! File: 3942C.PROP ! Database: PEPDB ! Date: 20-FEB-1994:00:58:51 coverpage: title_1: GTO - R136 - CYCLES 2-5 EXPOSURES sci_cat: STELLAR ASTROPHYSICS proposal_for: GTO/HRS pi_title: DR. pi_fname: DENNIS pi_mi: C. pi_lname: EBBETS pi_inst: BALL AEROSPACE SYSTEMS pi_country: USA pi_phone: (303) 939-5964 keywords_1: SUPERGIANT STAR, WOLF-RAYET STAR, MASS LOSS, LMC 30 keywords_2: DORADUS hours_pri: 16.04 num_pri: 6 realtime: X pi_position: PRIN MEM TECH STAFF ! end of coverpage abstract: line_1: R136 is the bright central object of the 30 Doradus nebula in the LMC. It line_2: contains an unusually tight grouping of very massive and luminous O and line_3: Wolf-Rayet type stars. The brightest recognizeable component, called R136A1, line_4: is itself a very close double. line_5: Detailed studies of the individual components line_6: have been hampered by a lack of sufficient spatial resolution. The High line_7: Resolution Spectrograph will be used to obtain detailed ultraviolet spatial and line_8: spectral information about the five or so brightest discrete components. The line_9: goal of the program is to study the spectral morphology, stellar wind line_10: characteristics, ultraviolet luminosities and ultimately the masses included line_11: in this unusual and interesting object. line_13: redlined for phase 2, 7/19/88, dce line_14: updated for cycle 1 phase 2 9/21/89 line_15: revised lines 1-7 for cycle zero 11/15/90 line_16: Revised for cycle 1 exposures February 09, 1991 line_17: Revised for cycles 2-5 May 22, 1991 line_18: This prop contains only cycle 2-5 exposures ! ! end of abstract general_form_proposers: lname: SAVAGE fname: BLAIR mi: D. inst: WISCONSIN, UNIVERSITY OF country: USA ! lname: EBBETS fname: DENNIS mi: C. inst: BALL AEROSPACE CORPORATION country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: Cycle 2 baseline time: line_2: R136A1 SSA G160M line_3: Wavelengths = 1250, 1380, 1542 S/N = 10 line_4: Cycle 2 augmentation requested line_5: R136A1 SSA G160M S/N > 20 to be recovered line_6: partial recovery of science in original plan line_7: Cycle 2 augmentation requested line_8: R136A3 plus nearby sky SSA G140L line_9: Cycle 5 post costar baseline time line_10: R136A1, R136A4, R136B, R136C line_11: SSA G140L Wavelengths 1362.5, 1642.5 ! question: 4 section: 1 line_1: R136 has been studied extensively from the ground with imagery and line_2: spectroscopy. Over a dozen observations have been made with the IUE. Much has line_3: been learned from these studies, but all have been ultimately limited by the line_4: finite spatial resolution allowed by the atmosphere and the instruments. line_5: The GHRS will have the spatial line_6: resolution, sensitivity and spectral resolving power to provide high quality line_7: ultraviolet spectra of each component. ! question: 5 section: 1 line_1: R136 is a very crowded field. Successful completion of this program requires line_2: that the component being observed be precisely centered in the 0.25 arc sec line_3: aperture. We request real time target acquisition capability, to ensure that line_4: the centering is adequate, and to make adjustments to the pointing if line_5: necessary. ! question: 7 section: 1 line_1: The spectra will be calibrated and reduced using standard procedures either in line_2: RSDP, or the IDT facilities. line_3: The spectrum of R136A1 will be studied in terms of gross spectral line_4: morphologhy, for the purposes of classification. Stellar wind diagnostics such line_5: as terminal velocities and mass loss rates will be derived from comparison of line_6: line profiles with model predictions and experience with similar stars. The line_7: ultraviolet spectral energy distributions will be studied by correcting for now line_8: known effects of galactic and LMC extinction. ! question: 13 section: 1 line_1: The High Resolution Spectrograph will be used to observe the UV spectrum of line_2: the bright components of R136. The brightest member, R136a1 will be observed line_3: in cycle 2 at medium resolution with G160M, to study important line_4: interstellar lines in the LMC and MW halo gas. The fainter line_5: stellar components, R136A3, R136A4, R136B and R136C will be line_6: observed with the G140L grating to study their stellar parameters. ! !end of general form text general_form_address: lname: SAVAGE fname: BLAIR mi: D. category: CON inst: UNIVERSITY OF WISCONSIN addr_1: DEPARTMENT OF ASTRONOMY addr_2: 475 N. CHARTER ST. city: MADISON state: WI zip: 53706 country: USA phone: (608) 262-4909 ! lname: EBBETS fname: DENNIS mi: C. title: DR. category: PI inst: BALL AEROSPACE SYSTEMS addr_1: GHRS PROJECT AR-1 addr_2: P.O. BOX 1062 city: BOULDER state: CO zip: 80306 country: USA phone: (303) 939-5964 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: R136A1 name_2: HD38268 descr_1: BRIGHTEST COMPONENT OF R136 pos_1: RA = 5H 38M 42.50S +/- 0.1S, pos_2: DEC = -69D 06' 02.8" +/- 1" equinox: 2000 pm_or_par: NO acqpr_1: COMP comment_1: POSITION FROM PC IMAGE MEASURED comment_2: BY ARCHIE BETWEEN A1 AND A2 comment_3: UV CONTINUUM FLUXES ESTIMATED FROM comment_4: IUE OBSERVATIONS OF TOTAL FLUX AND comment_5: RATIOS OF COMPONENT BRIGHTNESSES IN comment_6: VISIBLE LIGHT. comment_7: GS PLATE ID = 06B0 fluxnum_1: 1 fluxval_1: V = 10.1 fluxnum_2: 2 fluxval_2: F-CONT(1500) = 6.2 E-13 ! targnum: 2 name_1: R136A2 descr_1: RESOLVED COMPONENT pos_1: R = 0.1", pos_2: PA = 66D, pos_3: FROM 8 equinox: 2000 pm_or_par: NO acqpr_1: COMP fluxnum_1: 1 fluxval_1: F-CONT(1500) = 4.8 E-13 ! targnum: 3 name_1: R136B descr_1: RESOLVED COMPONENT pos_1: R = 2.2", pos_2: PA = 115D, pos_3: FROM 8 equinox: 2000 pm_or_par: NO acqpr_1: COMP fluxnum_1: 1 fluxval_1: F-CONT(1500) = 3.3 E-13 ! targnum: 4 name_1: R136C descr_1: RESOLVED COMPONENT pos_1: R = 3.4", pos_2: PA = 126D, pos_3: FROM 8 equinox: 2000 pm_or_par: NO acqpr_1: COMP fluxnum_1: 1 fluxval_1: F-CONT(1500) = 3.3 E-13 ! targnum: 5 name_1: R136A3 descr_1: RESOLVED COMPONENT pos_1: R = 0.5", pos_2: PA = 223D, pos_3: FROM 8 equinox: 2000 pm_or_par: NO acqpr_1: COMP fluxnum_1: 1 fluxval_1: F-CONT(1500) = 4.8 E-13 ! targnum: 6 name_1: R136A4 descr_1: RESOLVED COMPONENT pos_1: R = 0.4", pos_2: PA = 323D, pos_3: FROM 8 equinox: 2000 pm_or_par: NO acqpr_1: COMP fluxnum_1: 1 fluxval_1: F-CONT(1500) = 1.0 E-13 ! targnum: 7 name_1: SKY descr_1: WINGS OF PSF pos_1: R = 0.5", pos_2: PA = 270D, pos_3: FROM 8 equinox: 2000 pm_or_par: NO acqpr_1: COMP fluxnum_1: 1 fluxval_1: F-CONT(1500) = 1.0E-13 ! targnum: 8 name_1: R136-OFFSET name_2: HD38268 descr_1: REFERENCE POINT FOR COMPONENTS descr_2: BRIGHTEST COMPONENT OF R136 pos_1: RA = 5H 38M 42.50S +/- 0.1S, pos_2: DEC = -69D 06' 02.8" +/- 1" equinox: 2000 pm_or_par: NO acqpr_1: COMP comment_1: COORDS OF REF POINT MEASURED WITH comment_2: GASP BY ARCHIE WARNOCK. comment_3: OFFSETS TO COMPONENTS FROM comment_4: WEIGELT AND BAIER SPECKLE OBS comment_6: UPDATE AFTER EARLY ACQ IMAGES fluxnum_1: 1 fluxval_1: V = 10.1 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 10.000 targname: R136A1 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 477S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: SEARCH-SIZE=3, req_1: INT ACQ FOR 20-160; req_2: CYCLE 2 /10-160; ! linenum: 20.000 targname: R136A1 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 96.8S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=2, param_4: DELTA-Y=2, param_5: PRECISION=HIGH, ! linenum: 30.000 targname: R136A1 config: HRS opmode: IMAGE aperture: 0.25 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 96.8S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=1, param_4: DELTA-Y=1, param_5: PRECISION=HIGH, req_1: SEQ 30-50 NO GAP; ! linenum: 40.000 targname: WAVE config: HRS opmode: ACCUM aperture: SC1 sp_element: G160M wavelength: 1250 num_exp: 1 time_per_exp: 40.0S s_to_n: 25 priority: 2 param_1: STEP-PATT=2, req_1: CALIB FOR 50; ! linenum: 50.000 targname: R136A1 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1250 num_exp: 8 time_per_exp: 300.8S s_to_n: 25 fluxnum_1: 2 priority: 2 param_1: STEP-PATT=2, ! linenum: 60.000 targname: R136A1 config: HRS opmode: IMAGE aperture: 0.25 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 96.8S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=1, param_4: DELTA-Y=1, param_5: PRECISION=HIGH req_1: SEQ 60-80 NO GAP; ! linenum: 70.000 targname: WAVE config: HRS opmode: ACCUM aperture: SC1 sp_element: G160M wavelength: 1380 num_exp: 1 time_per_exp: 40.0S s_to_n: 25 priority: 2 param_1: STEP-PATT=2, req_1: CALIB FOR 80; ! linenum: 80.000 targname: R136A1 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1380 num_exp: 8 time_per_exp: 300.8S s_to_n: 25 fluxnum_1: 2 priority: 2 param_1: STEP-PATT=2, ! linenum: 90.000 targname: R136A1 config: HRS opmode: IMAGE aperture: 0.25 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 96.8S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=1, param_4: DELTA-Y=1, param_5: PRECISION=HIGH req_1: SEQ 90-110 NO GAP; ! linenum: 100.000 targname: WAVE config: HRS opmode: ACCUM aperture: SC1 sp_element: G160M wavelength: 1542 num_exp: 1 time_per_exp: 40.0S s_to_n: 25 priority: 2 param_1: STEP-PATT=2, req_1: CALIB FOR 110; ! linenum: 110.000 targname: R136A1 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1542 num_exp: 8 time_per_exp: 300.8S s_to_n: 25 fluxnum_1: 2 priority: 2 param_1: STEP-PATT=2, ! linenum: 140.000 targname: R136A1 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1250 num_exp: 30 time_per_exp: 300.8S s_to_n: 20 fluxnum_1: 2 priority: 2 param_1: STEP-PATT=2, req_1: COND IF TAC OK; ! linenum: 150.000 targname: R136A1 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1380 num_exp: 20 time_per_exp: 300.8S s_to_n: 20 fluxnum_1: 2 priority: 2 param_1: STEP-PATT=2, req_1: COND IF TAC OK; ! linenum: 160.000 targname: R136A1 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G160M wavelength: 1542 num_exp: 20 time_per_exp: 300.8S s_to_n: 20 fluxnum_1: 2 priority: 2 param_1: STEP-PATT=2, req_1: COND IF TAC OK; ! linenum: 300.000 targname: R136A3 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 477S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: SEARCH-SIZE=3, req_1: INT ACQ FOR 310-410; req_2: CYCLE 2 / 300-410; req_3: COND IF TAC OK; ! linenum: 310.000 targname: R136A3 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 96.8S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=2, param_4: DELTA-Y=2, param_5: PRECISION=HIGH, req_1: COND IF TAC OK; ! linenum: 320.000 targname: R136A3 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N1 num_exp: 1 time_per_exp: 484S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=2, param_4: DELTA-Y=2, param_5: PRECISION=HIGH, req_1: COND IF TAC OK; ! linenum: 330.000 targname: R136A3 config: HRS opmode: IMAGE aperture: 0.25 sp_element: MIRROR-N1 num_exp: 1 time_per_exp: 96.8S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=1, param_4: DELTA-Y=1, param_5: PRECISION=HIGH, req_1: COND IF TAC OK; ! linenum: 340.000 targname: R136A3 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G140L wavelength: 1362.5 num_exp: 2 time_per_exp: 1203.2S s_to_n: 20 fluxnum_1: 1 priority: 2 param_1: STEP-PATT=2, param_2: FP-SPLIT=STD, req_1: COND IF TAC OK; ! linenum: 350.000 targname: R136A3 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G140L wavelength: 1642.5 num_exp: 2 time_per_exp: 1203.2S s_to_n: 15 fluxnum_1: 1 priority: 2 param_1: STEP-PATT=2, param_2: FP-SPLIT=STD, req_1: COND IF TAC OK; ! linenum: 360.000 targname: R136A3 config: HRS opmode: IMAGE aperture: 0.25 sp_element: MIRROR-N1 num_exp: 1 time_per_exp: 96.8S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=1, param_4: DELTA-Y=1, param_5: PRECISION=HIGH, req_1: COND IF TAC OK; ! linenum: 370.000 targname: R136A3 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N1 num_exp: 1 time_per_exp: 96.8S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=2, param_4: DELTA-Y=2, param_5: PRECISION=HIGH, req_1: COND IF TAC OK; ! linenum: 380.000 targname: SKY config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N1 num_exp: 1 time_per_exp: 96.8S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=2, param_4: DELTA-Y=2, param_5: PRECISION=HIGH, req_1: COND IF TAC OK; ! linenum: 390.000 targname: SKY config: HRS opmode: IMAGE aperture: 0.25 sp_element: MIRROR-N1 num_exp: 1 time_per_exp: 96.8S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=1, param_4: DELTA-Y=1, param_5: PRECISION=HIGH, req_1: COND IF TAC OK; ! linenum: 400.000 targname: SKY config: HRS opmode: ACCUM aperture: 0.25 sp_element: G140L wavelength: 1362.5 num_exp: 1 time_per_exp: 1203.2S s_to_n: 15 fluxnum_1: 1 priority: 2 param_1: STEP-PATT=2, param_2: FP-SPLIT=STD, req_1: COND IF TAC OK; ! linenum: 410.000 targname: SKY config: HRS opmode: ACCUM aperture: 0.25 sp_element: G140L wavelength: 1642.5 num_exp: 1 time_per_exp: 1203.2S s_to_n: 15 fluxnum_1: 1 priority: 2 param_1: STEP-PATT=2, param_2: FP-SPLIT=STD, req_1: COND IF TAC OK; ! linenum: 500.000 targname: R136A1 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N1 num_exp: 1 time_per_exp: 477S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: SEARCH-SIZE=3, req_1: INT ACQ FOR 510-830; req_2: CYCLE 5 / 500-830; ! linenum: 510.000 targname: R136A1 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N1 num_exp: 1 time_per_exp: 96.8S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=2, param_4: DELTA-Y=2, param_5: PRECISION=HIGH, ! linenum: 520.000 targname: R136A1 config: HRS opmode: IMAGE aperture: 0.25 sp_element: MIRROR-N1 num_exp: 1 time_per_exp: 96.8S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=1, param_4: DELTA-Y=1, param_5: PRECISION=HIGH, ! linenum: 530.000 targname: R136A1 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G140L wavelength: 1362.5 num_exp: 1 time_per_exp: 320.0S s_to_n: 50 fluxnum_1: 2 priority: 2 param_1: STEP-PATT=2, ! linenum: 540.000 targname: R136A1 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G140L wavelength: 1642.5 num_exp: 1 time_per_exp: 320.0S s_to_n: 50 fluxnum_1: 2 priority: 2 param_1: STEP-PATT=2, ! linenum: 550.000 targname: R136A1 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N1 num_exp: 1 time_per_exp: 96.8S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=2, param_4: DELTA-Y=2, param_5: PRECISION=HIGH, ! linenum: 600.000 targname: R136B config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N1 num_exp: 1 time_per_exp: 46S s_to_n: 10 fluxnum_1: 1 priority: 2 req_1: ONBOARD ACQ FOR 610-640; req_2: SEQ 600-640 NO GAP; ! linenum: 610.000 targname: R136B config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N1 num_exp: 1 time_per_exp: 96.8S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=2, param_4: DELTA-Y=2, param_5: PRECISION=HIGH, ! linenum: 620.000 targname: R136B config: HRS opmode: IMAGE aperture: 0.25 sp_element: MIRROR-N1 num_exp: 1 time_per_exp: 96.8S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=1, param_4: DELTA-Y=1, param_5: PRECISION=HIGH, ! linenum: 630.000 targname: R136B config: HRS opmode: ACCUM aperture: 0.25 sp_element: G140L wavelength: 1362.5 num_exp: 1 time_per_exp: 320.0S s_to_n: 50 fluxnum_1: 1 priority: 2 param_1: STEP-PATT=2, ! linenum: 640.000 targname: R136B config: HRS opmode: ACCUM aperture: 0.25 sp_element: G140L wavelength: 1642.5 num_exp: 1 time_per_exp: 320.0S s_to_n: 50 fluxnum_1: 1 priority: 2 param_1: STEP-PATT=2, ! linenum: 700.000 targname: R136C config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N1 num_exp: 1 time_per_exp: 46S s_to_n: 10 fluxnum_1: 1 priority: 2 req_1: ONBOARD ACQ FOR 710-740; req_2: SEQ 700-740 NO GAP; ! linenum: 710.000 targname: R136C config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N1 num_exp: 1 time_per_exp: 96.8S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=2, param_4: DELTA-Y=2, param_5: PRECISION=HIGH, ! linenum: 720.000 targname: R136C config: HRS opmode: IMAGE aperture: 0.25 sp_element: MIRROR-N1 num_exp: 1 time_per_exp: 96.8S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=1, param_4: DELTA-Y=1, param_5: PRECISION=HIGH, ! linenum: 730.000 targname: R136C config: HRS opmode: ACCUM aperture: 0.25 sp_element: G140L wavelength: 1362.5 num_exp: 1 time_per_exp: 320.0S s_to_n: 50 fluxnum_1: 1 priority: 2 param_1: STEP-PATT=2, ! linenum: 740.000 targname: R136C config: HRS opmode: ACCUM aperture: 0.25 sp_element: G140L wavelength: 1642.5 num_exp: 1 time_per_exp: 320.0S s_to_n: 50 fluxnum_1: 1 priority: 2 param_1: STEP-PATT=2, ! linenum: 800.000 targname: R136A4 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N1 num_exp: 1 time_per_exp: 96.8S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=2, param_4: DELTA-Y=2, param_5: PRECISION=HIGH, ! linenum: 810.000 targname: R136A4 config: HRS opmode: IMAGE aperture: 0.25 sp_element: MIRROR-N1 num_exp: 1 time_per_exp: 96.8S s_to_n: 10 fluxnum_1: 1 priority: 2 param_1: NX=22, param_2: NY=22, param_3: DELTA-X=1, param_4: DELTA-Y=1, param_5: PRECISION=HIGH, ! linenum: 820.000 targname: R136A4 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G140L wavelength: 1362.5 num_exp: 1 time_per_exp: 320.0S s_to_n: 50 fluxnum_1: 1 priority: 2 param_1: STEP-PATT=2, ! linenum: 830.000 targname: R136A4 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G140L wavelength: 1642.5 num_exp: 1 time_per_exp: 320.0S s_to_n: 50 fluxnum_1: 1 priority: 2 param_1: STEP-PATT=2, ! ! end of exposure logsheet ! No scan data records found