! File: 1073C.PROP ! Database: PEPDB ! Date: 16-FEB-1994:00:41:36 coverpage: title_1: EXTRAGALACTIC DISTANCE INDICATORS-CYCLE9 sci_cat: GALAXIES & CLUSTERS proposal_for: GTO/OS pi_title: PROF. pi_fname: C. pi_mi: R. pi_lname: O'DELL pi_inst: RICE UNIVERSITY pi_country: USA pi_phone: 713-527-8101 X3633 keywords_1: HII REGIONS, EXTRAGALACTIC DISTANCES hours_pri: 8.00 num_pri: 12 wf_pc: X pi_position: PROF. SP.PHYS.ASTR. ! end of coverpage abstract: line_1: Ground based observations have shown that extragalactic H II Complexes can be line_2: fit by a simple standard model, whose parameters can be determined by line_3: observation of the recombination line surface brightness. WF/PC H-beta images line_4: will be obtained of a series of H II Complexes in successively more distant line_5: galaxies in order to refine the zero point calibration and to apply this method line_6: to distant galaxies. ! ! end of abstract general_form_proposers: lname: O'DELL fname: C. mi: R. inst: RICE UNIVERSITY country: USA ! lname: SPITZER JR. fname: LYMAN inst: PRINCETON UNIVERSITY country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: Images with emission line filters will be made with the WF/PC in the WF mode line_2: for five H II Complexes. line_4: Exposure 2 should be made during cycle 1. ! question: 4 section: 1 line_1: Only the HST allows the high angular resolution needed for this program. ! question: 7 section: 1 line_1: After standard image processing at the STScI, the images will be enhanced with line_2: the Rice University Image Processing Facility, with each H II complex's surface line_3: brightness distribution determined. This data will be tested against the line_4: standard model supported by ground based observations and then used to line_5: calibrate the zero point of this new distance scale method. ! question: 10 section: 1 line_1: The principal resources at Rice University are the Image Processing Facility line_2: and availability of graduate student assistants. ! question: 13 section: 1 line_1: Ground based observations have shown that extragalactic H II Complexes can be line_2: fit by a simple standard model, whose parameters can be determined by line_3: observation of the recombination line surface brightness. WF/PC H-beta images line_4: will be obtained of a series of H II Complexes in successively more distant line_5: galaxies in order to refine the zero point calibration and to apply this method line_6: to distant galaxies. ! !end of general form text general_form_address: lname: SPITZER JR. fname: LYMAN inst: PRINCETON UNIVERSITY OBSERVATORY addr_1: PEYTON HALL city: PRINCETON state: NJ zip: 08544 country: USA phone: (609)452-3809 ! lname: O'DELL fname: C. mi: R. title: PROF. category: PI inst: RICE UNIVERSITY addr_1: DEPT. OF SPACE PHYSICS & ASTRONOMY addr_2: P.O. BOX 1892 city: HOUSTON state: TX zip: 77251 country: USA phone: 713-527-8101 X3633 telex: 556457 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: NGC5457-1 descr_1: H,503 pos_1: RA=14H02M43.5S+/-0.2S, pos_2: DEC=+54D38'09"+/-5" equinox: 1950 pm_or_par: NO fluxnum_1: 1 fluxval_1: F-LINE(6563)=3.9+/-0.5E-12, fluxval_2: W-LINE(6563)=1+/-0 ! targnum: 2 name_1: NGC5457-4 descr_1: H,503 pos_1: RA=14H01M56.0S+/-0.2S, pos_2: DEC=+54D33'26"+/-5" equinox: 1950 pm_or_par: NO fluxnum_1: 1 fluxval_1: F-LINE(6563)=3.5+/-0.5E-12, fluxval_2: W-LINE(6563)=1+/-0 ! targnum: 3 name_1: NGC6822-1 descr_1: H,503 pos_1: RA=19H42M15.6S+/-0.2S, pos_2: DEC=-14D50'36"+/-5" equinox: 1950 pm_or_par: NO fluxnum_1: 1 fluxval_1: F-LINE(6563)=6.3+/-0.5E-12, fluxval_2: W-LINE(6563)=1+/-0 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 targname: NGC5457-1 config: WFC opmode: IMAGE aperture: ALL sp_element: F487N num_exp: 1 time_per_exp: 35M s_to_n: 30 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 req_1: CYCLE 9 / 1-21 ! linenum: 2.000 targname: NGC5457-1 config: WFC opmode: IMAGE aperture: ALL sp_element: F487N num_exp: 1 time_per_exp: 5M s_to_n: 30 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! linenum: 3.000 targname: NGC5457-1 config: WFC opmode: IMAGE aperture: ALL sp_element: F547M num_exp: 1 time_per_exp: 5M s_to_n: 20 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! linenum: 4.000 targname: NGC5457-1 config: WFC opmode: IMAGE aperture: ALL sp_element: F502N num_exp: 1 time_per_exp: 12M s_to_n: 20 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! linenum: 5.000 targname: NGC5457-1 config: WFC opmode: IMAGE aperture: ALL sp_element: F375N num_exp: 1 time_per_exp: 30M s_to_n: 30 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! linenum: 6.000 targname: NGC5457-1 config: WFC opmode: IMAGE aperture: ALL sp_element: F284W num_exp: 1 time_per_exp: 5M s_to_n: 20 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! linenum: 7.000 targname: NGC5457-1 config: WFC opmode: IMAGE aperture: ALL sp_element: F656N num_exp: 1 time_per_exp: 5M s_to_n: 10 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! linenum: 8.000 targname: NGC5457-4 config: WFC opmode: IMAGE aperture: ALL sp_element: F487N num_exp: 1 time_per_exp: 40M s_to_n: 10 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! linenum: 9.000 targname: NGC5457-4 config: WFC opmode: IMAGE aperture: ALL sp_element: F547M num_exp: 1 time_per_exp: 8M s_to_n: 10 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! linenum: 10.000 targname: NGC5457-4 config: WFC opmode: IMAGE aperture: ALL sp_element: F487N num_exp: 1 time_per_exp: 8M s_to_n: 10 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! linenum: 11.000 targname: NGC5457-4 config: WFC opmode: IMAGE aperture: ALL sp_element: F502N num_exp: 1 time_per_exp: 13M s_to_n: 30 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! linenum: 12.000 targname: NGC5457-4 config: WFC opmode: IMAGE aperture: ALL sp_element: F375N num_exp: 1 time_per_exp: 25M s_to_n: 30 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! linenum: 13.000 targname: NGC5457-4 config: WFC opmode: IMAGE aperture: ALL sp_element: F284W num_exp: 1 time_per_exp: 5M s_to_n: 30 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! linenum: 14.000 targname: NGC5457-4 config: WFC opmode: IMAGE aperture: ALL sp_element: F656N num_exp: 1 time_per_exp: 10M s_to_n: 30 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! linenum: 15.000 targname: NGC6822-1 config: WFC opmode: IMAGE aperture: ALL sp_element: F487N num_exp: 1 time_per_exp: 20M s_to_n: 30 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! linenum: 16.000 targname: NGC6822-1 config: WFC opmode: IMAGE aperture: ALL sp_element: F547M num_exp: 1 time_per_exp: 4M s_to_n: 30 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! linenum: 17.000 targname: NGC6822-1 config: WFC opmode: IMAGE aperture: ALL sp_element: F487N num_exp: 1 time_per_exp: 4M s_to_n: 30 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! linenum: 18.000 targname: NGC6822-1 config: WFC opmode: IMAGE aperture: ALL sp_element: F502N num_exp: 1 time_per_exp: 7M s_to_n: 30 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! linenum: 19.000 targname: NGC6822-1 config: WFC opmode: IMAGE aperture: ALL sp_element: F375N num_exp: 1 time_per_exp: 15M s_to_n: 30 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! linenum: 20.000 targname: NGC6822-1 config: WFC opmode: IMAGE aperture: ALL sp_element: F284W num_exp: 1 time_per_exp: 5M s_to_n: 30 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! linenum: 21.000 targname: NGC6822-1 config: WFC opmode: IMAGE aperture: ALL sp_element: F656N num_exp: 1 time_per_exp: 5M s_to_n: 30 fluxnum_1: 1 priority: 1 param_1: SUM=2X2 ! ! end of exposure logsheet ! No scan data records found