.91 ! targnum: 27 name_1: HD214511 name_2: ADS16111 descr_1: A pos_1: RA=22H 34M 51.6S +/- 0.1S, pos_2: DEC=+72D 37' 15" +/- 1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: 0.006674 ra_pm_unct: 0.000603 dec_pm_val: 0.0630 dec_pm_unct: 0.0090 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=7.50 ! targnum: 28 name_1: HD217166 name_2: ADS16417 descr_1: A pos_1: RA=22H 56M 02.9S +/- 0.1S, pos_2: DEC=+09D 05' 28" +/- 1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: 0.021936 ra_pm_unct: 0.000331 dec_pm_val: -0.1360 dec_pm_unct: 0.0040 plate_req: N plate_avail: N fluxnum_1: 1 fluxval_1: V=7.50 ! targnum: 29 name_1: UPGREN69 descr_1: A pos_1: RA=9.46625D +/- .0004D, pos_2: DEC=84.9632778D +/- .002D equinox: 1950.0 comment_1: THIS STAR IS FOR REFERENCE comment_2: TRANSFER SCANS fluxnum_1: 1 fluxval_1: V=9.58 +/- 0.05 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 sequence_1: DEFINE sequence_2: BTF targname: # config: FGS opmode: TRANS aperture: 3 sp_element: # num_exp: 1 time_per_exp: 300S fluxnum_1: 1 priority: # param_1: DATA-RATE=32 param_2: STEP-SIZE=1.0 param_3: SCANS=10 param_4: ACQ-MODE=SEARCH req_1: POS TARG 0.0, 0.0; req_2: CYCLE 3 comment_1: FINE LOCK GUIDING comment_2: OFFSET KB=0.6 ARCSEC FROM COARSE TRACK comment_3: POSITION TO START OF SCAN ! linenum: 2.000 sequence_1: USE BTF targname: HD16739 sp_element: F5ND priority: 1 req_1: REPEAT 2 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 3.000 sequence_1: USE BTF targname: HD22262 sp_element: F5ND priority: 1 req_1: REPEAT 3 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 4.000 sequence_1: USE BTF targname: BD+31D637 sp_element: PUPIL priority: 3 req_1: REPEAT 4 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 5.000 sequence_1: USE BTF targname: HD32923 sp_element: F5ND priority: 1 req_1: REPEAT 5 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 6.000 sequence_1: USE BTF targname: HD41511 sp_element: F5ND priority: 2 req_1: REPEAT 6 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 7.000 sequence_1: USE BTF targname: BD+14D1690 sp_element: PUPIL priority: 2 req_1: REPEAT 7 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 8.000 sequence_1: USE BTF targname: HD60414 sp_element: F5ND priority: 1 req_1: REPEAT 8 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 9.000 sequence_1: USE BTF targname: HD61994 sp_element: PUPIL priority: 1 req_1: REPEAT 9 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 10.000 sequence_1: USE BTF targname: HD64606 sp_element: PUPIL priority: 1 req_1: REPEAT 10 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 11.000 sequence_1: USE BTF targname: HD73900 sp_element: F5ND priority: 1 req_1: REPEAT 11 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 12.000 sequence_1: USE BTF targname: HD80671 sp_element: F5ND priority: 1 req_1: REPEAT 12 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; comment_1: OBSERVE EARLY IN CYCLE 3 ! linenum: 13.000 sequence_1: USE BTF targname: HD88021 sp_element: PUPIL priority: 3 req_1: REPEAT 13 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 14.000 sequence_1: USE BTF targname: HD115488 sp_element: F5ND priority: 2 req_1: REPEAT 14 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 15.000 sequence_1: USE BTF targname: GLIESE568 sp_element: PUPIL priority: 1 req_1: REPEAT 15 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 16.000 sequence_1: USE BTF targname: GLIESE660 sp_element: PUPIL priority: 3 req_1: REPEAT 16 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 17.000 sequence_1: USE BTF targname: HD163840 sp_element: F5ND priority: 3 req_1: REPEAT 17 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 18.000 sequence_1: USE BTF targname: BD+4D3562 sp_element: PUPIL priority: 2 req_1: REPEAT 18 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 19.000 sequence_1: USE BTF targname: HD166988 sp_element: F5ND priority: 3 req_1: REPEAT 19 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 20.000 sequence_1: USE BTF targname: HD179950 sp_element: F5ND priority: 2 req_1: REPEAT 20 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 21.000 sequence_1: USE BTF targname: HD181391 sp_element: F5ND priority: 2 req_1: REPEAT 21 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 22.000 sequence_1: USE BTF targname: HD182369 sp_element: F5ND priority: 1 req_1: REPEAT 22 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; comment_1: OBSERVE EARLY IN CYCLE 3 ! linenum: 23.000 sequence_1: USE BTF targname: HD193194 sp_element: F5ND priority: 1 req_1: REPEAT 23 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 24.000 sequence_1: USE BTF targname: HD195987 sp_element: PUPIL priority: 2 req_1: REPEAT 24 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 25.000 sequence_1: USE BTF targname: HD201038 sp_element: PUPIL priority: 2 req_1: REPEAT 25 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 26.000 sequence_1: USE BTF targname: HD207964 sp_element: F5ND priority: 1 req_1: REPEAT 26 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 27.000 sequence_1: USE BTF targname: HD208816 sp_element: F5ND priority: 1 req_1: REPEAT 27 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 28.000 sequence_1: USE BTF targname: HD214511 sp_element: PUPIL priority: 3 req_1: REPEAT 28 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; ! linenum: 29.000 sequence_1: USE BTF targname: HD217166 sp_element: PUPIL priority: 1 req_1: REPEAT 29 EVERY 45D +/- 15D FOR 1 MORE req_2: TIMES; comment_1: OBSERVE EARLY IN CYCLE 3 ! linenum: 30.000 sequence_1: USE BTF targname: UPGREN69 sp_element: F5ND priority: 1 req_1: COND IF SECONDARY MIRROR MOVED; comment_1: THIS STAR MUST BE OBSERVED ONCE comment_2: FOR EVERY SECONDARY MIRROR POSITION comment_3: AT WHICH A BINARY TARGET IS OBSERVED comment_4: WITH SPECTRAL ELEMENT F5ND. ! linenum: 31.000 sequence_1: USE BTF targname: UPGREN69 sp_element: PUPIL priority: 1 req_1: COND IF SECONDARY MIRROR MOVED; comment_1: THIS STAR MUST BE OBSERVED ONCE comment_2: FOR EVERY SECONDARY MIRROR POSITION comment_3: AT WHICH A BINARY TARGET IS OBSERVED comment_4: WITH SPECTRAL ELEMENT PUPIL. ! ! end of exposure logsheet ! No scan data records found