! $Id: 12,v 4.1 1994/07/26 20:46:36 pepsa Exp $ coverpage: title_1: THIS IS A TEST PROPOSAL AND BELONGS TO THE PEPDBA. title_2: ONE proposal_for: GO longterm: 1 pi_fname: JAMES pi_mi: T pi_lname: JONES pi_inst: SPACE TELESCOPE SCIENCE INSTITUTE pi_country: USA pi_phone: 301 338 4549 keywords_1: ROTATION, GALAXY, QUASAR keywords_2: NOT HERE, BUCKO. THIS IS TONY LAZAR'S TEST. hours_pri: 999.99 hours_par: 999.99 num_pri: 9999 num_par: 9999 wf_pc: X foc: X fos: X hrs: X hsp: X fgs: X realtime: X time_crit: X funds_amount: 108000 funds_length: 11 funds_date: MAR-87 pi_position: JACK FROST off_fname: SMITH off_mi: G off_lname: JONES off_title: CONTROLLER off_inst: JOHN HOPKINS UNIVERSITY off_addr_1: ROWLAND HALL off_addr_2: JOHN HOPKINS UNIVERSITY off_city: BALTIMORE off_state: MD off_zip: 21218 off_country: USA off_phone: 123 4567 off_telex: 123456 ! end of coverpage abstract: line_1: THE WFC is used to observe the host galaxy around 3C273 and the FOS will be line_2: used 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. line_7: ^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^ line_8: TEST=TEST=TEST=TEST=TEST=TEST=TEST=TEST=TEST=TEST=TEST=TEST=TEST=TEST line_9: ##################################################################### line_10: ################################################################ line_11: ############################################################ line_12: #########################################JIM###JONES#### line_13: @@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@ line_14: ^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^ line_16: bloop line_17: da-da-da-da-da-da-da-da-da line_18: duh-duh-duh-duh-duh ! ! end of abstract general_form_proposers: lname: RICHON fname: JOEL title: PROF mi: G inst: SPACE TELESCOPE SCIENCE INSTITUTE country: USA esa: N ! lname: RICHON fname: KAREN title: PROF mi: V inst: SPACE TELESCOPE SCIENCE INSTITUTE country: USA esa: N ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 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 nuetral density spot so the host galaxy can be more line_3: easily seen. This can be done blind because very accurate coordinates are 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_6: ================================================================================ line_7: (2)A 10 minute FOS exposure of a positions 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 used 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 longer exposures. The observation is made three days before line_13: exposures 3 - 5 so that a decision on which branch to use can be made. line_14: - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - line_15: (3) (default path) A 10 minute exposure of the other side of the host galaxy line_16: to measure the emission-line velocity. line_17: ================================================================================ 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_21: ================================================================================ line_22: (5) (branch) A 60 minute exposure on the other side of the host galaxy. line_23: ================================================================================ ! !end of general form text general_form_address: lname: KIRK fname: JAMES mi: T title: DR category: CON inst: USS ENTERPRISE addr_1: TAU-CETI addr_2: QUADRANT A-12'23" zip: 999999999 ! ! end of general_form_address records fixed_targets: targnum: 4 name_1: HAHA-HOHO-STAR descr_1: A VERY FUNNY STAR IN THE CONSTELLATION descr_2: WITH MORE DESCRIPTION pos_1: RA=10H10M10S,DEC=10D10'10" equinox: 1950 comment_1: THIS STAR JUST CRACKS ME UP ! targnum: 6 name_1: HAHA-HOHO-STAR2 descr_1: A VERY FUNNY STAR IN THE CONSTELLATION descr_2: FUNNYBONE - HAHAHAHAHA pos_1: RA=1H1M1S,DEC=1D1'1" equinox: 1950 comment_1: THIS STAR JUST CRACKS ME UP comment_2: YOU ONLY HAVE T. LAZAR TO comment_3: BLAME FOR THIS. ! targnum: 7 name_1: HAHA-HOHO-STAR4 descr_1: A VERY FUNNY STAR IN THE CONSTELLATION descr_2: FUNNYBONE - HAHAHAHAHA pos_1: RA=1H1M1S,DEC=1D1'1" equinox: 1950 comment_1: THIS STAR JUST CRACKS ME UP comment_2: YOU ONLY HAVE T. LAZAR TO comment_3: BLAME FOR THIS. ! targnum: 1 name_1: 3C273 descr_1: NEARBY QUASAR pos_1: RA=12H 26M 33.35S +/- 0.01S, pos_2: DEC=+2D 19' 42.4" +/- 0.05" equinox: 1950 pos_epoch_bj: J pos_epoch_yr: 2000.00 ra_pm_val: -0.100000 ra_pm_unct: 0.000267 dec_pm_val: 99.9000 dec_pm_unct: 0.0010 an_prlx_val: 3.2500 an_prlx_unct: 111.1100 rv_or_z: Z=0.245 comment_1: JIM'S PROVISIONAL FIXED TARGETS fluxnum_1: 1 fluxval_1: V=12.5 +/- 0.1 fluxnum_2: 2 fluxval_2: B=13.0 +/- 0.1 ! targnum: 2 name_1: 3C273A descr_1: NEARBY QUASAR pos_1: RA=12H 26M 33.35S +/- 0.01S, pos_2: DEC=+2D 19' 42.4" +/- 0.05" equinox: 1950 pos_epoch_bj: J pos_epoch_yr: 2000.00 ra_pm_val: 0.005333 ra_pm_unct: 0.005333 dec_pm_val: 0.0800 dec_pm_unct: 0.0890 an_prlx_val: 0.0070 an_prlx_unct: 43.6800 rv_or_z: Z=0.245 comment_1: JIM'S PROVISIONAL FIXED TARGETS fluxnum_1: 1 fluxval_1: V=12.5 +/- 0.1 fluxnum_2: 2 fluxval_2: B=13.0 +/- 0.1 ! targnum: 3 name_1: 3C273-HOST-B descr_1: ONE SIDE OF HOST GALAXY AROUND 3C273 pos_1: ^ equinox: ^ pos_epoch_bj: J pos_epoch_yr: 2000.00 ra_pm_val: 3.646667 ra_pm_unct: 0.000667 dec_pm_unct: 0.9000 an_prlx_val: 864.0700 rv_or_z: ^ comment_1: COORDINATES DETERMINED BY EARLY comment_2: ACQUISITION OF TARGET # 1. fluxval_1: ^ ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 100.000 sequence_1: DEFINE sequence_2: OBSSEQ targname: # config: FOC/48 opmode: ACQ aperture: 512X512 sp_element: F140W num_exp: 1 time_per_exp: 100S s_to_n: 1 priority: 1 req_1: COND IF IN TOP 20 ! linenum: 101.000 sequence_1: ^ targname: # config: FOC/48 opmode: SPEC aperture: 512X512-SLIT sp_element: G450M wavelength: 4400 num_exp: 1 time_per_exp: 100M s_to_n: 1 priority: 1 req_1: COND IF IN TOP 20 ! linenum: 102.000 sequence_1: USE sequence_2: OBSSEQ targname: 3C273 req_1: DO FOR TARG 1-4 ! ! end of exposure logsheet ! No scan data records found