! File: 4863C.PROP ! Database: PEPDB ! Date: 23-FEB-1994:06:56:12 coverpage: title_1: OPTICAL COUNTERPARTS OF RADIO PULSARS (FOS 38) title_2: AUGMENTATION: CYCLE 3 - HIGH sci_cat: STELLAR ASTROPHYSICS proposal_for: AUG/FOS cont_id: 3651 pi_title: PROF. pi_fname: BRUCE pi_lname: MARGON pi_inst: WASHINGTON, UNIVERSITY OF pi_country: USA pi_phone: 206-543-0089 hours_pri: 2.31 num_pri: 1 fos: Y ! end of coverpage abstract: line_1: The FOS GTO program includes a systematic study of degenerate stars. FOS line_2: spectra of the Crab will be used to measure the spectral index (especially line_3: UV) of the nonthermal pulsar radiation, to verify synchrotron mechanism and line_4: search for spectral breaks. Absorption may be seen due to intervening gas, line_5: whose abundance and physical state could then be probed. ! ! end of abstract general_form_proposers: lname: MARGON fname: BRUCE inst: UNIVERSITY OF WASHINGTON country: USA ! lname: HARMS fname: RICHARD title: PI mi: J. inst: APPLIED RESEARCH CORPORATION country: USA ! lname: BOHLIN fname: RALPH inst: SPACE TELESCOPE SCIENCE INSTITUTE country: USA ! lname: ANGEL fname: J. ROGER mi: P. inst: UNIVERSITY OF ARIZONA country: USA ! lname: BARTKO fname: FRANK inst: UNIVERSITY OF CALIFORNIA, SAN DIEGO country: USA ! lname: BEAVER fname: EDWARD inst: UNIVERSITY OF CALIFORNIA, SAN DIEGO country: USA ! lname: BURBIDGE fname: E. MARGARET inst: UNIVERSITY OF CALIFORNIA, SAN DIEGO country: USA ! lname: DAVIDSEN fname: ARTHUR mi: F. inst: JOHNS HOPKINS UNIVERSITY country: USA ! lname: FORD fname: HOLLAND mi: C. inst: JOHNS HOPKINS UNIVERSITY country: USA ! lname: HARTIG fname: GEORGE mi: F. inst: SPACE TELESCOPE SCIENCE INSTITUTE country: USA ! lname: ANDERSON fname: SCOTT mi: F. inst: UNIVERSITY OF WASHINGTON country: USA ! lname: DOWNES fname: RONALD mi: A. inst: SPACE TELESCOPE SCIENCE INSTITUTE country: USA ! lname: ALLEN fname: RICHARD mi: P. inst: UNIVERSITY OF ARIZONA country: USA ! ! end of general_form_proposers block general_form_text: question: 2 section: 1 line_1: ! question: 3 section: 1 line_1: UV FOS spectra of the Crab pulsar will be obtained. line_2: On the first visit a G160L spectrum will be taken. line_3: Based on quick analysis of this spectrum, gratings line_4: will be chosen for 2nd visit. ! question: 5 section: 1 line_1: The UV flux and spectrum of the Crab pulsar are uncertain; an line_2: initial FOS prism spectrum (line number 2) will be taken to line_3: measure these. Based on the flux and spectrum in the UV line_4: determined from the initial spectrum, GTO will SELECT one of line_5: four COND IF gratings for an additional follow-up spectrum. ! question: 7 section: 1 line_1: Data reduction will be performed at the ST ScI, and the analysis will be line_2: performed using FOS IDT computer facilities. The EF Eri program involves line_3: analysis of FOS spectropolarimetry. The FOS IDT, of course, has extensive line_4: practical experience in the use of STSDAS (and other IRAF-related) software line_5: to reduce and analyze all the various types of FOS data. ! question: 8 section: 1 line_1: ! question: 10 section: 1 line_1: Data analysis, research assistant support, and funding will be provided under line_2: NASA's FOS GTO contract(s). The FOS IDT support includes a total of roughly line_3: 30 Ph.D. astronomers and graduate students at 5 different institutions. At line_4: each institution one or more workstations (typically Sparc 2's or the line_5: equivalent), plus one or more Microvaxes (or equivalent) are essentially line_6: devoted to processing of HST data. ! !end of general form text general_form_address: lname: MARGON fname: BRUCE category: PI inst: UNIVERSITY OF WASHINGTON addr_1: ASTRONOMY DEPARTMENT, FM-20 city: SEATTLE state: WA zip: 98195 country: USA phone: 206 543-0089 telex: 4740096 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: CRAB-PULSAR name_2: NP0531 descr_1: A,160 pos_1: RA=05H31M 31.41S+/-0.01S, pos_2: DEC=+21D 58' 54.4"+/-0.1" equinox: 1950 acqpr_1: BKG comment_1: PULSAR AT CENTER OF CRAB NEBULA. comment_2: E(B-V)=0.5 fluxnum_1: 1 fluxval_1: V = 16.4 +/- 0.3 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 targname: CRAB-PULSAR config: FOS/BL opmode: ACQ/PEAK aperture: 4.3 sp_element: MIRROR num_exp: 1 time_per_exp: 5.0S fluxnum_1: 1 priority: 1 req_1: ONBOARD ACQ FOR 1.5; req_2: CYCLE 3 /1-10; req_3: SPATIAL SCAN; ! linenum: 1.500 targname: CRAB-PULSAR config: FOS/BL opmode: ACQ/PEAK aperture: 1.0 sp_element: MIRROR num_exp: 1 time_per_exp: 7.5S fluxnum_1: 1 priority: 1 req_1: ONBOARD ACQ FOR 2; req_2: SPATIAL SCAN; ! linenum: 2.000 targname: CRAB-PULSAR config: FOS/BL opmode: ACCUM aperture: 4.3 sp_element: PRISM num_exp: 1 time_per_exp: 1300S fluxnum_1: 1 priority: 1 comment_1: CRAB PULSAR UV SPECTRUM, comment_2: INITIAL VISIT. ! linenum: 3.000 targname: CRAB-PULSAR config: FOS/BL opmode: ACQ/PEAK aperture: 4.3 sp_element: MIRROR num_exp: 1 time_per_exp: 5.0S fluxnum_1: 1 priority: 1 req_1: ONBOARD ACQ FOR 3.5; req_2: SELECT 1 OF 3-4 OR 5-6 req_3: OR 7-8 OR 9-10; req_4: SPATIAL SCAN; comment_1: AFTER 2 BY 60 DAYS. comment_2: GTO TO SELECT ONE OF comment_3: FOUR GRATINGS FOR 2ND comment_4: VISIT AND NOTIFY STSCI. ! linenum: 3.500 targname: CRAB-PULSAR config: FOS/BL opmode: ACQ/PEAK aperture: 1.0 sp_element: MIRROR num_exp: 1 time_per_exp: 7.5S fluxnum_1: 1 priority: 1 req_1: ONBOARD ACQ FOR 4; req_2: SPATIAL SCAN; ! linenum: 4.000 targname: CRAB-PULSAR config: FOS/BL opmode: ACCUM aperture: 4.3 sp_element: G130H num_exp: 1 time_per_exp: 2700S fluxnum_1: 1 priority: 1 ! linenum: 5.000 targname: CRAB-PULSAR config: FOS/BL opmode: ACQ/PEAK aperture: 4.3 sp_element: MIRROR num_exp: 1 time_per_exp: 5.0S fluxnum_1: 1 priority: 1 req_1: ONBOARD ACQ FOR 5.5; req_2: SPATIAL SCAN; ! linenum: 5.500 targname: CRAB-PULSAR config: FOS/BL opmode: ACQ/PEAK aperture: 1.0 sp_element: MIRROR num_exp: 1 time_per_exp: 7.5S fluxnum_1: 1 priority: 1 req_1: ONBOARD ACQ FOR 6; req_2: SPATIAL SCAN; ! linenum: 6.000 targname: CRAB-PULSAR config: FOS/BL opmode: ACCUM aperture: 4.3 sp_element: G190H num_exp: 1 time_per_exp: 2700S fluxnum_1: 1 priority: 1 ! linenum: 7.000 targname: CRAB-PULSAR config: FOS/BL opmode: ACQ/PEAK aperture: 4.3 sp_element: MIRROR num_exp: 1 time_per_exp: 5.0S fluxnum_1: 1 priority: 1 req_1: ONBOARD ACQ FOR 7.5; req_2: SPATIAL SCAN; ! linenum: 7.500 targname: CRAB-PULSAR config: FOS/BL opmode: ACQ/PEAK aperture: 1.0 sp_element: MIRROR num_exp: 1 time_per_exp: 7.5S fluxnum_1: 1 priority: 1 req_1: ONBOARD ACQ FOR 8; req_2: SPATIAL SCAN; ! linenum: 8.000 targname: CRAB-PULSAR config: FOS/BL opmode: ACCUM aperture: 4.3 sp_element: G270H num_exp: 1 time_per_exp: 2700S fluxnum_1: 1 priority: 1 ! linenum: 9.000 targname: CRAB-PULSAR config: FOS/BL opmode: ACQ/PEAK aperture: 4.3 sp_element: MIRROR num_exp: 1 time_per_exp: 5.0S fluxnum_1: 1 priority: 1 req_1: ONBOARD ACQ FOR 9.5; req_2: SPATIAL SCAN; ! linenum: 9.500 targname: CRAB-PULSAR config: FOS/BL opmode: ACQ/PEAK aperture: 1.0 sp_element: MIRROR num_exp: 1 time_per_exp: 7.5S fluxnum_1: 1 priority: 1 req_1: ONBOARD ACQ FOR 10; req_2: SPATIAL SCAN; ! linenum: 10.000 targname: CRAB-PULSAR config: FOS/BL opmode: ACCUM aperture: 4.3 sp_element: PRISM num_exp: 1 time_per_exp: 2700S fluxnum_1: 1 priority: 1 ! ! end of exposure logsheet scan_data: line_list: 1,3,5,7,9 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: 0.0 ! line_list: 1.5,3.5,5.5,7.5,9.5 fgs_scan: cont_dwell: D dwell_pnts: 6 dwell_secs: 1.00 scan_width: 6.7000 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 ! ! end of scan data