! File: 4094C.PROP ! Database: PEPDB ! Date: 20-FEB-1994:08:25:36 coverpage: title_1: SPECTROSCOPY OF MILKY WAY HALO GAS---AUGMENTED title_2: CYCLE 2 sci_cat: INTERSTELLAR MEDIUM proposal_for: AUG/HRS cont_id: 1165 pi_title: PROF. pi_fname: BLAIR pi_mi: D. pi_lname: SAVAGE pi_inst: WISCONSIN, UNIVERSITY OF pi_country: USA pi_phone: (608)262-3072 keywords_1: INTERSTELLAR, GAS SPECTROSCOPY, UV, HALO hours_pri: 12.00 num_pri: 11 hrs: X pi_position: PROFESSOR ! end of coverpage abstract: line_1: Milky Way halo gas will be studied at resolutions of E+5 line_2: and 2xE+4 by observing selected interstellar lines toward line_3: galactic and extragalactic objects. Information about line_4: kinematics, physical condition, and abundances in the as line_5: will be obtained. ! ! end of abstract general_form_proposers: lname: SAVAGE fname: BLAIR mi: D. inst: WISCONSIN, UNIVERSITY OF country: USA ! lname: EBBETS fname: DENNIS title: DR. mi: C. inst: SPACE TELESCOPE SCIENCE INSTITUTE country: USA ! lname: CARDELLI fname: JASON title: DR. mi: A. inst: WISCONSIN, UNIVERSITY OF country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: HRS scanning will be performed on one Milky Way halo star and on line_2: one extragalactic object. line_6: Cycle 2 (19-30 months) Exposures 1-12 line_7: Cycle 2 (19-30 months) Exposures 100-140 ! question: 4 section: 1 line_1: 1E5 and 2E4 resolution UV spectra are essential for obtaining line_2: accurate abundance and line profile information for a wide variety of line_3: interstellar ionic species. ! question: 6 section: 1 line_1: Occasional pt lamp comparison spectra will be required to obtain accurate line_2: wavelength calibrations. ! question: 7 section: 1 line_1: Data will be reduced in Madison using the MADRAF VAX. HRS team software line_2: will be available. ! question: 10 section: 1 line_1: The data reduction facility. ! question: 12 section: 1 line_1: line_4: HD 116852 line_5: E1821+643 ! question: 13 section: 1 line_1: Physical conditions and abundances in Milky Way halo gas will be studied line_2: by observing galactic and extragalactic sources with the HRS. ! !end of general form text general_form_address: lname: SAVAGE fname: BLAIR mi: D. title: PROF. category: PI inst: UNIVERSITY OF WISCONSIN, MADISON addr_1: DEPARTMENT OF ASTRONOMY addr_2: 475 N. CHARTER STREET city: MADISON state: WI zip: 53706 country: USA phone: 608-262-3072 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: HD116852 name_2: GSC9434-1988 descr_1: A,105,911 pos_1: RA=13H 30M 23.63S+/-.01S, pos_2: DEC=-78D 51' 20.1"+/-.1" equinox: J2000 pm_or_par: NO fluxnum_1: 1 fluxval_1: V=8.47, B-V=-0.09 ! targnum: 2 name_1: E1821+643 descr_1: E,313 pos_1: RA=18H 21M 57.11S+/-.01S, pos_2: DEC=+64D 20' 36.7"+/-0.1" equinox: 2000 pm_or_par: NO rv_or_z: Z=0.297 fluxnum_1: 1 fluxval_1: V=14.1 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 targname: HD116852 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 75S priority: 1 param_1: SEARCH-SIZE=5 param_2: BRIGHT=65535, param_3: FAINT=3000, req_1: ONBOARD ACQ FOR 1.1; req_2: CYCLE 2 / 1-12 comment_1: STEP-TIME=3S ! linenum: 1.100 targname: HD116852 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 163.2S priority: 1 req_1: ONBOARD ACQ FOR 1.2-1.3 comment_1: STEP-TIME=1.6S ! linenum: 1.200 targname: HD116852 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 153.6S priority: 1 param_1: NX=16, param_2: NY=16, comment_1: TAKE MAP AFTER CENTERING comment_2: EXPECT 48 COUNTS AT PEAK comment_3: STEP-TIME=0.6S ! linenum: 1.300 targname: HD116852 config: HRS opmode: IMAGE aperture: 0.25 sp_element: MIRROR-A2 num_exp: 1 time_per_exp: 204.8S priority: 1 param_1: NX=16, param_2: NY=16, param_3: DELTA-X=1, param_4: DELTA-Y=1 comment_1: STEP-TIME=0.8S ! linenum: 9.000 targname: HD116852 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G200M wavelength: 2045 num_exp: 1 time_per_exp: 25.96M priority: 1 param_1: STEP-PATT=4 param_2: FP-SPLIT=STD ! linenum: 10.000 targname: HD116852 config: HRS opmode: ACCUM aperture: 0.25 sp_element: G270M wavelength: 2600 num_exp: 1 time_per_exp: 9.60M priority: 1 param_1: STEP-PATT=4 param_2: FP-SPLIT=STD ! linenum: 11.000 targname: HD116852 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B22 wavelength: 2603 num_exp: 1 time_per_exp: 20.16M s_to_n: 49 priority: 1 param_1: FP-SPLIT=STD param_2: STEP-PATT=6 ! linenum: 12.000 targname: HD116852 config: HRS opmode: ACCUM aperture: 0.25 sp_element: ECH-B25 wavelength: 2260 num_exp: 1 time_per_exp: 30.72M s_to_n: 50 priority: 1 param_1: STEP-PATT=6 param_2: FP-SPLIT=STD ! linenum: 100.000 targname: E1821+643 config: HRS opmode: ACQ aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 100S priority: 1 param_1: SEARCH-SIZE=5 param_2: BRIGHT=65535, param_3: FAINT=1300, req_1: ONBOARD ACQ FOR 111; req_2: CYCLE 2 / 100-140; comment_1: STEP-TIME=4S ! linenum: 111.000 targname: E1821+643 config: HRS opmode: ACQ/PEAKUP aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 204S priority: 1 req_1: ONBOARD ACQ FOR 112-140; comment_1: STEP-TIME=2S ! linenum: 112.000 targname: E1821+643 config: HRS opmode: IMAGE aperture: 2.0 sp_element: MIRROR-N2 num_exp: 1 time_per_exp: 5.12M priority: 1 param_1: NX=16, param_2: NY=16, comment_1: TAKE MAP AFTER CENTERING comment_2: EXPECT 30 COUNTS AT PEAK comment_3: STEP-TIME=1.2S ! linenum: 120.000 targname: E1821+643 config: HRS opmode: ACCUM aperture: 2.0 sp_element: G160M wavelength: 1250 num_exp: 6 time_per_exp: 20.16M s_to_n: 23 priority: 1 param_1: STEP-PATT=4 param_2: FP-SPLIT=STD ! linenum: 140.000 targname: E1821+643 config: HRS opmode: ACCUM aperture: 2.0 sp_element: G270M wavelength: 2800 num_exp: 3 time_per_exp: 19.2M s_to_n: 15 priority: 1 param_1: STEP-PATT=4 param_2: FP-SPLIT=STD ! ! end of exposure logsheet ! No scan data records found