!   $Id: 27,v 4.1 1994/07/26 20:55:25 pepsa Exp $

coverpage:

  title_1:         NON-PROPRIETARY ("SNAPSHOT") SURVEY - 3
    sci_cat:       GALAXIES & CLUSTERS
    proposal_for:  GO/DD
    pi_title:      DR.
    pi_fname:      JOE
    pi_lname:      ASTRONOMER
    pi_inst:       STSCI
    pi_country:    USA
    pi_phone:      (301) 338-4700
    keywords_1:    GALAXIES
    num_pri:       3
    wf_pc:         X
    pi_position:   PROFESSOR
! end of coverpage

abstract:

    line_1:        Whenever the automatic scheduler produces a substantial gap
    line_2:        between observations, the Wide Field/Planetary Camera will
    line_3:        be used to image a nearby object selected from a list of
    line_4:        several hundred low redshift quasars, normal galaxies,
    line_5:        peculiar galaxies, and standard survey fields.  HST
    line_6:        observations will reveal details of the immediate
    line_7:        environment of quasars, the nuclei of normal galaxies, the
    line_8:        morphology of peculiar galaxies, and the star density in
    line_9:        selected fields.  The purpose of this program is to increase
    line_10:       the efficiency of the HST and to provide scientific data
    line_11:       that can be used by many different astronomers.  The images
    line_12:       acquired in this program will be non-proprietary and will be
    line_13:       made available to qualified astronomers via the HST archival
    line_14:       system.  With the approval of the Director of STScI, the
    line_15:       images can also be used for public relations purposes by
    line_16:       appropriate NASA anad STScI personnel.

!
! end of abstract

general_form_proposers:

  lname:           ASTRONOMER
    fname:         JOE
    title:         DR.
    inst:          SPACE TELESCOPE SCIENCE INSTITUTE
    country:       USA

!
! end of general_form_proposers block

general_form_text:

  question:        3
    section:       1
    line_1:        Images drawn from a set of several hundred targets will be
    line_2:        taken with the Wide Field/Planetary Camera whenever there is
    line_3:        a substantial time gap between previously scheduled
    line_4:        observations.  The images will be taken through the
    line_5:        F555W filter, and the exposure length will be the
    line_6:        maximum time that can be allowed without impacting the
    line_7:        scheduled observations.  No relative priorities have been
    line_8:        given to the individual observations as the order of
    line_9:        observation will be decided solely by whichever target will
    line_10:       produce a minimum of HST motion when an unscheduled block
    line_11:       of time occurs.

!

  question:        4
    section:       1
    line_1:        This proposal is designed to increase the efficiency of the
    line_2:        HST.

!

  question:        5
    section:       1
    line_1:        The exposure time for each observation will depend upon the
    line_2:        amount of unscheduled HST time.

!

  question:        6
    section:       1
    line_1:        Justification for any special calibrations, use of dark
    line_2:        time, or uninterupted exposures goes here.

!

  question:        7
    section:       1
    line_1:        Data will be stored in the HST archive system and made
    line_2:        available on a non-proprietary basis to anyone authorized by
    line_3:        STScI who wishes to use the images for astronomical research.
    line_4:        On special occasions, the Director of STScI may decide that
    line_5:        some of the images may be used by NASA personnel or
    line_6:        authorized scientists.

!

  question:        8
    section:       1
    line_1:        Targets must be examined on the GSSS display system to make
    line_2:        certain that there are no unacceptably bright stars in the
    line_3:        field.  This will be done by the PI with appropriate
    line_4:        STScI support.

!

  question:        9
    section:       1
    line_1:        A description of any previous HST data goes here.

!

  question:        10
    section:       1
    line_1:        Resources provided by your home institution goes here.

!
!end of general form text

general_form_address:

  lname:           ASTRONOMER
    fname:         JOE
    title:         DR.
    category:      PI
    inst:          STSCI
    addr_1:        3700 SAN MARTIN DRIVE
    city:          BALTIMORE
    state:         MD
    zip:           21218
    country:       USA
    phone:         (301) 338-4700

!
! end of general_form_address records

fixed_targets:

    targnum:       1
    name_1:        1017+1055
    descr_1:       E,313
    pos_1:         RA=10H 20M 10.00S +/- 0.1S ,
    pos_2:         DEC=+10D 40' 02.3" +/- 1.0"
    equinox:       2000.00
    rv_or_z:       Z=2.000
    comment_1:     NOTE THAT THE WIDE FIELD-OF-VEIW OF
    comment_2:     THE PC MEANS THAT COORDINATES IN
    comment_3:     THE GUIDE STAR FRAME ARE NOT
    comment_4:     REQUIRED (HENCE NO PLATE-ID=).
    fluxnum_1:     1
    fluxval_1:     V = 16.00 +/- 0.1

!

    targnum:       43
    name_1:        BSO1
    descr_1:       E,314
    pos_1:         RA=12H 48M 51.86S +/- 0.1S ,
    pos_2:         DEC=+37D 30' 28.5" +/- 1.0"
    equinox:       2000.00
    rv_or_z:       Z=2.000
    fluxnum_1:     1
    fluxval_1:     V = 16.00 +/- 0.1

!

    targnum:       99
    name_1:        PKS2021-330
    descr_1:       E,314
    pos_1:         RA=20H 24M 35.55S +/- 0.1S ,
    pos_2:         DEC=-32D 53' 36.4" +/- 1.0"
    equinox:       2000.00
    rv_or_z:       Z=2.000
    fluxnum_1:     1
    fluxval_1:     V = 16.00 +/- 0.1

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       1.000
    targname:      1017+1055
    config:        PC
    opmode:        IMAGE
    aperture:      PCALL
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  260S
    s_to_n:        5
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=NO,
    param_2:       PRE-FLASH=YES
    req_1:         CYCLE 0/1-100;

!

    linenum:       43.000
    targname:      BSO1
    config:        PC
    opmode:        IMAGE
    aperture:      PCALL
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  260S
    s_to_n:        5
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=NO,
    param_2:       PRE-FLASH=YES

!

    linenum:       100.000
    targname:      PKS2021-330
    config:        PC
    opmode:        IMAGE
    aperture:      PCALL
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  260S
    s_to_n:        5
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=NO,
    param_2:       PRE-FLASH=YES

!
! end of exposure logsheet

! No scan data records found