!   $Id: 5611,v 7.1 1994/07/27 19:45:30 pepsa Exp $
coverpage:

  title_1:         A PHOTOMETRIC SEARCH FOR PLANETS OF NEARBY STARS:
    title_2:       EPSILON ERIDANI
    sci_cat:       SOLAR SYSTEM
    sci_subcat:    EXTRASOLAR PLANETS
    proposal_for:  GTO/OS
    cont_id:       5132
    pi_title:      PROF.
    pi_fname:      WILLIAM
    pi_mi:         G
    pi_lname:      FASTIE
    pi_inst:       JOHNS HOPKINS UNIVERSITY
    pi_country:    USA
    pi_phone:      (410) 516-5185,7302
    keywords_1:    PHOTOMETRIC EXTRA SOLAR PLANETS, PESP
    keywords_2:    GTO PROPOSAL 5132
    hours_pri:     87.24
    num_pri:       18
    wf_pc:         Y
    pi_position:   RESEARCH PROF
! end of coverpage

abstract:

    line_1:        The proposed research is a search for planets of nearby
    line_2:        stars.  The technique involves use of the Planetary Camera
    line_3:        with narrow and wide band pass filters to photometrically
    line_4:        measure the presence of resolved dark companions. The
    line_5:        exposures are calculated to provide 70000 electrons per
    line_6:        pixel at 1.2 arcsec from the target stars.  Multiple
    line_7:        exposures will be required.  This proposal describes
    line_8:        observations of Epsilon Eridani only for early scheduling.
    line_9:        The remainder of the the program is decribed in proposal
    line_10:       5132.

!
! end of abstract

general_form_proposers:

  lname:           FASTIE
    fname:         WILLIAM
    title:         PROF.
    mi:            G
    inst:          JOHNS HOPKINS UNIVERSITY
    country:       USA

!

  lname:           CALDWELL
    fname:         JOHN
    title:         PROF.
    inst:          YORK UNIVERSITY
    country:       CANADA

!

  lname:           SCHROEDER
    fname:         DANIEL
    title:         PROF.
    mi:            J
    inst:          BELOIT COLLEGE
    country:       USA

!
! end of general_form_proposers block

general_form_text:


!

  question:        3
    section:       1
    line_1:        Only nearby stars will be observed. Except for Priority IV
    line_2:        targets, repeated observations at specified intervals
    line_3:        will be required to determine whether faint
    line_4:        background objects are companions. Two or three color
    line_5:        filters will be used to differentiate between faint
    line_6:        cool stars and planets. This time should be split between
    line_7:        W. Fastie, D. Schroeder, J. Caldwell.

!

  question:        5
    section:       1
    line_1:        Implementation Notes from Peg Stanley:
    line_2:        There are 3 visits in this proposal.  The goal is to get on the same
    line_3:        pixel in visits 2 and 3 as in 1.  For this reason, I have changed the
    line_4:        aperture name to the fixed aperture and have changed the observer's
    line_5:        EARLY ACQ on lines 229 and 329 to INT ACQ (the observer incorrectly
    line_6:        thought the early acq could be handled quickly).  Original
    line_7:        specification of EARLY ACQ FOR and USE THE SAME GUIDE STARS would not
    line_8:        work.
    line_10:       If there are any questions during planning and scheduling, please call
    line_11:       me at x4536.

!
!end of general form text

general_form_address:

  lname:           FASTIE
    fname:         WILLIAM
    mi:            G
    title:         PROF.
    category:      PI
    inst:          JOHNS HOPKINS UNIVERSITY
    addr_1:        HOMEWOOD CAMPUS
    city:          BALTIMORE
    state:         MD
    zip:           21218
    country:       USA
    phone:         (410) 516-5185,7302

!

  lname:           SCHROEDER
    fname:         DANIEL
    mi:            J
    category:      PI
    inst:          BELOIT COLLEGE
    addr_1:        DEPT. OF PHYS. & ASTRON.
    city:          BELOIT
    state:         WI
    zip:           53511
    country:       USA
    phone:         (608) 363-2258

!
! end of general_form_address records

fixed_targets:

    targnum:       22
    name_1:        HD22049
    name_2:        EPSILON-ERI
    descr_1:       A,139
    pos_1:         RA  =  3H 32M 55.7S +/- 1.0",
    pos_2:         DEC = -9D 27' 30" +/- 1"
    equinox:       2000
    pm_or_par:     Y
    pos_epoch_bj:  J
    pos_epoch_yr:  2000.00
    ra_pm_val:     -0.066099
    ra_pm_unct:    0.000067
    dec_pm_val:    0.0230
    dec_pm_unct:   0.0010
    an_prlx_val:   0.3000
    an_prlx_unct:  0.0100
    comment_1:     K2V STAR
    fluxnum_1:     1
    fluxval_1:     V = 3.73 +/- 0.1
    fluxnum_2:     1
    fluxval_2:     TYPE = K2V
    fluxnum_3:     1
    fluxval_3:     A(V) = 0.0 +/- 0

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       10.000
    sequence_1:    DEFINE
    sequence_2:    OBS-4
    targname:      #
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1-FIX
    sp_element:    #
    num_exp:       1
    time_per_exp:  1S
    fluxnum_1:     1
    priority:      #
    param_1:       CR-SPLIT=NO
    param_2:       CLOCKS=YES
    param_3:       ATD-GAIN=15
    req_1:         NON-INT;
    comment_1:     EXPOSURE TO BE +/- 10 PERCENT OF
    comment_2:     SPECIFIED VALUE.

!

    linenum:       12.000
    sequence_1:    DEFINE
    sequence_2:    OBS-5
    targname:      #
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1-FIX
    sp_element:    #
    num_exp:       4
    time_per_exp:  1S
    fluxnum_1:     1
    priority:      #
    param_1:       CR-SPLIT=NO
    param_2:       CLOCKS=YES
    param_3:       ATD-GAIN=15
    req_1:         NON-INT;
    comment_1:     EXPOSURE TO BE +/- 10 PERCENT OF
    comment_2:     SPECIFIED VALUE.

    linenum:       14.000
    sequence_1:    DEFINE
    sequence_2:    OBS-6
    targname:      #
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1-FIX
    sp_element:    #
    num_exp:       5
    time_per_exp:  1S
    fluxnum_1:     1
    priority:      #
    param_1:       CR-SPLIT=NO
    param_2:       CLOCKS=YES
    param_3:       ATD-GAIN=15
    req_1:         NON-INT;

!
    linenum:       30.000
    sequence_1:    USE
    sequence_2:    OBS-4
    targname:      HD22049
    sp_element:    F160BW
    time_per_exp:  X200
    priority:      1
    req_1:         CYCLE 4;
    req_2:         SEQ 30-32 NO GAP;
    comment_1:     EPSILON ERI;
    comment_2:     USE SAME GUIDE STARS FOR 30-32;

!

    linenum:       31.000
    sequence_1:    USE
    sequence_2:    OBS-5
    targname:      HD22049
    sp_element:    F631N
    time_per_exp:  X500
    priority:      1
    req_1:         CYCLE 4;

!

    linenum:       32.000
    sequence_1:    USE
    sequence_2:    OBS-6
    targname:      HD22049
    sp_element:    F953N
    time_per_exp:  X2200
    priority:      1
    req_1:         CYCLE 4;


    linenum:       229.000
    sequence_1:    USE
    sequence_2:    OBS-4
    targname:      HD22049
    sp_element:    F122M, F622W
    time_per_exp:  X14
    priority:      1
    req_1:         CYCLE 4;
    req_2:         INT ACQ FOR 230;
    req_3:         AFTER 30 BY 160D +/- 30D;
    comment_1:     EPSILON ERI;
    comment_2:     USE SAME GUIDE STARS FOR 229-234

!

    linenum:       230.000
    sequence_1:    USE
    sequence_2:    OBS-4
    targname:      HD22049
    sp_element:    F122M, F622W
    time_per_exp:  X14
    priority:      1
    req_1:         CYCLE 4;
    req_2:         SEQ 230-234 NO GAP;

!

    linenum:       231.000
    sequence_1:    USE
    sequence_2:    OBS-5
    targname:      HD22049
    sp_element:    F622W
    time_per_exp:  X80
    priority:      1
    req_1:         CYCLE 4;

!
    linenum:       232.000
    sequence_1:    USE
    sequence_2:    OBS-5
    targname:      HD22049
    sp_element:    F850LP
    time_per_exp:  X300
    priority:      1
    req_1:         CYCLE 4;

    linenum:       233.000
    sequence_1:    USE
    sequence_2:    OBS-5
    targname:      HD22049
    sp_element:    F622W
    time_per_exp:  X20
    priority:      1
    req_1:         CYCLE 4;

!
    linenum:       234.000
    sequence_1:    USE
    sequence_2:    OBS-5
    targname:      HD22049
    sp_element:    F850LP
    time_per_exp:  X70
    priority:      1
    req_1:         CYCLE 4;

!

    linenum:       329.000
    sequence_1:    USE
    sequence_2:    OBS-4
    targname:      HD22049
    sp_element:    F122M, F622W
    time_per_exp:  X14
    priority:      1
    req_1:         CYCLE 4;
    req_2:         INT ACQ FOR 330;
    req_3:         AFTER 230 BY 60D +/- 10D;
    comment_1:     EPSILON ERI;
    comment_2:     USE SAME GUIDE STARS FOR 329-334

!

    linenum:       330.000
    sequence_1:    USE
    sequence_2:    OBS-4
    targname:      HD22049
    sp_element:    F122M, F622W
    time_per_exp:  X14
    priority:      1
    req_1:         CYCLE 4;
    req_2:         SEQ 330-334 NO GAP;

!

    linenum:       331.000
    sequence_1:    USE
    sequence_2:    OBS-5
    targname:      HD22049
    sp_element:    F622W
    time_per_exp:  X80
    priority:      1
    req_1:         CYCLE 4;

!
    linenum:       332.000
    sequence_1:    USE
    sequence_2:    OBS-5
    targname:      HD22049
    sp_element:    F850LP
    time_per_exp:  X300
    priority:      1
    req_1:         CYCLE 4;


    linenum:       333.000
    sequence_1:    USE
    sequence_2:    OBS-5
    targname:      HD22049
    sp_element:    F622W
    time_per_exp:  X20
    priority:      1
    req_1:         CYCLE 4;

!
    linenum:       334.000
    sequence_1:    USE
    sequence_2:    OBS-5
    targname:      HD22049
    sp_element:    F850LP
    time_per_exp:  X70
    priority:      1
    req_1:         CYCLE 4;

!
! end of exposure logsheet

! No scan data records found

!