! 5708_v3.prop ! $Id: 5708,v 6.1 1995/02/02 21:40:43 pepsa Exp $ ! New ID=5708 coverpage: title_1: BULGE STELLAR POPULATIONS IN SO GALAXIES: title_2: CYCLE 4 CARRY-OVER sci_cat: GALAXIES & CLUSTERS sci_subcat: NEARBY GALAXIES proposal_for: AUG/FOC cont_id: 4070 pi_fname: JEAN-MICHEL pi_lname: DEHARVENG pi_inst: LABORATOIRE ASTRONOMIE SPATIALE pi_country: FRANCE pi_phone: 91 05 59 17 keywords_1: EARLY-TYPE GALAXIES, STAR FORMATION hours_pri: 5.89 num_pri: 3 foc: Y ! end of coverpage abstract: line_1: It is proposed to study the origin of the UV flux in elliptical-type line_2: population and to determine the respective contribution from young line_3: stars and from hot evolved stars. Two SO galaxies NGC 5102 and NGC line_4: 3115, at reasonable distance and with very different gas contents, line_5: have been selected. Observations through several filters line_6: (especially a far UV filter) will allow to resolve and study the line_7: massive stars, if they exist. The UV surface brightness of the line_8: unresolved background will be measured and will set constraints on line_9: the characteristics of hot evolved stars. ! ! end of abstract general_form_proposers: lname: ROCCA-VOLMERANGE fname: BRIGITTE inst: INSTITUTE OF ASTROPHYSICS, PARIS country: FRANCE esa: X ! lname: DEHARVENG fname: J. mi: M. inst: MARSEILLE OBSERVATORY country: FRANCE esa: X ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: It is proposed to observe the two galaxies with the UV filter line_2: F175W in order to reveal the massive and young stars if any; line_3: a complementary observation of NGC 5102 is made with the filter line_4: F320W and F320W+F4ND+F1ND (at f/96). A dwarf elliptical is observed line_5: for comparison with the F175W filter. line_6: NOTE: Due to problems with image shift and elongated PSF in F320W line_7: we have requested to change to F342W and we have been granted permission line_8: to make this change by STScI ( Nolan Walborn ) on 20 Sept., 1994. We line_9: have just made a straight substitution of F342W for F320W. No other line_10: changes are required. ! question: 4 section: 1 line_1: The high spatial resolution of the FOC will provide the possibility to resolve line_2: the young and massive stars, if they exist, in two examples of relatively line_3: nearby elliptical-type population. This capability is further improved by the line_4: good response of the FOC in the ultra-violet. At these wavelengths, the line_5: contrast of young and hot stars would be enhanced against the contribution of line_6: the main-sequence and giant-branch components of the old stellar population. ! ! question: 9 section: 1 line_1: GTO program ID 1246 ! !end of general form text general_form_address: lname: DEHARVENG fname: JEAN-MICHEL category: PI inst: LABORATOIRE ASTRONOMIE SPATIALE addr_1: C.N.R.S. addr_2: TRAVERSE DU SIPHON addr_3: LE TROIS LUCS city: BP8-13376 MARSEILLE CEDEX12 country: FRANCE phone: (33) 91 05 59 17 telex: ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: NGC5102 descr_1: E,302 pos_1: RA=13H 21M 57.5S +/- 1", pos_2: DEC=-36D 37' 49" +/- 1" equinox: 2000 rv_or_z: V=454 acqpr_1: EXT fluxnum_1: 1 fluxval_1: SURF(V)=17.5 fluxnum_2: 2 fluxval_2: V=25.2, TYPE=B1V ! targnum: 2 name_1: NGC3115 descr_1: E,302 pos_1: RA=10H 05M 14.2S +/- 1", pos_2: DEC=-7D 43' 5" +/- 1" equinox: 2000 rv_or_z: V=698 acqpr_1: EXT fluxnum_1: 1 fluxval_1: V=25.7, TYPE=B1V ! targnum: 3 name_1: NGC4321-DW5 descr_1: E,304 pos_1: RA=12H 23M 21.28S +/- 1", pos_2: DEC=15D 52' 5" +/- 1" equinox: 2000 rv_or_z: V=1610 acqpr_1: EXT fluxnum_1: 1 fluxval_1: V=26, TYPE=O8 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 targname: NGC5102 config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: F175W num_exp: 1 time_per_exp: 900S s_to_n: 6 fluxnum_1: 2 priority: 1 req_1: CYCLE 4 / 1-5.5; ! linenum: 1.500 targname: NGC5102 config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: F175W num_exp: 3 time_per_exp: 1000S s_to_n: 6 fluxnum_1: 2 priority: 1 req_1: GROUP 1-1.5 NO GAP; ! linenum: 2.000 targname: NGC5102 config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: F342W num_exp: 2 time_per_exp: 900S s_to_n: 6 fluxnum_1: 2 priority: 1 ! linenum: 3.000 targname: NGC5102 config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: F342W,F4ND,F1ND num_exp: 1 time_per_exp: 900S s_to_n: 6 fluxnum_1: 1 priority: 1 ! linenum: 4.000 targname: NGC3115 config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: F175W num_exp: 1 time_per_exp: 900S s_to_n: 6 fluxnum_1: 1 priority: 1 ! linenum: 4.500 targname: NGC3115 config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: F175W num_exp: 3 time_per_exp: 1000S s_to_n: 6 fluxnum_1: 1 priority: 1 req_1: GROUP 4-4.5 NO GAP; ! linenum: 5.000 targname: NGC4321-DW5 config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: F175W num_exp: 1 time_per_exp: 900S s_to_n: 6 fluxnum_1: 1 priority: 1 ! linenum: 5.500 targname: NGC4321-DW5 config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: F175W num_exp: 3 time_per_exp: 1000S s_to_n: 6 fluxnum_1: 1 priority: 1 req_1: GROUP 5-5.5 NO GAP; ! ! end of exposure logsheet ! No scan data records found