!   $Id: 5298,v 4.1 1994/07/27 16:18:59 pepsa Exp $

coverpage:

  title_1:         UV IMAGING OF THE NEARBY QSO 2130+099 HOST GALAXY
    sci_cat:       QUASARS & AGN
    sci_subcat:    QUASAR ABSORPTION
    proposal_for:  SMC/ERO
    pi_fname:      SARA
    pi_lname:      HEAP
    pi_inst:       NASA/GSFC
    pi_country:    USA
    pi_phone:      301-286-5359
    keywords_1:    QUASARS, SPIRAL GALAXY, STELLAR POPULATION, MORPHOLOGY
    hours_pri:     2.91
    num_pri:       1
! end of coverpage

abstract:

    line_1:        The host galaxy of QSO 2130+099 is suspected to be a
    line_2:        barred spiral (Hickson & Hutchings 1987, Heap 1986).
    line_3:        We will use the unique imaging capabilities of the
    line_4:        GHRS to map the nucleus of QSO 2130+099 in UV (1200-
    line_5:        3200A) light. These observations will (1) demonstrate
    line_6:        that the GHRS' imaging capabilites have been recovered
    line_7:        by COSTAR, and (2) provide the first high-resolution
    line_8:        optical map of the nucleus/inner host galaxy of a
    line_9:        quasar. THIS IS PART OF HEAP'S CYCLE-4 GTO PROGRAM.

!
! end of abstract

general_form_proposers:

  lname:           HEAP
    fname:         SARA
    inst:          NASA/GSFC
    country:       USA

!
! end of general_form_proposers block

general_form_text:

  question:        2
    section:       1
    line_1:        QSO 2130+099 is a nearby QSO with z=0.061 and V=14.4. Our
    line_2:        recent studies of this object including image-deconvolution
    line_3:        suggest that the host is a barred spiral with a central
    line_4:        surface brightness, mu(B)=21.3 mag per sq. arcsec and a scale
    line_5:        length of 4 kpc. Observing the inner region of this or any
    line_6:        QSO poses two severe observational challenges: (1) high
    line_7:        spatial resolution, and (2) high dynamic range. (The FOC
    line_8:        coronograph won't work for this problem because it blots
    line_9:        out the inner 0.5"?) The GHRS is the ONLY instrument on HST
    line_10:       that can obtain direct images of the inner host galaxy. We
    line_11:       therefore will use this unique capability to obtain UV maps
    line_12:       of the nucleus/inner host galaxy with the GHRS.

!

  question:        3
    section:       1
    line_1:
    line_2:        Schedule the GHRS observations in dark time, so that
    line_3:        geocoronal Ly alpha emission doesn't swamp the target.

!

  question:        4
    section:       1
    line_1:        Only the HST can give the required angular resolution
    line_2:        and UV throughput.

!

  question:        5
    section:       1
    line_1:        Lines 20-22 call for GHRS field maps that are not standard.
    line_2:        The GHRS field maps should carried out during periods
    line_3:        when there is NO JITTER.

!

  question:        7
    section:       1
    line_1:        Reduction and analysis of the data will be done at GSFC.

!
!end of general form text

general_form_address:

  lname:           HEAP
    fname:         SARA
    category:      PI
    inst:          NASA/GSFC
    addr_1:        CODE 681
    city:          GREENBELT,
    state:         MD
    zip:           20771
    country:       USA
    phone:         (301)-286-9545

!
! end of general_form_address records

fixed_targets:

    targnum:       1
    name_1:        QSO2130+099-NUCLEUS
    name_2:        II-ZW-136
    descr_1:       E, 313,321,910,928
    pos_1:         RA=21H32M27.91S+/-0.75",
    pos_2:         DEC=10D08'20.2"+/-0.75",
    pos_3:         PLATE-ID=02KW
    equinox:       2000
    pm_or_par:     NO
    rv_or_z:       Z=0.061
    comment_1:     POSITION DETERMINED FROM GSSS.
    fluxnum_1:     1
    fluxval_1:     V=14.4+/-0.2
    fluxnum_2:     2
    fluxval_2:     F-LINE(1216)=2.6E-12

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       10.000
    targname:      QSO2130+099-NUCLEUS
    config:        HRS
    opmode:        ACQ
    aperture:      2.0
    sp_element:    MIRROR-N2
    num_exp:       1
    time_per_exp:  18.0S
    priority:      1
    param_1:       LOCATE=YES,
    param_2:       BRIGHT=RETURN
    req_1:         ONBOARD ACQ FOR 20-21;
    req_2:         DARK TIME / 10-21;
    req_3:         CYCLE 4/10-21;
    comment_1:     EXPECT 1360 C/S AT N2
    comment_2:     BASED ON TACOUNTS,IUE SPECTRA.

!

    linenum:       11.000
    targname:      QSO2130+099-NUCLEUS
    config:        HRS
    opmode:        ACQ/PEAKUP
    aperture:      2.0
    sp_element:    MIRROR-N2
    num_exp:       1
    time_per_exp:  102S
    priority:      1
    req_1:         ONBOARD ACQ FOR 20-21;

!

    linenum:       20.000
    targname:      QSO2130+099-NUCLEUS
    config:        HRS
    opmode:        IMAGE
    aperture:      2.0
    sp_element:    MIRROR-N2
    num_exp:       4
    time_per_exp:  1280S
    priority:      1
    param_1:       NX=16,
    param_2:       DELTA-X=4,NY=16, DELTA-Y=4
    req_1:         SEQ 20-21 NO GAP;
    comment_1:     FULL MAP OF THE GHRS LSA
    comment_2:     STEP-TIME=5S

!

    linenum:       21.000
    targname:      QSO2130+099-NUCLEUS
    config:        HRS
    opmode:        IMAGE
    aperture:      2.0
    sp_element:    MIRROR-N2
    num_exp:       2
    time_per_exp:  16M
    priority:      1
    param_1:       NX=64,DELTA-X=1,
    param_2:       NY=3,DELTA-Y=4
    comment_1:     HIGH-RESOLUTION PROFILE
    comment_2:     OF THE NUCLES/HOST GALAXY.
    comment_3:     STEP-TIME=5S

!
! end of exposure logsheet

! No scan data records found