! $Id: 5235,v 4.1 1994/07/27 16:02:39 pepsa Exp $ coverpage: title_1: STRUCTURE OF QUASARS AND RELATED OBJECTS (WC10): title_2: CYCLE 4 sci_cat: QUASARS & AGN proposal_for: GTO/WFC pi_title: PROF. pi_fname: JAMES pi_mi: A. pi_lname: WESTPHAL pi_inst: CALTECH pi_country: USA pi_phone: (818)395-4900 keywords_1: QUASAR, AGN,RADIO GALAXY, EMISSION LINE GALAXY,BL LAC keywords_2: OBJECT hours_pri: 8.50 num_pri: 3 wf_pc: Y pi_position: PROFESSOR OF PLANETA ! end of coverpage abstract: line_1: The aims of the program are (1) to detect, and to study the morphology of line_2: galaxies underlying QSOs and AGNs, galaxies associated with them in groups and line_3: clusters, and associated structures such as jets; (2) to detect bright nuclear line_4: and extranuclear structure on small angular scales; (3) to detect and examine line_5: additional images and lensing galaxies in gravitational lenses; (4) to detect line_6: extended emission line structure in quasars. ! ! end of abstract general_form_proposers: lname: WESTPHAL fname: JAMES mi: A. inst: CALTECH country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: The general sequence of observations is two or more short observations in V and line_2: I, in which the quasar or nucleus is unsaturated, in order to look for bright line_3: small scale structure close to the nucleus, and longer exposures to examine line_4: the parent galaxy, nearby galaxies, and other extended structure. ! question: 6 section: 1 line_1: Dark time and uninterrupted exposures are required to maximize signal/noise. line_3: For all exposures >=1000sec, we request dark time. This is needed to minimize line_4: scattered light. By dark time we mean that the telescope should be beyond the line_5: brightly lit limb of the Earth in the dark half of the orbit. We do not require line_6: that the telescope actually be within the Earth's shadow. See note on exposure line_7: logsheet. The above guidline of 1000 sec may need revision after experience in line_8: orbit. ! question: 13 section: 1 line_1: The aims of the program are (1) to detect, and to study the morphology of line_2: galaxies underlying QSOs and AGNs, galaxies associated with them in groups and line_3: clusters, and associated structures such as jets; (2) to detect bright nuclear line_4: and extranuclear structures on small angular scales; (3) to detect and examine line_5: additional images and lensing galaxies in gravitational lenses; (4) to detect line_6: extended emission line structure in quasars. ! !end of general form text general_form_address: lname: KRISTIAN fname: JEROME category: CON inst: MT. WILSON & LAS addr_1: CAMPANAS OBSERVS. addr_2: 813 SANTA BARBARA ST. city: PASADENA state: CA zip: 91101 country: USA phone: (818)577-1122 ! lname: SHAYA fname: E. mi: J. category: CON inst: UNIV. OF MARYLAND addr_1: DEPT. OF PHYSICS & ASTRONOMY city: COLLEGE PARK state: MD zip: 20742 country: USA phone: (301) 405-6044 ! lname: LYNDS fname: C. mi: R. category: CON inst: NOAO, KITT PEAK NATIONAL OBSERVATORY addr_1: 950 N CHERRY city: TUCSON state: AZ zip: 86726 country: USA phone: (602)327-5511 ! lname: WESTPHAL fname: JAMES mi: A. title: PROF. category: PI inst: CALTECH addr_1: M/S 170-25 addr_2: DIVISION OF GEOLOGICAL addr_3: & PLANETARY SCIENCES city: PASADENA state: CA zip: 91125 country: USA phone: 818-395-4900 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: 3C48 descr_1: E, 314 pos_1: RA=01H34M49.8S+/-0.7S, pos_2: DEC=+32D54'20"+/-10" equinox: 1950 pm_or_par: N rv_or_z: Z=0.37 plate_req: NO comment_1: QUASAR fluxnum_1: 1 fluxval_1: V=16.2 ! targnum: 2 name_1: 3C345 descr_1: E, 314 pos_1: RA=16H41M17.6S+/-0.7S, pos_2: DEC=+39D54'11"+/-10" equinox: 1950 pm_or_par: N rv_or_z: Z=0.59 plate_req: NO comment_1: QUASAR fluxnum_1: 1 fluxval_1: V=16 ! targnum: 3 name_1: B21425+267 name_2: TON202 descr_1: E, 314 pos_1: RA=14H25M21.9S+/-1S, pos_2: DEC=+26D45'38"+/-15" equinox: 1950 pm_or_par: N rv_or_z: Z=0.37 plate_req: NO comment_1: QUASAR fluxnum_1: 1 fluxval_1: V=15.7 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 sequence_1: DEFINE sequence_2: COLOR2 targname: # config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F555W num_exp: 2 time_per_exp: 1455S priority: # param_1: CR-SPLIT=0.0345, param_2: CR-TOLERANCE=0.0, req_1: GROUP 1-2 NO GAP; comment_1: CYCLE 4-5 VERSION comment_2: JAK 6/9/93 17:30 ! linenum: 2.000 sequence_1: DEFINE sequence_2: COLOR2 targname: # config: WFPC2 opmode: IMAGE aperture: PC1 sp_element: F814W num_exp: 2 time_per_exp: 1755S priority: # param_1: CR-SPLIT=0.0286, param_2: CR-TOLERANCE=0.0, req_1: SAME POS FOR 2 AS 1; req_2: SAME ORIENT FOR 2 AS 1; ! linenum: 11.000 sequence_1: USE sequence_2: COLOR2 targname: 3C48 priority: 1 req_1: CYCLE 4 / 11-13; ! linenum: 12.000 targname: B21425+267 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F555W num_exp: 2 time_per_exp: 1455S priority: 1 param_1: CR-SPLIT=.0345, param_2: CR-TOLERANCE=0.0, req_1: GROUP 12-12.5 NO GAP; ! linenum: 12.500 targname: B21425+267 config: WFPC2 opmode: IMAGE aperture: WF3 sp_element: F814W num_exp: 2 time_per_exp: 1755S priority: 1 param_1: CR-SPLIT=.0286, param_2: CR-TOLERANCE=0.0, req_1: SAME POS FOR 12.5 AS 12; req_2: SAME ORIENT FOR 12.5 AS 12; ! linenum: 13.000 sequence_1: USE sequence_2: COLOR2 targname: 3C345 priority: 1 ! ! end of exposure logsheet ! No scan data records found