! $Id: 5153,v 7.1 1994/10/04 20:08:50 pepsa Exp $ coverpage: title_1: UV-BRIGHT STARS IN LEO I sci_cat: GALAXIES & CLUSTERS sci_subcat: STELLAR POPULATIONS proposal_for: GTO/FOC longterm: 2 cont_id: 3105 pi_title: DR. pi_fname: JEAN-MICHEL pi_lname: DEHARVENG pi_inst: LABORATOIRE D'ASTRONOMIE SPATIALE, CNRS, MARSEILLE pi_country: FRANCE pi_phone: (33) 91055917 hours_pri: 3.50 hours_par: 3.50 num_pri: 1 num_par: 1 wf_pc: Y foc: Y pi_position: DR. ! end of coverpage abstract: line_1: FOC ultraviolet images have resolved PAGB (Post-Asymptotic-Giant- line_2: Branch) stars in the inner bulge of the galaxy M31. These stars, line_3: however, contribute to less than 20 % of the total observed UV flux. line_4: The bulk of the UV emission should be explained by stars which, line_5: in metal-rich population, are predicted to move from the giant line_6: branch to the left of the HR diagram while skipping the AGB line_7: (Asymptotic-Giant-Branch) either partially or totally. line_8: The dwarf spheroidal galaxy Leo I provides an opportunity to line_9: resolve these categories of stars at intrinsically fainter level line_10: than possible in M31, down to the AGB-manque or HB phases of line_11: evolution. Observations will be performed with the FOC and the line_12: WFPC2 in parallel mode. ! ! end of abstract general_form_proposers: lname: DEHARVENG fname: JEAN-MICHEL title: DR. inst: LABORATOIRE D'ASTRONOMIE SPATIALE, CNRS, MARSEILLE country: FRANCE esa: Y ! lname: KING fname: IVAN title: PROF. inst: ASTRONOMY DEPT., UNIVERSITY OF CALIFORNIA, BERKELEY country: USA ! ! end of general_form_proposers block general_form_text: question: 3 section: 1 line_1: Observations with the FOC F175W and F320W filters will allow to line_2: detect the UV-bright stars and to give their temperature and line_3: luminosity distribution. line_4: The angular extent of the galaxy allows parallel observations with line_5: the WFPC2 and comparable UV filters (F170W and F300W). ! !end of general form text general_form_address: lname: DEHARVENG fname: JEAN-MICHEL title: DR. category: PI inst: LABORATOIRE D'ASTRONOMIE SPATIALE, CNRS addr_1: TRAVERSE DU SIPHON, LES TROIS LUCS, BP 8 city: MARSEILLE CEDEX 12 zip: 13376 country: FRANCE phone: (33) 91055917 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: LEOI descr_1: E,308 pos_1: RA = 10H 8M 26.7S +/- 1", pos_2: DEC = 12D 18' 29" +/- 1" equinox: 2000 rv_or_z: V = 168 fluxnum_1: 1 fluxval_1: SURF(V) = 22.3 +/- 0.2 ! ! end of fixed targets ! No solar system records found generic_targets: targnum_1: 2 name_1: LEOI-GEN descr_1: E,308 criteria_1: RA=10H 08M 26.7S, criteria_2: DEC=12D 18' 29", criteria_3: R=10' fluxnum_1: 1 fluxval_1: SURF(V) = 22.3 +/- 0.2 ! ! end of generic targets exposure_logsheet: linenum: 1.000 targname: LEOI config: FOC/96 opmode: IMAGE aperture: 512X1024 sp_element: F175W num_exp: 1 time_per_exp: 8400S s_to_n: 10 fluxnum_1: 1 priority: 1 param_1: PIXEL = 50X25 req_1: CYCLE 4 ! linenum: 2.000 targname: LEOI config: FOC/96 opmode: IMAGE aperture: 512X1024 sp_element: F342W num_exp: 1 time_per_exp: 4200S s_to_n: 10 fluxnum_1: 1 priority: 1 param_1: PIXEL = 50X25 req_1: CYCLE 4 ! linenum: 5.000 targname: LEOI-GEN config: WFPC2 opmode: IMAGE aperture: WFALL sp_element: F170W num_exp: 1 time_per_exp: 8400S s_to_n: 10 fluxnum_1: 1 priority: 1 req_1: PAR; CYCLE 4 comment_1: PARALLEL WITH 1 ! linenum: 6.000 targname: LEOI-GEN config: WFPC2 opmode: IMAGE aperture: WFALL sp_element: F300W num_exp: 1 time_per_exp: 4200S s_to_n: 10 fluxnum_1: 1 priority: 1 req_1: PAR; CYCLE 4 comment_1: PARALLEL WITH 2 ! ! end of exposure logsheet ! No scan data records found