!  File:  4131C.PROP
!  Database:  PEPDB
!  Date:  20-FEB-1994:09:58:33

coverpage:

  title_1:         M87'S JET, NUCLEUS, AND HOT CORONA (FOS NO. 12):
    title_2:       FUTURE-CYCLE CONTINUATION
    sci_cat:       QUASARS & AGN
    proposal_for:  GTO/FOS
    cont_id:       1034
    pi_title:      DR.
    pi_fname:      HOLLAND
    pi_mi:         C.
    pi_lname:      FORD
    pi_inst:       SPACE TELESCOPE SCIENCE INSTITUTE
    pi_country:    USA
    pi_phone:      (410) 338-4803
    keywords_1:    JET, CORONA, M87, IONIZED GAS
    hours_pri:     1.39
    num_pri:       1
    wf_pc:         Y
! end of coverpage

abstract:

    line_1:        WF/PC narrow band images of M87 will be used to isolate emission line regions
    line_2:        near the nucleus and jet. FOS spectra of these clouds will be used to i) map
    line_3:        the velocity field near the nucleus, ii) understand physical conditions and
    line_4:        ionization mechanisms in these clouds, and iii) measure chemical composition of
    line_5:        the clouds. FOS spectra of the stellar nucleus and synchotron knots in the
    line_6:        jet will be used to establish long-base-line spectral indices and to look for
    line_7:        spectral features. Long exposure ultraviolet spectra of the nucleus and jet
    line_8:        will be used to look for absorption lines from M87's hot corona.

!
! 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:          APPLIED RESEARCH 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:        Cycle 9: 901-902

!

  question:        5
    section:       2
    line_1:        The SV prerequisite programs for all FOS
    line_2:        observations in this program are:
    line_3:        Prop ID 2195 FOS Target Acquisition Tests
    line_4:        - All observations
    line_5:        Prop ID 1317 Int./Ext. Wavelength Offsets
    line_6:        - 1st target
    line_7:        Prop ID 1318 Spectral Flat Fields
    line_8:        - 1st target
    line_9:        Prop ID 1320 Absolute Spectrophotometry
    line_10:       - 1st visit of bright targets
    line_11:       All WF/PC imaging with a center wavelength
    line_12:       blueward of 5000 Angstroms requires UV flood

!

  question:        12
    section:       1
    line_1:        This is an integrated scientific program investigating the jet and nucleus
    line_2:        of M87, and will not be complete until 80% of the observations have been
    line_3:        obtained. Data release should not begin until 1 year after the 80% completion
    line_4:        point.

!

  question:        13
    section:       1
    line_1:        WF/PC narrow band images and FOS spectra will be used to isolate emission
    line_2:        line regions, measure their velocities, and establish physical conditions and
    line_3:        chemical compositions in the gas. FOS spectra of the nucleus and jet will
    line_4:        establish their spectral energy distributions from the UV to the optical. Long
    line_5:        exposure FOS UV spectra of the nucleus and jet will be used to search for
    line_6:        absorption lines from M87's hot corona.

!
!end of general form text

general_form_address:

  lname:           FORD
    fname:         HOLLAND
    mi:            C.
    title:         DR.
    category:      PI
    inst:          SPACE TELESCOPE SCIENCE INSTITUTE
    addr_1:        HOMEWOOD CAMPUS
    addr_2:        3700 SAN MARTIN DRIVE
    city:          BALTIMORE
    state:         MD
    zip:           21218
    country:       USA
    phone:         (410) 338-4803

!
! end of general_form_address records

fixed_targets:

    targnum:       1
    name_1:        M87
    descr_1:       E,303,910
    pos_1:         RA=12H 28M 17.549S +/- 0.014S,
    pos_2:         DEC=+12D 40' 01.46" +/- 0.2"
    equinox:       1950
    rv_or_z:       V=1100
    acqpr_1:       EXT
    fluxnum_1:     1
    fluxval_1:     V=16.7, E(B-V)=0.01

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       901.000
    targname:      M87
    config:        PC
    opmode:        IMAGE
    aperture:      PCALL
    sp_element:    F664N
    num_exp:       1
    time_per_exp:  2000S
    priority:      1
    param_1:       CR-SPLIT=0.33,
    param_2:       PRE-FLASH=YES
    req_1:         GROUP 901-902 WITHIN 15D;
    req_2:         SAME POS FOR 902 AS 901;
    req_3:         CYCLE 9 / 901-902

!

    linenum:       902.000
    targname:      M87
    config:        PC
    opmode:        IMAGE
    aperture:      PCALL
    sp_element:    F547M
    num_exp:       1
    time_per_exp:  600S
    priority:      1
    param_1:       CR-SPLIT=0.33,
    param_2:       PRE-FLASH=YES

!
! end of exposure logsheet

! No scan data records found