! File: 3351O.PROP ! Database: PEPDB ! Date: 19-FEB-1994:04:25:53 coverpage: title_1: SEYFERT GALAXY SURVEY (FOS 14A)-FUTURE CYCLES sci_cat: QUASARS & AGN proposal_for: GTO/FOS pi_fname: ARTHUR pi_mi: F. pi_lname: DAVIDSEN pi_inst: JOHNS HOPKINS UNIVERSITY pi_country: USA pi_phone: 301-338-7000 keywords_1: SEYFERT GALAXIES hours_pri: 5.14 num_pri: 1 wf_pc: Y fos: Y ! end of coverpage abstract: line_1: The purpose of this program is to establish the optical and UV spectral energy line_2: distribution for one of the nearest and brightest Seyfert 2 galaxies, line_3: using the small (0.3") FOS aperture to isolate the broad line and continuum line_4: emission regions. Early PC exposures with filters F502N and F547M will line_5: be used to isolate the exact location of the maximum continuum brightness line_6: from the emission of the narrow line region. The UV continuum line_7: spectra will be used to look for absorption due to the halo of line_8: the Seyfert or intervening clouds. Emission line intensities and profiles line_9: for the broad components will be measured uncontaminated by emission from line_10: the galactic disk or narrow line region. In conjunction with the more line_11: detailed information obtained on brighter Seyferts (FOS 14), this study line_12: will provide another point of comparison for more generally line_13: understanding the Seyfert phenomenon. ! ! end of abstract general_form_proposers: lname: BEAVER fname: EDWARD inst: UC, SAN DIEGO country: USA ! lname: BURBIDGE fname: E. MARGARET inst: UC, SAN DIEGO country: USA ! lname: BARTKO fname: FRANK inst: APPLIED RESEARCH CORP. country: USA ! lname: MARGON fname: BRUCE inst: WASHINGTON, UNIVERSITY OF country: USA ! lname: ANGEL fname: J. ROGER mi: P. inst: ARIZONA, UNIVERSITY OF country: USA ! lname: DAVIDSEN fname: ARTHUR mi: F. inst: JOHNS HOPKINS UNIVERSITY country: USA ! lname: HARMS fname: RICHARD mi: J. inst: APPLIED RESEARCH CORPORATION country: USA ! lname: BOHLIN fname: RALPH inst: SPACE TELESCOPE SCIENCE INSTITUTE country: USA ! lname: FORD fname: HOLLAND mi: C. inst: SPACE TELESCOPE SCIENCE INSTITUTE country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: Exposures with the PC will be used to determine the location of line_2: maximum brightness of the nonthermal continuum line_3: (which may differ from the peak starlight and narrow line emission.) line_4: All observations will be made with the 0.3" circular slit. line_5: Exposure times for T0109-38 are scaled by the ratio of H-alpha flux line_6: to that of NGC1068 over the central 2 x 4 arc seconds. line_7: Exposures are calculated to give a S/N of 10 line_8: per diode for each spectral range from the UV to 6500 A. line_9: Cycle 3 1.03 hours primary, 0 hours parallel line_10: Cycle 4 4.11 hours primary, 0 hours parallel ! question: 5 section: 1 line_1: The SV prerequisite programs for all FOS observations in this line_2: program are: line_3: Prop ID 2195 FOS Target Acquisition Tests All observations line_4: Prop ID 1317 Int./Ext. Wavelength Offsets 1st target line_5: Prop ID 1318 Spectral Flat Fields 1st target line_6: Prop ID 1320 Absolute Spectrophotometry 1st visit of line_7: bright targets line_8: For those programs performing polarimetry, all include the following: line_9: Prop ID 1430 Polarimetric Calibration All observations ! question: 12 section: 1 line_1: ! question: 13 section: 1 line_1: This program will establish the optical and UV spectral energy line_2: distributions of one of the brightest and nearest Seyfert 2 line_3: galaxies using the small FOS aperture (0.3") to isolate the broad line_4: line and continuum emission regions. The UV continuum will be used line_5: as a probe of the Seyfert halo and intervening clouds, and line line_6: intensities and profiles will be used as diagnostics of the dynamics line_7: and physical conditions of the broad line region. ! !end of general form text general_form_address: lname: DAVIDSEN fname: ARTHUR mi: F. category: PI inst: JOHNS HOPKINS UNIVERSITY ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: T0109-38 descr_1: SEYFERT 2 pos_1: TBD-EARLY, pos_2: RA=01H 09M 09.8S +/- 0.2S, pos_3: DEC=-38D 20' 56" +/- 2" equinox: 1950.0 rv_or_z: V=3300 acqpr_1: EXT acqpr_2: BKG fluxnum_1: 1 fluxval_1: V=14.0 +/- 0.10, E(B-V)=0.1 +/- 0.1 ! targnum: 2 name_1: T0109-NUC descr_1: SEYFERT 2 pos_1: TBD-EARLY, pos_2: RA-OFF=0S +/- 40.00S, pos_3: DEC-OFF=0' +/- 10', pos_4: FROM 1 equinox: 1950.0 rv_or_z: V=3300 acqpr_1: EXT acqpr_2: BKG comment_1: POSITION OF NUCLEUS WILL BE comment_2: IDENTIFIED FROM PC PICTURES. fluxnum_1: 1 fluxval_1: V=14.0 +/- 0.10, E(B-V)=0.1 +/- 0.1 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 targname: T0109-38 config: PC opmode: IMAGE aperture: ALL sp_element: F502N num_exp: 1 time_per_exp: 1200S fluxnum_1: 1 priority: 2 param_1: CR-SPLIT=NO, param_2: PRE-FLASH=YES, req_1: EARLY ACQ FOR 3-9; req_2: CYCLE 3 / 1-2; req_3: COND IF TAC OK; ! linenum: 2.000 targname: T0109-38 config: PC opmode: IMAGE aperture: ALL sp_element: F547M num_exp: 1 time_per_exp: 600S fluxnum_1: 1 priority: 2 param_1: CR-SPLIT=NO, param_2: PRE-FLASH=YES, req_1: EARLY ACQ FOR 3-9; req_2: COND IF TAC OK; ! linenum: 3.000 targname: T0109-NUC config: FOS/RD opmode: ACQ/BINARY aperture: 4.3 sp_element: MIRROR num_exp: 1 time_per_exp: 11S fluxnum_1: 1 priority: 2 param_1: BRIGHT = 33000, param_2: FAINT = 660, req_1: ONBOARD ACQ FOR 3.5-6; req_2: REQ DATA FROM 2; req_3: CYCLE 4 / 3 - 9; req_4: SEQ 3-6 NO GAP; req_5: COND IF TAC OK; comment_1: SET REALISTIC BRIGHT AND FAINT LIMITS comment_2: BASED ON PC EXPOSURES. ! linenum: 3.500 targname: T0109-NUC config: FOS/RD opmode: ACQ aperture: 4.3 sp_element: MIRROR num_exp: 1 time_per_exp: 64S priority: 1 req_1: REQ DATA FROM 1-2; req_2: COND IF TAC OK; comment_1: EXPOSURE TIME WILL BE UPDATED comment_2: BASED ON PC PICTURES. comment_3: PICTURE TO VERIFY ACQUISITION. ! linenum: 4.000 targname: T0109-NUC config: FOS/RD opmode: ACCUM aperture: 0.3 sp_element: G270H num_exp: 1 time_per_exp: 1000S fluxnum_1: 1 priority: 2 req_1: COND IF TAC OK; ! linenum: 5.000 targname: T0109-NUC config: FOS/RD opmode: ACCUM aperture: 0.3 sp_element: G570H num_exp: 1 time_per_exp: 1000S fluxnum_1: 1 priority: 2 req_1: COND IF TAC OK; ! linenum: 6.000 targname: T0109-NUC config: FOS/RD opmode: ACCUM aperture: 0.3 sp_element: G400H num_exp: 1 time_per_exp: 2400S fluxnum_1: 1 priority: 2 req_1: COND IF TAC OK; ! linenum: 7.000 targname: T0109-NUC config: FOS/BL opmode: ACQ/BINARY aperture: 4.3 sp_element: MIRROR num_exp: 1 time_per_exp: 11S fluxnum_1: 1 priority: 2 param_1: BRIGHT = 33000, param_2: FAINT = 660, req_1: ONBOARD ACQ FOR 8-9; req_2: REQ DATA FROM 2; req_3: SEQ 7-9 NO GAP; req_4: COND IF TAC OK; comment_1: SET REALISTIC BRIGHT AND FAINT LIMITS comment_2: BASED ON PC EXPOSURES. ! linenum: 7.500 targname: T0109-NUC config: FOS/BL opmode: ACQ aperture: 4.3 sp_element: MIRROR num_exp: 1 time_per_exp: 64S priority: 1 req_1: REQ DATA FROM 1-2; req_2: COND IF TAC OK; comment_1: EXPOSURE TIME WILL BE UPDATED comment_2: BASED ON PC PICTURES. comment_3: PICTURE TO VERIFY ACQUISITION. ! linenum: 8.000 targname: T0109-NUC config: FOS/BL opmode: ACCUM aperture: 0.3 sp_element: G130H num_exp: 1 time_per_exp: 4000S fluxnum_1: 1 priority: 2 req_1: COND IF TAC OK; comment_1: LONG EXPOSURE MAY BE SPLIT BY SAA comment_2: OR EARTH OCCULTATION. ! linenum: 9.000 targname: T0109-NUC config: FOS/BL opmode: ACCUM aperture: 0.3 sp_element: G190H num_exp: 1 time_per_exp: 2400S fluxnum_1: 1 priority: 2 req_1: COND IF TAC OK; ! ! end of exposure logsheet ! No scan data records found