! File: 2251C.PROP ! Database: PEPDB ! Date: 17-FEB-1994:04:02:10 coverpage: title_1: THE PROPERTIES OF SINGLE INTERSTELLAR CLOUDS: title_2: MODIFIED CYCLE 1 OBSERVATIONS sci_cat: INTERSTELLAR MEDIUM proposal_for: GO longterm: 2 cont_id: 2251 pi_title: PROF. pi_fname: L. pi_mi: M. pi_lname: HOBBS pi_inst: CHICAGO, UNIVERSITY OF pi_country: USA pi_phone: (414) 245-5555 keywords_1: INTERSTELLAR CLOUDS hours_pri: 21.46 num_pri: 8 hrs: Y funds_amount: 170528 funds_length: 12 funds_date: JUL-91 pi_position: PROFESSOR off_fname: JOYCE off_lname: FREEDMAN off_title: ASST. VICE PRES. off_inst: THE UNIVERSITY OF CHICAGO off_addr_1: 970 E. 58TH ST. off_city: CHICAGO off_state: IL off_zip: 60637 off_country: USA off_phone: (312) 702-8604 off_telex: 282-131 ! end of coverpage abstract: line_1: WE PROPOSE TO USE THE ECHELLE AND 160M GRATINGS OF THE HIGH RESOLUTION line_2: SPECTROGRAPH OVER A TWO-YEAR PERIOD TO OBSERVE THE PROFILES OF line_3: INTERSTELLAR ABSORPTION LINES. THE COLUMN DENSITES OF 18 NEUTRAL OR line_4: IONIZED FORMS OF THE ELEMENTS C,N,O,Mg,Si,P,S,Fe, AND Zn WILL BE line_5: MEASURED IN THE APPROXIMATELY 100 INDIVIDUAL INTERSTELLAR CLOUDS ALONG line_6: THE LIGHT PATHS TO 18 BRIGHT, BROAD-LINED STARS OF EARLY SPECTRAL TYPE line_7: WITHIN 1 KPC OF THE SUN. THE PRIMARY PURPOSE OF THE OBSERVATIONS IS TO line_8: DETERMINE MORE ACCURATELY THAN WAS HITHERTO POSSIBLE THE FUNDAMENTAL line_9: PHYSICAL PROPERTIES OF THE RESOLVED CLOUDS, INCLUDING LINEAR SIZE, line_10: TEMPERATURE, TOTAL DENSITY, FRACTIONAL IONIZATION AND THE RELATIVE line_11: ABUNDANCES OF THE 9 SELECTED ELEMENTS. line_13: THE REST OF THIS OBSERVING PROGRAM IS CONTAINED IN APPROVED PROPOSAL ID = line_14: 3993; THE PROGRAM ENUMERATED HERE CONSISTS OF THAT PART OF OUR ORIGINAL line_15: PROGRAM, ID = 2251, WHICH REQUIRED MODIFICATION IN ORDER TO BE CARRIED line_16: OUT USING ONLY SIDE 2 OF THE GHRS. THIS PROGRAM THEREFORE CONSISTS OF line_17: ECH-B AND G160M OBSERVATIONS OF EACH OF 8 STARS AT 14 OR MORE WAVELENGTHS. line_18: PROGRAMS 2251 AND 3993 SHOULD BE CONSULTED FOR ADDITIONAL DETAILS. ! ! end of abstract general_form_proposers: lname: HOBBS fname: L. title: P.I. mi: M. inst: CHICAGO, UNIVERSITY OF country: USA ! lname: MORTON fname: D. title: DR. mi: C. inst: HERZBERG INSTITUTE OF ASTROPHYSICS country: CANADA ! lname: SPITZER JR. fname: L. title: DR. inst: PRINCETON UNIVERSITY country: USA ! lname: WELTY fname: D. title: DR. mi: E. inst: CHICAGO, UNIVERSITY OF country: USA ! lname: YORK fname: D. title: DR. mi: G. inst: CHICAGO, UNIVERSITY OF country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: FOR EACH OF 8 STARS, A SERIES OF 14 OR MORE EXPOSURES IS TO BE OBTAINED line_2: THROUGH THE SMALL SCIENCE APERTURE IN THE ACCUMULATION MODE, WITH THE line_3: 160M OR ECH GRATINGS. NINE OBSERVATIONS OF A FEW MINUTES EACH ARE MADE line_4: WITH THE 160M GRATING, IN THE INTERVAL BETWEEN 1120 AND 1680 ANGSTROMS; line_5: 5 OBSERVATIONS OF A FEW MINUTES EACH ARE MADE IN THE ECH-B MODE IN THE line_6: INTERVAL BETWEEN 1850 AND 2810 ANGSTROMS. FOR THE 4 BRIGHTEST STARS, line_7: UP TO 10 SIMILAR, ADDITIONAL ECH-B EXPOSURES ARE OBTAINED. IN THE ECH-B line_8: CASE, EXPOSURE TIMES ARE CHOSEN TO YIELD APPROXIMATELY 10,000 COUNTS line_9: PER DIODE; FOR EACH SPECTRAL SETTING, THREE SEPARATE SUBEXPOSURES WILL line_10: BE MADE IN THE WSCAN MODE, WITH THE SPECTRUM MOVED PARALLEL TO THE line_11: DISPERSION TO THREE DIFFERENT POSITIONS ON THE PHOTOCATHODE, TO ALLOW line_12: SOME CORRECTION FOR NON-UNIFORMITIES OF THE CATHODE. IN THE 160M CASE, line_13: EXPOSURE TIMES ARE CHOSEN TO YIELD APPROXIMATELY 40,000 COUNTS PER line_14: DIODE. ! question: 3 section: 2 line_1: ALL OF OUR TARGETS ARE BRIGHT STARS WITH WELL DETERMINED POSITIONS, line_2: FOR WHICH THE ONBOARD ACQUISITION MODE SHOULD SUFFICE. MOST OF THE line_3: STARS ARE EITHER SPECTROSCOPIC BINARIES OR KNOWN VISUAL BINARIES WITH line_4: SEPARATIONS LESS THAN 1 ARCSEC. IN ALL SUCH CASES, THE BRIGHTEST line_5: MEMBER OF THE MULTIPLE SYSTEM SHOULD BE CENTERED IN THE SMALL SCIENCE line_6: APERTURE. line_8: NO UNUSUALLY STRINGENT REQUIREMENTS WITH RESPECT TO THE USE OF THE line_9: PT/NE OR FLAT-FIELD LAMPS OR OF THE SUBSTEPPING ROUTINES ARE line_10: ANTICIPATED, ALTHOUGH WE DO REQUIRE ABOUT 1% SPECTROPHOTOMETRIC line_11: ACCURACY (S/N = 100) AS WELL AS ACCURATE (1 KM/S) HELIOCENTRIC line_12: WAVELENGTH SCALES. ! question: 4 section: 1 line_1: THE PROPOSED SCIENTIFIC PROGRAM CANNOT BE CARRIED OUT WITH ANY OTHER line_2: EXISTING TELESCOPE AND SPECTROGRAPH. THE HIGHEST POSSIBLE SPECTRAL RE- line_3: SOLVING POWER IS REQUIRED TO INVESTIGATE SEPARATELY THE INDIVIDUAL line_4: CLOUDS. IN ADDITION, ONLY THE LARGE ARRAY OF ULTRAVIOLET RESONANCE line_5: LINES OF THE PRINCIPAL IONIZATION STAGES OF MANY ELEMENTS PROVIDES SUF- line_6: FICIENT SPECTROSCOPIC DIAGNOSTIC POWER TO ANALYZE RELIABLY EACH CLOUD'S line_7: PHYSICAL PROPERTIES. line_9: THE REST OF THIS OBSERVING PROGRAM IS CONTAINED IN APPROVED PROPOSAL ID = line_10: 3993; THE PROGRAM ENUMERATED HERE CONSISTS OF THAT PART OF OUR ORIGINAL line_11: PROGRAM, ID = 2251, WHICH REQUIRED MODIFICATION IN ORDER TO BE CARRIED line_12: OUT USING ONLY SIDE 2 OF THE GHRS. THIS PROGRAM THEREFORE CONSISTS OF line_13: ECH-B AND G160M OBSERVATIONS OF EACH OF 8 STARS AT 14 OR MORE WAVELENGTHS. line_14: PROGRAMS 2251 AND 3993 SHOULD BE CONSULTED FOR ADDITIONAL DETAILS. ! question: 5 section: 1 line_1: THE PROGRAM STARS,THE NUMBER OF EXPOSURES FOR EACH, AND THE ESTIMATED line_2: TOTAL TIME UTILIZED IN ALL OF THOSE EXPOSURES FOR EACH STAR ARE GIVEN line_3: BELOW IN THE EXPOSURE LOGSHEET. OBSERVED ABSOLUTE UV FLUXES EXTENDING line_4: TYPICALLY TO BELOW 1400 ANGSTROMS HAVE BEEN PUBLISHED FOR NEARLY ALL line_5: OF THE PROGRAM STARS; SEE THE UV BRIGHT-STAR SPECTROPHOTOMETRIC line_6: CATALOGUE OF JAMAR ET AL (1976). THE ABSOLUTE SENSITIVITY OF THE HRS line_7: IS GIVEN IN THE GHRS INSTRUMENT HANDBOOK, VERSION 2.0. THIS line_8: COMBINATION ALLOWS STRAIGHTFORWARD ESTIMATES OF THE REQUIRED EXPOSURE line_9: TIMES. line_11: AS AN EXAMPLE, CONSIDER THE OBSERVATION OF THE 1827.9 A LINE OF Mg I line_12: IN THE SPECTRUM OF HD72127. FROM JAMAR ET AL, THE INCIDENT FLUX IS F = line_13: 4.89(-10) ERG/S/CM2/A; FROM THE GHRS HANDBOOK, A SENSITIVITY OF S = ! question: 5 section: 2 line_1: 2.0(+11) (COUNT/DIODE/S)/(ERG/S/CM2/A) APPLIES TO THE OTA + 0.25 line_2: ARCSEC APERTURE + ECH-B SYSTEM. IN AN INTEGRATION TIME T = 27 SEC, line_3: THEREFORE, FxSxT = 4000 COUNTS/DIODE. AFTER SLIGHT DISPLACEMENTS OF line_4: THE SPECTRUM ALONG THE DIGICON ARRAY, TWO MORE IDENTICAL EXPOSURES ARE line_5: THEN OBTAINED. IN A TOTAL OF 81 SEC = 1.3 MIN, ALMOST ALL DIODES WILL line_6: RECORD ABOUT 12,000 COUNTS, AS DESIRED. ! question: 6 section: 1 line_1: IN ADDITION TO THE STELLAR EXPOSURES DESCRIBED ABOVE, OBSERVATIONS line_2: OF THE ONBOARD PT/NE CALIBRATION LAMP WILL BE REQUIRED FOR THE 4 line_3: BRIGHTEST STARS, UNDER INSTRUMENTAL SETUPS IDENTICAL TO THOSE FOR line_4: THE CORRESPONDING STELLAR EXPOSURES. THE PURPOSE OF THESE COM- line_5: PARISON LAMP SPECTRA IS TO CALIBRATE THE ABSOLUTE WAVELENGTH SCALES TO line_6: AN ACCURACY OF ABOUT 1 KM/S. DETAILS ARE GIVEN IN THE EXPOSURE LOGSHEET line_7: BELOW. ! question: 7 section: 1 line_1: OUR PLAN IS TO USE THE CALIBRATED SCIENCE DATA WHICH ARE PROVIDED AS line_2: THE OUTPUT OF THE ROUTINE SCIENCE DATA PROCESSING (RSDP) AND THE line_3: CALIBRATION DATA BASE (CDBS) SOFTWARE, AT THE ST ScI. SINCE WE WILL line_4: ANALYZE ALMOST EXCLUSIVELY ABSORPTION LINE PROFILES, WE DO NOT line_5: REQUIRE PRECISE INFORMATION ABOUT THE ABSOLUTE FLUXES. line_7: ALTHOUGH WE WILL UNDOUBTEDLY MAKE ADDITIONAL USE OF THE SCIENCE DATA line_8: ANALYSIS SYSTEM (SDAS) AT THE INSTITUTE, ESPECIALLY AS WE GAIN EXPERI- line_9: ENCE WITH ITS DETAILED FEATURES, THE BULK OF THE ENSUING SCIENTIFIC line_10: ANALYSES, SUCH AS LINE-PROFILE FITTING AND EQUIVALENT-WIDTH INTEGRA- line_11: TIONS, PROBABLY WILL BE CARRIED OUT AT OUR HOME INSTITUTIONS. FOR MORE line_12: THAN FIFTEEN YEARS WE HAVE BEEN REDUCING AND ANALYZING SUCH UV AND OP- line_13: TICAL DATA, INCLUDING GROUND-BASED ECHELLE/DIGICON SPECTA, STARTING IN line_14: ITS RAW FORM. THEREFORE, A FLEXIBLE AND POWERFUL ARRAY OF APPROPRIATE line_15: PROGRAMS HAS BEEN THOROUGHLY TESTED AND USED. line_17: WHILE THIS NUMERICAL ANALYSIS IS STRAIGHTFORWARD AND RELATIVELY SIM- line_18: PLE, THE AMOUNT OF DATA TO BE PROCESSED AND ANALYZED WILL BE MODERATELY line_19: LARGE. THE PRINCIPAL RESPONSIBILITY FOR THIS TASK THEREFORE HAS BEEN line_20: ASSIGNED TO WELTY, WHO WILL WORK CLOSELY WITH HOBBS AND YORK. line_22: IN THE ANALYSIS OF THE INTERSTELLAR LINES, WE SHALL TAKE ADVANTAGE OF line_23: THE CONTINUING EFFORTS OF MORTON AND HIS COLLEAGUES IN COLLECTING THE ! question: 7 section: 2 line_1: BEST AVAILABLE LABORATORY DATA ON THE WAVELENGTHS AND THE OSCILLATOR line_2: STRENGTHS OF THE LINES OBSERVED. THUS, WE WILL BE ABLE TO OBTAIN THE line_3: MOST RELIABLE RADIAL VELOCITIES, COLUMN DENSITIES, AND LINE WIDTH line_4: PARAMETERS FROM THE DATA. ! question: 10 section: 1 line_1: AS INDICATED IN QUESTION 7 ABOVE, EXTENSIVE DATA-ANALYSIS CAPABILITIES line_2: WHICH ARE TAILORED PRECISELY FOR THIS KIND OF OBSERVATIONAL DATA AND line_3: ITS INTERPRETATION EXIST AT, AND WILL BE MADE AVAILABLE BY, OUR HOME line_4: INSTITUTIONS. ! !end of general form text general_form_address: lname: HOBBS fname: L. mi: M. title: PROF. category: PI inst: UNIVERSITY OF CHICAGO addr_1: YERKES OBSERVATORY city: WILLIAMS BAY state: WI zip: 531910258 country: USA ! ! end of general_form_address records fixed_targets: targnum: 5 name_1: HD035149 name_2: 23 ORI descr_1: STAR; TYPE=B1 V pos_1: RA= 05H 20M 12.191S +/- 0.05S, pos_2: DEC= +03D 29' 52.65" +/- 1.0" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: -0.001267 dec_pm_val: 0.0010 an_prlx_val: 0.0020 an_prlx_unct: 0.0050 rv_or_z: V= +18 fluxnum_1: 1 fluxval_1: V=4.99+/-0.02, TYPE=B1V, E(B-V)=0.11 fluxnum_2: 2 fluxval_2: F-CONT(1480)=8.80 E-10 fluxnum_3: 3 fluxval_3: F-CONT(1600)=6.42 E-10 fluxnum_4: 4 fluxval_4: F-CONT(2000)=4.10 E-10 fluxnum_5: 5 fluxval_5: F-CONT(2400)=3.12 E-10 ! targnum: 9 name_1: HD047839 name_2: 15 MON name_3: S MON descr_1: STAR; TYPE=O7 V pos_1: RA= 06H 38M 13.43S +/- 0.01S, pos_2: DEC= +09D 56' 37.0" +/- 0.1" equinox: 1950 pos_epoch_bj: B pos_epoch_yr: 1950.00 rv_or_z: V= +33 fluxnum_1: 1 fluxval_1: V=4.70+/-0.05, TYPE=07V, E(B-V)=0.07 fluxnum_2: 2 fluxval_2: F-CONT(1480)=2.12 E-09 fluxnum_3: 3 fluxval_3: F-CONT(1600)=1.64 E-09 fluxnum_4: 4 fluxval_4: F-CONT(2000)=1.03 E-09 fluxnum_5: 5 fluxval_5: F-CONT(2400)=6.05 E-10 ! targnum: 10 name_1: HD057061 name_2: TAU CMA descr_1: STAR; TYPE=O9 III pos_1: RA= 07H 16M 38.01S +/- 0.01S, pos_2: DEC= -24D 51' 42.5" +/- 0.1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: -0.001000 dec_pm_val: 0.0080 an_prlx_val: 0.0010 an_prlx_unct: 0.0050 rv_or_z: V= +40 acqpr_1: COMP comment_1: OBSERVE BRIGHTEST MEMBER OF BINARY fluxnum_1: 1 fluxval_1: V=4.39+/-0.05, TYPE=O9III, E(B-V)=0.17 fluxnum_2: 2 fluxval_2: F-CONT(1480)=1.90 E-09 fluxnum_3: 3 fluxval_3: F-CONT(1600)=1.41 E-09 fluxnum_4: 4 fluxval_4: F-CONT(2000)=1.01 E-09 fluxnum_5: 5 fluxval_5: F-CONT(2400)=6.56 E-10 ! targnum: 11 name_1: HD072127 descr_1: STAR; TYPE=B2 IV pos_1: RA= 08H 27M 46.39S +/- 0.01S, pos_2: DEC= -44D 33' 24.8" +/- 0.1" equinox: 1950 pos_epoch_bj: B pos_epoch_yr: 1950.00 rv_or_z: V= +22 acqpr_1: COMP comment_1: OBSERVE BRIGHTEST MEMBER OF BINARY fluxnum_1: 1 fluxval_1: V=5.22+/-0.02, TYPE=B2IV, E(B-V)=0.02 fluxnum_2: 2 fluxval_2: F-CONT(1480)=7.44 E-10 fluxnum_3: 3 fluxval_3: F-CONT(1600)=5.57 E-10 fluxnum_4: 4 fluxval_4: F-CONT(2000)=3.61 E-10 fluxnum_5: 5 fluxval_5: F-CONT(2400)=2.54 E-10 ! targnum: 12 name_1: HD091316 name_2: RHO LEO descr_1: STAR; TYPE=B1 IB pos_1: RA= 10H 30M 10.76S +/- 0.01S, pos_2: DEC= +09D 33' 52.2" +/- 0.1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: -0.000600 dec_pm_val: -0.0060 an_prlx_val: 0.0020 an_prlx_unct: 0.0050 rv_or_z: V= +42 fluxnum_1: 1 fluxval_1: V=3.85+/-0.02, TYPE=B1IB, E(B-V)=0.05 fluxnum_2: 2 fluxval_2: F-CONT(1480)=1.51 E-09 fluxnum_3: 3 fluxval_3: F-CONT(1600)=1.19 E-09 fluxnum_4: 4 fluxval_4: F-CONT(2000)=6.75 E-10 fluxnum_5: 5 fluxval_5: F-CONT(2400)=8.28 E-10 ! targnum: 14 name_1: HD141637 name_2: 1 SCO descr_1: STAR; TYPE=B2.5 V pos_1: RA= 15H 47M 57.94S +/- 0.01S, pos_2: DEC= -25D 36' 03.0" +/- 0.1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: -0.001333 dec_pm_val: -0.0270 an_prlx_val: 0.0050 an_prlx_unct: 0.0050 rv_or_z: V= +03 fluxnum_1: 1 fluxval_1: V=4.68+/-0.02, TYPE=B2.5V, E(B-V)=0.16 fluxnum_2: 2 fluxval_2: F-CONT(1480)=7.27 E-10 fluxnum_3: 3 fluxval_3: F-CONT(1600)=5.65 E-10 fluxnum_4: 4 fluxval_4: F-CONT(2000)=2.96 E-10 fluxnum_5: 5 fluxval_5: F-CONT(2400)=2.17 E-10 ! targnum: 15 name_1: HD143018 name_2: PI SCO descr_1: STAR; TYPE=B1 V pos_1: RA= 15H 55M 49.30S +/- 0.01S, pos_2: DEC= -25D 58' 18.1" +/- 0.1" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: -0.000733 dec_pm_val: -0.0270 an_prlx_val: 0.0050 an_prlx_unct: 0.0050 rv_or_z: V= -03 fluxnum_1: 1 fluxval_1: V=2.88+/-0.02, TYPE=B1V, E(B-V)=0.07 fluxnum_2: 2 fluxval_2: F-CONT(1480)=7.10 E-09 fluxnum_3: 3 fluxval_3: F-CONT(1600)=5.32 E-09 fluxnum_4: 4 fluxval_4: F-CONT(2000)=3.07 E-09 fluxnum_5: 5 fluxval_5: F-CONT(2400)=2.02 E-09 ! targnum: 17 name_1: HD212571 name_2: PI AQR descr_1: STAR; TYPE=B1 VPE; descr_2: BE STAR pos_1: RA= 22H 22M 43.381S +/- 0.05S, pos_2: DEC= +01D 07' 23.55" +/- 1.0" equinox: 1950 pm_or_par: Y pos_epoch_bj: B pos_epoch_yr: 1950.00 ra_pm_val: 0.000867 dec_pm_val: 0.0410 an_prlx_val: 0.0050 an_prlx_unct: 0.0050 rv_or_z: V= +04 fluxnum_1: 1 fluxval_1: V=4.68+/-0.04, TYPE=B1VPE, E(B-V)=0.12 fluxnum_2: 2 fluxval_2: F-CONT(1480)=1.04 E-09 fluxnum_3: 3 fluxval_3: F-CONT(1600)=7.73 E-10 fluxnum_4: 4 fluxval_4: F-CONT(2000)=4.45 E-10 fluxnum_5: 5 fluxval_5: F-CONT(2400)=3.57 E-10 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 sequence_1: DEFINE 161 targname: # config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1133.7 num_exp: 1 time_per_exp: 15.3M s_to_n: # fluxnum_1: 2 priority: # param_1: FP-SPLIT=DSFOUR req_1: SEQ 001-009 NO GAP comment_1: FE III, (3)N I, (3)FE II; comment_2: STANDARD S/N=150, NOT 200; comment_3: 161 USES IN-ORBIT RESPONSE FN ! linenum: 2.000 sequence_1: DEFINE 161 targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 1175.0 num_exp: 1 time_per_exp: 12.4M s_to_n: # fluxnum_1: 2 priority: # param_1: FP-SPLIT=FOUR comment_1: (2)N I, V II, S III ! linenum: 3.000 sequence_1: DEFINE 161 targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 1249.7 num_exp: 1 time_per_exp: 6.2M s_to_n: # fluxnum_1: 2 priority: # param_1: FP-SPLIT=DSFOUR comment_1: (2)MG II, (3)S II ! linenum: 4.000 sequence_1: DEFINE 161 targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 1290.9 num_exp: 1 time_per_exp: 6.2M s_to_n: # fluxnum_1: 2 priority: # param_1: FP-SPLIT=DSFOUR comment_1: (NUM)C I, S I, PII, O I, SI II ! linenum: 5.000 sequence_1: DEFINE 161 targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 1345.1 num_exp: 1 time_per_exp: 6.2M s_to_n: # fluxnum_1: 3 priority: # param_1: FP-SPLIT=DSFOUR comment_1: C II*, CL I, O I ! linenum: 6.000 sequence_1: DEFINE 161 targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 1398.3 num_exp: 1 time_per_exp: 6.2M s_to_n: # fluxnum_1: 3 priority: # param_1: FP-SPLIT=DSFOUR comment_1: (2)SI IV ! linenum: 7.000 sequence_1: DEFINE 161 targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 1554.3 num_exp: 1 time_per_exp: 7.3M s_to_n: # fluxnum_1: 3 priority: # param_1: FP-SPLIT=DSFOUR comment_1: (2)C IV, (NUM) C I ! linenum: 9.000 sequence_1: DEFINE 161 targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 1663.9 num_exp: 1 time_per_exp: 6.7M s_to_n: # fluxnum_1: 3 priority: # param_1: FP-SPLIT=DSFOUR comment_1: (NUM)C I, AL II ! linenum: 101.000 sequence_1: DEFINE OLB targname: # config: HRS opmode: WSCAN aperture: 0.25 sp_element: ECH-B wavelength: 1826.83-1829.05 num_exp: 1 time_per_exp: 9.0M s_to_n: # fluxnum_1: 4 priority: # param_1: WAVE-STEP=0.74 req_1: SEQ 101-107 NO GAP comment_1: MG I; comment_2: WAVE-STEP = 8 CAROUSEL STEPS; comment_3: 3 SUBEXPOSURES, EACH .74A APART; comment_4: CEN WAV=1827.20,1827.94,1828.68; comment_5: 180 SEC PER SUBEXPOSURE; comment_6: OLB USES IN-ORBIT RESPONSE FN ! linenum: 102.000 sequence_1: DEFINE OLB targname: # config: HRS opmode: WSCAN aperture: 0.25 sp_element: ECH-B wavelength: 2025.11-2027.51 num_exp: 1 time_per_exp: 4.4M s_to_n: # fluxnum_1: 4 priority: # param_1: WAVE-STEP=0.80 comment_1: MG I, ZN II; comment_2: WAVE-STEP = 8 CAROUSEL STEPS; comment_3: 3 SUBEXPOSURES, EACH .80A APART; comment_4: CEN WAV=2025.51,2026.31,2027.11; comment_5: VACUUM WAVELENGTHS; comment_6: 88 SEC PER SUBEXPOSURE ! linenum: 103.000 sequence_1: DEFINE OLB targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 2369.65-2372.41 num_exp: 1 time_per_exp: 2.5M s_to_n: # fluxnum_1: 5 priority: # param_1: WAVE-STEP=0.92 comment_1: (2)FE II; comment_2: WAVE-STEP = 8 CAROUSEL STEPS; comment_3: 3 SUBEXPOSURES, EACH .92A APART; comment_4: CEN WAV=2370.11,2371.03,2371.95; comment_5: VACUUM WAVELENGTHS; comment_6: 50 SEC PER SUBEXPOSURE ! linenum: 104.000 sequence_1: DEFINE OLB targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 1806.52-1808.80 num_exp: 1 time_per_exp: 10.8M s_to_n: # fluxnum_1: 4 priority: # param_1: WAVE-STEP=0.76 comment_1: SI II, S I; comment_2: WAVE-STEP = 8 CAROUSEL STEPS; comment_3: 3 SUBEXPOSURES, EACH .76A APART; comment_4: CEN WAV=1806.90,1807.66,1808.42; comment_5: 216 SEC PER SUBEXPOSURE ! linenum: 105.000 sequence_1: DEFINE OLB targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 2058.11-2060.81 num_exp: 1 time_per_exp: 4.7M s_to_n: # fluxnum_1: 4 priority: # param_1: WAVE-STEP=0.90 comment_1: ZN II, CR II; comment_2: WAVE-STEP = 8 CAROUSEL STEPS; comment_3: 3 SUBEXPOSURES, EACH .90A APART; comment_4: CEN WAV=2058.56,2059.46,2060.36; comment_5: VACUUM WAVELENGTHS; comment_6: 94 SEC PER SUBEXPOSURE ! linenum: 106.100 sequence_1: DEFINE OLB targname: # config: ^ opmode: ACCUM aperture: 0.25 sp_element: ^ wavelength: 2324.41 num_exp: 1 time_per_exp: 2.1M s_to_n: # fluxnum_1: 5 priority: # comment_1: C II; comment_2: VACUUM WAVELENGTH ! linenum: 106.200 sequence_1: DEFINE OLB targname: WAVE config: ^ opmode: ^ aperture: SC2 sp_element: ^ wavelength: 2324.41 num_exp: 1 time_per_exp: DEF s_to_n: 30 fluxnum_1: 1 priority: # req_1: CALIB FOR 106.100 NO SLEW comment_1: 0.25 ARCSEC APERTURE ! linenum: 106.300 sequence_1: DEFINE OLB targname: # config: ^ opmode: ^ aperture: 0.25 sp_element: ^ wavelength: 2325.40 num_exp: 1 time_per_exp: 2.1M s_to_n: # fluxnum_1: 5 priority: # comment_1: C II; comment_2: VACUUM WAVELENGTH ! linenum: 106.400 sequence_1: DEFINE OLB targname: WAVE config: ^ opmode: ^ aperture: SC2 sp_element: ^ wavelength: 2325.40 num_exp: 1 time_per_exp: DEF s_to_n: 30 fluxnum_1: 1 priority: # req_1: CALIB FOR 106.300 NO SLEW comment_1: 0.25 ARCSEC APERTURE ! linenum: 106.500 sequence_1: DEFINE OLB targname: # config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2326.39 num_exp: 1 time_per_exp: 2.1M s_to_n: # fluxnum_1: 5 priority: # comment_1: C II; comment_2: VACUUM WAVELENGTH ! linenum: 106.600 sequence_1: DEFINE OLB targname: WAVE config: ^ opmode: ^ aperture: SC2 sp_element: ^ wavelength: 2326.39 num_exp: 1 time_per_exp: DEF s_to_n: 30 fluxnum_1: 1 priority: # req_1: CALIB FOR 106.500 NO SLEW comment_1: 0.25 ARCSEC APERTURE ! linenum: 107.000 sequence_1: DEFINE OLB targname: # config: HRS opmode: WSCAN aperture: 0.25 sp_element: ECH-B wavelength: 1743.56-1745.78 num_exp: 1 time_per_exp: 9.0M s_to_n: # fluxnum_1: 3 priority: # param_1: WAVE-STEP=0.74 comment_1: MG I, NI II; comment_2: WAVE-STEP = 8 CAROUSEL STEPS; comment_3: 3 SUBEXPOSURES, EACH .74A APART; comment_4: CEN WAV=1743.93,1744.67,1745.41; comment_5: 180 SEC PER SUBEXPOSURE; comment_6: STANDARD S/N=80, NOT 100 ! linenum: 201.100 sequence_1: DEFINE AUX targname: # config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2324.31 num_exp: 1 time_per_exp: 2.1M s_to_n: # fluxnum_1: 5 priority: # req_1: SEQ 201.1-203.6 NO GAP comment_1: C II; comment_2: VACUUM WAVELENGTH; comment_3: AUX USES IN-ORBIT RESPONSE FN ! linenum: 201.200 sequence_1: DEFINE AUX targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2324.31 num_exp: 1 time_per_exp: DEF s_to_n: 30 fluxnum_1: 1 priority: # req_1: CALIB FOR 201.100 NO SLEW comment_1: 0.25 ARCSEC APERTURE ! linenum: 201.300 sequence_1: DEFINE AUX targname: # config: ^ opmode: ^ aperture: 0.25 sp_element: ^ wavelength: 2325.30 num_exp: 1 time_per_exp: 2.1M s_to_n: # fluxnum_1: 5 priority: # comment_1: C II; comment_2: VACUUM WAVELENGTH ! linenum: 201.400 sequence_1: DEFINE AUX targname: WAVE config: ^ opmode: ^ aperture: SC2 sp_element: ^ wavelength: 2325.30 num_exp: 1 time_per_exp: DEF s_to_n: 30 fluxnum_1: 1 priority: # req_1: CALIB FOR 201.300 NO SLEW comment_1: 0.25 ARCSEC APERTURE ! linenum: 201.500 sequence_1: DEFINE AUX targname: # config: ^ opmode: ^ aperture: 0.25 sp_element: ^ wavelength: 2326.29 num_exp: 1 time_per_exp: 2.1M s_to_n: # fluxnum_1: 5 priority: # comment_1: C II; comment_2: VACUUM WAVELENGTH ! linenum: 201.600 sequence_1: DEFINE AUX targname: WAVE config: ^ opmode: ^ aperture: SC2 sp_element: ^ wavelength: 2326.29 num_exp: 1 time_per_exp: DEF s_to_n: 30 fluxnum_1: 1 priority: # req_1: CALIB FOR 201.500 NO SLEW comment_1: 0.25 ARCSEC APERTURE ! linenum: 203.100 sequence_1: DEFINE AUX targname: # config: ^ opmode: ^ aperture: 0.25 sp_element: ^ wavelength: 2324.51 num_exp: 1 time_per_exp: 2.1M s_to_n: # fluxnum_1: 5 priority: # comment_1: C II; comment_2: VACUUM WAVELENGTH ! linenum: 203.200 sequence_1: DEFINE AUX targname: WAVE config: ^ opmode: ^ aperture: SC2 sp_element: ^ wavelength: 2324.51 num_exp: 1 time_per_exp: DEF s_to_n: 30 fluxnum_1: 1 priority: # req_1: CALIB FOR 203.100 NO SLEW comment_1: 0.25 ARCSEC APERTURE ! linenum: 203.300 sequence_1: DEFINE AUX targname: # config: ^ opmode: ^ aperture: 0.25 sp_element: ^ wavelength: 2325.50 num_exp: 1 time_per_exp: 2.1M s_to_n: # fluxnum_1: 5 priority: # comment_1: C II; comment_2: VACUUM WAVELENGTH ! linenum: 203.400 sequence_1: DEFINE AUX targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2325.50 num_exp: 1 time_per_exp: DEF s_to_n: 30 fluxnum_1: 1 priority: # req_1: CALIB FOR 203.300 NO SLEW comment_1: 0.25 ARCSEC APERTURE ! linenum: 203.500 sequence_1: DEFINE AUX targname: # config: ^ opmode: ^ aperture: 0.25 sp_element: ^ wavelength: 2326.49 num_exp: 1 time_per_exp: 2.1M s_to_n: # fluxnum_1: 5 priority: # comment_1: C II; comment_2: VACUUM WAVELENGTH ! linenum: 203.600 sequence_1: DEFINE AUX targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2326.49 num_exp: 1 time_per_exp: DEF s_to_n: 30 fluxnum_1: 1 priority: # req_1: CALIB FOR 203.500 NO SLEW comment_1: 0.25 ARCSEC APERTURE ! linenum: 301.000 sequence_1: DEFINE 160 targname: # config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1133.7 num_exp: 1 time_per_exp: 15.3M s_to_n: # fluxnum_1: 2 priority: # param_1: FP-SPLIT=DSFOUR param_2: STEP-PATT=5 req_1: SEQ 301-309 NO GAP comment_1: FE III, (3)N I, (3)FE II; comment_2: STANDARD S/N=150, NOT 200; comment_3: 160 USES IN-ORBIT RESPONSE FN ! linenum: 302.000 sequence_1: DEFINE 160 targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 1175.0 num_exp: 1 time_per_exp: 12.4M s_to_n: # fluxnum_1: 2 priority: # param_1: FP-SPLIT=FOUR param_2: STEP-PATT=5 comment_1: (2)N I, V II, S III ! linenum: 303.000 sequence_1: DEFINE 160 targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 1249.7 num_exp: 1 time_per_exp: 3.7M s_to_n: # fluxnum_1: 2 priority: # param_1: FP-SPLIT=DSFOUR param_2: STEP-PATT=5 comment_1: (2)MG II, (3)S II ! linenum: 304.000 sequence_1: DEFINE 160 targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 1290.9 num_exp: 1 time_per_exp: 2.8M s_to_n: # fluxnum_1: 2 priority: # param_1: FP-SPLIT=DSFOUR param_2: STEP-PATT=5 comment_1: (NUM)C I, S I, PII, O I, SI II ! linenum: 305.000 sequence_1: DEFINE 160 targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 1345.1 num_exp: 1 time_per_exp: 3.3M s_to_n: # fluxnum_1: 3 priority: # param_1: FP-SPLIT=DSFOUR param_2: STEP-PATT=5 comment_1: C II*, CL I, O I ! linenum: 306.000 sequence_1: DEFINE 160 targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 1398.3 num_exp: 1 time_per_exp: 4.8M s_to_n: # fluxnum_1: 3 priority: # param_1: FP-SPLIT=DSFOUR param_2: STEP-PATT=5 comment_1: (2)SI IV ! linenum: 307.000 sequence_1: DEFINE 160 targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 1554.3 num_exp: 1 time_per_exp: 7.3M s_to_n: # fluxnum_1: 3 priority: # param_1: FP-SPLIT=DSFOUR param_2: STEP-PATT=5 comment_1: (2)C IV, (NUM) C I ! linenum: 308.000 sequence_1: DEFINE 160 targname: # config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1608.5 num_exp: 1 time_per_exp: 6.8M s_to_n: # fluxnum_1: 3 priority: # param_1: FP-SPLIT=DSFOUR param_2: STEP-PATT=5 comment_1: FE II ! linenum: 309.000 sequence_1: DEFINE 160 targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 1663.9 num_exp: 1 time_per_exp: 6.7M s_to_n: # fluxnum_1: 3 priority: # param_1: FP-SPLIT=DSFOUR param_2: STEP-PATT=5 comment_1: (NUM)C I, AL II ! linenum: 401.000 sequence_1: DEFINE NEB targname: # config: HRS opmode: WSCAN aperture: 0.25 sp_element: ECH-B wavelength: 1857.56-1859.96 num_exp: 1 time_per_exp: 8.6M s_to_n: # fluxnum_1: 4 priority: # param_1: WAVE-STEP=0.80 req_1: SEQ 401-405 NO GAP comment_1: (2) AL III; comment_2: WAVE-STEP = 8 CAROUSEL STEPS; comment_3: 3 SUBEXPOSURES, EACH .80A APART; comment_4: CEN WAV=1857.96,1858.76,1859.56; comment_5: 172 SEC PER SUBEXPOSURE; comment_6: NEB USES IN-ORBIT RESPONSE FN ! linenum: 402.000 sequence_1: DEFINE NEB targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 2248.50-2251.26 num_exp: 1 time_per_exp: 1.9M s_to_n: # fluxnum_1: 5 priority: # param_1: WAVE-STEP=0.92 comment_1: (1) FE II; comment_2: WAVE-STEP = 8 CAROUSEL STEPS; comment_3: 3 SUBEXPOSURES, EACH .92A APART; comment_4: CEN WAV=2248.96,2249.88,2250.80; comment_5: VACUUM WAVELENGTHS; comment_6: 38 SEC PER SUBEXPOSURE ! linenum: 403.000 sequence_1: DEFINE NEB targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 2482.58-2485.46 num_exp: 1 time_per_exp: 3.2M s_to_n: # fluxnum_1: 5 priority: # param_1: WAVE-STEP=0.96 comment_1: FE I; comment_2: WAVE-STEP = 8 CAROUSEL STEPS; comment_3: 3 SUBEXPOSURES, EACH .96A APART; comment_4: CEN WAV=2483.06,2484.02,2484.98; comment_5: VACUUM WAVELENGTHS; comment_6: 64 SEC PER SUBEXPOSURE ! linenum: 404.000 sequence_1: DEFINE NEB targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 2517.69-2520.99 num_exp: 1 time_per_exp: 3.5M s_to_n: # fluxnum_1: 5 priority: # param_1: WAVE-STEP=1.10 comment_1: FE I, SI I; comment_2: WAVE-STEP = 8 CAROUSEL STEPS; comment_3: 3 SUBEXPOSURES, EACH 1.1A APART; comment_4: CEN WAV=2518.24,2519.34,2520.44; comment_5: VACUUM WAVELENGTHS; comment_6: 70 SEC PER SUBEXPOSURE ! linenum: 405.000 sequence_1: DEFINE NEB targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 2798.17-2801.71 num_exp: 1 time_per_exp: 2.2M s_to_n: # fluxnum_1: 5 priority: # param_1: WAVE-STEP=1.18 comment_1: (2) MG II; comment_2: WAVE-STEP = 8 CAROUSEL STEPS; comment_3: 3 SUBEXPOSURES, EACH 1.18A APART; comment_4: CEN WAV=2798.76,2799.94,2801.12; comment_5: VACUUM WAVELENGTHS; comment_6: 44 SEC PER SUBEXPOSURE ! linenum: 509.100 targname: HD047839 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 5S s_to_n: 175 fluxnum_1: 3 priority: 1 param_1: SEARCH-SIZE=5 param_2: FAINT=6600 param_3: LOCATE=YES req_1: ONBOARD ACQ FOR 509.2; req_2: SEQ 509.1-509.5 NO GAP; req_3: CYCLE 1 / 509.1-515.7 comment_1: STEP-TIME = 0.2 SEC; comment_2: 15 MON ! linenum: 509.200 targname: HD047839 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 9.2S fluxnum_1: 3 priority: 1 req_1: ONBOARD ACQ FOR 509.3-509.5 comment_1: STEP-TIME = 0.2 SEC; comment_2: 15 MON ! linenum: 509.300 targname: HD047839 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 96.8S fluxnum_1: 3 priority: 1 comment_1: STEP-TIME = 0.2 SEC; comment_2: TAKE MAP AFTER CENTERING; comment_3: 15 MON ! linenum: 509.400 sequence_1: USE OLB targname: HD047839 time_per_exp: X0.53 s_to_n: 100 priority: 1 comment_1: 15 MON ! linenum: 509.500 sequence_1: USE NEB targname: HD047839 time_per_exp: X0.53 s_to_n: 100 priority: 1 comment_1: 15 MON ! linenum: 509.510 targname: HD047839 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 5S s_to_n: 175 fluxnum_1: 3 priority: 1 param_1: SEARCH-SIZE=5 param_2: FAINT=6600 param_3: LOCATE=YES req_1: ONBOARD ACQ FOR 509.52; req_2: SEQ 509.51-509.6 NO GAP; comment_1: STEP-TIME = 0.2 SEC; comment_2: 15 MON ! linenum: 509.520 targname: HD047839 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 9.2S fluxnum_1: 3 priority: 1 req_1: ONBOARD ACQ FOR 509.53-509.6 comment_1: STEP-TIME = 0.2 SEC; comment_2: 15 MON ! linenum: 509.530 targname: HD047839 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 96.8S fluxnum_1: 3 priority: 1 comment_1: STEP-TIME = 0.2 SEC; comment_2: TAKE MAP AFTER CENTERING; comment_3: 15 MON ! linenum: 509.600 sequence_1: USE 160 targname: HD047839 time_per_exp: X0.65 s_to_n: 200 priority: 1 comment_1: 15 MON ! linenum: 510.100 targname: HD057061 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 5S s_to_n: 175 fluxnum_1: 3 priority: 1 param_1: SEARCH-SIZE=5 param_2: FAINT=6100 param_3: LOCATE=YES req_1: ONBOARD ACQ FOR 510.2; req_2: SEQ 510.1-510.5 NO GAP comment_1: STEP-TIME = 0.2 SEC; comment_2: TAU CMA ! linenum: 510.200 targname: HD057061 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 9.2S fluxnum_1: 3 priority: 1 req_1: ONBOARD ACQ FOR 510.3-510.5 comment_1: STEP-TIME = 0.2 SEC; comment_2: TAU CMA ! linenum: 510.300 targname: HD057061 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 96.8S fluxnum_1: 3 priority: 1 comment_1: STEP-TIME = 0.2 SEC; comment_2: TAKE MAP AFTER CENTERING; comment_3: TAU CMA ! linenum: 510.400 sequence_1: USE OLB targname: HD057061 time_per_exp: X0.59 s_to_n: 100 priority: 1 comment_1: TAU CMA ! linenum: 510.500 sequence_1: USE AUX targname: HD057061 time_per_exp: X0.59 s_to_n: 100 priority: 1 comment_1: TAU CMA ! linenum: 510.510 targname: HD057061 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 5S s_to_n: 175 fluxnum_1: 3 priority: 1 param_1: SEARCH-SIZE=5 param_2: FAINT=6100 param_3: LOCATE=YES req_1: ONBOARD ACQ FOR 510.52; req_2: SEQ 510.51-510.7 NO GAP comment_1: STEP-TIME = 0.2 SEC; comment_2: TAU CMA ! linenum: 510.520 targname: HD057061 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 9.2S fluxnum_1: 3 priority: 1 req_1: ONBOARD ACQ FOR 510.53-510.7 comment_1: STEP-TIME = 0.2 SEC; comment_2: TAU CMA ! linenum: 510.530 targname: HD057061 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 96.8S fluxnum_1: 3 priority: 1 comment_1: STEP-TIME = 0.2 SEC; comment_2: TAKE MAP AFTER CENTERING; comment_3: TAU CMA ! linenum: 510.600 sequence_1: USE NEB targname: HD057061 time_per_exp: X0.59 s_to_n: 100 priority: 1 comment_1: TAU CMA ! linenum: 510.700 sequence_1: USE 160 targname: HD057061 time_per_exp: X0.65 s_to_n: 200 priority: 1 comment_1: TAU CMA ! linenum: 512.100 targname: HD091316 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 5S s_to_n: 170 fluxnum_1: 3 priority: 1 param_1: SEARCH-SIZE=5 param_2: FAINT=5800 param_3: LOCATE=YES req_1: ONBOARD ACQ FOR 512.2; req_2: SEQ 512.1-512.5 NO GAP comment_1: STEP-TIME = 0.2 SEC; comment_2: RHO LEO ! linenum: 512.200 targname: HD091316 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 9.2S fluxnum_1: 3 priority: 1 req_1: ONBOARD ACQ FOR 512.3-512.5 comment_1: STEP-TIME = 0.2 SEC; comment_2: RHO LEO ! linenum: 512.300 targname: HD091316 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 96.8S fluxnum_1: 3 priority: 1 comment_1: STEP-TIME = 0.2 SEC; comment_2: TAKE MAP AFTER CENTERING; comment_3: RHO LEO ! linenum: 512.400 sequence_1: USE OLB targname: HD091316 time_per_exp: X0.75 s_to_n: 100 priority: 1 comment_1: RHO LEO ! linenum: 512.500 sequence_1: USE NEB targname: HD091316 time_per_exp: X0.75 s_to_n: 100 priority: 1 comment_1: RHO LEO ! linenum: 512.510 targname: HD091316 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 5S s_to_n: 170 fluxnum_1: 3 priority: 1 param_1: SEARCH-SIZE=5 param_2: FAINT=5800 param_3: LOCATE=YES req_1: ONBOARD ACQ FOR 512.52; req_2: SEQ 512.51-512.6 NO GAP comment_1: STEP-TIME = 0.2 SEC; comment_2: RHO LEO ! linenum: 512.520 targname: HD091316 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 9.2S fluxnum_1: 3 priority: 1 req_1: ONBOARD ACQ FOR 512.53-512.6 comment_1: STEP-TIME = 0.2 SEC; comment_2: RHO LEO ! linenum: 512.530 targname: HD091316 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 96.8S fluxnum_1: 3 priority: 1 comment_1: STEP-TIME = 0.2 SEC; comment_2: TAKE MAP AFTER CENTERING; comment_3: RHO LEO ! linenum: 512.600 sequence_1: USE 160 targname: HD091316 time_per_exp: X0.75 s_to_n: 200 priority: 1 comment_1: RHO LEO ! linenum: 515.100 targname: HD143018 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 5S s_to_n: 300 fluxnum_1: 3 priority: 1 param_1: SEARCH-SIZE=5 param_2: FAINT=20000 param_3: LOCATE=YES req_1: ONBOARD ACQ FOR 515.2; req_2: SEQ 515.1-515.7 NO GAP comment_1: STEP-TIME = 0.2 SEC; comment_2: PI SCO ! linenum: 515.200 targname: HD143018 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 9.2S fluxnum_1: 3 priority: 1 req_1: ONBOARD ACQ FOR 515.3-515.7 comment_1: STEP-TIME = 0.2 SEC; comment_2: PI SCO ! linenum: 515.300 targname: HD143018 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 96.8S fluxnum_1: 3 priority: 1 comment_1: STEP-TIME = 0.2 SEC; comment_2: TAKE MAP AFTER CENTERING; comment_3: PI SCO ! linenum: 515.700 sequence_1: USE 161 targname: HD143018 time_per_exp: X0.16 s_to_n: 200 priority: 1 comment_1: PI SCO ! linenum: 705.100 targname: HD035149 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 5S s_to_n: 120 fluxnum_1: 3 priority: 1 param_1: SEARCH-SIZE=5 param_2: FAINT=2500 param_3: LOCATE=YES req_1: ONBOARD ACQ FOR 705.2; req_2: SEQ 705.1-705.5 NO GAP; req_3: CYCLE 1 / 705.1-717.5 comment_1: STEP-TIME = 0.2 SEC; comment_2: 23 ORI ! linenum: 705.200 targname: HD035149 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 9.2S fluxnum_1: 3 priority: 1 req_1: ONBOARD ACQ FOR 705.3-705.5 comment_1: STEP-TIME = 0.2 SEC; comment_2: 23 ORI ! linenum: 705.300 targname: HD035149 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 96.8S fluxnum_1: 3 priority: 1 comment_1: STEP-TIME = 0.2 SEC; comment_2: TAKE MAP AFTER CENTERING; comment_3: 23 ORI ! linenum: 705.400 sequence_1: USE 160 targname: HD035149 time_per_exp: X1.29 s_to_n: 200 priority: 1 comment_1: 23 ORI ! linenum: 705.500 sequence_1: USE NEB targname: HD035149 time_per_exp: X1.29 s_to_n: 100 priority: 1 comment_1: 23 ORI ! linenum: 711.100 targname: HD072127 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 5S s_to_n: 95 fluxnum_1: 3 priority: 1 param_1: SEARCH-SIZE=5 param_2: FAINT=2400 param_3: LOCATE=YES req_1: ONBOARD ACQ FOR 711.2; req_2: SEQ 711.1-711.5 NO GAP comment_1: STEP-TIME = 0.2 SEC; comment_2: HD 72127 ! linenum: 711.200 targname: HD072127 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 9.2S fluxnum_1: 3 priority: 1 req_1: ONBOARD ACQ FOR 711.3-711.5 comment_1: STEP-TIME = 0.2 SEC; comment_2: HD 72127 ! linenum: 711.300 targname: HD072127 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 96.8S fluxnum_1: 3 priority: 1 comment_1: STEP-TIME = 0.2 SEC; comment_2: TAKE MAP AFTER CENTERING; comment_3: HD 72127 ! linenum: 711.400 sequence_1: USE 160 targname: HD072127 time_per_exp: X1.52 s_to_n: 200 priority: 1 comment_1: HD 72127 ! linenum: 711.500 sequence_1: USE NEB targname: HD072127 time_per_exp: X1.52 s_to_n: 100 priority: 1 comment_1: HD 72127 ! linenum: 714.100 targname: HD141637 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 5S s_to_n: 95 fluxnum_1: 3 priority: 1 param_1: SEARCH-SIZE=5 param_2: FAINT=2200 param_3: LOCATE=YES req_1: ONBOARD ACQ FOR 714.2; req_2: SEQ 714.1-714.5 NO GAP comment_1: STEP-TIME = 0.2 SEC; comment_2: 1 SCO ! linenum: 714.200 targname: HD141637 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 9.2S fluxnum_1: 3 priority: 1 req_1: ONBOARD ACQ FOR 714.3-714.5 comment_1: STEP-TIME = 0.2 SEC; comment_2: 1 SCO ! linenum: 714.300 targname: HD141637 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 96.8S fluxnum_1: 3 priority: 1 comment_1: STEP-TIME = 0.2 SEC; comment_2: TAKE MAP AFTER CENTERING; comment_3: 1 SCO ! linenum: 714.400 sequence_1: USE 160 targname: HD141637 time_per_exp: X1.59 s_to_n: 200 priority: 1 comment_1: 1 SCO ! linenum: 714.500 sequence_1: USE NEB targname: HD141637 time_per_exp: X1.59 s_to_n: 100 priority: 1 comment_1: 1 SCO ! linenum: 717.100 targname: HD212571 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 5S s_to_n: 100 fluxnum_1: 3 priority: 1 param_1: SEARCH-SIZE=5 param_2: FAINT=3200 param_3: LOCATE=YES req_1: ONBOARD ACQ FOR 717.2; req_2: SEQ 717.1-717.5 NO GAP comment_1: STEP-TIME = 0.2 SEC; comment_2: PI AQR ! linenum: 717.200 targname: HD212571 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 9.2S fluxnum_1: 3 priority: 1 req_1: ONBOARD ACQ FOR 717.3-717.5 comment_1: STEP-TIME = 0.2 SEC; comment_2: PI AQR ! linenum: 717.300 targname: HD212571 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 96.8S fluxnum_1: 3 priority: 1 comment_1: STEP-TIME = 0.2 SEC; comment_2: TAKE MAP AFTER CENTERING; comment_3: PI AQR ! linenum: 717.400 sequence_1: USE 160 targname: HD212571 time_per_exp: X1.09 s_to_n: 200 priority: 1 comment_1: PI AQR ! linenum: 717.500 sequence_1: USE NEB targname: HD212571 time_per_exp: X1.09 s_to_n: 100 priority: 1 comment_1: PI AQR ! ! end of exposure logsheet ! 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