!   $Id: 5603,v 4.1 1994/07/27 19:41:39 pepsa Exp $

coverpage:

  title_1:         THE STELLAR DENSITY DISTRIBUTIONS IN THE CENTERS OF
    title_2:       GALACTIC GLOBULAR CLUSTERS:  CYCLE 4 OBSERVATIONS
    sci_cat:       STELLAR POPULATIONS
    proposal_for:  GTO/OS
    cont_id:       1019
    pi_title:      DR.
    pi_fname:      JOHN
    pi_mi:         N.
    pi_lname:      BAHCALL
    pi_inst:       INSTITUTE FOR ADVANCED STUDY
    pi_country:    USA
    pi_phone:      (609) 734-8054
    keywords_1:    GLOBULAR CLUSTER, POPULATION II, BLACK HOLE
    hours_pri:     0.52
    num_pri:       20
    wf_pc:         X
    pi_position:   DR. JOHN N. BAHCALL
    off_fname:     ALLEN
    off_lname:     ROWE
    off_title:     ASSOC DIR ADM/FIN
    off_addr_1:    INSTITUTE FOR ADVANCED STUDY
    off_addr_2:    OLDEN LANE
    off_city:      PRINCETON
    off_state:     NJ
    off_zip:       08540
    off_country:   USA
    off_phone:     (609) 734-8205
    off_telex:     837680
! end of coverpage

abstract:

    line_1:        A single exposure in the F336W filter will be made of
    line_2:        M30 using the PC CCD of the WFPC2.

!
! end of abstract

general_form_proposers:

  lname:           BAHCALL
    fname:         JOHN
    mi:            N.
    inst:          INSTITUTE FOR ADVANCED STUDY
    country:       USA

!

  lname:           BAHCALL
    fname:         NETA
    mi:            A.
    inst:          SPACE TELESCOPE SCIENCE INSTITUTE
    country:       USA

!
! end of general_form_proposers block

general_form_text:

  question:        3
    section:       1
    line_1:        One F336W exposure will be taken.
    line_2:        The target position (center of cluster) should be placed
    line_3:        at the center of the single PC chip.

!

  question:        4
    section:       1
    line_1:        ST observations are required in order to resolve individual
    line_2:        stars in the cores of the globular clusters in sufficient
    line_3:        numbers to permit a determination of the stellar density law.

!

  question:        5
    section:       1
    line_1:

!


!

  question:        8
    section:       1
    line_1:        The target position should be placed at the center of
    line_2:        the PC detector in the WFPC2.

!

  question:        10
    section:       1
    line_1:        Computing support and research associates will be available
    line_2:        at both IAS and STScI as required by the science.

!

  question:        13
    section:       1
    line_1:        A F336W exposure will be made of the center of M30.
    line_2:        A search will be made for cusps in the stellar density
    line_3:        distribution and thecolors will be measured for the
    line_4:        brightest stars in the core.

!
!end of general form text

general_form_address:

  lname:           BAHCALL
    fname:         JOHN
    mi:            N.
    category:      PI
    inst:          INSTITUTE FOR ADVANCED STUDY

!
! end of general_form_address records

fixed_targets:

    targnum:       1
    name_1:        NGC7099
    name_2:        M30
    descr_1:       C,201
    pos_1:         RA = 21H 37M 31.64S +/- 0.1S,
    pos_2:         DEC = -23D 24' 23.1" +/- 1"
    equinox:       1950
    pm_or_par:     NO
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 15.12 +/- 0.2

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       1.000
    targname:      NGC7099
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F336W
    num_exp:       1
    time_per_exp:  600S
    fluxnum_1:     1
    priority:      1
    req_1:         CYCLE 4

!
! end of exposure logsheet

! No scan data records found