!   $Id: 5098,v 4.1 1994/07/27 15:08:48 pepsa Exp $

coverpage:

  title_1:         UV SPECTRA OF LOW-REDSHIFT-QSOS:
    title_2:       CYCLE 4 OBSERVATIONS
    sci_cat:       QUASARS & AGN
    sci_subcat:    GTO/FOS
    proposal_for:  GTO/FOS
    cont_id:       1026
    pi_fname:      E. MARGARET
    pi_lname:      BURBIDGE
    pi_inst:       UNIVERSITY OF CALIFORNIA, SAN DIEGO
    pi_country:    USA
    pi_phone:      619-534-4477
    hours_pri:     2.48
    num_pri:       3
    wf_pc:         Y
! end of coverpage

abstract:

    line_1:        This proposal contains observations which will help to complete a number of FOS
    line_2:        IDT scientific programs.  1) Nearly simultaneous HST and optical observations
    line_3:        of emission line profiles will be used for models of the emission line region.
    line_4:        2) Images of QSOs with low redshift absorption line systems will characterize
    line_5:        the type and impact parameter of the absorbing galaxy.

!
! end of abstract

general_form_proposers:

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

!

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

!

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

!

  lname:           BARTKO
    fname:         FRANK
    inst:          UNAFFILIATED
    country:       USA

!

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

!

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

!

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

!

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

!

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

!

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

!

  lname:           MARGON
    fname:         BRUCE
    mi:            H.
    inst:          UNIVERSITY OF WASHINGTON
    country:       USA

!
! end of general_form_proposers block

general_form_text:

  question:        3
    section:       1
    line_1:        PKS0454-220: A 1200s exposure with WFC 2 and F702W.
    line_2:        3C 286: A 1200s exposure with WFC 2 and F702W.
    line_5:        PG2302+029: A 1500s exposure with G270H, the RED detector and the
    line_6:        1" round aperture will be done after a binary search target acq.
    line_7:        with the large aperture.

!

  question:        4
    section:       1
    line_1:        HST observations are required because the seeing of ground-based
    line_2:        observations is not good enough to reveal the absorbing objects
    line_3:        hidden in the glare of the background QSOs.

!


!

  question:        9
    section:       1
    line_1:        Collaborators have received data from a number of GTO programs, SAT,
    line_2:        and ERO programs.  Related programs which have had observations are as
    line_3:        follows:
    line_4:        1026 - ``UV Spectra of Low-Redshift-QSOs'',
    line_5:        1027 - ``UV Spectra of QSOs with z$>  3.1$'',
    line_6:        1029 - ``Spectropolarimetry of QSOs, Blazars, and AGN'', and
    line_7:        1033 - ``Search for Misdirected BL Lac Objects''.
    line_8:        Low resolution observations of three high redshift QSOs have not
    line_9:        revealed any with light at He II lambda 304.  Observations of UM 675
    line_10:       have shown that any He I Gunn--Peterson effect is small, that He I
    line_11:       absorption lines are not strong, that predictions of the ``Lyman
    line_12:       valley'' may be correct, and that low redshift Ly-alpha is more
    line_13:       prevalent than expected.  Observations of low redshift QSOs (including
    line_14:       3C 273) have shown even more clearly that Ly-alpha absorption occurs
    line_15:       in greater numbers than expected, as well as showing emission--line
    line_16:       profile differences more clearly than from earlier data.
    line_17:       Unexpectedly, Ly-alpha is narrower than H-alpha.

!

  question:        9
    section:       2
    line_1:        ``HST Imaging of the Inner 3 Arcseconds of NGC 1068 in the Light of [O
    line_2:        III] lambda5007'', I.N.Evans, H.C.Ford, A.L.Kinney, R.R.J.Antonucci,
    line_3:        L.Armus, and S.Caganoff, {\it Ap.J.(Lett.)}, {\bf 369}, L27, 1991.
    line_4:        ``Faint Object Camera Observations of a Globular Cluster Nova Field'',
    line_5:        B.Margon, S.F.Anderson, R.A.Downes, R.C.Bohlin, and P.Jakobsen, {\it
    line_6:        Ap.J.(Lett.)}, {\bf 369}, L71, 1991.
    line_7:        ``Far--Ultraviolet Spectroscopy of the Quasar UM 675 with the Faint
    line_8:        Object Spectrograph on the Hubble Space Telescope'', E.A.Beaver,
    line_9:        E.M.Burbidge, R.D.Cohen, V.T.Junkkarinen, R.W.Lyons, E.I.Rosenblatt,
    line_10:       G.F.Hartig, B.Margon, and A.F.Davidsen, {\it Ap.J.(Lett.)}, {\bf 377},
    line_11:       L1, 1991.
    line_12:       ``The Ultraviolet Absorption Spectrum of 3C 273'', J.N.Bahcall,
    line_13:       B.T.Jannuzi, D.P.Schneider, G.F.Hartig, R.Bohlin, and V.Junkkarinen,
    line_14:       {\it Ap.J.(Lett.)}, {\bf 377}, L5, 1991.
    line_15:       ``Faint Object Spectrograph Spectroscopy of Resolved Structure in the
    line_16:       Nucleus of NGC 1068'', S.Caganoff, R.R.J.Antonucci, H.C.Ford,
    line_17:       G.A.Kriss, G.Hartig, L.Armus, I.N.Evans, E.Rosenblatt, R.C.Bohlin, and
    line_18:       A.L.Kinney, {\it Ap.J.(Lett.)}, {\bf 377}, L9, 1991.
    line_19:       ``Faint Object Spectrograph Observations of the Low-Luminosity Seyfert
    line_20:       Galaxy NGC 1566'', G.A.Kriss, G.F.Hartig, L.Armus, W.P.Blair,
    line_21:       S.Caganoff, and L.Dressel, {\it Ap.J.(Lett.)}, {\bf 377}, L13, 1991.

!

  question:        10
    section:       1
    line_1:        The majority of the resources required for this project other than the
    line_2:        normal facilities of a university (librarys, offices, etc.) were
    line_3:        supplied by NASA to the members of the FOS IDT for these projects.
    line_4:        These include all the computing facilities required for the completion
    line_5:        of data reduction and analysis.
    line_6:        Optical and IR ground--based observing facilities and support are
    line_7:        provided by the University of California and the University of
    line_8:        Arizona.

!
!end of general form text

general_form_address:

  lname:           BURBIDGE
    fname:         E. MARGARET
    category:      PI
    inst:          UNIVERSITY OF CALIFORNIA, SAN DIEGO
    addr_1:        CASS 0111, UCSD
    addr_2:        9500 GILMAN DRIVE
    city:          LA JOLLA
    state:         CA
    zip:           920930111
    country:       USA
    phone:         619-534-4477

!
! end of general_form_address records

fixed_targets:

    targnum:       1
    name_1:        PKS0454-22
    descr_1:       E,314,
    descr_2:       H,515,516
    pos_1:         RA = 4H 56M 8.903S +/- 0.3",
    pos_2:         DEC = -21D 59' 9.38" +/- 0.3",
    pos_3:         PLATE-ID = 029V
    equinox:       2000
    pm_or_par:     NO
    rv_or_z:       Z=0.534
    fluxnum_1:     1
    fluxval_1:     V=16.1 +/- 0.5

!

    targnum:       2
    name_1:        3C286
    descr_1:       E,314,
    descr_2:       H,515,516
    pos_1:         RA=13H 31M 8.293S +/- 0.3",
    pos_2:         DEC=30D 30' 32.86" +/- 0.3",
    pos_3:         PLATE-ID = 009L
    equinox:       2000
    pm_or_par:     NO
    rv_or_z:       Z=0.849
    fluxnum_1:     1
    fluxval_1:     V=17.25+/-1.0

!

    targnum:       12
    name_1:        PG2302+029
    descr_1:       E,313,923,
    descr_2:       H,515,519
    pos_1:         RA = 23H 4M 44.956S +/- 0.3",
    pos_2:         DEC = 3D 11' 46.42" +/- 0.3",
    pos_3:         PLATE-ID = 02JH
    equinox:       2000
    pm_or_par:     NO
    rv_or_z:       Z=1.044
    fluxnum_1:     1
    fluxval_1:     V=16.0 +/- 0.5
    fluxnum_2:     2
    fluxval_2:     F(2700)=4.0 +/- 0.3 E-15

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       1.000
    targname:      PKS0454-22
    config:        WFPC2
    opmode:        IMAGE
    aperture:      WF3
    sp_element:    F702W
    num_exp:       1
    time_per_exp:  1200S
    fluxnum_1:     1
    priority:      1
    req_1:         CYCLE 4 /1

!

    linenum:       2.000
    targname:      3C286
    config:        WFPC2
    opmode:        IMAGE
    aperture:      WF3
    sp_element:    F702W
    num_exp:       1
    time_per_exp:  1200S
    fluxnum_1:     1
    priority:      1
    req_1:         CYCLE 4 / 2

!

    linenum:       6.000
    targname:      PG2302+029
    config:        FOS/RD
    opmode:        ACQ/BINARY
    aperture:      4.3
    sp_element:    MIRROR
    num_exp:       1
    time_per_exp:  3.3S
    fluxnum_1:     1
    priority:      1
    param_1:       BRIGHT = 700000
    req_1:         ONBOARD ACQ FOR 6.1;
    req_2:         SEQ 6.0-6.1 NO GAP;
    req_3:         CYCLE 4 / 6.0-6.1

!

    linenum:       6.100
    targname:      PG2302+029
    config:        FOS/RD
    opmode:        ACCUM
    aperture:      1.0
    sp_element:    G270H
    wavelength:    2700
    num_exp:       1
    time_per_exp:  1500S
    s_to_n:        30
    fluxnum_1:     2
    priority:      1

!
! end of exposure logsheet

! No scan data records found