!  File:  2982C.PROP
!  Database:  PEPDB
!  Date:  18-FEB-1994:02:30:16

coverpage:

  title_1:         FOC DIAGNOSTIC EXPOSURES
    proposal_for:  OV/OTA
    pi_title:      DR.
    pi_fname:      DUCCIO
    pi_lname:      MACCHETTO
    pi_inst:       SPACE TELESCOPE SCIENCE INSTITUTE
    pi_country:    USA
    foc:           Y
! end of coverpage

abstract:

    line_1:        This proposal will be used to understand the OTA during
    line_2:        Boostrap Phase B. It consists of a series of FOC exposures
    line_3:        with an interference filter, F501N, which will give the PSF
    line_4:        as a function of position in the chip, and will be used to
    line_5:        derive the aberrations of the OTA (FOC image quality is
    line_6:        known to be much better than the present OTA alignments).
    line_7:        These measurements will complement the WFPC images and
    line_8:        the existing LOS scan data and the OCS measurements.

!
! end of abstract

general_form_proposers:

  lname:           MACCHETTO
    fname:         DUCCIO
    title:         DR.
    inst:          SPACE TELESCOPE SCIENCE INSTITUTE
    country:       USA

!

  lname:           BURROWS
    fname:         CHRIS
    title:         DR.
    inst:          SPACE TELESCOPE SCIENCE INSTITUTE
    country:       USA

!

  lname:           MEYLAN
    fname:         GEORGES
    title:         DR.
    inst:          SPACE TELESCOPE SCIENCE INSTITUTE
    country:       USA

!

  lname:           NAGEL
    fname:         LAURETTA
    inst:          SPACE TELESCOPE SCIENCE INSTITUTE
    country:       USA

!
! end of general_form_proposers block

general_form_text:

  question:        2
    section:       1
    line_1:        In order to do photometry with the FOC, it is necessary to

!

  question:        2
    section:       2
    line_1:        It is assumed that the calibration fields will provide the

!

  question:        6
    section:       0
    line_1:        Prerequisities: this test must be done when the preformance

!

  question:        8
    section:       0
    line_1:        This test is stray light sensitive with an allowable

!
!end of general form text

general_form_address:

  lname:           MACCHETTO
    fname:         DUCCIO
    category:      PI
    inst:          SPACE TELESCOPE SCIENCE INSTITUTE

!

  lname:           MACCHETTO
    fname:         DUCCIO
    mi:            F
    title:         DR.
    inst:          SPACE TELESCOPE SCIENCE INSTITUTE
    addr_1:        3700 SAN MARTIN DRIVE
    city:          BALTIMORE
    state:         MD
    zip:           21218
    country:       USA

!
! end of general_form_address records

fixed_targets:

    targnum:       1
    name_1:        EPSSCOFIELD
    descr_1:       FIELD AROUND EPSILON SCORPIO
    pos_1:         RA=16H 50M 44.091S +/- 0.33",
    pos_2:         DEC=-34D 18' 24.70" +/- 0.33",
    pos_3:         PLATE-ID=06Q4
    equinox:       2000
    fluxnum_1:     1
    fluxval_1:     V=15 +/- 2

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       1.000
    targname:      EPSSCOFIELD
    config:        FOC/96
    opmode:        IMAGE
    aperture:      512X512
    sp_element:    F501N, F2ND
    num_exp:       2
    time_per_exp:  15M
    s_to_n:        100
    fluxnum_1:     1
    priority:      1

!

    linenum:       2.000
    targname:      ^
    config:        ^
    opmode:        ^
    aperture:      ^
    sp_element:    F501N, F2ND
    num_exp:       2
    time_per_exp:  ^
    s_to_n:        ^
    fluxnum_1:     ^
    priority:      ^

!
! end of exposure logsheet

! No scan data records found