! File: 1170C.PROP ! Database: PEPDB ! Date: 16-FEB-1994:04:31:29 coverpage: title_1: UV SPECTROSCOPY OF LOW-REDSHIFT ACTIVE GALAXIES -- CYCLE 0 sci_cat: QUASARS & AGN sci_subcat: QUASAR EMISSION proposal_for: GTO/HRS pi_title: DR. pi_fname: ALBERT pi_lname: BOGGESS pi_inst: NASA, GODDARD SPACE FLIGHT CENTER pi_country: USA pi_phone: (301)344-5975 keywords_1: ACTIVE GALACTIC NUCLEI, SEYFERT, LINE PROFILES, BROAD keywords_2: LINE REGION, NARROW LINE REGION hours_pri: 12.70 num_pri: 9 pi_position: DR ! end of coverpage abstract: line_1: HRS will be used to measure the ultraviolet spectrum of active galaxies. line_2: Complementary and simultaneous visual and infrared data will also be obtained. line_3: The profile of the emission lines will provide information on the broadening line_4: mechanism and dynamics of the emitting regions. Comparison of the profile and line_5: radial velocity of the emission lines produced by species of different ioni- line_6: zation potential will allow the study of the thermal and density stratification line_7: of the emitting regions. The degree of asymmetry of lines at different wave- line_8: lengths will allow the absorbing material be identified and located. The ratio line_9: of the UV to visible lines, such as those for O I and He II will be used to line_10: estimate the reddening along the line of sight. Ratio of emission line fluxes line_11: will be compared with models in order to derive the ionization mechanism, elec- line_12: tron temperature and density, and chemical composition of the emitting gas. line_13: The emission line properties of low luminosity will be compared with those of line_14: high luminosity objects in order to investigate the covering factor and line_15: evolutionary effects. The continumm spectrum from the UV to the IR will be line_16: used to establish the emission mechanism and the nature and luminosity of the line_17: energy source. The weak absorption lines will be used to establish the line_18: physical conditions and the chemical composition of the gas in: our Galaxy, line_19: intergalactic medium and the parent galaxy. Absorption produced by broad line line_20: clouds will give information on cloud motion and covering factor. ! ! end of abstract general_form_proposers: lname: WU fname: CHI-CHAO inst: COMPUTER SCIENCE CORPORATION country: USA ! lname: BOGGESS fname: ALBERT inst: NASA, GODDARD SPACE FLIGHT CENTER country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: Cycle 0: Object: Fairall 9 Exposures: 1-13 line_4: Cycle 1: Object: NGC 5548 26-38 line_5: Cycle 1: Object: Mrk 509 51-61 line_6: Cycle 2: Object: ESO 141-G55 Exposures: 14-25 line_7: Cycle 2: Object: Mrk 335 99-106 line_8: Cycle 2: Object: Akn 120 62-72 line_9: Cycle 3: Object: NGC 1068 39-50 line_10: Cycle 3: Object: MCG-2-58-22 73-87 line_11: Cycle 3: Object: NGC 3783 88-98 line_13: All these objects have semi-point-source nucleus. ! question: 12 section: 1 line_1: Data for Fairall 9 (cycle 0) will be published shortly after they are line_2: taken and analyzed, so they can be released according to normal procedures. line_3: However, for the cycle 1 objects, we need to combine the data from all of them line_4: for several studies, such as comparison of line profiles and their correlation line_5: with luminosity (e.g. with optical observations of high redshift quasars), the line_6: range of properties of active galaxies and the statistical significance of line_7: various observed phenomena, etc. Therefore, we request that the data for the line_8: cycle 1 objects not be released until one year after all the exposures are line_9: taken and all the data sent to our group. ! question: 13 section: 1 line_1: HRS UV spectra of active galaxies, complemented by visible and IR data line_2: will be used to study: the dynamics, physical conditions (and their line_3: stratification), chemical composition and the emission mechanism(s) of the line_4: emitting regions. Reddening in the emitting regions and along the line of line_5: sight will be estimated. The effects of luminosity and covering factor will be line_6: investigated. The absorption lines will be used to estimate the covering line_7: factor in the broad line region and the gas along the line of sight. ! !end of general form text general_form_address: lname: BOGGESS fname: ALBERT title: DR. category: PI inst: NASA, GODDARD SPACE FLIGHT CENTER addr_1: CODE 400.2 city: GREENBELT state: MD zip: 20771 country: USA phone: 301-344-5975 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: FAIRALL9 name_2: ESO 113-IG45 descr_1: GALAXY; AGN; SEYFERT; TYPE 1 pos_1: RA=01H23M45.721S +/-0.5", pos_2: DEC=-58D48'21.84" +/-0.5" equinox: 2000 rv_or_z: V=13630 fluxnum_1: 1 fluxval_1: V=13.2+/-0.5 fluxnum_2: 2 fluxval_2: F-CONT(1520)=9.4+/-2.E-14 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 targname: FAIRALL9 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 57.8S s_to_n: 10 fluxnum_1: 1 priority: 1 param_1: SEARCH-SIZE=5, param_2: MAP=END-POINT, param_3: FAINT=100, param_4: LOCATE=NO req_1: ONBOARD ACQ FOR 1.4; req_2: CYCLE 0 / 1-13 comment_1: STEP-TIME = 0.2 SEC ! linenum: 1.400 targname: ^ config: ^ opmode: ACQ/PEAKUP aperture: ^ sp_element: ^ num_exp: 1 time_per_exp: 73.6S s_to_n: ^ fluxnum_1: 1 priority: 1 req_1: ONBOARD ACQ FOR 1.5 comment_1: STEP-TIME = 1.6 SEC ! linenum: 1.500 targname: ^ config: ^ opmode: ACQ aperture: ^ sp_element: ^ num_exp: 1 time_per_exp: 53.0S s_to_n: ^ fluxnum_1: 1 priority: 1 param_1: SEARCH-SIZE=1, param_2: MAP=END-POINT, param_3: LOCATE=NO, param_4: FAINT=0 req_1: ONBOARD ACQ FOR 2-13 comment_1: TAKE MAP AFTER CENTERING comment_2: 200 MSEC INTEGRATIONS ! linenum: 2.000 targname: ^ config: ^ opmode: ACCUM aperture: ^ sp_element: G140L wavelength: 1315 num_exp: ^ time_per_exp: 18M s_to_n: 50 fluxnum_1: 2 priority: 1 param_1: FP-SPLIT = STD ! linenum: 3.000 targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 1590 num_exp: ^ time_per_exp: 25M s_to_n: ^ fluxnum_1: ^ priority: 2 param_1: FP-SPLIT = STD ! linenum: 4.000 targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: G200M wavelength: 1940 num_exp: ^ time_per_exp: 4M s_to_n: 5 fluxnum_1: ^ priority: 3 ! linenum: 5.000 targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 1978 num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ ! linenum: 6.000 targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 2014 num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ ! linenum: 7.000 targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 2052 num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ ! linenum: 8.000 targname: FAIRALL9 config: HRS opmode: ACCUM aperture: 2.0 sp_element: G270M wavelength: 2829 num_exp: 1 time_per_exp: 2M s_to_n: 5 fluxnum_1: 2 priority: 3 ! linenum: 9.000 targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 2869 num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ ! linenum: 10.000 targname: FAIRALL9 config: HRS opmode: ACCUM aperture: 2.0 sp_element: G270M wavelength: 2909 num_exp: 1 time_per_exp: 3M s_to_n: 5 fluxnum_1: 2 priority: 3 ! linenum: 11.000 targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 2945 num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ ! linenum: 12.000 targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 2985 num_exp: ^ time_per_exp: ^ s_to_n: ^ fluxnum_1: ^ priority: ^ ! linenum: 13.000 targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: ^ wavelength: 3025 num_exp: ^ time_per_exp: 4M s_to_n: ^ fluxnum_1: ^ priority: ^ ! ! end of exposure logsheet ! No scan data records found