!  File:  3352C.PROP
!  Database:  PEPDB
!  Date:  19-FEB-1994:04:28:15

coverpage:

  title_1:         BINARY PULSAR PSR1913+16 IMAGING: FUTURE-CYCLES CONTINUATION
    sci_cat:       STELLAR ASTROPHYSICS
    sci_subcat:    SUBLUMINOUS STARS
    proposal_for:  GTO/OS
    cont_id:       1061
    pi_fname:      PHILIPPE
    pi_lname:      CRANE
    pi_inst:       EUROPEAN SOUTHERN OBSERVATORY
    pi_country:    GERMANY, WEST
    pi_phone:      +49-89-320-06-230
    keywords_1:    PULSARS, ASTROMETRY, GRAVITATIONAL RADIATION
    hours_pri:     0.25
    num_pri:       1
    pi_position:   ASTRONOMER/PHYSICIST
! end of coverpage

abstract:

    line_1:        A candidate star for the binary pulsar has previously been identified but the
    line_2:        precision of the astrometric measurement needs to be improved in order to
    line_3:        finally put to rest the question of whether or not this object lies at the
    line_4:        radio position. A single 10 minute PC image in the R band will provide the
    line_5:        initial data to determine if it is worth using the FGS to get results at the 2
    line_6:        milliarcsec level of precision.

!
! end of abstract

general_form_proposers:

  lname:           CRANE
    fname:         PHILIPPE
    inst:          EUROPEAN SOUTHERN OBSERVATORY
    country:       GERMANY, WEST
    esa:           N

!

  lname:           BOESHAAR
    fname:         P.
    mi:            T.
    inst:          DREW UNIVERSITY
    country:       USA
    esa:           N

!

  lname:           TYSON
    fname:         J.
    mi:            A.
    inst:          BELL LABORITORIES
    country:       USA
    esa:           N

!
! end of general_form_proposers block

general_form_text:

  question:        3
    section:       1
    line_1:

!

  question:        12
    section:       1
    line_1:        Note that the region near the binary pulsar should fall entirely into a single
    line_2:        PC chip and not be split among 2 or 3. Thus the pointing requirements are not
    line_3:        crucial within this constraint.

!

  question:        13
    section:       1
    line_1:        FOC  images of the binary pulsar PSR1913+16 will follow up investigations
    line_2:        of the PC images obtained in Cycke 0 and which showed strong
    line_3:        evidence of a distortion in the optitcal candidate.

!
!end of general form text

general_form_address:

  lname:           CRANE
    fname:         PHILIPPE
    category:      PI
    inst:          EUROPEAN SOUTHERN OBSERVATORY
    addr_1:        KARL-SCWARZSCHILD-STR. 2
    city:          D-8046 GARCHING BEI MUNCHEN
    country:       GERMANY, WEST
    phone:         +49-89-320-06-230

!
! end of general_form_address records

fixed_targets:

    targnum:       1
    name_1:        PSR1913+16
    descr_1:       BINARY PULSAR
    pos_1:         RA = 19H 13M 12.47S+/-.1S,
    pos_2:         DEC = 16D 01' 08.0"+/-1.0"
    equinox:       1950
    comment_1:     R>20.9

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       1.000
    targname:      PSR1913+16
    config:        FOC/96
    opmode:        IMAGE
    aperture:      512X512
    sp_element:    F480LP
    wavelength:    4940
    num_exp:       1
    time_per_exp:  7200S
    priority:      1
    req_1:         CYCLE 2;
    req_3:         COND IF TAC OK

!

    linenum:       2.000
    targname:      PSR1913+16
    config:        FOC/96
    opmode:        IMAGE
    aperture:      512X512
    sp_element:    F342W
    wavelength:    3500
    num_exp:       1
    time_per_exp:  180M
    priority:      1
    req_1:         CYCLE 2;
    req_3:         COND IF TAC OK

!
! end of exposure logsheet

! No scan data records found