!  File:  3335C.PROP
!  Database:  PEPDB
!  Date:  19-FEB-1994:03:50:12

coverpage:

  title_1:         BULGE STELLAR POPULATIONS IN SO GALAXIES - CYCLE 3
    sci_cat:       GALAXIES & CLUSTERS
    sci_subcat:    NEARBY GALAXIES
    proposal_for:  AUG/FOC
    longterm:      2
    cont_id:       3487
    pi_title:      DR.
    pi_fname:      JEAN
    pi_mi:         M
    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:     4.39
    num_pri:       4
    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:        following cycle2 observations it is proposed to observe
    line_2:        NGC3115 with the F342W filter and NGC5102 with the F220W filter
    line_3:        in order to get color information on the massive stars, if any.

!

  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:        7
    section:       1
    line_1:        we plan to use IRAF/STSDAS on workstations

!

  question:        9
    section:       1
    line_1:        GTO program ID 1246 and cycle 2 observations on this program

!
!end of general form text

general_form_address:

  lname:           DEHARVENG
    fname:         J.
    mi:            M.
    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:         420584F

!
! end of general_form_address records

fixed_targets:

    targnum:       1
    name_1:        NGC5102
    descr_1:       E,302
    pos_1:         RA=13H 21M 57.5S +/- 4",
    pos_2:         DEC=-36D 37' 49" +/- 4"
    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 +/- 4",
    pos_2:         DEC=-7D 43' 5" +/- 4"
    equinox:       2000
    rv_or_z:       V=698
    acqpr_1:       EXT
    fluxnum_1:     1
    fluxval_1:     V=25.7, TYPE=B1V

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       1.000
    targname:      NGC5102
    config:        FOC/48
    opmode:        IMAGE
    aperture:      512X512
    sp_element:    F220W
    num_exp:       1
    time_per_exp:  2280S
    s_to_n:        6
    fluxnum_1:     2
    priority:      1
    req_1:         CYCLE 3 / 1-2

!

    linenum:       2.000
    targname:      NGC3115
    config:        FOC/48
    opmode:        IMAGE
    aperture:      512X512
    sp_element:    F342W
    num_exp:       1
    time_per_exp:  1400S
    s_to_n:        6
    fluxnum_1:     1
    priority:      2

!
! end of exposure logsheet

! No scan data records found