!  File:  3282C.PROP
!  Database:  PEPDB
!  Date:  19-FEB-1994:01:16:51

coverpage:

  title_1:         BINARIES IN GLOBULAR CLUSTERS (FOS 37): CYCLE 2 OBSERVATIONS
    sci_cat:       STELLAR ASTROPHYSICS
    proposal_for:  GTO/FOS
    cont_id:       1053
    pi_title:      PROF.
    pi_fname:      BRUCE
    pi_lname:      MARGON
    pi_inst:       WASHINGTON, UNIVERSITY OF
    pi_country:    USA
    pi_phone:      206-543-0089
    keywords_1:    X-RAY STAR, NOVA, GLOBULAR CLUSTER, NEUTRON STAR
    num_pri:       1
    wf_pc:         Y
    pi_position:   CHAIR AND PROFESSOR
! end of coverpage

abstract:

    line_1:        Imaging and spectroscopy will be used to attempt an optical identification
    line_2:        of a low luminosity X-ray source removed from the core, and thus to
    line_3:        verify the conjecture that these objects are related to CVs.

!
! end of abstract

general_form_proposers:

  lname:           BEAVER
    fname:         EDWARD
    inst:          UC, SAN DIEGO
    country:       USA

!

  lname:           BURBIDGE
    fname:         E. MARGARET
    inst:          UC, SAN DIEGO
    country:       USA

!

  lname:           MARGON
    fname:         BRUCE
    inst:          WASHINGTON, UNIVERSITY OF
    country:       USA

!

  lname:           ANGEL
    fname:         J. ROGER
    mi:            P.
    inst:          ARIZONA, UNIVERSITY OF
    country:       USA

!

  lname:           BARTKO
    fname:         FRANK
    inst:          UC, SAN DIEGO
    country:       USA

!

  lname:           DAVIDSEN
    fname:         ARTHUR
    mi:            F.
    inst:          JOHNS HOPKINS UNIVERSITY
    country:       USA

!

  lname:           HARMS
    fname:         RICHARD
    mi:            J.
    inst:          APPLIED RESEARCH CORPORATION
    country:       USA

!

  lname:           BOHLIN
    fname:         RALPH
    inst:          SPACE TELESCOPE SCIENCE INSTITUTE
    country:       USA

!

  lname:           FORD
    fname:         HOLLAND
    mi:            C.
    inst:          SPACE TELESCOPE SCIENCE INSTITUTE
    country:       USA

!
! end of general_form_proposers block

general_form_text:

  question:        3
    section:       1
    line_1:        WF/PC images of globular cluster interacting binaries will
    line_2:        be obtained as acquistions for follow-up FOS spectra in
    line_3:        cycle 3. If no interesting candidates are found, no
    line_4:        followup spectra will be taken. If an interesting looking
    line_5:        candidate is found, then follow-up spectra will be obtained
    line_6:        in a later cycle, with the specific gratings to be used
    line_7:        determined by the quality of the candidate.

!

  question:        5
    section:       1
    line_1:        The images must be obtained NON-INT to avoid unecessary
    line_2:        readout noise in these low S/N data

!

  question:        7
    section:       1
    line_1:        Data reduction will be performed at the ST ScI, and the analysis will be
    line_2:        performed using FOS IDT computer facilities.

!

  question:        10
    section:       1
    line_1:        Data analysis, research assistant support, and funding will be provided under
    line_2:        NASA's FOS GTO contract(s).

!

  question:        13
    section:       1
    line_1:        Multicolor WF/PC images will be used to search for the optical counterparts of
    line_2:        both central and noncentral X-ray sources. Objects identified through unusual
    line_3:        colors will be observed with the FOS. The recovery of two historical novae in
    line_4:        globular clusters, and spectra to yield abundances and possibly expansion
    line_5:        parallaxes, is also proposed.

!
!end of general form text

general_form_address:

  lname:           MARGON
    fname:         BRUCE
    category:      PI
    inst:          UNIVERSITY OF WASHINGTON
    addr_1:        ASTRONOMY DEPARTMENT, FM-20
    city:          SEATTLE
    state:         WA
    zip:           98195
    country:       USA
    phone:         206 543-0089
    telex:         4740096

!
! end of general_form_address records

fixed_targets:

    targnum:       1
    name_1:        NGC1851
    descr_1:       C,201,I,605
    pos_1:         RA=05H 12M 27.9S+/-0.1S,
    pos_2:         DEC=-40D 05' 59.7"+/-1"
    equinox:       1950
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 14.7+/-0.5

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       1.000
    sequence_1:    DEFINE
    sequence_2:    PC
    targname:      #
    config:        PC
    opmode:        IMAGE
    aperture:      PC8-FIX
    sp_element:    F336W
    wavelength:    3363
    num_exp:       1
    time_per_exp:  2000S
    fluxnum_1:     1
    priority:      1
    param_1:       PRE-FLASH=YES,
    param_2:       CR-SPLIT=NO
    req_1:         SEQ 1-3 NO GAP;
    req_2:         NON-INT / 1-3;
    req_3:         POS TARG -5.4,+5.4  / 1-3;
    comment_1:     PC PICTURES FOR SOURCE IDENTIFICATION.

!

    linenum:       2.000
    sequence_1:    DEFINE
    sequence_2:    PC
    targname:      #
    config:        PC
    opmode:        IMAGE
    aperture:      PC8-FIX
    sp_element:    F439W
    wavelength:    4385
    num_exp:       1
    time_per_exp:  2000S
    fluxnum_1:     1
    priority:      1
    param_1:       PRE-FLASH=YES,
    param_2:       CR-SPLIT=0.1

!

    linenum:       3.000
    sequence_1:    DEFINE
    sequence_2:    PC
    targname:      #
    config:        PC
    opmode:        IMAGE
    aperture:      PC8-FIX
    sp_element:    F336W
    wavelength:    3363
    num_exp:       1
    time_per_exp:  2000S
    fluxnum_1:     1
    priority:      1
    param_1:       PRE-FLASH=YES,
    param_2:       CR-SPLIT=NO

!

    linenum:       4.000
    sequence_1:    USE
    sequence_2:    PC
    targname:      NGC1851
    req_2:         CYCLE 2/ 1-4;

!
! end of exposure logsheet

! No scan data records found