!  File:  1167C.PROP
!  Database:  PEPDB
!  Date:  16-FEB-1994:04:24:20

coverpage:

  title_1:         METALLIC ABSORPTION LINES IN THE HALO OF NGC 3067
    sci_cat:       QUASARS & AGN
    sci_subcat:    ABSORPTION LINES
    proposal_for:  GTO/HRS
    pi_title:      PROF.
    pi_fname:      BLAIR
    pi_mi:         D.
    pi_lname:      SAVAGE
    pi_inst:       WISCONSIN, UNIVERSITY OF
    pi_country:    USA
    pi_phone:      (608)262-3072
    keywords_1:    SPECTROSCOPY, QUASAR, GALAXY HALOS, ABSORPTION LINES
    hours_pri:     2.60
    num_pri:       1
    hrs:           X
    pi_position:   PROFESSOR
! end of coverpage

abstract:

    line_1:        This program will investigate the velocity structure and abundances of Fe II
    line_2:        and Mg II in the halo and/or extended disk of NGC 3067. HRS 20,000 resolution
    line_3:        spectra will be obtained at 2800 and 2590 A for 3C232.

!
! end of abstract

general_form_proposers:

  lname:           WEYMANN
    fname:         RAY
    mi:            J.
    inst:          ARIZONA, UNIVERSITY OF
    country:       USA

!

  lname:           SAVAGE
    fname:         BLAIR
    mi:            D.
    inst:          WISCONSIN, UNIVERSITY OF
    country:       USA

!

  lname:           BRANDT
    fname:         JOHN
    mi:            C.
    inst:          NASA, GODDARD SPACE FLIGHT CENTER
    country:       USA

!
! end of general_form_proposers block

general_form_text:

  question:        3
    section:       1
    line_1:        PKS 0955+326 (3C232) will be observed with the HRS G270M grating at 2800
    line_2:        and 2590 A. The total integration time is 2 1/2 hrs.
    line_4:        Obtain these data in Cycle 1 (7-18 months).

!

  question:        4
    section:       1
    line_1:        The lines being studied require satellite observations.

!

  question:        7
    section:       1
    line_1:        The data will be reduced in Madison using the MADRAF VAX. HRS team
    line_2:        software will be available for this analysis.

!

  question:        10
    section:       1
    line_1:        The data analysis facility.

!

  question:        13
    section:       1
    line_1:        The middle UV lines of Mg II and Fe II will be observed at 20,000
    line_2:        resolution to investigate the velocity structure and abundance of these ions in
    line_3:        the halo and/or extended disk of NGC 3067.

!
!end of general form text

general_form_address:

  lname:           SAVAGE
    fname:         BLAIR
    mi:            D.
    title:         PROF.
    category:      PI
    inst:          UNIVERSITY OF WISCONSIN
    addr_1:        DEPARTMENT OF ASTRONOMY
    addr_2:        475 N. CHARTER ST.
    city:          MADISON
    state:         WI
    zip:           53706
    country:       USA
    phone:         608-262-3072

!
! end of general_form_address records

fixed_targets:

    targnum:       1
    name_1:        PKS0955+326
    name_2:        3C232
    descr_1:       QUASAR BEHIND
    descr_2:       NGC 3067
    pos_1:         RA=9H55M25.44S +/-.05S,
    pos_2:         DEC=32D38'23.2"+/- .5"
    equinox:       1950
    pm_or_par:     NO
    rv_or_z:       Z=.53
    comment_1:     COORDINATES ARE FROM HEWITT AND
    comment_2:     BURBIDGE (1980) AND AGREE WITH
    comment_3:     VERON-VERON (1984).
    fluxnum_1:     1
    fluxval_1:     V=15.8

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       1.000
    targname:      PKS0955+326
    config:        HRS
    opmode:        ACQ
    aperture:      2.0
    sp_element:    MIRROR-N2
    num_exp:       1
    time_per_exp:  5M
    priority:      2
    param_1:       BRIGHT=30000.0,
    param_2:       FAINT=3000.0,
    req_1:         ONBOARD ACQ FOR 2-3;
    req_2:         CYCLE 2 /1-3
    comment_1:     STEP-TIME=12.0

!

    linenum:       2.000
    targname:      ^
    config:        ^
    opmode:        ACCUM
    aperture:      ^
    sp_element:    G270M
    wavelength:    2600
    num_exp:       6
    time_per_exp:  10M
    priority:      ^
    param_1:       STEP-PATT=4

!

    linenum:       3.000
    targname:      ^
    config:        ^
    opmode:        ^
    aperture:      ^
    sp_element:    ^
    wavelength:    2805
    num_exp:       9
    time_per_exp:  10M
    priority:      ^
    param_1:       STEP-PATT=4
    comment_1:     EXPOSURES 2 AND 3 MUST BE OBTAINED
    comment_2:     WITH AN OBSERVING SCHEME WHICH
    comment_3:     PROPERLY MONITORS THE RADIATION
    comment_4:     BACKGROUND (SPENDING ABOUT 5 PERCENT
    comment_5:     OF THE INTEGRATION TIME IN THE
    comment_6:     BACKGROUND).

!
! end of exposure logsheet

! No scan data records found