! File: 3149C.PROP ! Database: PEPDB ! Date: 18-FEB-1994:19:24:44 coverpage: title_1: WF/PC SV CALIBRATION THROUGH title_2: OBSERVATION OF FIELD OF STARS-REVISED 1/91 proposal_for: SV/WFC pi_fname: JAMES pi_mi: A. pi_lname: WESTPHAL pi_inst: CALTECH pi_country: USA pi_phone: (818) 356-4900 keywords_1: CALIBRATION, WF/PC PHOTOMETRIC SYSTEM, NGC 5139 hours_pri: 11.00 wf_pc: Y ! end of coverpage abstract: line_1: The objective of this calibration test is to observe a field of stars that will line_2: allow an adequate number of calibrated stars to appear in each CCD to line_3: efficiently produce an instrument-defined photmetric system for each filter. line_4: The selected field is in the outer regions of the globular clusters NGC 5139 line_9: Revised 1/9/90 by PStanley to expand out SEQ to avoid AFTER conflicts line_10: during transformation. Mod'ed by JAW 2 Sept 90 to do post flood cals. line_11: This is a temporary fix to increase exposures for the line_12: monitor part of the proposal: Jan. 22 - shaya ! ! end of abstract general_form_proposers: lname: fname: WF/PC IDT inst: VARIOUS country: USA ! lname: WESTPHAL fname: JAMES mi: A. inst: CALIFORNIA INSTITUTE OF TECHNOLOGY country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: line_4: In order to verify the scientific photometric line_5: measurement capabilities of selected filters in the WF/PC. ! question: 4 section: 1 line_1: Instrument calibration which is coordinated with the appropriate ground-based line_2: observations. ! question: 5 section: 1 line_1: SV Prerequisites: line_2: This activity should start approximately one week after the line_3: UV Flood in SV (prop 1431) is completed. line_7: Target Information: line_8: NGC 5139 is the preferred target and will be available 12/90. line_9: The same target should be used consistently for this proposal line_10: and for WF/PC-03 (prop 1323). ! question: 6 section: 1 line_1: This is a normal calibration observation. ! question: 7 section: 1 line_1: These data will be part of the calibration data base at the ScI and will be line_2: used to determine the photometric sensitivity of each of the CCDs through each line_3: of the filters. These data will be analyzed by the WF/PC IDT. The output line_4: products will be published in the Calibrations Report whcih will be delivered line_5: to the ScI. ! question: 8 section: 1 line_1: Ground-based observations of these fields is essential to line_2: establish the absolute flux for each star. ! !end of general form text general_form_address: lname: WESTPHAL fname: JAMES mi: A. category: PI inst: CALTECH ! lname: DANIELSON fname: G. mi: E. inst: CALTECH M/S 170-25 addr_1: GEOLOGICAL & PLANETARY SCIENCES city: PASADENA state: CA zip: 91125 country: USA phone: (818) 356-6861 ! lname: GUNN fname: JAMES mi: E. inst: PRINCETON UNIVERSITY addr_1: ASTROPHYSICAL SCIENCE addr_2: PEYTON HALL city: PRINCETON state: NJ zip: 08540 country: USA phone: (609) 452-3803 ! lname: BAUM fname: WILLIAM mi: A. inst: LOWELL OBSERVATORY addr_1: PLANETARY RESEARCH CENTER addr_2: 1400 W. MARS HILL ROAD city: FLAGSTAFF state: AZ zip: 86002 country: USA phone: (818) 774-3358 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: NGC5139 descr_1: GLOBULAR CLUSTER pos_1: RA = 13H 25M 37.04S +/- 0.1S, pos_2: DEC = -47D 35' 38.3" +/- 1.0" equinox: 2000 comment_1: PRIMARY TARGET. fluxnum_1: 1 fluxval_1: V = 14.5 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 282.000 sequence_1: DEF SEQMON targname: NGC5139 config: WFC opmode: IMAGE aperture: ALL sp_element: F336W num_exp: 1 time_per_exp: 1000S priority: 1 param_1: CR-SPLIT=NO,PRE-FLASH=YES req_1: GUID TOL 0.030" / 282-289.00; req_2: CYCLE 0/282-370; ! linenum: 283.000 sequence_1: DEF SEQMON targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F439W num_exp: 1 time_per_exp: 180S priority: ^ param_1: ^ ! linenum: 284.000 sequence_1: DEF SEQMON targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F555W num_exp: 1 time_per_exp: 35S priority: ^ param_1: ^ ! linenum: 284.500 sequence_1: DEF SEQMON targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F555W num_exp: 1 time_per_exp: 400S priority: ^ param_1: ^ ! linenum: 285.000 sequence_1: DEF SEQMON targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F785LP num_exp: 1 time_per_exp: 60S priority: ^ param_1: ^ ! linenum: 285.500 sequence_1: DEF SEQMON targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F785LP num_exp: 1 time_per_exp: 600S priority: ^ param_1: ^ ! linenum: 286.000 sequence_1: DEF SEQMON targname: NGC5139 config: PC opmode: IMAGE aperture: ALL sp_element: F336W num_exp: 2 time_per_exp: 1000S priority: 1 param_1: CR-SPLIT=NO,PRE-FLASH=YES ! linenum: 287.000 sequence_1: DEF SEQMON targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: F439W num_exp: 1 time_per_exp: 500S priority: ^ param_1: ^ ! linenum: 288.000 sequence_1: DEF SEQMON targname: NGC5139 config: PC opmode: IMAGE aperture: ALL sp_element: F555W num_exp: 1 time_per_exp: 60S priority: 1 param_1: CR-SPLIT=NO,PRE-FLASH=YES, ! linenum: 288.500 sequence_1: DEF SEQMON targname: NGC5139 config: PC opmode: IMAGE aperture: ALL sp_element: F555W num_exp: 1 time_per_exp: 600S priority: 1 param_1: CR-SPLIT=NO,PRE-FLASH=YES, ! linenum: 289.000 sequence_1: DEF SEQMON targname: NGC5139 config: PC opmode: IMAGE aperture: ALL sp_element: F785LP num_exp: 1 time_per_exp: 100S priority: 1 param_1: ^ ! linenum: 289.500 sequence_1: DEF SEQMON targname: NGC5139 config: PC opmode: IMAGE aperture: ALL sp_element: F785LP num_exp: 1 time_per_exp: 1000S priority: 1 param_1: ^ ! linenum: 360.000 sequence_1: USE SEQMON comment_1: AFTER 350 OF OLD 1321 BY comment_2: 30D +/- 10D, comment_3: IE. INSERT IN EXISTING comment_4: SCHEDULE FOR 1321 MONITOR. ! linenum: 370.000 sequence_1: USE SEQMON req_1: AFTER 360 BY 30D +/- 10D ! ! end of exposure logsheet ! No scan data records found