! File: 1514C.PROP ! Database: PEPDB ! Date: 16-FEB-1994:21:28:48 coverpage: title_1: FOC F/48 LONG-SLIT PHOTOMETRIC CALIB-REVISED proposal_for: SV/FOC pi_title: DR. pi_fname: FRANCESCO pi_lname: PARESCE pi_inst: SPACE TELESCOPE SCIENCE INSTITUTE pi_country: USA foc: X ! end of coverpage abstract: line_1: The aim of this SV task is to establish the spectrophotometric response of the line_2: FOC f/48 spectrograph. Because it is not anticipated that observers will want line_3: to try and put a star down the 0.1 arcsecond wide slit, the slitless operation line_4: of the spectrograph will be emphasized. Two standard stars will separately be line_5: placed near the spectrographic finger and spectra obtained in each of the four line_6: orders, as well as using the FOCPD prism as a cross-disperser. line_7: An initial attempt at using the spectrograph slit will also be performed, but line_8: in first order only. line_9: The study will also provide the only in-orbit check on the wavelength line_10: sensitivity of the f/48 mode (particularly in the UV). The data are needed for line_11: updating the SOGS RSDP calibration files. line_12: Real time downlink/uplink required. ! ! end of abstract general_form_proposers: lname: PARESCE fname: F. title: DR. inst: SPACE TELESCOPE SCIENCE INSTITUTE country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: Standard stars will be placed near the slit, in both echelle and filter modes, line_2: and used to calibrate the photometric response of the f/48 spectrograph with line_3: wavelength. The standards have absolute flux measures from IUE and line_4: ground-based studies which in combination cover the required wavelength region line_5: from 1200-6000 A. The observed counts will lead directly to the derivation of line_6: a sensitivity curve. Comparison with the predicted OTA+FOC throughput for line_7: different wavelengths will enable any deterioration of FOC response to be line_8: measured and monitored. line_10: The targets will be placed near the slit finger, and on the slit. These line_11: spectra will yield the plate scale of the spectrograph and the photometric line_12: response of the spectrograph in the spatial direction. ! question: 5 section: 1 line_1: Real time observations are required to monitor positioning of the star with line_2: respect to the slit template and the slit. line_4: note to scheduler: line_10: Prerequisites: line_11: To plan after thesecond visit of SV aperture location (2764). line_12: Detector focus (FOC-i2;1506) and line_13: Optical Focus (FOC-03; 1507); For data analysis, Point line_14: Source Linearity (FOC-04, 1508). ! !end of general form text general_form_address: lname: PARESCE fname: FRANCESCO title: DR. category: PI inst: SPACE TELESCOPE SCIENCE INSTITUTE addr_1: 3700 SAN MARTIN DRIVE city: BALTIMORE state: MD zip: 21218 country: USA phone: 301-338-4823 telex: 684-9101-STSCI ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: HZ21 descr_1: UV-OPTICAL STANDARD pos_1: RA=12H 13M 56.42S +/- 1.0", pos_2: DEC=+32D 56' 30.8" +/- 1.0", equinox: 2000 fluxnum_1: 1 fluxval_1: V=14.68,TYPE= DO2 ! targnum: 2 name_1: AGK+81D266 descr_1: SPECTROPHOTOMETRIC STANDARD pos_1: RA=9H 21M 19.06S +/- 1.0", pos_2: DEC=+81D 43' 28.6" +/- 1.0", equinox: 2000 fluxnum_1: 1 fluxval_1: V=11.92,TYPE= SD0 ! targnum: 3 name_1: NGC4151 descr_1: EMISSION LINE GALAXY pos_1: RA=12H 08M 01.07S +/- 2", pos_2: DEC=+39D 41' 02.2" +/- 1" equinox: 1950 rv_or_z: Z=0.0033 fluxnum_1: 1 fluxval_1: V=12.5 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 6.000 targname: HZ21 config: FOC/48 opmode: ACQ aperture: 512X512-SF sp_element: F150W,F275W num_exp: 1 time_per_exp: 600S fluxnum_1: 1 priority: 1 param_1: PIXEL=50X25 req_1: INT ACQ FOR 7-10; req_2: CYCLE 0 / 6-26; comment_1: ONCE IMAGE IS READ-DOWN, POSITION OF comment_2: STAR CAN BE DETERMINED IN DETECTOR comment_3: COORDS.A SMALL-ANGLE MANEUVER IS NOW comment_4: REQUIRED TO POSITION STAR NEAR THE comment_5: SLIT FINGER. ! linenum: 7.000 targname: ^ config: ^ opmode: IMAGE aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ comment_1: THIS EXPOSURE CONFIRMS comment_2: THE MANEUVER AND ALLOWS comment_3: US TO SEE EXACTLY WHERE comment_4: THE STAR ENDED UP. ! linenum: 8.000 targname: ^ config: ^ opmode: SPEC aperture: 512X1024-CD sp_element: G450M num_exp: 2 time_per_exp: 500S fluxnum_1: ^ priority: ^ param_1: PIXEL=25X25, ! linenum: 9.000 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: G225M num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 10.000 sequence_1: ^ targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: GRATING,PRISM3 num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 11.000 targname: AGK+81D266 config: ^ opmode: IMAGE aperture: 512X512-SF sp_element: F140W,F342W num_exp: 1 time_per_exp: 600S fluxnum_1: ^ priority: ^ param_1: PIXEL=50X25 req_1: INT ACQ FOR 12-15; ! linenum: 12.000 sequence_1: ^ targname: ^ config: ^ opmode: IMAGE aperture: 512X512-SF sp_element: ^ num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 13.000 targname: ^ config: ^ opmode: SPEC aperture: 512X1024-CD sp_element: G150M num_exp: 2 time_per_exp: 500S fluxnum_1: ^ priority: ^ param_1: PIXEL=25X25 ! linenum: 14.000 targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: G130M num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 15.000 targname: AGK+81D266 config: FOC/48 opmode: SPEC aperture: 512X1024-CD sp_element: GRATING,PRISM3 num_exp: 2 time_per_exp: 500S fluxnum_1: 1 priority: 1 param_1: PIXEL=25X25 ! linenum: 16.000 targname: HZ21 config: FOC/48 opmode: ACQ aperture: 512X512-SF sp_element: F150W,F275W num_exp: 1 time_per_exp: 600S fluxnum_1: ^ priority: ^ param_1: PIXEL=50X25 req_1: INT ACQ FOR 17-22; ! linenum: 17.000 targname: ^ config: ^ opmode: IMAGE aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 18.000 targname: ^ config: ^ opmode: SPEC aperture: 256X1024-SLIT sp_element: G450M num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ req_1: POS TARG 0,+0.10; ! linenum: 19.000 targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ req_1: POS TARG 0,+0.05; ! linenum: 20.000 targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ req_1: POS TARG 0,0; ! linenum: 21.000 targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ req_1: POS TARG 0,-0.05; ! linenum: 22.000 targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ req_1: POS TARG 0,-0.10; ! linenum: 23.000 targname: NGC4151 config: FOC/48 opmode: ACQ aperture: 512X512-SF sp_element: F150W num_exp: 1 time_per_exp: 600S fluxnum_1: ^ priority: ^ param_1: PIXEL=50X25 req_1: INT ACQ FOR 24-26 ! linenum: 24.000 targname: ^ config: ^ opmode: IMAGE aperture: ^ sp_element: ^ num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! linenum: 25.000 targname: NGC4151 config: FOC/48 opmode: SPEC aperture: 256X1024-SLIT sp_element: G450M num_exp: 3 time_per_exp: 600S fluxnum_1: 1 priority: 1 param_1: PIXEL=50X25 ! linenum: 26.000 targname: ^ config: ^ opmode: ^ aperture: ^ sp_element: G150M num_exp: ^ time_per_exp: ^ fluxnum_1: ^ priority: ^ param_1: ^ ! ! end of exposure logsheet ! No scan data records found