!   $Id: 5630,v 5.1 1994/07/27 19:55:07 pepsa Exp $
coverpage:
  title_1:         LUMINOUS STARS IN OLD STELLAR POPULATIONS
    sci_cat:       GALAXIES & CLUSTERS
    sci_subcat:    STELLAR POPULATIONS
    proposal_for:  GTO/WF2
cont_id: 5209
    pi_fname:      JOHN
    pi_mi:         T
    pi_lname:      TRAUGER
    pi_country:    USA
    hours_pri:     6.889
    num_pri:       5
    wf_pc:         Y
    sc_time:       9.880
    pgm_eff:       69.7
abstract:
    line_1:        Two outstanding problems in Stellar Populations are the existence
    line_2:        of luminous asymptotic giant branch stars in the bulges of Local
    line_3:        Group galaxies and the existence of an ultraviolet upturn in the
    line_4:        spectral energy distribution of many early type galaxies. It is likely
    line_5:        that the UV upturn is due to the presence of very hot luminous
    line_6:        post-AGB stars of some kind. The aim of these observations is to
    line_7:        resolve the source of the UV upturn into stars and to learn more
    line_8:        about the AGB luminosity function in early type galaxies.
general_form_proposers:
  lname:           TRAUGER
    fname:         JOHN
    title:         PI
    mi:            T
    inst:          JPL
    country:       USA
  lname:           MOULD
    fname:         JEREMY
    inst:          CALTECH
    country:       USA
  lname:           CLARKE
    fname:         JOHN
    inst:          UNIV. OF MICHIGAN
    country:       USA
  lname:           HOESSEL
    fname:         JOHN
    inst:          UNIV. OF WISCONSIN
    country:       USA
  lname:           GALLAGHER
    fname:         JAY
    inst:          UNIV. OF WISCONSIN
    country:       USA
  lname:           HOLTZMAN
    fname:         JOHN
    inst:          LOWELL OBSERVATORY
    country:       USA
  lname:           HESTER
    fname:         JEFF
    inst:          ARIZONA STATE UNIV.
    country:       USA
  lname:           WESTPHAL
    fname:         JAMES
    inst:          CALTECH
    country:       USA
  lname:           BURROWS
    fname:         CHRIS
    inst:          STSCI
    country:       USA
  lname:           CRISP
    fname:         DAVID
    inst:          JPL
    country:       USA
  lname:           GRIFFITHS
    fname:         RICHARD
    inst:          JOHNS HOPKINS UNIV
    country:       USA
general_form_text:
  question:        3
    section:       1
    line_1:        Most of these observations are UV imaging designed to resolve the ultraviolet
    line_2:        sources at S/N = 10.
    line_3:        The following targets require deep imaging in the optical: NGC 6397, the Fornax
    line_4:        dE, NGC 3115, & NGC 5128. With WFPC2 we expect a limiting V magnitude in 75
    line_5:        minutes of V = 27.6 mag.
  question:        4
    section:       1
    line_1:        WFPC2 offers the highest spatial resolution UV imaging yet proposed.  WFPC2
    line_2:        offers the deepest optical imaging likely to be achieved this decade.
    line_3:        stlook2 says 0.106 electrons/second for a V=25 B0 star through nf160w.
general_form_address:
  lname:           Trauger
    fname:         John
    mi:            T
    category:      PI
    inst:          JPL
    addr_1:        4800 Oak Grove Drive
    city:          Pasadena
    state:         CA
    zip:           91109
    country:       USA
    phone:         818 354 9594
fixed_targets:
    targnum:       1
    name_1:        NGC6397
    descr_1:       C,201
    pos_1:         RA=17h40m41.5s        +/- 2",
    pos_2:         DEC=-53d30'25"          +/- 2"
    equinox:       2000
    pm_or_par:     N
    fluxnum_1:     1
    targnum:       2
    name_1:        NGC7099
    descr_1:       C,201
    pos_1:         RA=21H40M22.0S        +/- 2",
    pos_2:         DEC=-23D10'44"          +/- 2"
    equinox:       2000
    pm_or_par:     N
    fluxnum_1:     1
    targnum:       3
    name_1:        NGC1978
    descr_1:       D,201
    pos_1:         RA=5H28M41.3S           +/- 2",
    pos_2:         DEC=-66D16'24"           +/- 2"
    equinox:       1950
    pm_or_par:     N
    fluxnum_1:     1
    targnum:       4
    name_1:        M32
    descr_1:       E,304
    pos_1:         RA=0H42M41.7S         +/- 2",
    pos_2:         DEC=40D50'29"           +/- 2"
    equinox:       2000
    pm_or_par:     N
    comment_1:     THIS FIELD IS 85"S OF NUCLEUS
    comment_2:     AS REQUESTED BY WFPC1 TEAM
    fluxnum_1:     1
    targnum:       5
    name_1:        NGC205
    descr_1:       E,304
    pos_1:         RA=0H40M22.0S         +/- 2",
    pos_2:         DEC=41D41'7"            +/- 2"
    equinox:       2000
    pm_or_par:     N
    fluxnum_1:     1
exposure_logsheet:
    linenum:       1.000
    sequence_1:    DEFINE
    sequence_2:    UV
    targname:      #
    config:        WFPC2
    opmode:        IMAGE
    aperture:      WFALL-FIX
    sp_element:    F160BW
    num_exp:       2
    time_per_exp:  2000S
    priority:      1
    param_1:       CR-SPLIT=0.6,
    param_2:       CR-TOLERANCE=0.2,
    param_3:       ATD-GAIN=7
    req_1:         GROUP 1-2.1 NO GAP;
    req_2:         GROUP 1-2.1 WITHIN 1D;
    req_3:         POS TARG 33,33 / 1-2;
    linenum:       2.000
    sequence_1:    DEFINE
    sequence_2:    UV
    targname:      #
    config:        WFPC2
    opmode:        IMAGE
    aperture:      WFALL-FIX
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  10S
    priority:      1
    param_1:       CR-SPLIT=NO
    param_2:       ATD-GAIN=15
    req_1:         SAME POS FOR 2-2.1 AS 1;
    req_2:         SAME ORIENT FOR 2-2.1 AS 1
    linenum:       2.100
    sequence_1:    DEFINE
    sequence_2:    UV
    targname:      #
    config:        WFPC2
    opmode:        IMAGE
    aperture:      WFALL-FIX
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  100S
    priority:      1
    param_1:       CR-SPLIT=NO
    param_2:       ATD-GAIN=15
    linenum:       3.000
    sequence_1:    DEFINE
    sequence_2:    VIS
    targname:      #
    config:        WFPC2
    opmode:        IMAGE
    aperture:      WFALL-FIX
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  2000s
    param_1:       CR-SPLIT=0.6,
    param_2:       CR-TOLERANCE=0.2,
    param_3:       ATD-GAIN=7
    req_1:         GROUP 3-4 NO GAP;
    req_2:         GROUP 3-4 WITHIN 1D;
    linenum:       4.000
    sequence_1:    DEFINE
    sequence_2:    VIS
    targname:      #
    config:        WFPC2
    opmode:        IMAGE
    aperture:      WFALL-FIX
    sp_element:    F814W
    num_exp:       2
    time_per_exp:  2000s
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=0.6,
    param_2:       CR-TOLERANCE=0.2,
    param_3:       ATD-GAIN=15
    req_1:         SAME POS FOR 4 AS 3;
    req_2:         SAME ORIENT FOR 4 AS 3
    linenum:       6.000
    sequence_1:    USE
    sequence_2:    VIS
    targname:      NGC6397
    req_1:         CYCLE 4
    linenum:       7.000
    sequence_1:    USE
    sequence_2:    UV
    targname:      NGC7099
    req_1:         CYCLE 4
    linenum:       8.000
    sequence_1:    USE
    sequence_2:    UV
    targname:      NGC1978
    req_1:         CYCLE 4
    linenum:       9.000
    sequence_1:    USE
    sequence_2:    UV
    targname:      M32
    req_1:         CYCLE 4;
    req_2:         ORIENT 180D +/- 10D
    comment_1:     THIS ANGLE SPECIFIED BY WFPC1 TEAM
    linenum:       10.000
    sequence_1:    USE
    sequence_2:    UV
    targname:      NGC205
    req_1:         CYCLE 4
!~~~RPSS~~~,PSTANLEY,5209.prop, 8-MAR-1994 09:06