!   $Id: 5127,v 4.1 1994/07/27 15:18:11 pepsa Exp $

coverpage:

  title_1:         BINARIES IN GLOBULAR CLUSTERS (FOS 37) N6712 SPECTROSCOPY:
    title_2:       CYCLE 4
    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:       2
    fos:           X
    pi_position:   CHAIR AND PROFESSOR
! end of coverpage

abstract:

    line_1:        UV spectroscopy will be used to probe the nature of the
    line_2:        likely counterpart, star S, to the luminous central X-ray
    line_3:        burst source in NGC6712.

!
! 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:          MARTIN MARIETTA CORPORATION
    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:        Based on a WFPC image, we have identified the likely
    line_2:        optical/UV counterpart to a globular cluster X-ray
    line_3:        source. Using astrometry from that PC image, we now wish
    line_4:        to take a UV FOS spectrum of the likely counterpart (called
    line_5:        star S) using the G160L grating. An offset star will be
    line_6:        acquired first, and then a blind pointing (based on
    line_11:       the PC image astrometry) will be performed to star S.

!

  question:        4
    section:       1
    line_1:        HST is essential, because of the need for spatially-resolved
    line_2:        UV spectra in the corwded globular cluster core.

!


!

  question:        9
    section:       1
    line_1:        All FOS IDT (GTO and AUG) data.

!

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

!
!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:       17
    name_1:        NGC6712-OFFSET
    descr_1:       A,139
    pos_1:         RA = 18H 53M 04.97S +/- 0.01S,
    pos_2:         DEC = -08D 42' 18.2" +/- 0.3"
    equinox:       2000
    comment_1:     E(B-V) FOR THE CLUSTER IS 0.48.
    comment_2:     SPECTRAL TYPE IS G (IF IN
    comment_3:     CLUSTER) OR K (IF FOREGROUND).
    fluxnum_1:     1
    fluxval_1:     V = 16.00 +/- 0.05
    fluxnum_2:     2
    fluxval_2:     B = 17.00 +/- 0.05
    fluxnum_3:     3
    fluxval_3:     U = 17.54 +/- 0.05

!

    targnum:       28
    name_1:        NGC6712-STAR
    name_2:        STAR-S
    descr_1:       A,165
    pos_1:         RA-OFF = -0.13S +/- 0.01S,
    pos_2:         DEC-OFF = -2.31" +/- 0.1",
    pos_3:         FROM 17
    equinox:       2000
    acqpr_1:       COMP
    fluxnum_1:     1
    fluxval_1:     B = 20.9 +/- 0.5

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       2.000
    targname:      NGC6712-OFFSET
    config:        FOS/BL
    opmode:        ACQ/BINARY
    aperture:      4.3
    sp_element:    MIRROR
    num_exp:       1
    time_per_exp:  68.0S
    fluxnum_1:     1
    priority:      1
    req_1:         ONBOARD ACQ FOR 3;
    req_2:         CYCLE 4/2-4;
    comment_1:     ACQUIRE OFFSET STAR

!

    linenum:       3.000
    targname:      NGC6712-OFFSET
    config:        FOS/BL
    opmode:        ACQ/PEAK
    aperture:      0.3
    sp_element:    MIRROR
    num_exp:       1
    time_per_exp:  25.0S
    fluxnum_1:     1
    priority:      1
    param_1:       SEARCH-SIZE-X=3,
    param_2:       SCAN-STEP-X=0.10,
    param_3:       SEARCH-SIZE-Y=3,
    param_4:       SCAN-STEP-Y=0.10
    req_1:         ONBOARD ACQ FOR 4;
    comment_1:     ACQUIRE OFFSET STAR.
    comment_2:     SINCE THE 0.5" APERTURE IS
    comment_3:     USED FOR THE SCIENCE OBS,
    comment_4:     WE NEED TO PEAK UP TO REFINE THE
    comment_5:     CENTERING.

!

    linenum:       4.000
    targname:      NGC6712-STAR
    config:        FOS/BL
    opmode:        ACCUM
    aperture:      0.5
    sp_element:    G160L
    num_exp:       1
    time_per_exp:  6100S
    fluxnum_1:     1
    priority:      1
    comment_1:     BLIND OFFSET TO SCIENCE
    comment_2:     TARGET.

!
! end of exposure logsheet

! No scan data records found