! File: 3993C.PROP ! Database: PEPDB ! Date: 20-FEB-1994:03:01:17 coverpage: title_1: THE PROPERTIES OF SINGLE INTERSTELLAR CLOUDS: title_2: CYCLE 1, SIDE-2 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: 9.06 num_pri: 4 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 GRATING 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: 2251; THE PROGRAM EUNUMERATED HERE CONSISTS OF THAT PART OF OUR ORIGINAL line_15: PROGRAM WHICH CAN BE CARRIED OUT USING ONLY SIDE 2 OF THE GHRS. THIS PROGRAM line_16: THEREFORE CONSISTS OF ECH-B OBSERVATIONS OF EACH OF 4 STARS AT 7 line_17: WAVELENGTHS. PROGRAM 2251 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 4 STARS, A SERIES OF 7 OR 8 EXPOSURES IS TO BE OBTAINED line_2: THROUGH THE SMALL SCIENCE APERTURE IN THE WSCAN MODE, WITH THE ECHELLE line_3: GRATING. SEVEN OBSERVATIONS, TYPICALLY OF ABOUT FOUR MINUTES EACH, ARE line_4: MADE IN THE ECH-B MODE (I.E. WITH THE CsTe DIGICON) IN THE WAVELENGTH line_5: INTERVAL BETWEEN 1740 AND 2380 ANGSTROMS. ONE ADDITIONAL SET OF line_6: EXPOSURES IS OBTAINED AT ONE OF THESE WAVELENGTHS FOR 2 OF THE STARS. line_7: THE VARIOUS EXPOSURE TIMES ARE CHOSEN TO YIELD APPROXIMATELY 10,000 line_8: COUNTS PER DIODE. FOR EACH SPECTRAL SETTING, THREE SEPARATE line_9: SUBEXPOSURES WILL BE MADE, WITH THE SPECTRUM MOVED PARALLEL TO THE line_10: DISPERSION TO THREE DIFFERENT POSITIONS ON THE PHOTOCATHODE, TO ALLOW line_11: SOME CORRECTION FOR NON-UNIFORMITIES OF THE CATHODE. ! 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 FULL OBSERVING PROGRAM IS line_10: CONTAINED IN APPROVED PROPOSAL ID = 2251; THE PROGRAM EUNUMERATED HERE line_11: CONSISTS OF THAT PART OF 2251 WHICH CAN BE CARRIED OUT USING ONLY SIDE line_12: 2 OF THE GHRS. THIS PROGRAM THEREFORE CONSISTS OF ECH-B OBSERVATIONS line_13: OF EACH OF 4 STARS AT 7 WAVELENGTHS. PROGRAM 2251 SHOULD BE CONSULTED line_14: FOR ADDITIONAL DETAILS; BEFORE 2251 IS SUBSEQUENTLY EXECUTED, HOWEVER, line_15: IT MUST BE MODIFIED IN ACCORDANCE WITH THIS PROGRAM AND WITH THE line_16: LIMITATIONS IMPOSED BY THE CURRENT FAILURE OF SIDE 1 OF THE line_17: SPECTROGRAPH. ! 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 ALL OF THE line_5: 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: THE REGIONS CENTERED NEAR THE FOLLOWING SPECTRAL LINES ARE TO BE line_12: OBSERVED: Mg I 1747.8, Si II 1808.0, Mg I 1827.9, Mg I 2025.8, line_13: ZN II 2062.0, C II 2324.7, AND FE II 2366.9. AT LEAST ONE ADDITIONAL line_14: LINE NOT LISTED HERE WHICH IS OF IMPORTANCE TO OUR INVESTIGATION WILL line_15: BE RECORDED SIMULTANEOUSLY IN NEARLY ALL EXPOSURES; AN EXAMPLE IS line_16: ZN II 2025.5. line_18: AS AN EXAMPLE, CONSIDER THE OBSERVATION OF THE 1827.9 A LINE OF Mg I line_19: IN THE SPECTRUM OF HD72127. FROM JAMAR ET AL, THE INCIDENT FLUX IS F = line_20: 4.89(-10) ERG/S/CM2/A; FROM THE GHRS HANDBOOK, A SENSITIVITY OF S = ! question: 5 section: 2 line_1: 8.2(+10) (COUNT/DIODE/S)/(ERG/S/CM2/A) APPLIES TO THE OTA + 0.25 line_2: ARCSEC APERTURE + GHRS SYSTEM. IN AN INTEGRATION TIME T = 81 SEC, line_3: THEREFORE, FxSxT = 3250 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 243 SEC = 4.1 MIN, ALMOST ALL DIODES WILL line_6: RECORD ABOUT 10,000 COUNTS, AS DESIRED. THE TOTAL EXPOSURE TIME line_7: UTILIZED FOR HD 72127 AT 7 SUCH SPECTRAL LINES WORKS OUT SIMILARLY TO line_8: BE 53 MIN. ! question: 6 section: 1 line_1: IN ADDITION TO THE 7 STELLAR EXPOSURES DESCRIBED ABOVE, ONE OBSERVA- line_2: TION OF THE ONBOARD PT/NE CALIBRATION LAMP WILL TYPICALLY BE line_3: REQUIRED FOR EACH STAR, UNDER INSTRUMENTAL SETUPS IDENTICAL TO THOSE line_4: FOR 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: 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: 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: 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: 101.000 sequence_1: DEFINE FUL targname: # config: HRS opmode: WSCAN aperture: 0.25 sp_element: ECH-B wavelength: 1826.83-1829.05 num_exp: 1 time_per_exp: 81S 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: 27 SEC PER SUBEXPOSURE ! linenum: 102.000 sequence_1: DEFINE FUL targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 2025.11-2027.51 num_exp: 1 time_per_exp: 57S 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: 19 SEC PER SUBEXPOSURE ! linenum: 103.000 sequence_1: DEFINE FUL targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 2369.65-2372.41 num_exp: 1 time_per_exp: 36S 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: 12 SEC PER SUBEXPOSURE ! linenum: 104.000 sequence_1: DEFINE FUL targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 1806.52-1808.80 num_exp: 1 time_per_exp: 69S 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: 23 SEC PER SUBEXPOSURE ! linenum: 105.000 sequence_1: DEFINE FUL targname: # config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 2058.11-2060.81 num_exp: 1 time_per_exp: 57S 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: 19 SEC PER SUBEXPOSURE ! linenum: 106.100 sequence_1: DEFINE FUL targname: # config: ^ opmode: ACCUM aperture: 0.25 sp_element: ^ wavelength: 2324.41 num_exp: 1 time_per_exp: 22S s_to_n: # fluxnum_1: 5 priority: # comment_1: C II; comment_2: STANDARD S/N=141, NOT 100; comment_3: VACUUM WAVELENGTH ! linenum: 106.200 sequence_1: DEFINE FUL 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 FUL targname: # config: ^ opmode: ^ aperture: 0.25 sp_element: ^ wavelength: 2325.40 num_exp: 1 time_per_exp: 22S s_to_n: # fluxnum_1: 5 priority: # comment_1: C II; comment_2: STANDARD S/N=141, NOT 100; comment_3: VACUUM WAVELENGTH ! linenum: 106.400 sequence_1: DEFINE FUL 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 FUL targname: # config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B wavelength: 2326.39 num_exp: 1 time_per_exp: 22S s_to_n: # fluxnum_1: 5 priority: # comment_1: C II; comment_2: STANDARD S/N=141, NOT 100; comment_3: VACUUM WAVELENGTH ! linenum: 106.600 sequence_1: DEFINE FUL 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 FUL targname: # config: ^ opmode: WSCAN aperture: 0.25 sp_element: ^ wavelength: 1743.56-1745.78 num_exp: 1 time_per_exp: 102S 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: 34 SEC PER SUBEXPOSURE ! 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: 22S s_to_n: # fluxnum_1: 5 priority: # req_1: SEQ 201.1-203.6 NO GAP comment_1: C II; comment_2: VACUUM WAVELENGTH ! 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: 22S 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: 22S 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: 202.100 sequence_1: DEFINE AUX targname: # config: ^ opmode: ^ aperture: 0.25 sp_element: ^ wavelength: 2324.41 num_exp: 1 time_per_exp: 22S s_to_n: # fluxnum_1: 5 priority: # comment_1: C II; comment_2: VACUUM WAVELENGTH ! linenum: 202.200 sequence_1: DEFINE AUX targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2324.41 num_exp: 1 time_per_exp: DEF s_to_n: 30 fluxnum_1: 1 priority: # req_1: CALIB FOR 202.100 NO SLEW comment_1: 0.25 ARCSEC APERTURE ! linenum: 202.300 sequence_1: DEFINE AUX targname: # config: ^ opmode: ^ aperture: 0.25 sp_element: ^ wavelength: 2325.40 num_exp: 1 time_per_exp: 22S s_to_n: # fluxnum_1: 5 priority: # comment_1: C II; comment_2: VACUUM WAVELENGTH ! linenum: 202.400 sequence_1: DEFINE AUX 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 202.300 NO SLEW comment_1: 0.25 ARCSEC APERTURE ! linenum: 202.500 sequence_1: DEFINE AUX targname: # config: ^ opmode: ^ aperture: 0.25 sp_element: ^ wavelength: 2326.39 num_exp: 1 time_per_exp: 22S s_to_n: # fluxnum_1: 5 priority: # comment_1: C II; comment_2: VACUUM WAVELENGTH ! linenum: 202.600 sequence_1: DEFINE AUX targname: WAVE config: HRS opmode: ACCUM aperture: SC2 sp_element: ECH-B wavelength: 2326.39 num_exp: 1 time_per_exp: DEF s_to_n: 30 fluxnum_1: 1 priority: # req_1: CALIB FOR 202.500 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: 22S 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: 22S 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: ^ opmode: ^ aperture: SC2 sp_element: ^ 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: 22S 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: 505.100 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=4700 param_3: LOCATE=YES req_1: ONBOARD ACQ FOR 505.2; req_2: SEQ 505.1-505.4 NO GAP; req_3: CYCLE 1 / 505.1-517.4 comment_1: STEP-TIME = 0.2 SEC; comment_2: 23 ORI ! linenum: 505.200 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 505.3-505.4 comment_1: STEP-TIME = 0.2 SEC; comment_2: 23 ORI ! linenum: 505.300 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: 505.400 sequence_1: USE FUL targname: HD035149 time_per_exp: X5.85 s_to_n: 100 priority: 1 comment_1: 23 ORI ! linenum: 511.100 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=2900 param_3: LOCATE=YES req_1: ONBOARD ACQ FOR 511.2; req_2: SEQ 511.1-511.4 NO GAP comment_1: STEP-TIME = 0.2 SEC; comment_2: HD 72127 ! linenum: 511.200 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 511.3-511.4 comment_1: STEP-TIME = 0.2 SEC; comment_2: HD 72127 ! linenum: 511.300 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: 511.400 sequence_1: USE FUL targname: HD072127 time_per_exp: X6.75 s_to_n: 100 priority: 1 comment_1: HD 72127 ! linenum: 514.100 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=3500 param_3: LOCATE=YES req_1: ONBOARD ACQ FOR 514.2; req_2: SEQ 514.1-514.4 NO GAP comment_1: STEP-TIME = 0.2 SEC; comment_2: 1 SCO ! linenum: 514.200 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 514.3-514.4 comment_1: STEP-TIME = 0.2 SEC; comment_2: 1 SCO ! linenum: 514.300 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: 514.400 sequence_1: USE FUL targname: HD141637 time_per_exp: X7.20 s_to_n: 100 priority: 1 comment_1: 1 SCO ! linenum: 517.100 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=4650 param_3: LOCATE=YES req_1: ONBOARD ACQ FOR 517.2; req_2: SEQ 517.1-517.4 NO GAP comment_1: STEP-TIME = 0.2 SEC; comment_2: PI AQR ! linenum: 517.200 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 517.3-517.4 comment_1: STEP-TIME = 0.2 SEC; comment_2: PI AQR ! linenum: 517.300 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: 517.400 sequence_1: USE FUL targname: HD212571 time_per_exp: X4.95 s_to_n: 100 priority: 1 comment_1: PI AQR ! linenum: 605.100 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=4700 param_3: LOCATE=YES req_1: ONBOARD ACQ FOR 605.2; req_2: SEQ 605.1-605.5 NO GAP; req_3: CYCLE 1 / 605.1-614.5 comment_1: STEP-TIME = 0.2 SEC; comment_2: 23 ORI ! linenum: 605.200 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 605.3-605.5 comment_1: STEP-TIME = 0.2 SEC; comment_2: 23 ORI ! linenum: 605.300 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: 605.500 sequence_1: USE AUX targname: HD035149 time_per_exp: X5.85 s_to_n: 141 priority: 1 comment_1: 23 ORI ! linenum: 614.100 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=3500 param_3: LOCATE=YES req_1: ONBOARD ACQ FOR 614.2; req_2: SEQ 614.1-614.5 NO GAP comment_1: STEP-TIME = 0.2 SEC; comment_2: 1 SCO ! linenum: 614.200 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 614.3-614.5 comment_1: STEP-TIME = 0.2 SEC; comment_2: 1 SCO ! linenum: 614.300 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: 614.500 sequence_1: USE AUX targname: HD141637 time_per_exp: X7.20 s_to_n: 141 priority: 1 comment_1: 1 SCO ! ! end of exposure logsheet ! No scan data records found