! File: 4847C.PROP ! Database: PEPDB ! Date: 23-FEB-1994:05:58:03 coverpage: title_1: SPECTROPOLARIMETRY OF QSOS, BLAZARS AND AGN: CYCLE 3 - HIGH sci_cat: QUASARS & AGN proposal_for: GTO/FOS cont_id: 1029 pi_fname: J. ROGER pi_mi: P pi_lname: ANGEL pi_inst: UNIVERSITY OF ARIZONA pi_country: USA keywords_1: QSOS, BLAZARS, SEYFERT, AGN, POLARIZATION hours_pri: 7.84 num_pri: 2 fos: Y ! end of coverpage abstract: line_1: Measurement of the spectrum of polarization has proven to be a powerful tool in line_2: deciphering emission processes and source geometry in AGN. This program will line_3: extend these observations into the UV below 3000A. These observations must be line_4: completed before COSTAR is installed in HST. ! ! end of abstract general_form_proposers: lname: BEAVER fname: EDWARD title: DR. inst: UC, SAN DIEGO country: USA ! lname: BURBIDGE fname: E. MARGARET title: DR. inst: UC, SAN DIEGO country: USA ! lname: ANGEL fname: J. ROGER title: DR. mi: P inst: UNIVERSITY OF ARIZONA country: USA ! lname: MARGON fname: BRUCE title: DR. inst: WASHINGTON, UNIVERSITY OF country: USA ! lname: FORD fname: HOLLAND title: DR. mi: C inst: JOHNS HOPKINS UNIVERSITY country: USA ! lname: BARTKO fname: FRANK title: DR. inst: MARTIN MARIETTA CORPORATION country: USA ! lname: DAVIDSEN fname: ARTHUR title: DR. mi: F inst: JOHNS HOPKINS UNIVERSITY country: USA ! lname: HARMS fname: RICHARD title: DR. mi: J inst: APPLIED RESEARCH CORPORATION country: USA ! lname: BOHLIN fname: RALPH title: DR. inst: SPACE TELESCOPE SCIENCE INSTITUTE country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: The spectrum of polarization for a number of AGN of diverse type will be line_2: observed with the FOS spectropolarimeter. Targets include a Seyfert line_3: galaxy and a BL Lac object. These observations must be completed before the line_4: corrective mirrors of COSTAR are placed in front of the FOS entrance apertures. ! question: 4 section: 1 line_1: The ST is needed to do spectropolarimetry below 3000A. ! question: 5 section: 1 line_1: Blazars are so rapidly variable that any observation must be completed within a line_2: few hours. line_3: The SV prerequisite programs for all FOS observations in this program are: line_4: Prop ID 2195 FOS Target Acquisition Tests All observations line_5: Prop ID 1317 Int./Ext. Wavelength Offsets 1st target line_6: Prop ID 1318 Spectral Flat Fields 1st target line_7: Prop ID 1320 Absolute Spectrophotometry 1st visit of bright targets line_8: Prop ID 1430 Polarimetric y-bases (lines 103,104) and polarimetric line_9: wavelength calibrations (lines 105,106) ! question: 13 section: 1 line_1: Spectropolarimetry of QSOs, BL Lac objects, Blazars, Seyferts, and other AGN, line_2: are obtained in order to decipher emission and scattering processes and source line_3: geometry. These observations must be completed before the corrective mirrors line_4: of COSTAR are placed in front of the FOS entrance apertures. ! !end of general form text general_form_address: lname: ALLEN fname: RICHARD title: DR. category: CON inst: STEWARD OBSERVATORY addr_1: UNIVERSITY OF ARIZONA city: TUCSON state: AZ zip: 85721 country: USA phone: 602-621-7661 telex: 467175 ! lname: ANGEL fname: J. ROGER mi: P. title: DR. category: PI inst: STEWARD OBSERVATORY addr_1: UNIVERSITY OF ARIZONA city: TUCSON state: AZ zip: 85721 country: USA phone: 602-621-7661 telex: 467175 ! ! end of general_form_address records fixed_targets: targnum: 18 name_1: H0323+022 descr_1: E,316 pos_1: RA=3H 26M 13.92S +/- 1", pos_2: DEC=2D 25' 14.7" +/- 1", pos_3: PLATE-ID=0174 equinox: 2000 pm_or_par: NO rv_or_z: Z=.147 comment_1: VARIABLE OBJECT; PHOTOMETRIC comment_2: RANGE OF ABOUT 1 MAG; comment_3: V MAGNITUDE GIVEN IS AVERAGE; comment_4: OBSERVATION MUST TAKE PLACE BEFORE comment_5: COSTAR IS INSTALLED fluxnum_1: 1 fluxval_1: V=16.60 +/- 0.5 fluxnum_2: 1 fluxval_2: B-V=0.50 fluxnum_3: 2 fluxval_3: E(B-V)=0.0 ! targnum: 22 name_1: MRK486 descr_1: E,312 pos_1: RA=15H 36M 38.36S +/- 1", pos_2: DEC=54D 33' 33.1" +/- 1", pos_3: PLATE-ID=01BT, equinox: 2000 pm_or_par: NO rv_or_z: Z=.039 comment_1: VARIABLE OBJECT; PHOTOMETRIC comment_2: RANGE ABOUT 0.5 MAG; comment_3: V MAGNITUDE GIVEN IS AVERAGE; comment_4: OBSERVATION MUST TAKE PLACE BEFORE comment_5: COSTAR IS INSTALLED fluxnum_1: 1 fluxval_1: V=14.80 +/- 0.25 fluxnum_2: 1 fluxval_2: B-V=0.40 +/- 0.20 fluxnum_3: 2 fluxval_3: E(B-V)=0.0 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 70.000 targname: H0323+022 config: FOS/BL opmode: ACQ/PEAK aperture: 4.3 sp_element: MIRROR num_exp: 1 time_per_exp: 8S priority: 1 req_1: CYCLE 3 / 70.0-72.0; req_2: SEQ 70.0-72.0 NO GAP; req_3: ONBOARD ACQ FOR 70.5; req_4: SPATIAL SCAN; req_5: AFTER 12-SEP-93; req_6: BEFORE 20-DEC-93; comment_1: PHASE REQUIREMENT TO COORDINATE comment_2: SIMULTANEOUS GROUND-BASED OBSERVATIONS comment_3: WITH "DARK" LUNAR PHASE comment_4: (BETWEEN FIRST AND LAST QUARTERS) ! linenum: 70.500 targname: H0323+022 config: FOS/BL opmode: ACQ/PEAK aperture: 1.0 sp_element: MIRROR num_exp: 1 time_per_exp: 12S priority: 1 req_1: ONBOARD ACQ FOR 71.0-72.0; req_2: SPATIAL SCAN; req_3: PERIOD 29.531D +/- .001D; req_4: ZERO-PHASE JD2449158.578 +/- .001D; req_5: PHASE 0.0 +/- .125 ! linenum: 71.000 targname: H0323+022 config: FOS/BL opmode: ACCUM aperture: 4.3 sp_element: G190H wavelength: 1600-2300 num_exp: 1 time_per_exp: 1440S priority: 1 param_1: POLSCAN=8B ! linenum: 71.100 targname: H0323+022 config: FOS/BL opmode: ACCUM aperture: 4.3 sp_element: G270H wavelength: 2227-3306 num_exp: 1 time_per_exp: 1440S priority: 1 param_1: POLSCAN=8B ! linenum: 71.200 targname: H0323+022 config: FOS/BL opmode: ACCUM aperture: 4.3 sp_element: G190H wavelength: 1600-2300 num_exp: 1 time_per_exp: 1440S priority: 1 param_1: POLSCAN=8B ! linenum: 71.300 targname: H0323+022 config: FOS/BL opmode: ACCUM aperture: 4.3 sp_element: G190H wavelength: 1600-2300 num_exp: 1 time_per_exp: 1440S priority: 1 param_1: POLSCAN=8B ! linenum: 71.400 targname: H0323+022 config: FOS/BL opmode: ACCUM aperture: 4.3 sp_element: G270H wavelength: 2227-3306 num_exp: 1 time_per_exp: 1440S priority: 1 param_1: POLSCAN=8B ! linenum: 72.000 targname: H0323+022 config: FOS/BL opmode: ACCUM aperture: 4.3 sp_element: G190H wavelength: 1600-2300 num_exp: 1 time_per_exp: 1440S priority: 1 param_1: POLSCAN=8B ! linenum: 88.000 targname: MRK486 config: FOS/BL opmode: ACQ/BINARY aperture: 4.3 sp_element: MIRROR num_exp: 1 time_per_exp: 6.6S priority: 1 param_1: BRIGHT = 720000 req_1: CYCLE 3 / 88.0-89.3; req_2: SEQ 88.0-89.3 NO GAP; req_3: ONBOARD ACQ FOR 89.1-89.3; req_4: PHASE 0.0 +/- .125 OF REF 70.5 ! linenum: 89.100 targname: MRK486 config: FOS/BL opmode: ACCUM aperture: 4.3 sp_element: G190H wavelength: 1600-2300 num_exp: 1 time_per_exp: 1440S priority: 1 param_1: POLSCAN=8B ! linenum: 89.200 targname: MRK486 config: FOS/BL opmode: ACCUM aperture: 4.3 sp_element: G270H wavelength: 2227-3306 num_exp: 1 time_per_exp: 1440S priority: 1 param_1: POLSCAN=8B ! linenum: 89.300 targname: MRK486 config: FOS/BL opmode: ACCUM aperture: 4.3 sp_element: G190H wavelength: 1600-2300 num_exp: 1 time_per_exp: 1440S priority: 1 param_1: POLSCAN=8B ! ! end of exposure logsheet scan_data: line_list: 70.0 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: 70.5 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 ! ! end of scan data