! File: 1233C.PROP ! Database: PEPDB ! Date: 16-FEB-1994:07:06:02 coverpage: title_1: NARROW BAND IMAGING OF QUASARS -- CYCLE 0 sci_cat: QUASARS & AGN sci_subcat: HOST GALAXY proposal_for: GTO/FOC pi_fname: F. DUCCIO pi_lname: MACCHETTO pi_inst: ESA, SPACE TELESCOPE SCIENCE INSTITUTE pi_country: USA pi_phone: (301) 338-4790 keywords_1: QUASARS, IMAGING, NARROW LINE EMISSION hours_pri: 10.00 num_pri: 11 pi_position: CHIEF, ISB ! end of coverpage abstract: line_1: It has long been thought that quasars may be powered by the infall of gas, line_2: either from within the parent galaxy or from outside. It has also been thought line_3: that quasars may expel gas into the intergalactic medium, leading to line_4: large-scale enrichment at an early epoch. In either case, one may expect to line_5: find gas within the parent galaxies of quasars, and large gaseous halos around line_6: them. Other possibilities have been suggested - protogalactic disks, line_7: protoclusters, residual pancake structures - the remains of which might also line_8: appear as halos around quasars. Narrow-band observations of quasars with the line_9: ST will not only address these fundamental issues, but will at the same time line_10: touch on several others, including the nature of the parent galaxy, its line_11: evolution with redshift, the presence of nearby galaxies and possible line_12: protogalaxies, and the nature of the objects causing quasar absorption lines. ! ! end of abstract general_form_proposers: lname: PERRYMAN fname: M. A. C. inst: ESA, ESTEC country: NETHERLANDS esa: X ! lname: SHAVER fname: P. inst: EUROPEAN SOUTHERN OBSERVATORY country: GERMANY, WEST esa: X ! lname: MACCHETTO fname: F. DUCCIO inst: ESA, SPACE TELESCOPE SCIENCE INSTITUTE country: USA esa: X ! lname: DI SEREGO ALIGHIERI fname: S. inst: ESA, EUROPEAN COORDINATING FACILITY country: ITALY esa: X ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: Observations for Cycle 0 are those in Exposure Logsheet Nos.: 22 and 23. line_3: The total duration is 1 hour. line_5: All other observations will be done in subsequent cycles. ! question: 13 section: 1 line_1: It has long been thought that quasars may be powered by the infall of gas, line_2: either from within the parent galaxy or from outside. It has also been thought line_3: that quasars may expel gas into the intergalactic medium, leading to line_4: large-scale enrichment at an early epoch. In either case, one may expect to line_5: find gas within the parent galaxies of quasars, and large gaseous halos around line_6: thhem. Other possibilities have been suggested - protogalactic disks, line_7: protoclusters, residual pancake structures - the remains of which might also line_8: appear as halos around quasars. Narrow-band observations of quasars with the line_9: ST will not only address these fundamental issues, but will at the same time line_10: touch on several others, including the nature of the parent galaxy, its line_11: evolutin with redshift, the presence of nearby galaxies and possible line_12: protogalaxies, and the nature of the objects causing quasar absorption lines. ! !end of general form text general_form_address: lname: MACCHETTO fname: F. DUCCIO title: DR. category: PI inst: SPACE TELESCOPE SCIENCE INSTITUTE addr_1: HOMEWOOD CAMPUS city: BALTIMORE state: MD zip: 21218 country: USA phone: 301-338-4790 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: UM253 descr_1: ASSOCIATED ABSORPTION QSO PAIR pos_1: RA = 00H 29M 01.8S +/- 0.1S, pos_2: DEC = 00D 17' 49" +/- 1" equinox: 1950 rv_or_z: Z=1.732 fluxnum_1: 1 fluxval_1: V=18.5 ! targnum: 2 name_1: PHL1186-GROUP descr_1: QSO WITH COMPANION GALAXY pos_1: RA = 01H 47M 46.69S +/- 0.02S, pos_2: DEC = 09D 00' 01.7" +/- 0.5" equinox: 1950 rv_or_z: Z=0.270 acqpr_1: EXT fluxnum_1: 1 fluxval_1: V=17.4 ! targnum: 3 name_1: MARK1014 descr_1: INTERACTING SEYFERT 1 GALAXY pos_1: RA = 01H 57M 15.8S +/- 0.1S, pos_2: DEC = 00D 09' 10" +/- 1" equinox: 1950 rv_or_z: Z=0.163 acqpr_1: EXT fluxnum_1: 1 fluxval_1: V=15.69 ! targnum: 4 name_1: PKS0349-27 descr_1: RADIO GALAXY WITH IONIZED GAS AND JET pos_1: RA = 03H 49M 31.93S +/- 0.02S, pos_2: DEC = -27D 53' 31.0" +/- 0.7" equinox: 1950 rv_or_z: Z=0.066 acqpr_1: EXT fluxnum_1: 1 fluxval_1: V=16 fluxnum_2: 2 fluxval_2: B=16.8 ! targnum: 5 name_1: PKS0952+179 descr_1: QSO WITH LOW-REDSHIFT NARROW ABSORPTION SY descr_2: STEM pos_1: RA = 09H 52M 11.84S +/- 0.02S, pos_2: DEC = 17D 57' 44.5" +/- 0.2" equinox: 1950 rv_or_z: Z=0.238 fluxnum_1: 1 fluxval_1: V=17.23 ! targnum: 6 name_1: PG1001+05 descr_1: RADIO-QUIET QSO pos_1: RA = 10H 01M 43.31S +/- 0.05S, pos_2: DEC = 05D 27' 35.3" +/- 0.5" equinox: 1950 rv_or_z: Z=0.161 fluxnum_1: 1 fluxval_1: V=16.38 ! targnum: 7 name_1: MC1548+114A+B descr_1: QSO PAIR WITH NEARBY GALAXIES pos_1: RA = 15H 48M 21.38S +/- 0.02S, pos_2: DEC = 11D 29' 47.0" +/- 0.2" equinox: 1950 rv_or_z: Z=0.436 comment_1: FLUXVAL_2 IS FOR THE GALAXY comment_2: UNDERLYING OBJECT A AT O.5" comment_3: FROM THE NUCLEUS. fluxnum_1: 1 fluxval_1: V=17.23 fluxnum_2: 2 fluxval_2: SURF(R) = 19.0 +/- 0.5 ! targnum: 8 name_1: 3C332.0 descr_1: RADIO-LOUD QSO pos_1: RA = 16H 15M 47.1S +/- 0.1S, pos_2: DEC = 32D 29' 50" +/- 1" equinox: 1950 rv_or_z: Z=0.152 acqpr_1: EXT fluxnum_1: 1 fluxval_1: V=16 ! targnum: 9 name_1: PKS2135-147 descr_1: QSO WITH NARROW ABSORPTION AT EMISSION RED descr_2: SHIFT pos_1: RA = 21H 35M 01.21S +/- 0.02S, pos_2: DEC = -14D 46' 27.3" +/- 0.2" equinox: 1950 rv_or_z: Z=0.200 fluxnum_1: 1 fluxval_1: V=15.53 ! targnum: 10 name_1: QSO2206-199N descr_1: QSO WITH TWO BROAD LYMAN-ALPHA ABSORP. FEA descr_2: TURES pos_1: RA = 22H 06M 06.9S +/- 0.1S, pos_2: DEC = -19D 58' 45" +/- 1" equinox: 1950 rv_or_z: Z=2.076 fluxnum_1: 1 fluxval_1: V=17.33 ! targnum: 11 name_1: MR2251-178 descr_1: QSO WITH LARGE GASEOUS HALO pos_1: RA = 22H 51M 25.89S +/- 0.1S, pos_2: DEC = -17D 50' 54" +/- 1" equinox: 1950 rv_or_z: Z=0.068 fluxnum_1: 1 fluxval_1: V=14.11 ! targnum: 12 name_1: 3C227 descr_1: GALAXY; AGN; RADIO GALAXY; TYPE=N pos_1: RA = 9H 45M 6.5S +/- 0.1S, pos_2: DEC = 7D 39' 17" +/- 1" equinox: 1950 rv_or_z: Z=0.0877 comment_1: FLUXVAL_2 AND FLUXVAL_3 ARE comment_2: FOR THE GALAXY AT 3" comment_3: FROM THE NUCLEUS. fluxnum_1: 1 fluxval_1: V=16.33 fluxnum_2: 2 fluxval_2: SURF-LINE(5007) = 20 +/- 5 E-16 fluxnum_3: 3 fluxval_3: SURF-CONT(5100) = 65 +/- 15 E-19 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 22.000 targname: MR2251-178 config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: F130M num_exp: 1 time_per_exp: 40M priority: 1 req_1: CYCLE 0 comment_1: CAN BE SPLIT INTO TWO 20M EXPOSURES comment_2: IF NECESSARY ! linenum: 23.000 targname: MR2251-178 config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: F190M num_exp: 1 time_per_exp: 40M priority: 1 req_1: CYCLE 0 comment_1: CAN BE SPLIT INTO TWO 20M EXPOSURES comment_2: IF NECESSARY ! linenum: 24.000 targname: MR2251-178 config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: F550M num_exp: 1 time_per_exp: 40M priority: 1 req_1: CYCLE 0 comment_1: CAN BE SPLIT INTO TWO 20M EXPOSURES comment_2: IF NECESSARY ! linenum: 24.100 targname: MR2251-178 config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: F502M num_exp: 1 time_per_exp: 40M priority: 1 req_1: CYCLE 0 comment_1: CAN BE SPLIT INTO TWO 20M EXPOSURES comment_2: IF NECESSARY ! ! end of exposure logsheet ! No scan data records found