! File: 4556C.PROP ! Database: PEPDB ! Date: 22-FEB-1994:17:31:31 coverpage: title_1: FUNDAMENTAL EVOLUTIONARY PARAMETERS OF HOT MASSIVE STARS IN THE LMC sci_cat: HOT STARS sci_subcat: MASSIVE STARS proposal_for: GO pi_fname: ROLF-PETER pi_lname: KUDRITZKI pi_inst: UNIVERSITAT MUENCHEN pi_country: GERMANY hours_pri: 9.82 num_pri: 6 fos: Y off_fname: ROLF-PETER off_lname: KUDRITZKI off_title: DIRECTOR off_inst: 5588 off_addr_1: SCHEINERSTRASSE 1 off_addr_2: 8000 MUENCHEN 80 off_city: MUNICH off_country: GERMANY off_phone: +49-89-9220940 ! end of coverpage abstract: line_1: We propose to use the FOS to obtain high S/N UV spectral data, covering the line_2: wavelength range 1150-2300 A, for six LMC O9-B1.5 Ia supergiants belonging line_3: to the morphologically normal and OBN/OBC subgroups. These data will be line_4: analysed together with high-resolution optical data already obtained by the line_5: applicants. This spectral coverage is necessary in order to derive reliable line_6: values of the effective temperature, surface gravity, chemical composition, line_7: mass-loss rate and stellar mass. Highly sophisticated model atmosphere, stellar line_8: wind and 'unified' model atmosphere codes will be used in this analysis. Our line_9: principal scientific objective is to determine the evolutionary status of the line_10: 'normal' and OBN/OBC supergiant subgroups, in particular we will investigate line_11: which of these objects are pre- or post-RSG (Red SuperGiant) stars by looking line_12: for evidence of anomalous H/He and C/N/O abundance ratios AND supporting line_13: evidence from unusally low stellar masses for the post-RSG stars as compared line_14: with the pre-RSG objects. Further analagous galactic objects, for which IUE line_15: data are available, will be analysed, providing valuable observational line_16: constraints for stellar evolution theory for different metallicities, so line_17: essential for our understanding of SN like SN1987A. The project will also be a line_18: valuable test of a new spectroscopic distance determination method for which line_19: the most luminous B-supergiants are ideal candidates being easily detectable line_20: as individual stars in other distant galaxies. ! ! end of abstract general_form_proposers: lname: KUDRITZKI fname: ROLF-PETER title: PI inst: UNIVERSITAT MUENCHEN country: GERMANY esa: Y ! lname: WALBORN fname: NOLAN mi: R inst: STSCI country: USA ! lname: FITZPATRICK fname: EDWARD mi: L inst: PRINCETON UNIVERSITY country: USA ! lname: BOHANNAN fname: BRUCE inst: NOAO country: USA ! lname: VOELS fname: STEPHEN mi: A inst: UNIVERSITAT MUENCHEN country: GERMANY esa: Y ! lname: LENNON fname: DANIEL mi: J inst: UNIVERSITAT MUENCHEN country: GERMANY esa: Y ! lname: HILLIER fname: JOHN mi: D inst: UNIVERSITAT MUENCHEN country: GERMANY esa: Y ! lname: BUTLER fname: KEITH inst: UNIVERSITAT MUENCHEN country: GERMANY esa: Y ! lname: HUSFELD fname: DIRK inst: UNIVERSITAT MUENCHEN country: GERMANY esa: Y ! lname: PAULDRACH fname: ADI inst: UNIVERSITAT MUENCHEN country: GERMANY esa: Y ! lname: PULS fname: JOACHIM inst: UNIVERSITAT MUENCHEN country: GERMANY esa: Y ! ! end of general_form_proposers block general_form_text: question: 2 section: 1 line_1: Justification not required for Phase 2 ! question: 3 section: 1 line_1: We will observe 5 luminosity class Ia OB-supergiant stars in the LMC, these line_2: being chosen to be one 'normal' and one 'peculiar' (OBN/OBC) object at each line_3: of the spectral types O9.7, B1 and B1.5. The V magnitudes are in the range line_4: 11.3 to 12.2 and the spectral types are well determined from both intermediate line_5: slit spectroscopy and high dispersion echelle spectroscopy. We require two line_6: spectra of each star using the FOS and the blue detector with gratings line_7: G130H and G190H at a S/N of approximately 100. The spectral coverage will line_8: thus run from 1150A to 2300A and will contain all the important wind lines line_9: needed for our analysis; NV 1239,1243, CII 1334,1336, SiIV 1394,1403, line_10: CIV 1548,1551 and AlIII 1855,1863, plus a large number of photospheric lines line_11: due to Fe and Ni. The resolution of FOS (200 km/s) is not a problem for the line_12: analysis of the wind features while the photospheric line spectrum suffers line_13: from such blending problems that spectral sysnthesis techniques are necessary line_14: to derive abundances in any case - provided the S/N is 100. This S/N is line_15: needed to ensure reliable synthesis of FeIII line blends and for accurate line_16: modelling of the stellar wind P-Cygni line profiles. ! question: 4 section: 1 line_1: The UV spectrum is essential for our analysis as it provides crucial information line_2: about the atmospheres and winds of our objects. The UV stellar wind lines line_3: provide us with estimates of v(infinity) as well as being important diagnostics line_4: of the stellar wind velocity and ionization structure. Futhermore, there are a line_5: number of elements with no, or very weak, optical lines but with a rich UV line_6: spectrum (Fe, Ni). Experience gained with IUE on targets of similar apparent line_7: magnitudes has demonstrated that the present program is not feasible with IUE line_8: given our combined requirements of S/N, resolution and crowding problems in our line_9: target fields. HST/FOS observations are therefore necessary for this project. line_11: Extensive ground based programs have been ongoing in this area for a number of line_12: years. NRW and EF have been involved in spectral classification of hot stars line_13: in the Magellanic Clouds using low and intermediate resolution observations for line_14: some time. In addition ALL of the targets have been observed in the visible at line_15: intermediate and high dispersions using, for example, ESO 3.6m and CTIO 4m line_16: telescopes. ! question: 4 section: 2 line_1: For all target stars, low dispersion SWP IUE spectra are available line_2: and thus it is possible to accurately estimate the exposure times needed line_3: to reach a photon counting S/N of 100 for each of the two gratings. line_5: ACQ/PEAK - Count rates were estimated from scaled blackbody values for line_6: the G400H grating as supplied to Steven Voels for the Cycle 1 proposal line_7: 2233/4110. All times are given to ensure approximately 10,000 counts line_8: in all cases. NOTE THAT ALL STARS EXCEED BRIGHT LIMITS FOR ACQ/BINARY. ! question: 5 section: 1 line_1: NO GAP is requested to avoid complications in the analsysis which might line_2: arise due to variability of stellar winds. ! question: 6 section: 1 line_1: No special calibrations required ! question: 7 section: 1 line_1: Data Reduction: The P.I.'s institute has a cluster of 12 DEC VAXStations line_2: (3 x 3200, 2 x 3100, 7 x 2000, 21 VUPS total, several with 8-bit color display) line_3: plus a cluster of DEC Decstations (2 x 5000, 1 x VT1300,all 8-bit color display) line_4: on which all major astronomical software environments (IDL, IRAF, IRAF/STSDAS line_5: and MIDAS) are installed. Data calibration and reduction will be performed line_6: using the latest software and calibration databases available locally or line_7: at the nearby ST-ECF in Garching. In addition, two scientific software line_8: specialists funded by the German research ministry as part of the Deutches line_9: AstroNetz (DAN) (a four University, eight position collaboration, software line_10: and hardware network which provides German astronomers with access to and line_11: expertise in astronomical software) are based at the institute. Note that line_12: personnel have already gained experience with FOS data reduction as a result line_13: of a Cycle 1 allocation of time and are familiar with the procedures and line_14: software. ! question: 7 section: 2 line_1: 2) Analysis: The analysis will be carried out by spectral synthesis using line_2: state-of-the-art NLTE model photosphere and stellar wind codes developed line_3: by the P.I. and his collaborators. Present plane parallel, hydrostatic line_4: equilibrium codes have been pushed to new limits of sophistication through line_5: the inclusion of more realistic model atoms and more complete atomic data, line_6: made possible in part by the Opacity Project. These particular codes have been line_7: further improved by the inclusion of velocity fields, a feature which is of line_8: great importance for the analysis of the OB-supergiants. The quantitative line_9: analysis of the stars will be carried out using a new generation of NLTE line_10: model atmospheres which include spherical extension and stellar winds. line_11: NLTE model atmosphere, line formation, and stellar wind codes are implemented line_12: on a CDC Cyber 990, 2 Cray YMP-4/32's and an HP730, all of which are line_13: fiber-optically linked to the institute's local VAXcluster. ! question: 8 section: 1 line_1: Revised target positions, obtained with GASP, are now supplied with line_2: the Phase 2 proposal. ! question: 9 section: 1 line_1: GO No. 2233/4110 THE PHYSICS OF MASSIVE O-STARS IN DIFFERENT PARENT GALAXIES line_3: GTO No. 1215 ULTRAVIOLET SPECTRAL ATLAS OF O-STARS IN THE MILKY WAY AND line_4: MAGELLANIC CLOUDS line_6: The present proposal is related to these in so far as they are all concerned line_7: with the general topic of the physics and nature of hot massive stars in other line_8: galaxies. This proposal however is more specific and is concerned with the line_9: particular problem of the evolutionary status of the B-supergiants viv-a-vis line_10: the OBN/OBC dichotomy and 'blue loop' scenario. ! question: 9 section: 2 line_1: Stellar parameters and abundances (including iron) have so far been obtained line_2: for 3 very massive early O-type stars in the LMC. In addition, estimates line_3: have been made of the mass-loss rates, terminal velocities and hence the line_4: stellar masses and distances. The 15 other targets from this project are line_5: due to be observed before the end of this year. ! question: 9 section: 3 line_1: First Results from the GHRS: Spectroscopic determination of stellar parameters line_2: of an O3f star, Melnick 42, in the Large Magellanic Cloud, line_3: Heap, S.R., Altner, B., Ebbets, D., Hubeny, I., Hutchings, J.S., line_4: Kudritzki, R.P. Voels, S.A., Haser, S., Pauldrach, A., Puls, J., line_5: Butler, K., 1991., Ap. J. Let., 377, L29. line_7: Kudritzki, R.P., Becker, S.R., Butler, K., Gabler, R., Haser, S., Husfeld, D., line_8: Lennon, D.J., Pauldrach, A., Puls, J., Voels, S. 1992b, 'Hot Stars and line_9: the Hubble Space Telescope', in 'Science with the Hubble Space Telescope', line_10: ESO, in press. ! question: 10 section: 1 line_1: Munich University: line_3: Data reduction and analysis facilities and personal are described under line_4: section 6. There are no problems with the funding of the necessary computer line_5: calculations required for this project. line_7: In addition to those people from Munich University listed under "Investigators" line_8: above, Dr. R. Gabler (research assistant funded by the German Ministry for line_9: Research), Dr. S.R. Becker (research assistant funded by the the Deutsche line_10: Forschungsgemeinschaft) and several Ph.D. students (S. Haser, F. Sellmaier, line_11: U. Springmann) will work full time on the project. line_13: Funds for travel, preparation of observations, reduction, etc will also be line_14: available. ! !end of general form text general_form_address: lname: KUDRITZKI fname: ROLF-PETER category: PI inst: Universitat Muenchen addr_1: SCHEINERSTRASSE 1 addr_2: 8000 MUENCHEN 80 city: MUENCHEN/MUNICH country: GERMANY phone: +49-89-9220940 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: SK-69D43 name_2: HDE268809 name_3: GSC9161-00737 descr_1: B,113; descr_2: HOST=LMC descr_3: TYPE=B1IA pos_1: PLATE-ID=05ZW, pos_2: RA = 04H 56M 10.51S +/- 0.5", pos_3: DEC = -69D 15' 38.5" +/- 0.5" equinox: 2000 rv_or_z: V = +279 fluxnum_1: 1 fluxval_1: V = 11.9 , TYPE=B1IA fluxnum_2: 2 fluxval_2: B-V = -0.1 fluxnum_3: 3 fluxval_3: E(B-V) = 0.10 fluxnum_4: 4 fluxval_4: F-CONT(1300) = 1.0 +/- 0.1 E-12 fluxnum_5: 5 fluxval_5: F-CONT(1600) = 0.6 +/- 0.1 E-12 ! targnum: 2 name_1: SK-67D256 name_2: GSC8904-01409 descr_1: B,113; descr_2: HOST=LMC descr_3: TYPE=BC1IA pos_1: PLATE-ID=05ZW, pos_2: RA = 05H 44M 25.19S +/- 0.5", pos_3: DEC = -67D 13' 49.8" +/- 0.5" equinox: 2000 rv_or_z: V = +280 fluxnum_1: 1 fluxval_1: V = 11.9 , TYPE=BC1IA fluxnum_2: 2 fluxval_2: B-V = -0.1 fluxnum_3: 3 fluxval_3: E(B-V) = 0.09 fluxnum_4: 4 fluxval_4: F-CONT(1300) = 1.1 +/- 0.1 E-12 fluxnum_5: 5 fluxval_5: F-CONT(1600) = 0.7 +/- 0.1 E-12 ! targnum: 3 name_1: SK-67D14 name_2: HDE268685 name_3: GSC8889-00517 descr_1: B,113; descr_2: HOST=LMC descr_3: TYPE=B1.5IA pos_1: PLATE-ID=06AF, pos_2: RA = 04H 54M 31.92S +/- 0.5", pos_3: DEC = -67D 15' 24.9" +/- 0.5" equinox: 2000 rv_or_z: V = +270 fluxnum_1: 1 fluxval_1: V = 11.5 , TYPE=B1.5IA fluxnum_2: 2 fluxval_2: B-V = -0.1 fluxnum_3: 3 fluxval_3: E(B-V) = 0.06 fluxnum_4: 4 fluxval_4: F-CONT(1300) = 1.4 +/- 0.1 E-12 fluxnum_5: 5 fluxval_5: F-CONT(1600) = 1.0 +/- 0.1 E-12 ! targnum: 4 name_1: SK-69D228 name_2: GSC9163-00764 descr_1: B,113; descr_2: HOST=LMC descr_3: TYPE=BC1.5IA pos_1: PLATE-ID=05ZW, pos_2: RA = 05H 37M 9.36S +/- 0.5", pos_3: DEC = -69D 20' 19.1" +/- 0.5" equinox: 2000 rv_or_z: V = +270 fluxnum_1: 1 fluxval_1: V = 12.1 , TYPE=BC1.5IA fluxnum_2: 2 fluxval_2: B-V = 0.1 fluxnum_3: 3 fluxval_3: E(B-V) = 0.23 fluxnum_4: 4 fluxval_4: F-CONT(1300) = 0.3 +/- 0.05 E-12 fluxnum_5: 5 fluxval_5: F-CONT(1600) = 0.3 +/- 0.05 E-12 ! targnum: 5 name_1: SK-68D135 name_2: HDE269896 name_3: GSC9163-00806 descr_1: B,105; descr_2: HOST=LMC descr_3: TYPE=ON9.7IA+ pos_1: PLATE-ID=05ZW, pos_2: RA = 05H 37M 49.25S +/- 0.5", pos_3: DEC = -68D 55' 1.5" +/- 0.5" equinox: 2000 rv_or_z: V = +266 fluxnum_1: 1 fluxval_1: V = 11.4 , TYPE=ON9.7IA+ fluxnum_2: 2 fluxval_2: B-V = 0.0 fluxnum_3: 3 fluxval_3: E(B-V) = 0.29 fluxnum_4: 4 fluxval_4: F-CONT(1300) = 0.8 +/- 0.1 E-12 fluxnum_5: 5 fluxval_5: F-CONT(1600) = 0.7 +/- 0.1 E-12 ! targnum: 6 name_1: SK-66D169 name_2: HDE269889 name_3: GSC8891-00008 descr_1: B,105; descr_2: HOST=LMC descr_3: TYPE=O9.7IA+ pos_1: PLATE-ID=02I7, pos_2: RA = 05H 36M 54.70S +/- 0.5", pos_3: DEC = -66D 38' 21.9" +/- 0.5" equinox: 2000 rv_or_z: V = +270 fluxnum_1: 1 fluxval_1: V = 11.6 , TYPE=O9.7IA+ fluxnum_2: 2 fluxval_2: B-V = -0.1 fluxnum_3: 3 fluxval_3: E(B-V) = 0.09 fluxnum_4: 4 fluxval_4: F-CONT(1300) = 2.4 +/- 0.1 E-12 fluxnum_5: 5 fluxval_5: F-CONT(1600) = 1.5 +/- 0.1 E-12 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 11.000 targname: SK-69D43 config: FOS/BL opmode: ACQ/PEAK aperture: 4.3 sp_element: G400H num_exp: 1 time_per_exp: 0.26S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP req_1: ONBOARD ACQ FOR 12; req_2: SPATIAL SCAN; req_3: SEQ 11-16 NO GAP; req_4: CYCLE 3 / 11-16; ! linenum: 12.000 targname: SK-69D43 config: FOS/BL opmode: ACQ/PEAK aperture: 1.0 sp_element: G400H num_exp: 1 time_per_exp: 0.40S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP req_1: ONBOARD ACQ FOR 13; req_2: SPATIAL SCAN; ! linenum: 13.000 targname: SK-69D43 config: FOS/BL opmode: ACQ/PEAK aperture: 0.5 sp_element: G400H num_exp: 1 time_per_exp: 0.62S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP, param_2: SEARCH-SIZE-X=3, param_3: SCAN-STEP-X=0.35, param_4: SEARCH-SIZE-Y=3, param_5: SCAN-STEP-Y=0.35 req_1: ONBOARD ACQ FOR 14; ! linenum: 14.000 targname: SK-69D43 config: FOS/BL opmode: ACQ/PEAK aperture: 0.25X2.0 sp_element: G400H num_exp: 1 time_per_exp: 0.62S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP req_1: ONBOARD ACQ FOR 15; req_2: SPATIAL SCAN; ! linenum: 15.000 targname: SK-69D43 config: FOS/BL opmode: ACCUM aperture: 0.25X2.0 sp_element: G130H num_exp: 1 time_per_exp: 2299.0S s_to_n: 70 fluxnum_1: 4 priority: 1 ! linenum: 16.000 targname: SK-69D43 config: FOS/BL opmode: ACCUM aperture: 0.25X2.0 sp_element: G190H num_exp: 1 time_per_exp: 2299.0S s_to_n: 75 fluxnum_1: 5 priority: 1 ! linenum: 21.000 targname: SK-67D256 config: FOS/BL opmode: ACQ/PEAK aperture: 4.3 sp_element: G400H num_exp: 1 time_per_exp: 0.26S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP req_1: ONBOARD ACQ FOR 22; req_2: SPATIAL SCAN; req_3: SEQ 21-26 NO GAP; req_4: CYCLE 3 / 21-26; ! linenum: 22.000 targname: SK-67D256 config: FOS/BL opmode: ACQ/PEAK aperture: 1.0 sp_element: G400H num_exp: 1 time_per_exp: 0.40S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP req_1: ONBOARD ACQ FOR 23; req_2: SPATIAL SCAN; ! linenum: 23.000 targname: SK-67D256 config: FOS/BL opmode: ACQ/PEAK aperture: 0.5 sp_element: G400H num_exp: 1 time_per_exp: 0.60S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP, param_2: SEARCH-SIZE-X=3, param_3: SCAN-STEP-X=0.35, param_4: SEARCH-SIZE-Y=3, param_5: SCAN-STEP-Y=0.35 req_1: ONBOARD ACQ FOR 24; ! linenum: 24.000 targname: SK-67D256 config: FOS/BL opmode: ACQ/PEAK aperture: 0.25X2.0 sp_element: G400H num_exp: 1 time_per_exp: 0.60S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP req_1: ONBOARD ACQ FOR 25; req_2: SPATIAL SCAN; ! linenum: 25.000 targname: SK-67D256 config: FOS/BL opmode: ACCUM aperture: 0.25X2.0 sp_element: G130H num_exp: 1 time_per_exp: 2299.0S s_to_n: 75 fluxnum_1: 4 priority: 1 ! linenum: 26.000 targname: SK-67D256 config: FOS/BL opmode: ACCUM aperture: 0.25X2.0 sp_element: G190H num_exp: 1 time_per_exp: 2299.0S s_to_n: 85 fluxnum_1: 5 priority: 1 ! linenum: 31.000 targname: SK-67D14 config: FOS/BL opmode: ACQ/PEAK aperture: 4.3 sp_element: G400H num_exp: 1 time_per_exp: 0.16S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP req_1: ONBOARD ACQ FOR 32; req_2: SPATIAL SCAN; req_3: SEQ 31-36 NO GAP; req_4: CYCLE 3 / 31-36; ! linenum: 32.000 targname: SK-67D14 config: FOS/BL opmode: ACQ/PEAK aperture: 1.0 sp_element: G400H num_exp: 1 time_per_exp: 0.26S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP req_1: ONBOARD ACQ FOR 33; req_2: SPATIAL SCAN; ! linenum: 33.000 targname: SK-67D14 config: FOS/BL opmode: ACQ/PEAK aperture: 0.5 sp_element: G400H num_exp: 1 time_per_exp: 0.40S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP, param_2: SEARCH-SIZE-X=3, param_3: SCAN-STEP-X=0.35, param_4: SEARCH-SIZE-Y=3, param_5: SCAN-STEP-Y=0.35 req_1: ONBOARD ACQ FOR 34; ! linenum: 34.000 targname: SK-67D14 config: FOS/BL opmode: ACQ/PEAK aperture: 0.25X2.0 sp_element: G400H num_exp: 1 time_per_exp: 0.40S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP req_1: ONBOARD ACQ FOR 35; req_2: SPATIAL SCAN; ! linenum: 35.000 targname: SK-67D14 config: FOS/BL opmode: ACCUM aperture: 0.25X2.0 sp_element: G130H num_exp: 1 time_per_exp: 2299.0S s_to_n: 85 fluxnum_1: 4 priority: 1 ! linenum: 36.000 targname: SK-67D14 config: FOS/BL opmode: ACCUM aperture: 0.25X2.0 sp_element: G190H num_exp: 1 time_per_exp: 2299.0S s_to_n: 100 fluxnum_1: 5 priority: 1 ! linenum: 41.000 targname: SK-69D228 config: FOS/BL opmode: ACQ/PEAK aperture: 4.3 sp_element: G400H num_exp: 1 time_per_exp: 0.36S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP req_1: ONBOARD ACQ FOR 42; req_2: SPATIAL SCAN; req_3: SEQ 41-46 NO GAP; req_4: CYCLE 3 / 41-46; ! linenum: 42.000 targname: SK-69D228 config: FOS/BL opmode: ACQ/PEAK aperture: 1.0 sp_element: G400H num_exp: 1 time_per_exp: 0.58S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP req_1: ONBOARD ACQ FOR 43; req_2: SPATIAL SCAN; ! linenum: 43.000 targname: SK-69D228 config: FOS/BL opmode: ACQ/PEAK aperture: 0.5 sp_element: G400H num_exp: 1 time_per_exp: 0.86S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP, param_2: SEARCH-SIZE-X=3, param_3: SCAN-STEP-X=0.35, param_4: SEARCH-SIZE-Y=3, param_5: SCAN-STEP-Y=0.35 req_1: ONBOARD ACQ FOR 44; ! linenum: 44.000 targname: SK-69D228 config: FOS/BL opmode: ACQ/PEAK aperture: 0.25X2.0 sp_element: G400H num_exp: 1 time_per_exp: 0.86S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP req_1: ONBOARD ACQ FOR 45; req_2: SPATIAL SCAN; ! linenum: 45.000 targname: SK-69D228 config: FOS/BL opmode: ACCUM aperture: 0.25X2.0 sp_element: G130H num_exp: 1 time_per_exp: 7497.0S s_to_n: 70 fluxnum_1: 4 priority: 1 ! linenum: 46.000 targname: SK-69D228 config: FOS/BL opmode: ACCUM aperture: 0.25X2.0 sp_element: G190H num_exp: 1 time_per_exp: 3885.0S s_to_n: 70 fluxnum_1: 5 priority: 1 ! linenum: 51.000 targname: SK-68D135 config: FOS/BL opmode: ACQ/PEAK aperture: 4.3 sp_element: G400H num_exp: 1 time_per_exp: 0.18S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP req_1: ONBOARD ACQ FOR 52; req_2: SPATIAL SCAN; req_3: SEQ 51-56 NO GAP; req_4: CYCLE 3 / 51-56; ! linenum: 52.000 targname: SK-68D135 config: FOS/BL opmode: ACQ/PEAK aperture: 1.0 sp_element: G400H num_exp: 1 time_per_exp: 0.30S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP req_1: ONBOARD ACQ FOR 53; req_2: SPATIAL SCAN; ! linenum: 53.000 targname: SK-68D135 config: FOS/BL opmode: ACQ/PEAK aperture: 0.5 sp_element: G400H num_exp: 1 time_per_exp: 0.44S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP, param_2: SEARCH-SIZE-X=3, param_3: SCAN-STEP-X=0.35, param_4: SEARCH-SIZE-Y=3, param_5: SCAN-STEP-Y=0.35 req_1: ONBOARD ACQ FOR 54; ! linenum: 54.000 targname: SK-68D135 config: FOS/BL opmode: ACQ/PEAK aperture: 0.25X2.0 sp_element: G400H num_exp: 1 time_per_exp: 0.44S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP req_1: ONBOARD ACQ FOR 55; req_2: SPATIAL SCAN; ! linenum: 55.000 targname: SK-68D135 config: FOS/BL opmode: ACCUM aperture: 0.25X2.0 sp_element: G130H num_exp: 1 time_per_exp: 2812.0S s_to_n: 70 fluxnum_1: 4 priority: 1 ! linenum: 56.000 targname: SK-68D135 config: FOS/BL opmode: ACCUM aperture: 0.25X2.0 sp_element: G190H num_exp: 1 time_per_exp: 2299.0S s_to_n: 85 fluxnum_1: 5 priority: 1 ! linenum: 61.000 targname: SK-66D169 config: FOS/BL opmode: ACQ/PEAK aperture: 4.3 sp_element: G400H num_exp: 1 time_per_exp: 0.18S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP req_1: ONBOARD ACQ FOR 62; req_2: SPATIAL SCAN; req_3: SEQ 61-66 NO GAP; req_4: CYCLE 3 / 61-66; ! linenum: 62.000 targname: SK-66D169 config: FOS/BL opmode: ACQ/PEAK aperture: 1.0 sp_element: G400H num_exp: 1 time_per_exp: 0.28S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP req_1: ONBOARD ACQ FOR 63; req_2: SPATIAL SCAN; ! linenum: 63.000 targname: SK-66D169 config: FOS/BL opmode: ACQ/PEAK aperture: 0.5 sp_element: G400H num_exp: 1 time_per_exp: 0.42S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP, param_2: SEARCH-SIZE-X=3, param_3: SCAN-STEP-X=0.35, param_4: SEARCH-SIZE-Y=3, param_5: SCAN-STEP-Y=0.35 req_1: ONBOARD ACQ FOR 64; ! linenum: 64.000 targname: SK-66D169 config: FOS/BL opmode: ACQ/PEAK aperture: 0.25X2.0 sp_element: G400H num_exp: 1 time_per_exp: 0.42S fluxnum_1: 1,3 priority: 1 param_1: TYPE=UP req_1: ONBOARD ACQ FOR 65; req_2: SPATIAL SCAN; ! linenum: 65.000 targname: SK-66D169 config: FOS/BL opmode: ACCUM aperture: 0.25X2.0 sp_element: G130H num_exp: 1 time_per_exp: 2299.0S s_to_n: 110 fluxnum_1: 4 priority: 1 ! linenum: 66.000 targname: SK-66D169 config: FOS/BL opmode: ACCUM aperture: 0.25X2.0 sp_element: G190H num_exp: 1 time_per_exp: 2299.0S s_to_n: 120 fluxnum_1: 5 priority: 1 ! ! end of exposure logsheet scan_data: line_list: 11.00 fgs_scan: cont_dwell: D dwell_pnts: 3 dwell_secs: 1.00 scan_width: 0.0000 scan_length: 2.8000 sides_angle: 90.0000 number_lines: 1 scan_rate: 0.0000 first_line_pa: 0.0000 scan_frame: S/C len_offset: 1.4 wid_offset: ! line_list: 12.00 fgs_scan: cont_dwell: D dwell_pnts: 6 dwell_secs: 1.00 scan_width: 0.7000 scan_length: 3.5000 sides_angle: 90.0000 number_lines: 2 scan_rate: 0.0000 first_line_pa: 90.0000 scan_frame: S/C len_offset: 1.75 wid_offset: 0.35 ! line_list: 14.00 fgs_scan: cont_dwell: D dwell_pnts: 7 dwell_secs: 1.00 scan_width: 0.0000 scan_length: 0.4000 sides_angle: 0.0000 number_lines: 1 scan_rate: 0.0000 first_line_pa: 90.0000 scan_frame: S/C len_offset: 0.2 wid_offset: ! line_list: 21.00 fgs_scan: cont_dwell: D dwell_pnts: 3 dwell_secs: 1.00 scan_width: 0.0000 scan_length: 2.8000 sides_angle: 90.0000 number_lines: 1 scan_rate: 0.0000 first_line_pa: 0.0000 scan_frame: S/C len_offset: 1.4 wid_offset: ! line_list: 22.00 fgs_scan: cont_dwell: D dwell_pnts: 6 dwell_secs: 1.00 scan_width: 0.7000 scan_length: 3.5000 sides_angle: 90.0000 number_lines: 2 scan_rate: 0.0000 first_line_pa: 90.0000 scan_frame: S/C len_offset: 1.75 wid_offset: 0.35 ! line_list: 24.00 fgs_scan: cont_dwell: D dwell_pnts: 7 dwell_secs: 1.00 scan_width: 0.0000 scan_length: 0.4000 sides_angle: 0.0000 number_lines: 1 scan_rate: 0.0000 first_line_pa: 90.0000 scan_frame: S/C len_offset: 0.2 wid_offset: ! line_list: 31.00 fgs_scan: cont_dwell: D dwell_pnts: 3 dwell_secs: 1.00 scan_width: 0.0000 scan_length: 2.8000 sides_angle: 90.0000 number_lines: 1 scan_rate: 0.0000 first_line_pa: 0.0000 scan_frame: S/C len_offset: 1.4 wid_offset: ! line_list: 32.00 fgs_scan: cont_dwell: D dwell_pnts: 6 dwell_secs: 1.00 scan_width: 0.7000 scan_length: 3.5000 sides_angle: 90.0000 number_lines: 2 scan_rate: 0.0000 first_line_pa: 90.0000 scan_frame: S/C len_offset: 1.75 wid_offset: 0.35 ! line_list: 34.00 fgs_scan: cont_dwell: D dwell_pnts: 7 dwell_secs: 1.00 scan_width: 0.0000 scan_length: 0.4000 sides_angle: 0.0000 number_lines: 1 scan_rate: 0.0000 first_line_pa: 90.0000 scan_frame: S/C len_offset: 0.2 wid_offset: ! line_list: 41.00 fgs_scan: cont_dwell: D dwell_pnts: 3 dwell_secs: 1.00 scan_width: 0.0000 scan_length: 2.8000 sides_angle: 90.0000 number_lines: 1 scan_rate: 0.0000 first_line_pa: 0.0000 scan_frame: S/C len_offset: 1.4 wid_offset: ! line_list: 42.00 fgs_scan: cont_dwell: D dwell_pnts: 6 dwell_secs: 1.00 scan_width: 0.7000 scan_length: 3.5000 sides_angle: 90.0000 number_lines: 2 scan_rate: 0.0000 first_line_pa: 90.0000 scan_frame: S/C len_offset: 1.75 wid_offset: 0.35 ! line_list: 44.00 fgs_scan: cont_dwell: D dwell_pnts: 7 dwell_secs: 1.00 scan_width: 0.0000 scan_length: 0.4000 sides_angle: 0.0000 number_lines: 1 scan_rate: 0.0000 first_line_pa: 90.0000 scan_frame: S/C len_offset: 0.2 wid_offset: ! line_list: 51.00 fgs_scan: cont_dwell: D dwell_pnts: 3 dwell_secs: 1.00 scan_width: 0.0000 scan_length: 2.8000 sides_angle: 90.0000 number_lines: 1 scan_rate: 0.0000 first_line_pa: 0.0000 scan_frame: S/C len_offset: 1.4 wid_offset: ! line_list: 52.00 fgs_scan: cont_dwell: D dwell_pnts: 6 dwell_secs: 1.00 scan_width: 0.7000 scan_length: 3.5000 sides_angle: 90.0000 number_lines: 2 scan_rate: 0.0000 first_line_pa: 90.0000 scan_frame: S/C len_offset: 1.75 wid_offset: 0.35 ! line_list: 54.00 fgs_scan: cont_dwell: D dwell_pnts: 7 dwell_secs: 1.00 scan_width: 0.0000 scan_length: 0.4000 sides_angle: 0.0000 number_lines: 1 scan_rate: 0.0000 first_line_pa: 90.0000 scan_frame: S/C len_offset: 0.2 wid_offset: ! line_list: 61.00 fgs_scan: cont_dwell: D dwell_pnts: 3 dwell_secs: 1.00 scan_width: 0.0000 scan_length: 2.8000 sides_angle: 90.0000 number_lines: 1 scan_rate: 0.0000 first_line_pa: 0.0000 scan_frame: S/C len_offset: 1.4 wid_offset: ! line_list: 62.00 fgs_scan: cont_dwell: D dwell_pnts: 6 dwell_secs: 1.00 scan_width: 0.7000 scan_length: 3.5000 sides_angle: 90.0000 number_lines: 2 scan_rate: 0.0000 first_line_pa: 90.0000 scan_frame: S/C len_offset: 1.75 wid_offset: 0.35 ! line_list: 64.00 fgs_scan: cont_dwell: D dwell_pnts: 7 dwell_secs: 1.00 scan_width: 0.0000 scan_length: 0.4000 sides_angle: 0.0000 number_lines: 1 scan_rate: 0.0000 first_line_pa: 90.0000 scan_frame: S/C len_offset: 0.2 wid_offset: ! ! end of scan data