! File: 1194C.PROP ! Database: PEPDB ! Date: 16-FEB-1994:05:28:33 coverpage: title_1: IMAGING AND SPECTROSCOPY OF THE NEARBY QSO 2130+099: title_2: FUTURE-CYCLE CONTINUATION sci_cat: QUASARS & AGN sci_subcat: QUASAR ABSORPTION proposal_for: GTO/HRS pi_fname: SARA pi_lname: HEAP pi_inst: NASA/GSFC pi_country: USA pi_phone: 301-286-5359 keywords_1: QUASARS, SPIRAL GALAXY, STELLAR POPULATION, MORPHOLOGY hours_pri: 5.00 num_pri: 1 ! end of coverpage abstract: line_1: We will make four types of observations of the nearby QSO line_2: 2130+099: (1) images with the PC: (2) UV maps of the nucleus line_3: with the GHRS N2 mirror; (3) UV spectrum of the nucleus line_4: with either FOS or GHRS/D1 and (4) UV spectrum of a knot line_5: in the spiral arm of the host galaxy. ! ! end of abstract general_form_proposers: lname: HEAP fname: SARA inst: NASA/GSFC country: USA ! ! end of general_form_proposers block general_form_text: question: 2 section: 1 line_1: QSO 2130+099 is a nearby QSO with z=0.061 and v=14.4. Our line_2: recent studies of this object including image-deconvolution line_3: indicate that the host galaxy is a barred spiral with a central line_4: surface brightness, mu(B)=21.3 mag per sq. arcsec and a scale line_5: length of 4 kpc. We will continue our studies of this object line_6: with the HST/WFPC and GHRS by making four types of line_7: observations: (1) images of the quasar-host galaxy with the line_8: PC; (2) UV maps of the nucleus with the GHRS; (3) UV spectrum line_9: of the nucleus with the GHRS; and (4) off-nuclear ultraviolet line_10: spectrum of the host galaxy with the GHRS. We shall use the line_11: UV spectrum of the nucleus to search for "nearby" Lyman line_12: alpha clouds. ! question: 3 section: 1 line_1: Schedule in Cycle 3 AFTER the repair mission. line_2: Schedule the GHRS observations in dark time, so that line_3: geocoronal Ly alpha emission doesn't swamp the target. ! question: 4 section: 1 line_1: Only the HST can give the required angular resolution and line_2: UV throughput and spectral resolution. ! question: 5 section: 1 line_1: Lines 20-22 call for GHRS field maps that are not standard. ! question: 7 section: 1 line_1: Astrometric reduction of the PC images will be done at the line_2: STScI in order to obtain precise coordinates of the region line_3: for GHRS observations. Reduction and analysis of the data line_4: will be done at GSFC. ! question: 13 section: 1 line_1: We will obtain images and UV spectra of QSO 2130+099. ! !end of general form text general_form_address: lname: HEAP fname: SARA category: PI inst: NASA/GSFC addr_1: CODE 681 city: GREENBELT, state: MD zip: 20771 country: USA phone: (301)-286-5359 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: QSO2130+099-NUCLEUS name_2: II-ZW-136 descr_1: E, 313,321,910,928 pos_1: RA=21H32M27.91S+/-0.75", pos_2: DEC=10D08'20.2"+/-0.75", pos_3: PLATE-ID=02KW equinox: 2000 pm_or_par: NO rv_or_z: Z=0.061 comment_1: POSITION DETERMINED FROM GSSS. fluxnum_1: 1 fluxval_1: V=14.4+/-0.2 fluxnum_2: 2 fluxval_2: F-LINE(1216)=2.6E-12 ! targnum: 2 name_1: QSO2130+099-OFFSET descr_1: SPIRAL ARM OF HOST GALAXY pos_1: R=10" +/- 2", pos_2: PA=240D +/- 40D, pos_3: FROM 1 equinox: ^ pm_or_par: ^ rv_or_z: ^ fluxnum_1: 1 fluxval_1: SURF(V)=22.0+/-1.0 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 3.000 targname: QSO2130+099-NUCLEUS config: PC opmode: IMAGE aperture: PC6 sp_element: F547M num_exp: 1 time_per_exp: 20M priority: 1 param_1: PRE-FLASH=YES req_1: EARLY ACQ FOR 4-22; req_2: CYCLE 3 comment_1: F547M INCLUDES REDSHIFTED H-BETA comment_2: AND [OIII] SPIRAL INDICATORS . ! linenum: 4.000 targname: QSO2130+099-NUCLEUS config: PC opmode: IMAGE aperture: PC6 sp_element: F547M num_exp: 1 time_per_exp: 20M priority: 1 param_1: PRE-FLASH=YES req_1: EARLY ACQ FOR 10-12; req_2: CYCLE 9 comment_1: REPEAT OF LINE 3, comment_2: DO AFTER THE REPAIR WITH WFPC2 ! linenum: 10.000 targname: QSO2130+099-NUCLEUS config: FOS/BL opmode: ACQ/BINARY aperture: 4.3 sp_element: MIRROR num_exp: 1 time_per_exp: 10S priority: 1 req_1: ONBOARD ACQ FOR 11; req_2: CYCLE 3 comment_1: DO 10-12 BEFORE THE REPAIR OF HST ! linenum: 11.000 targname: QSO2130+099-NUCLEUS config: FOS/BL opmode: ACCUM aperture: 1.0 sp_element: G130H wavelength: 1150-1608 num_exp: 1 time_per_exp: 60M priority: 1 req_1: CYCLE 3 ! linenum: 12.000 targname: QSO2130+099-OFFSET config: FOS/BL opmode: ACCUM aperture: 1.0 sp_element: G130H wavelength: 1150-1608 num_exp: 1 time_per_exp: 60M priority: 1 req_1: CYCLE 3 ! linenum: 20.000 targname: QSO2130+099-NUCLEUS config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 18.0S priority: 1 param_1: LOCATE=YES, param_2: FAINT=100 req_1: ONBOARD ACQ FOR 21-22; req_2: DARK TIME; SEQ 21-22 NON-INT; req_3: CYCLE 9 comment_1: EXPECTED COUNT/RATE > 2200, comment_2: BASED ON IUE SPECTRA. GEOCORONA comment_3: NOT A PROBLEM FOR FAINT HOST comment_4: GALAXY IF SCHEDULED DURING DARK comment_5: TIME. FORMERLY CYCLE 0 ! linenum: 21.000 targname: QSO2130+099-NUCLEUS config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N2 num_exp: 2 time_per_exp: 256S priority: 1 param_1: NX=16, param_2: DELTA-X=4,NY=16, DELTA-Y=4 req_1: CYCLE 9 comment_1: SHOULD PRODUCE A FULL MAP OF comment_2: THE LARGE APERTURE. STEP-TIME=1. comment_3: FORMERLY CYCLE 0. ! linenum: 22.000 targname: QSO2130+099-NUCLEUS config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 3.2M priority: 1 param_1: NX=64,DELTA-X=1, param_2: NY=3,DELTA-Y=4 req_1: CYCLE 9 comment_1: THIS SCAN SHOULD BE CENTERED comment_2: ON THE CENTER OF THE LSAP. comment_3: STEP-TIME=1. FORMERLY CYCLE 0. ! ! end of exposure logsheet ! No scan data records found