! File: 3219C.PROP ! Database: PEPDB ! Date: 18-FEB-1994:22:21:19 coverpage: title_1: IMAGING OF M31-GROUP GALAXIES: FUTURE-CYCLE CONTINUATION sci_cat: GALAXIES & CLUSTERS sci_subcat: NEARBY GALAXIES proposal_for: GTO/OS cont_id: 1277 pi_title: PROF. pi_fname: IVAN pi_mi: R. pi_lname: KING pi_inst: UNIVERSITY OF CALIFORNIA, BERKELEY pi_country: USA pi_phone: (510)642-2206 keywords_1: LOCAL GROUP hours_pri: 4.00 hours_par: 4.00 num_pri: 2 num_par: 2 wf_pc: Y foc: Y pi_position: PROF. OF ASTRONOMY ! end of coverpage abstract: line_1: This is the remainder of proposal OS-1277, consisting of the line_2: parts that can be done only after the spherical aberration is line_3: corrected. It consists of B and V FOC/96 imaging of M31 and M32, line_4: far enough off the centers that there should be resolution down line_5: to the limiting magnitude, so that color-magnitude arrays can be line_6: derived. line_8: Parallel exposures with the PC will be used to derive line_9: color-magnitude arrays of two M31 globular clusters. ! ! end of abstract general_form_proposers: lname: KING fname: IVAN title: PROF. mi: R. inst: UNIV. OF CALIFORNIA country: U.S.A. ! lname: DISNEY fname: MICHAEL title: PROF. mi: J. inst: UNIV. OF CARDIFF country: U.K. esa: Y ! lname: DEHARVENG fname: JEAN-MICHEL title: DR. inst: LABORATOIRE D'ASTRONOMIE SPATIALE, MARSEILLE country: FRANCE esa: Y ! lname: CRANE fname: PHILIPPE title: DR. inst: EUROPEAN SOUTHERN OBSERVATORY country: GERMANY ! ! end of general_form_proposers block general_form_text: question: 3 section: 0 line_1: A field 6 arcmin from the center of M31, and another 2 arcmin line_2: from the center of M32. Exposures will be 60M each in line_3: F430W and F480LP, for color-magnitude arrays. line_5: Parallel exposures with PC on M31 globular clusters G233 and G142, line_6: in F555W and F785LP, for color-magnitude arrays. line_8: All exposures in Cycle 9. ! question: 4 section: 0 line_1: In all of these exposures, resolving power and faintness are of line_2: the essence. They cannot be done in the present condition of line_3: imagery. ! question: 5 section: 0 line_1: Simulations indicate that we should reach to 26th or 27th magnitude line_2: in these fields, without excessive crowding. ! question: 6 section: 1 line_1: Note that all FOC exposures have parallel WFC exposures (so that line_2: the true efficiency of HST usage is much higher than indicated by line_3: the percentage on the cover page). At Phase II, ORIENT will be a line_4: requirement on all primary exposures. If any exposures turn out to line_5: have orientations that have no guide stars, the orientation will be line_6: changed to cover some other field of interest. In this region, line_7: nearly every field is of interest. ! question: 6 section: 2 line_1: It is assumed that PSF's will be available without the need to add line_2: observations to this program to secure them. (Yes, PSF's will line_3: still be needed, on account of the diffraction pattern.) ! question: 7 section: 0 line_1: At Berkeley we have a VMS cluster and a Sun cluster. I have a line_2: Microvax II GPX and a Sun IPC with a gigabyte disk. For software line_3: we have been using Vista, DAOPHOT, and IRAF/STSDAS. Although it is line_4: an unhappy fact that no one has yet arrived at the ideal method of line_5: doing stellar photometry on HST images, I am doing at least as well line_6: as anyone else and am in contact with most of those who are making line_7: efforts in this direction. line_9: My collaborators on the FOC IDT have access to all the resources of line_10: the Institute in general, and of the FOC group in particular. line_11: Crane has all sorts of resources at ESO, and Deharveng is well line_12: provided at Marseille. ! question: 9 section: 1 line_1: SAO-3121, MORPHOLOGY OF FAINT GALAXIES - PART II line_2: GTO-1277, IMAGING OF M31-GROUP GALAXIES line_3: GTO-1278, SPECTROSCOPY OF THE CENTERS OF M31, M32, AND NGC 205 line_4: GTO-1279, STRUCTURE OF GLOBULAR CLUSTERS line_5: GTO-1280, COLLAPSED CORES OF GLOBULAR CLUSTERS line_6: GTO-1281, THE FAINT POPULATION IN BAADE'S WINDOW line_7: GTO-1282, IMAGING OF HIGH-REDSHIFT FIELD GALAXIES AND CLUSTERS line_8: GTO-3217, (continuation of 1280) line_9: GTO-3218, (continuation of 1279) line_10: GTO-3219, (continuation of 1277) line_11: GTO-3325, (continuation of 1279, 3218) ! question: 9 section: 2 line_1: 3121 produced a report that I am told was quite useful to the Cycle line_2: 1 Re-TAC, and also the publication below. line_4: Otherwise all I have gotten up to now is a pair of exposures on the line_5: center of Omega Centauri, which are in the early stages of line_6: reduction; the center of M32 and of the collapsed-core line_7: globular cluster NGC7099, also under reduction. line_9: In Cycle 1 I have put all of 1281 and all of the 1279 exposures on line_10: NGC6624. ! question: 9 section: 3 line_1: "The Current Ability of HST to Reveal Morphological Structure in line_2: Medium-Redshift Galaxies", King, I.R., et al. (8 other authors), line_3: Astron. J., to appear in Oct. 1991 issue. ! question: 10 section: 0 line_1: Hardware/software as above. Postdoc + RA's. GTO funding (from line_2: NASA). ! !end of general form text general_form_address: lname: KING fname: IVAN mi: R. title: PROF. category: PI inst: UNIVERSITY OF CALIFORNIA, BERKELEY addr_1: ASTRONOMY DEPARTMENT addr_2: UNIVERSITY OF CALIFORNIA city: BERKELEY state: CA zip: 94720 country: U.S.A. phone: (510)642-2206 telex: (910)366-7114 from_date: 15-MAR-92 to_date: 31-DEC-99 ! ! end of general_form_address records fixed_targets: targnum: 1 name_1: NGC224-OFF-4 descr_1: E,301,913 pos_1: RA = 00H 40M 17.9S +/- 0.1S, pos_2: DEC = +40D 54' 03" +/- 1" equinox: 1950 ! targnum: 2 name_1: NGC221-OFF-3 descr_1: E,303,913 pos_1: RA = 00H 40M 01.54S +/- 0.1S, pos_2: DEC = +40D 33' 38.1" +/- 1" equinox: 1950 comment_1: THE FOLLOWING ARE TARGETS FOR comment_2: PARALLEL EXPOSURES. ! targnum: 3 name_1: G142 descr_1: D,201 pos_1: RA = 00H 39M 29.9S +/- 0.1S, pos_2: DEC = +40D 32' 13" +/- 1" equinox: 1950 ! targnum: 4 name_1: G233 descr_1: D,201 pos_1: RA = 00H 40M 52.5S +/- 0.1S, pos_2: DEC = +40D 51' 47" +/- 1" equinox: 1950 ! ! end of fixed targets ! No solar system records found ! No generic target records found exposure_logsheet: linenum: 1.000 sequence_1: DEFINE sequence_2: STD targname: # config: FOC/96 opmode: IMAGE aperture: 512X512 sp_element: # num_exp: 1 time_per_exp: 60M priority: # ! linenum: 2.000 sequence_1: DEFINE sequence_2: PAR targname: # config: PC opmode: IMAGE aperture: ALL sp_element: # num_exp: 1 time_per_exp: 60M priority: # param_1: CR-SPLIT=NO, param_2: PRE-FLASH=YES ! linenum: 3.000 sequence_1: USE STD targname: NGC224-OFF-4 sp_element: F430W priority: 1 req_1: ORIENT 52.2D +/- 0.1D; req_2: CYCLE 9 /3-10; req_3: GROUP 3,5 NO GAP ! linenum: 4.000 sequence_1: USE PAR targname: G233 sp_element: F555W priority: 1 req_1: PAR WITH 3 ! linenum: 5.000 sequence_1: USE STD targname: NGC224-OFF-4 sp_element: F480LP priority: 1 req_1: SAME ORIENT FOR 5 AS 3; req_2: SAME POS FOR 5 AS 3; ! linenum: 6.000 sequence_1: USE PAR targname: G233 sp_element: F785LP priority: 1 req_1: PAR WITH 5 ! linenum: 7.000 sequence_1: USE STD targname: NGC221-OFF-3 sp_element: F430W priority: 1 req_1: ORIENT 198.6D +/- 0.1D; req_2: GROUP 7,9 NO GAP ! linenum: 8.000 sequence_1: USE PAR targname: G142 sp_element: F555W priority: 1 req_1: PAR WITH 7 ! linenum: 9.000 sequence_1: USE STD targname: NGC221-OFF-3 sp_element: F480LP priority: 1 req_1: SAME ORIENT FOR 9 AS 7; req_2: SAME POS FOR 9 AS 7 ! linenum: 10.000 sequence_1: USE PAR targname: G142 sp_element: F785LP priority: 1 req_1: PAR WITH 9 ! ! end of exposure logsheet ! No scan data records found