!   $Id: 5665,v 27.1 1994/11/30 18:43:25 pepsa Exp $

coverpage:

  title_1:         MASS EXCHANGE BINARIES (FOS 34) CARRYOVER OBSERVATIONS
    sci_cat:       STELLAR ASTROPHYSICS
    proposal_for:  AUG/FOS
    cont_id:       4058
    pi_title:      PROF.
    pi_fname:      BRUCE
    pi_lname:      MARGON
    pi_inst:       WASHINGTON, UNIVERSITY OF
    pi_country:    USA
    pi_phone:      206-543-0089
    hours_pri:     7.10
    num_pri:       1
    fos:           Y
! end of coverpage

abstract:

    line_1:        The pre-launch FOS GTO program proposed a systematic study of degenerate stars
    line_2:        in binary systems, both in the field and in globular clusters, plus a handful
    line_3:        of related objects. For the isolated field systems, the emphasis is on spectro-
    line_4:        photometry (in many cases time-resolved over a pulse or orbital period) and
    line_5:        spectropolarimetry, to observe the effects of the intense ionizing flux emitted
    line_6:        by the compact object on the nearby normal star and/or accretion disk. While
    line_7:        some such effects are seen from the ground, they should be far more spectacular
    line_8:        in the UV. The GTO program for the globular cluster systems typically proposes
    line_9:        WF/PC or FOC images to locate candidates for cluster X-ray sources, followed by
    line_10:       confirming FOS spectroscopy. Our published FOC observations of M14 show that
    line_11:       even with the primary's spherical aberration, it is possible to reach flux
    line_12:       levels relevant to these problems with angular resolution far better than
    line_13:       achievable from the ground. Even one or two new close binaries identified
    line_14:       through this program will be extremely important, as these systems are thought
    line_15:       to dominate the kinetic energy budget of globular clusters, yet virtually none
    line_16:       are currently known. Also proposed for augmentation are two related programs:
    line_17:       FOS observations of the Crab pulsar and a study of UV-bright objects in
    line_18:       globular cluster cores. The increased FOS integration times caused by the
    line_19:       spherical aberration have drastically disrupted the original intended
    line_20:       scientific program; augmentation proposed here partially restores these efforts.

!
! end of abstract

general_form_proposers:

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

!

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

!

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

!

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

!

  lname:           BARTKO
    fname:         FRANK
    inst:          UNIVERSITY OF CALIFORNIA, SAN DIEGO
    country:       USA

!

  lname:           BEAVER
    fname:         EDWARD
    inst:          UNIVERSITY OF CALIFORNIA, SAN DIEGO
    country:       USA

!

  lname:           BURBIDGE
    fname:         E. MARGARET
    inst:          UNIVERSITY OF CALIFORNIA, SAN DIEGO
    country:       USA

!

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

!

  lname:           FORD
    fname:         HOLLAND
    mi:            C.
    inst:          JOHNS HOPKINS UNIVERSITY
    country:       USA

!

  lname:           HARTIG
    fname:         GEORGE
    mi:            F.
    inst:          SPACE TELESCOPE SCIENCE INSTITUTE
    country:       USA

!

  lname:           ANDERSON
    fname:         SCOTT
    mi:            F.
    inst:          UNIVERSITY OF WASHINGTON
    country:       USA

!

  lname:           DOWNES
    fname:         RONALD
    mi:            A.
    inst:          STSCI
    country:       USA

!

  lname:           ALLEN
    fname:         RICHARD
    mi:            P.
    inst:          UNIVERSITY OF ARIZONA
    country:       USA

!
! end of general_form_proposers block

general_form_text:

  question:        3
    section:       1
    line_1:        The intermediate polar DQ Her will be observed, including
    line_2:        UV FOS spectrophotometry of modest spectral resolution at
    line_3:        binary orbital phases of max light and time-resolved
    line_4:        FOS UV spectrophotometry through the 71S white dwarf
    line_5:        rotation period.

!

  question:        5
    section:       1
    line_1:        All observations in this program are time critical.  The 
    line_2:        observations have been organized to allow lines 18-22 to be 
    line_3:        scheduled in consecutive orbits in one visit, and lines 
    line_4:        23-27 in a second visit.  The visits should be GROUPed
    line_5:        WITHIN 6D.

!


  question:        8
    section:       1
    line_1:        Although not essential to our scientific programs, we will 
    line_2:        try to obtain simultaneous (or contemporaneous) observations 
    line_3:        of DQ Her from the ground.  

!
!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:        DQ-HER
    descr_1:       A,154
    pos_1:         RA= 18H 07M 30.35S +/-0.01S,
    pos_2:         DEC = +45D 51' 31.7"+/-0.3",
    pos_3:         PLATE-ID=00TB
    equinox:       2000
    fluxnum_1:     1
    fluxval_1:     V = 14.2 +/- 0.3
    fluxnum_2:     2
    fluxval_2:     V = 17.7 +/- 0.3

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       18.000
    targname:      DQ-HER
    config:        FOS/BL
    opmode:        ACQ/PEAK
    aperture:      4.3
    sp_element:    G400H
    num_exp:       1
    time_per_exp:  1.0S
    fluxnum_1:     1
    priority:      1
    param_1:       SCAN-STEP-Y=1.204,
    param_2:       SEARCH-SIZE-X=1,
    param_3:       SEARCH-SIZE-Y=3
    req_1:         ONBOARD ACQ FOR 18.1;
    req_2:         ZERO-PHASE JD2434954.94425 +/- 0.00001D;
    req_3:         PERIOD 0.19362087D +/- 0.001S;
    req_5:         CYCLE 4 /18-27;
    req_6:         GROUP 18-27 WITHIN 6D;
    req_7:         NON-INT /18-18.2
    comment_1:     THE PHASE IS TO AVOID THE
    comment_2:     TA OCCURRING DURING ECLIPSE.
    comment_3:     TA MUST OCCUR BETWEEN PHASES 0.5 AND
    comment_4:     0.25 DUE TO ECLIPSING NATURE OF OBJECT

!

    linenum:       18.100
    targname:      DQ-HER
    config:        FOS/BL
    opmode:        ACQ/PEAK
    aperture:      1.0
    sp_element:    G400H
    num_exp:       1
    time_per_exp:  1.0S
    fluxnum_1:     1
    priority:      1
    param_1:       SCAN-STEP-X=0.602,
    param_2:       SCAN-STEP-Y=0.602,
    param_3:       SEARCH-SIZE-X=6,
    param_4:       SEARCH-SIZE-Y=2
    req_1:         ONBOARD ACQ FOR 18.2;

!

    linenum:       18.200
    targname:      DQ-HER
    config:        FOS/BL
    opmode:        ACQ/PEAK
    aperture:      0.5
    sp_element:    G400H
    num_exp:       1
    time_per_exp:  9.0S
    fluxnum_1:     1
    priority:      1
    param_1:       SCAN-STEP-X=0.30,
    param_2:       SCAN-STEP-Y=0.30,
    param_3:       SEARCH-SIZE-X=3,
    param_4:       SEARCH-SIZE-Y=3
    req_1:         ONBOARD ACQ FOR 19.01-22;

!

    linenum:       19.010
    targname:      DARK
    config:        S/C
    opmode:        POINTING
    aperture:      V1
    num_exp:       1
    time_per_exp:  1S
    fluxnum_1:     1
    priority:      1
    req_1:         PHASE 0.61 +/- 0.004 OF REF18;
    req_2:         NON-INT /19.01-22;
    req_3:         SEQ 19.01-22 WITHIN 7.5H
    comment_1:     DQ HER TIME-RESOLVED DATA

!

    linenum:       19.100
    targname:      DQ-HER
    config:        FOS/BL
    opmode:        RAPID
    aperture:      1.0
    sp_element:    G160L
    wavelength:    1150-2510
    num_exp:       1
    time_per_exp:  1918.08S
    fluxnum_1:     1
    priority:      1
    param_1:       READ-TIME=4.44
    comment_1:     DQ HER TIME-RESOLVED DATA

!

    linenum:       20.000
    targname:      DQ-HER
    config:        FOS/BL
    opmode:        RAPID
    aperture:      1.0
    sp_element:    G160L
    wavelength:    1150-2510
    num_exp:       1
    time_per_exp:  1918.08S
    fluxnum_1:     2
    priority:      1
    param_1:       READ-TIME=4.44
    comment_1:     DQ HER TIME-RESOLVED AT MIN

!

    linenum:       21.000
    targname:      DQ-HER
    config:        FOS/BL
    opmode:        RAPID
    aperture:      1.0
    sp_element:    G160L
    wavelength:    1150-2510
    num_exp:       1
    time_per_exp:  1918.08S
    fluxnum_1:     1
    priority:      1
    param_1:       READ-TIME=4.44
    comment_1:     DQ HER TIME-RESOLVED

!

    linenum:       22.000
    targname:      DQ-HER
    config:        FOS/BL
    opmode:        ACCUM
    aperture:      1.0
    sp_element:    G130H
    num_exp:       1
    time_per_exp:  2400S
    fluxnum_1:     1
    priority:      1
    comment_1:     DQ HER AT MAX

!


    linenum:       23.000
    targname:      DQ-HER
    config:        FOS/BL
    opmode:        ACQ/PEAK
    aperture:      4.3
    sp_element:    G400H
    num_exp:       1
    time_per_exp:  1.0S
    fluxnum_1:     1
    priority:      2
    param_1:       SCAN-STEP-Y=1.204,
    param_2:       SEARCH-SIZE-X=1,
    param_3:       SEARCH-SIZE-Y=3
    req_1:         ONBOARD ACQ FOR 23.1;
    req_2:         NON-INT /23-23.2
    comment_1:     TA MUST OCCUR BETWEEN PHASES 0.5 AND
    comment_2:     0.25 DUE TO ECLIPSING NATURE OF OBJECT

!

    linenum:       23.100
    targname:      DQ-HER
    config:        FOS/BL
    opmode:        ACQ/PEAK
    aperture:      1.0
    sp_element:    G400H
    num_exp:       1
    time_per_exp:  1.0S
    fluxnum_1:     1
    priority:      2
    param_1:       SCAN-STEP-X=0.602,
    param_2:       SCAN-STEP-Y=0.602,
    param_3:       SEARCH-SIZE-X=6,
    param_4:       SEARCH-SIZE-Y=2
    req_1:         ONBOARD ACQ FOR 23.2;

!

    linenum:       23.200
    targname:      DQ-HER
    config:        FOS/BL
    opmode:        ACQ/PEAK
    aperture:      0.5
    sp_element:    G400H
    num_exp:       1
    time_per_exp:  9.0S
    fluxnum_1:     1
    priority:      2
    param_1:       SCAN-STEP-X=0.30,
    param_2:       SCAN-STEP-Y=0.30,
    param_3:       SEARCH-SIZE-X=3,
    param_4:       SEARCH-SIZE-Y=3
    req_1:         ONBOARD ACQ FOR 24.01-27;


!


    linenum:       24.010
    targname:      DARK
    config:        S/C
    opmode:        POINTING
    aperture:      V1
    num_exp:       1
    time_per_exp:  1S
    fluxnum_1:     1
    priority:      1
    req_1:         PHASE 0.61 +/- 0.004 OF REF18;
    req_2:         NON-INT /24.01-22;
    req_3:         SEQ 24.01-22 WITHIN 7.5H
    comment_1:     DQ HER TIME-RESOLVED DATA

!

    linenum:       24.100
    targname:      DQ-HER
    config:        FOS/BL
    opmode:        RAPID
    aperture:      1.0
    sp_element:    G160L
    wavelength:    1150-2510
    num_exp:       1
    time_per_exp:  1918.08S
    fluxnum_1:     1
    priority:      2
    param_1:       READ-TIME=4.44
    comment_1:     DQ HER TIME-RESOLVED DATA

!

    linenum:       25.000
    targname:      DQ-HER
    config:        FOS/BL
    opmode:        RAPID
    aperture:      1.0
    sp_element:    G160L
    wavelength:    1150-2510
    num_exp:       1
    time_per_exp:  1918.08S
    fluxnum_1:     2
    priority:      2
    param_1:       READ-TIME=4.44
    comment_1:     DQ HER TIME-RESOLVED AT MIN

!

    linenum:       26.000
    targname:      DQ-HER
    config:        FOS/BL
    opmode:        RAPID
    aperture:      1.0
    sp_element:    G160L
    wavelength:    1150-2510
    num_exp:       1
    time_per_exp:  1918.08S
    fluxnum_1:     1
    priority:      2
    param_1:       READ-TIME=4.44
    comment_1:     DQ HER TIME-RESOLVED

!

    linenum:       27.000
    targname:      DQ-HER
    config:        FOS/BL
    opmode:        ACCUM
    aperture:      1.0
    sp_element:    G190H
    num_exp:       1
    time_per_exp:  2400S
    fluxnum_1:     1
    priority:      2
    comment_1:     DQ HER AT MAX

!
! end of exposure logsheet