! $Id: 5124,v 11.1 1994/12/08 20:45:38 pepsa Exp $ coverpage: title_1: IMAGING AND SPECTROPHOTOMETRY OF SEYFERT NUCLEI (FOS 14): title_2: CYCLE 4 OBSERVATIONS sci_cat: QUASARS & AGN proposal_for: GTO/FOS cont_id: 1036 pi_title: DR. pi_fname: HOLLAND pi_mi: C. pi_lname: FORD pi_inst: SPACE TELESCOPE SCIENCE INSTITUTE pi_country: USA pi_phone: (410) 338-4803 keywords_1: SEYFERT, AGN, IONIZED GAS, NUCLEUS, NARROW LINE keywords_2: REGION, BROAD LINE REGION hours_pri: 9.14 num_pri: 3 wf_pc: Y ! end of coverpage abstract: line_1: WF/PC narrow band images will be used to isolate clouds near the nucleus and to line_2: look for organized structure such as disks, bubbles, and jets. FOS line_3: spectrophotometry from 1200A to 7000A will be used to establish density, line_4: temperature, chemical composition, ionization mechanisms, and reddening in the line_5: emission regions near the nucleus. Line profiles and radial velocities will be line_6: used to investigate broadening mechanisms near the nucleus such as turbulence, line_7: gas flows, and rotation. Small aperture FOS spectra of the nuclei will be used line_8: to separate the broad line region from the narrow line region. The spectra line_9: will be used to investigate physical conditions and gas dynamics in the broad line_10: line region. Absorption lines in the nuclear spectra will be used to measure line_11: the amount and distribution of gas along the line of sight through the parent line_12: galaxy. ! ! 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: MARGON fname: BRUCE inst: WASHINGTON, UNIVERSITY OF country: USA ! lname: ANGEL fname: J. ROGER mi: P. inst: ARIZONA, UNIVERSITY OF country: USA ! lname: BARTKO fname: FRANK inst: APPLIED RESEARCH CORPORATION 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: We will obtain WFPC2 images of NGC4151 and line_2: NGC4261 as specified in the exposure logsheet. For each target line_3: all exposures should be obtained at the same pointing and roll line_4: angle. CR-SPLITs should be as specified, normally 0.333 (2:1) line_5: for long exposures to maximize dynamic range, and upsplit for short line_6: exposures. NGC4151 and NGC4261 should be placed at the PC1 line_7: aperture location. ANY CHANGES TO THIS PROGRAM MUST HAVE SIGNED line_11: APPROVAL BY THE PI OR HIS DESIGNEE. Cycle 4: 401-422 ! question: 5 section: 2 line_1: The SV prerequisite programs for all FOS line_2: observations in this program are: line_3: Prop ID 2195 FOS Target Acquisition Tests line_4: - All observations line_5: Prop ID 1317 Int./Ext. Wavelength Offsets line_6: - 1st target line_7: Prop ID 1318 Spectral Flat Fields line_8: - 1st target line_9: Prop ID 1320 Absolute Spectrophotometry line_10: - 1st visit of bright targets line_11: All WF/PC imaging with a center wavelength line_12: blueward of 5000 Angstroms requires UV flood ! question: 12 section: 1 line_1: This is an integrated program to study the morpholgy, dynamics, and ionization line_2: of the narrow line region in Type 1 and Type 2 Seyfert galaxies. The program line_3: will not be complete until 7 of the 12 Seyferts have been observed. Data line_4: release should not begin until one year after the seventh Seyfert has been line_5: completed. ! question: 13 section: 1 line_1: WF/PC images will be used to study the structure of the narrow line region line_2: (NLR) in low redshift Seyferts. FOS spectra will used to establish physical line_3: conditions, chemical composition, ionization mechanisms and dynamics of line_4: individual clouds in the NLR. Small-aperture spectra of the nucleus will be line_5: used to isolate the broad line region (BLR) and to study physical condition line_6: and gas motion in the BLR. ! !end of general form text general_form_address: lname: FORD fname: HOLLAND mi: C. title: DR. category: PI inst: SPACE TELESCOPE SCIENCE INSTITUTE addr_1: HOMEWOOD CAMPUS addr_2: 3700 SAN MARTIN DRIVE city: BALTIMORE state: MD zip: 21218 country: USA phone: (410) 338-4803 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: NGC4151 descr_1: E,301,312,910,923,924 pos_1: RA=12H 10M 32.537S +/- 0.3", pos_2: DEC=+39D 24' 21.12" +/- 0.3", pos_3: PLATE-ID=01QY equinox: 2000 rv_or_z: V=900 fluxnum_1: 1 fluxval_1: V=12.00, E(B-V)=0.050 ! targnum: 3 name_1: NGC4261 descr_1: E,312,910 pos_1: RA=12H 19M 23.165S +/- 0.3", pos_2: DEC=+05D 49' 30.89" +/- 0.3", pos_3: PLATE-ID=01UQ equinox: 2000 rv_or_z: V=2210 fluxnum_1: 1 fluxval_1: V=11.4 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 401.000 targname: NGC4151 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F502N num_exp: 1 time_per_exp: 900S fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.333 req_1: SAME POS FOR 402-414 AS 401; req_2: GROUP 401-412 NO GAP; req_3: CYCLE 4 / 401-422 ! linenum: 402.000 targname: NGC4151 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F502N num_exp: 1 time_per_exp: 10S fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=NO ! linenum: 403.000 targname: NGC4151 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F658N num_exp: 1 time_per_exp: 900S fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.333 ! linenum: 404.000 targname: NGC4151 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F658N num_exp: 1 time_per_exp: 10S fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=NO ! linenum: 405.000 targname: NGC4151 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F547M num_exp: 1 time_per_exp: 300S fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=NO ! linenum: 406.000 targname: NGC4151 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F547M num_exp: 1 time_per_exp: 10S fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=NO ! linenum: 407.000 targname: NGC4151 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F375N num_exp: 1 time_per_exp: 1800S fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.333 ! linenum: 408.000 targname: NGC4151 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F375N num_exp: 1 time_per_exp: 10S fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=NO ! linenum: 409.000 targname: NGC4151 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F336W num_exp: 1 time_per_exp: 900S fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.333 ! linenum: 410.000 targname: NGC4151 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F336W num_exp: 1 time_per_exp: 10S fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=NO ! linenum: 411.000 targname: NGC4151 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F218W num_exp: 1 time_per_exp: 2400S fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=0.333 ! linenum: 412.000 targname: NGC4151 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F218W num_exp: 1 time_per_exp: 90S fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=NO ! linenum: 413.000 targname: NGC4151 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F791W num_exp: 1 time_per_exp: 300S fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=NO ! linenum: 414.000 targname: NGC4151 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F791W num_exp: 1 time_per_exp: 10S fluxnum_1: 1 priority: 1 param_1: CR-SPLIT=NO ! linenum: 420.000 targname: NGC4261 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F675W num_exp: 1 time_per_exp: 2100S priority: 1 param_1: CR-SPLIT=0.5 req_1: GROUP 420-422 NO GAP; req_2: SAME POS FOR 421-422 AS 420 ! linenum: 421.000 targname: NGC4261 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F547M num_exp: 1 time_per_exp: 900S priority: 1 param_1: CR-SPLIT=0.5 ! linenum: 422.000 targname: NGC4261 config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F791W num_exp: 1 time_per_exp: 900S priority: 1 param_1: CR-SPLIT=0.5 ! ! end of exposure logsheet ! No scan data records found