! File: 1046C.PROP ! Database: PEPDB ! Date: 15-FEB-1994:23:40:03 coverpage: title_1: IMAGING AND UV SPECTROPHOTOMETRY OF LOCAL GROUP PLANETARY NEBULAE title_2: (FOS 26) -- CYCLE 0 sci_cat: INTERSTELLAR MEDIUM proposal_for: GTO/FOS pi_title: DR. pi_fname: HOLLAND pi_mi: C. pi_lname: FORD pi_inst: SPACE TELESCOPE SCIENCE INSTITUTE pi_country: USA pi_phone: (301) 338-4803 keywords_1: NEBULA, PLANETARIES, CENTRAL STARS, GALAXIES, K648 hours_pri: 9.54 num_pri: 29 wf_pc: X fos: X ! end of coverpage abstract: line_1: WF/PC interference filter pictures will be used to resolve the shells of line_2: planetary nebulae in the LMC and to resolve the shell of K648 in M15. The line_3: angular diameters of the shells will be combined with echelle expansion line_4: velocities to derive the ages of nebulae. Ultraviolet spectra of the central line_5: stars will be used to derive the stars' effective temperatures and magnitudes, line_6: with objective of placing the stars on evolutionary tracks in an M-Teff line_7: diagram. UV spectra of the LMC nebulae, K648, and the brightest nebula in M32, line_8: NGC205, and NGC185 will be used to derive chemical compositions and physical line_9: conditions in the nebulae. ! ! end of abstract general_form_proposers: lname: BEAVER fname: EDWARD inst: UC, SAN DIEGO country: USA ! lname: BURBIDGE fname: E. MARGARET inst: UC, SAN DIEGO country: USA ! lname: MARGON fname: BRUCE inst: WASHINGTON, UNIVERSITY OF country: USA ! lname: ANGEL fname: J. ROGER mi: P. inst: ARIZONA, UNIVERSITY OF country: USA ! lname: BARTKO fname: FRANK inst: APPLIED RESEARCH CORPORATION country: USA ! lname: DAVIDSEN fname: ARTHUR mi: F. inst: JOHNS HOPKINS UNIVERSITY country: USA ! lname: HARMS fname: RICHARD mi: J. inst: APPLIED RESEARCH CORPORATION country: USA ! lname: BOHLIN fname: RALPH inst: SPACE TELESCOPE SCIENCE INSTITUTE country: USA ! lname: FORD fname: HOLLAND mi: C. inst: SPACE TELESCOPE SCIENCE INSTITUTE country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: Cycle 0: 56, 68, 74, 92 line_2: Cycle 1: 40-44, 80, 86, 94-102 line_3: Cycle 2: 9-20, 38, 46-54.1, 58-66.1, line_4: 70-72.1, 76-78.1, 82-84.1, 88-90.1 ! question: 5 section: 1 line_1: ! question: 5 section: 2 line_1: The SV prerequisite programs for all FOS line_2: observations in this program are: line_3: Prop ID 2195 FOS Target Acquisition Tests line_4: - All observations line_5: Prop ID 1317 Int./Ext. Wavelength Offsets line_6: - 1st target line_7: Prop ID 1318 Spectral Flat Fields line_8: - 1st target line_9: Prop ID 1320 Absolute Spectrophotometry line_10: - 1st visit of bright targets line_11: All WF/PC imaging with a center wavelength line_12: blueward of 5000 Angstroms requires UV flood ! question: 12 section: 1 line_1: The observations of the LMC planetaries constitute an integrated program to line_2: establish to evolution of central stars, and will not be complete until seven line_3: of the nine have been observed. Data should not be released until one year line_4: after completion of the seventh planetary nebula. Likewise, the three line_5: planetaries in NGC205, NGC185, and M32 constitute a program which will not be line_6: complete until two of the three planetaries have been observed. ! question: 13 section: 1 line_1: WF/PC pictures of K648 and LMC planetaries will be used to resolve their line_2: shells. Small aperture FOS UV spectra of the central stars will be used to line_3: place the central stars on evolutionary tracks in an M-Teff diagram. Chemical line_4: composition and physical conditions in the shells will be derived from UV line_5: spectra of the nebulae. ! !end of general form text general_form_address: lname: FORD fname: HOLLAND mi: C. title: DR. category: PI inst: SPACE TELESCOPE SCIENCE INSTITUTE addr_1: HOMEWOOD CAMPUS addr_2: 3700 SAN MARTIN DRIVE city: BALTIMORE state: MD zip: 21218 country: USA phone: (301) 338-4803 ! ! end of general_form_address records fixed_targets: targnum: 7 name_1: LMC-WS9 descr_1: PLANETARY NEBULA IN THE LMC pos_1: TBD-EARLY, pos_2: RA=05H 08M 2.21S +/- 0.3", pos_3: DEC=-68D 40' 29.6" +/- 0.3" equinox: 2000 rv_or_z: V=280 plate_req: Y fluxnum_1: 1 fluxval_1: F-LINE(5007)=5 +/- 2E-12, fluxval_2: E(B-V)=0.13 ! targnum: 9 name_1: LMC-WS33 descr_1: ^ pos_1: TBD-EARLY, pos_2: RA=5H 34M 21.25S +/- 0.3", pos_3: DEC=-68D 58' 25.0" +/- 0.3" equinox: 2000 rv_or_z: V=252 plate_req: Y fluxnum_1: 1 fluxval_1: F-LINE(5007)=5 +/- 2E-12, fluxval_2: E(B-V)=0.13 ! targnum: 10 name_1: LMC-WS35 descr_1: PLANETARY NEBULA IN THE LMC pos_1: TBD-EARLY, pos_2: RA=5H 36M 20.87S +/- 0.3", pos_3: DEC=-67D 18' 8.2" +/- 0.3" equinox: 2000 rv_or_z: V=287 plate_req: Y fluxnum_1: 1 fluxval_1: F-LINE(5007)=5 +/- 2E-12, fluxval_2: E(B-V)=0.13 ! targnum: 13 name_1: K648 descr_1: PLANETARY NEBULA IN M15 pos_1: TBD-EARLY, pos_2: RA=21H 27M 34.4S +/- 1", pos_3: DEC=+11D 57' 14.3" +/- 1" equinox: 1950 rv_or_z: V=-115 fluxnum_1: 1 fluxval_1: F-LINE(5007)=1.5E-12, E(B-V)=0.08 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 22.000 sequence_1: DEFINE PS1 targname: # config: PC opmode: IMAGE aperture: ALL sp_element: F664N num_exp: 1 time_per_exp: 150S priority: # param_1: CR-SPLIT=NO, param_2: PRE-FLASH=YES comment_1: PREFLASH ALL WFC AND PC EXPOSURES IN comment_2: THIS PROGRAM IF NEEDED TO ELIMINATE comment_3: DEFERRED CHARGE PROBLEMS. ! linenum: 26.000 sequence_1: ^ targname: # config: ^ opmode: ^ aperture: ^ sp_element: F502N num_exp: ^ time_per_exp: 150S priority: # param_1: CR-SPLIT=NO, param_2: PRE-FLASH=YES req_1: SAME POS FOR 26 AS 22 ! linenum: 56.000 sequence_1: USE PS1 targname: LMC-WS9 time_per_exp: X2.0 priority: 3 req_2: GUID TOL 0.020"; req_3: CYCLE 0 comment_1: EARLY ACQ FOR EXPOSURES IN LATER comment_2: CYCLES. ! linenum: 68.000 sequence_1: USE PS1 targname: LMC-WS33 time_per_exp: X2.0 priority: 3 req_2: GUID TOL 0.020"; req_3: CYCLE 0 comment_1: EARLY ACQ FOR EXPOSURES IN LATER comment_2: CYCLES. ! linenum: 74.000 sequence_1: USE PS1 targname: LMC-WS35 time_per_exp: X2.0 priority: 2 req_2: GUID TOL 0.020"; req_3: CYCLE 0 comment_1: EARLY ACQ FOR EXPOSURES IN LATER comment_2: CYCLES. ! linenum: 92.000 sequence_1: USE PS1 targname: K648 time_per_exp: X2.0 priority: 1 req_2: GUID TOL 0.020"; req_3: CYCLE 0 comment_1: EARLY ACQ FOR EXPOSURES IN LATER comment_2: CYCLES. ! ! end of exposure logsheet ! No scan data records found