!   $Id: 20,v 4.1 1994/07/26 20:51:05 pepsa Exp $

coverpage:

  title_1:         VARIABILITY OF HIGH LUMINOSITY STARS
    sci_cat:       STELLAR ASTROPHYSICS
    proposal_for:  GO
    pi_title:      DR.
    pi_fname:      JOE
    pi_lname:      ASTRONOMER
    pi_inst:       STSCI
    pi_country:    USA
    pi_phone:      (301) 338-4700
    keywords_1:    SUPERGIANT, VARIABLE
    hours_pri:     20.00
    num_pri:       1
! end of coverpage

abstract:

    line_1:        Some of the most luminous and massive stars in our galaxy and
    line_2:        in the Large Magellanic Cloud will be monitored for
    line_3:        variability in light. Knowledge of the time scales and
    line_4:        amplitudes of luminosity fluctuations can perhaps place
    line_5:        useful constraints on various stellar models.

!
! end of abstract

general_form_proposers:

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

!
! end of general_form_proposers block

general_form_text:

  question:        3
    section:       1
    line_1:        The object will be monitored for 30 minutes on four occasions
    line_2:        separated by a few days.

!

  question:        4
    section:       1
    line_1:        ST is required in order to observe in the ultraviolet where
    line_2:        the luminsoity variations are expected to be larger.

!

  question:        5
    section:       1
    line_1:        The observations are to be repeated for a total of 4 series
    line_2:        to search for long-term (i.e. days) periodicities.

!

  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:        A description of your data reduction plans go here.

!

  question:        8
    section:       1
    line_1:        Any additional comments go here.

!

  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:       6
    name_1:        HD193237
    name_2:        P-CYG
    descr_1:       A,117
    pos_1:         PLATE-ID=6TK9,
    pos_2:         RA = 20H 17M 47.07S +/- 0.5",
    pos_3:         DEC = +38D 01' 58.9" +/- 0.5"
    equinox:       2000
    fluxnum_1:     1
    fluxval_1:     V = 4.9+/-0.1

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       12.000
    targname:      HD193237
    config:        HSP/UV2
    opmode:        ACQ
    num_exp:       1
    time_per_exp:  10S
    s_to_n:        10
    fluxnum_1:     1
    priority:      1
    param_1:       DATA-FORMAT=ANALOG
    req_1:         ONBOARD ACQ FOR 12.2;
    req_2:         CYCLE 1 / 12.0-12.2;
    req_3:         REPEAT 12.0-12.2 EVERY 5D
    req_4:         +/- 2D FOR 3 MORE TIMES;

!

    linenum:       12.200
    targname:      HD193237
    config:        HSP/UV2
    opmode:        SINGLE
    aperture:      1.0
    sp_element:    F152M
    num_exp:       1
    time_per_exp:  1800S
    s_to_n:        40
    fluxnum_1:     1
    priority:      1
    param_1:       SAMPLE-TIME=0.1,
    param_2:       DATA-FORMAT=WORD

!
! end of exposure logsheet

! No scan data records found