! $Id: 14,v 4.1 1994/07/26 20:47:21 pepsa Exp $ coverpage: title_1: A TRAINING PROPOSAL sci_cat: QUASARS AND AGNS proposal_for: GO TIME longterm: 4 pi_title: DR pi_fname: ROBERT pi_mi: E pi_lname: JACKSON pi_inst: SPACE TELESCOPE SCIENCE INSTITUTE pi_country: USA pi_phone: 301-338-4754 keywords_1: ROTATION,GALAXY,QUASAR hours_pri: 3.00 hours_par: 2.00 num_pri: 800 num_par: 555 fos: X realtime: X funds_amount: 47000 funds_length: 24 funds_date: APR-89 pi_position: SYSTEM ANALYST off_fname: GORDON off_mi: G. off_lname: BELLWEATHER off_title: CONTROLLER off_inst: ROWLAND HALL off_addr_1: JOHNS HOPKINS UNIV. off_city: BALTIMORE off_state: MD off_zip: 21218 off_country: USA off_phone: 338-4109 off_telex: 987453 ! end of coverpage abstract: line_1: The WFC is use to observe the host galaxy around 3C273 and the FOS will be used line_2: to measure the rotation of the galaxy. The WFC image is taken a few months line_3: early so that positions can be determined for the FOS apertures. a branch is line_4: defined so that either an emission-line(3727 A) or an absorption-line region line_5: (around 4300 A) can be observed. ! ! end of abstract general_form_proposers: lname: PATTERSON fname: STEVEN mi: R. inst: LAWRENCE LIVERMORE LABORATORY country: USA ! lname: JACKSON fname: ROBERT title: DR. mi: E. inst: SPACE TELESCOPE SCIENCE INST. country: USA ! ! end of general_form_proposers block general_form_text: question: 0 section: 0 line_1: (1) A 10 minute WFC exposure for early acquisition.Only CCD number 4 is used line_2: and 3C273 is placed on the neutral density spot so the host galaxy can be more line_3: earily seen. this can be done blind because very accurate coordinates ave line_4: available. The resulting image is sent to the observer who uses it to finalize line_5: the positions for the FOS exposures. line_7: (2) A 10 minute Fos exposure of a position in the host galaxy to determine line_8: whether emission or absorption lines are present. The G400M grating is used to line_9: provide moderate resolution from 3200 A to 4700 A. If emission is found in the line_10: 3727 line of oxygen, the default path can be with short exposures. line_11: Otherwise a branch is made to exposure 4 so an absorption-line velocity can be line_12: determined from the longewr exposures. The observation is made three days line_13: before exposures 3-5 so that a decision on which branch to use can be made. line_15: (3) (default path) A 10 minute exposure of the other side of the host galaxy to line_16: measure the emission-line velocity. line_18: (4) (branch) A 50 minute exposure at the same location as exposure 2. This line_19: exposure will be added to exposure 2, so the relevant time for the S/N line_20: calculation (column 12) is 60 minutes. line_22: (5) (branch) A 60 minute exposure on the other side of the host galaxy. ! !end of general form text general_form_address: lname: PATERSON fname: STEVEN category: X inst: LAWRENCE LIVERMORE LAB. addr_1: LRL 32-281 city: LIVERMORE state: CA zip: 94409 country: USA phone: 415-449-5310 telex: 531535 ! lname: JACKSON fname: ROBERT category: X inst: SPACE TELESCOPE SCEINCE INST. addr_1: JOHNS HOPKINS UNIV. city: BALTIMORE state: MD zip: 21218 country: USA phone: 301-338-4754 telex: 421583 ! lname: COLLICK category: PI inst: SPACE TELESCOPE SCIENCE INSTITUTE addr_1: JOHNS HOPKINS UNIVERSITY addr_2: HOMEWOOD CAMPUS city: BALTIMORE state: MD zip: 21218 country: USA ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: 3C273 descr_1: NEARBY QUASAR pos_1: RA=12H 26M 33.35S+/-0.01S,DEC=+2D 19' pos_2: 42.4" +0.05" equinox: 1950 rv_or_z: Z=0.158 fluxnum_1: 1 fluxval_1: V=12.8+/- 0.1 fluxnum_2: 2 fluxval_2: B=13.0+/- 0.1 ! targnum: 2 name_1: 3C273-HOST-A descr_1: ONE SIDE OF HOST GALAXY AROUND 3C273 pos_1: TBD-PII,RA-OFF=0+/- 3",DEC-OFF=0" +/-3" equinox: 1950 rv_or_z: Z=0.158 fluxnum_1: 1 fluxval_1: SURF(V)=24+/- 1 fluxnum_2: 2 fluxval_2: F-LINE(3727)=5.0 +/-4.0 E-18 fluxnum_3: 3 fluxval_3: F-LINE-BKG(3727)=2.0 +/- 1.0 E-18 fluxnum_4: 4 fluxval_4: W-LINE(3727)=3 +/- 1 fluxnum_5: 5 fluxval_5: F-CONT(4300)=2.0 +/- 1.0 E-18 fluxnum_6: 6 fluxval_6: F-CONT-BKG(4300)=2.0+/-1.0 E-18 ! targnum: 3 name_1: 3C273-HOST-B descr_1: ONE SIDE OF HOST GALAXY AROUND 3C273 pos_1: ^ equinox: ^ rv_or_z: ^ comment_1: COORDINATES DETERMINED BY EARLY comment_2: ACQUISITION OF TARGET #1. fluxval_1: ^ ! targnum: 4 ! targnum: 5 ! targnum: 6 ! targnum: 7 ! targnum: 8 ! ! end of fixed targets solar_system_targets: targnum: 3 name_1: PLUTO descr_1: PLANET lev1_1: USE JPL EPHEMERIS fluxnum_1: 1 fluxval_1: V=14.9: ! ! end of solar system targets generic_targets: targnum_1: 6 name_1: SN descr_1: BRIGHT SUPERNOVA IN UNKNOWN GALAXY criteria_1: ANY SUPERNOVA BRIGHTER THAN B=15 AT DISCOVERY, AS REPORTED IN IAU criteria_2: CIRCULAR. PROPOSER WILL ALERT STSCI OF CANDIDATES. fluxnum_1: 1 fluxval_1: V=12 +/- 3 fluxnum_2: 2 fluxval_2: B=12 +/- 3 fluxnum_3: 3 fluxval_3: B=12.2 +/- 3 fluxnum_4: 4 fluxval_4: B=12.5 +/- 3 fluxnum_5: 5 fluxval_5: B=12.9 +/- 3 fluxnum_6: 6 fluxval_6: B=13.4 +/- 3 ! ! end of generic targets exposure_logsheet: linenum: 1.000 targname: 3C273 config: HSP/POL opmode: 1APER sp_element: F277M num_exp: 1 time_per_exp: 10M s_to_n: 100 s_to_n_time: 2M fluxnum_1: 2 priority: 1 param_1: SAMPLE-TIME=2.0 param_2: DATA-FORMAT=ALL req_1: EXTERNAL PARALLEL WITH 1 OF 13 ! linenum: 2.000 targname: ^ config: ^ opmode: ^ sp_element: ^ num_exp: 1 time_per_exp: 10M s_to_n: 100 s_to_n_time: 2M fluxnum_1: 2 priority: 1 ! linenum: 3.000 targname: ^ config: ^ opmode: ^ sp_element: ^ num_exp: 1 time_per_exp: 5M s_to_n: 100 fluxnum_1: ^ priority: ^ req_1: EXTERNAL PARALLEL WITH 3 OF 13 ! ! end of exposure logsheet ! No scan data records found