!  File:  3912C.PROP
!  Database:  PEPDB
!  Date:  19-FEB-1994:23:41:16

coverpage:

  title_1:         CORES OF EARLY-TYPE GALAXIES
    sci_cat:       GALAXIES & CLUSTERS
    sci_subcat:    NUCLEI/CORES
    proposal_for:  GO
    longterm:      2
    cont_id:       2600
    pi_title:      DR.
    pi_fname:      SANDRA
    pi_mi:         M.
    pi_lname:      FABER
    pi_inst:       CALIFORNIA, UNIVERSITY OF, SANTA CRUZ
    pi_country:    USA
    pi_phone:      408-459-2944
    keywords_1:    ELLIPTICAL GALAXY, S0 GALAXY, DWARF GALAXY,LOCAL
    keywords_2:    GROUP, GALACTIC NUCLEUS, GALACTIC BULGE, IMAGING
    hours_pri:     22.88
    num_pri:       38
    wf_pc:         Y
    pi_position:   PROFESSOR
    off_fname:     DAVID
    off_mi:        S.
    off_lname:     KLIGER
    off_title:     DEAN
    off_inst:      UNIVERSITY OF CALIFORNIA
    off_addr_1:    391 APPLIED SCIENCES
    off_addr_2:    UNIVERSITY OF CALIFORNIA, SANTA CRUZ
    off_city:      SANTA CRUZ
    off_state:     CA
    off_zip:       95064
    off_country:   USA
    off_phone:     408-459-2106
! end of coverpage

abstract:

    line_1:        We are conducting a comprehensive imaging survey of the cores
    line_2:        of early-type galaxies and spiral bulges.  The high spatial
    line_3:        resolving power of deconvolved HST images will be used to
    line_4:        measure core structure parameters over a wide range of core
    line_5:        size and luminosity.  PC images in F555W will be taken of 45
    line_6:        galaxies covering a range of 9 magnitudes in luminosity.  Ground-
    line_7:        based photometry and kinematic data will be obtained to augment
    line_8:        small-radii HST data.  Observations will be used to constuct
    line_9:        dynamical models of the core regions using a maximum-entropy
    line_10:       technique with the particular goal of searching for BHs in
    line_11:       selected galaxy candidates.  Existing HST images of galaxy cores
    line_12:       are revealing a wide variety of different types of structure
    line_13:       including the prevalence of nuclear cusps.  At the same time,
    line_14:       ground-based data suggest that cores can retain information
    line_15:       about merger processes and accretion events for up to Gyrs after
    line_16:       they occur.  In studying systematic core properties over a wide
    line_17:       range of galaxies, we expect to learn much about how spheroidal
    line_18:       galaxies were formed.

!
! end of abstract

general_form_proposers:

  lname:           FABER
    fname:         SANDRA
    mi:            M.
    inst:          UNIVERSITY OF CALIFORNIA
    country:       USA

!

  lname:           KORMENDY
    fname:         JOHN
    inst:          UNIVERSITY OF HAWAII
    country:       USA

!

  lname:           RICHSTONE
    fname:         DOUGLAS
    mi:            O.
    inst:          UNIVERSITY OF MICHIGAN
    country:       USA

!

  lname:           TREMAINE
    fname:         SCOTT
    mi:            D.
    inst:          UNIVERSITY OF TORONTO
    country:       CANADA

!

  lname:           DRESSLER
    fname:         ALAN
    inst:          CARNEGIE OBSERVATORIES
    country:       USA

!

  lname:           LAUER
    fname:         TOD
    mi:            R.
    inst:          KITT PEAK NATIONAL OBSERVATORY
    country:       USA

!
! end of general_form_proposers block

general_form_text:

  question:        2
    section:       1
    line_1:        F555W PC6 images of 45 representative eary-type galaxies and spheroidal
    line_2:        bulges covering a range of 9 magnitudes in intrinsic luminosity are planned.
    line_3:        Objects are centered at the newly defined aperture location PC6, to avoid
    line_4:        the bad column near the center of PC6.  Exposures are keyed to give 1300 DN
    line_5:        in the central pixel for our present best guess at central surface
    line_6:        brightness.  A safety exposure of 1/4 nominal is added in uncertain cases to
    line_7:        protect against saturation.
    line_9:        Accurate PSFs are crucial to this program because the images will have
    line_10:       high S/N and will be ideal for deconvolution.  We are relying on the
    line_11:       announced STScI weekly PSF monitoring program in F555W in P6 and have not
    line_12:       included any PSF exposures in the present program.  The galaxy exposures should
    line_13:       be centered at the same location in P6 as the PSF monitor exposures.
    line_15:       Long exposures are divided so as to provide appropriate CR splits.
    line_16:       We have switched to fine lock to improve the guiding, but coarse track
    line_17:       may be substituted if scheduling proves difficult.  We will require
    line_18:       jitter data to reconstruct the time-averaged PSFs.

!

  question:        3
    section:       1
    line_1:        Most nuclei are unresolved from the ground and will benefit from the
    line_2:        narrower PSF of HST.  In those nuclei that are resolved, we are searching
    line_3:        for sharp nuclear star clusters or power-law cusps that may have escaped
    line_4:        detection from the ground.   Existing HST images of galactic cores have
    line_5:        revealed much important structure that could not be seen in ground-based
    line_6:        images.

!

  question:        4
    section:       1
    line_1:        Exposure times are based on measured on-orbit PC throughput plus
    line_2:        estimates of the net surface brightness that will be observed with HST with
    line_3:        spherical aberration taken into account.  Times for most galaxies are adjusted
    line_4:        to yield 1300 DN in the central pixel (S/N = 100).  A safety exposure of
    line_5:        1/4 nominal is also included.  For a small number of very low surface
    line_6:        brightness galaxies, exposure times are less than nominal and the expected
    line_7:        S/N will be reduced.

!

  question:        5
    section:       1
    line_1:        None.

!

  question:        5
    section:       2
    line_1:        For all galaxies, we require accurate PSFs, but these should be
    line_2:        adequately provided by the weekly Observatory monitoring program in PC6/F555W.
    line_3:        We also require jitter data for all images, plus accurate flat fields in
    line_4:        F555W good to +/- 1% in the central 200x200 pixels of PC6 and 2%
    line_5:        over the entire chip.

!

  question:        6
    section:       1
    line_1:        PC images will be reduced and analyzed by Lauer and Kormendy.  The
    line_2:        team already has extensive experience with modelling HST galaxy images
    line_3:        and has proven software routines for deconvolution, isophote fitting,
    line_4:        and multiple-component fitting, as well as other options.  Supporting
    line_5:        ground-based data will be obtained by Dressler and Kormendy.  Richstone and
    line_6:        Tremaine will lead the dynamical modelling.  Faber will oversee
    line_7:        manuscript preparation and coordinate the team.

!

  question:        7
    section:       1
    line_1:        All target coordinates have been verified with the STScI GASP system
    line_2:        and are accurate to +/- 1".

!

  question:        8
    section:       1
    line_1:        Faber and Lauer are members of the WFPC IDT.  The IDT programs related
    line_2:        to this proposal include 1118 (Nuclei of Galaxies), 1105 (Peculiar and
    line_3:        Interacting Galaxies), and 1112 (Cores of Globular Clusters).

!

  question:        8
    section:       2
    line_1:        GO 2600 has very good data on 19 galaxies. GTO programs 1105 and 1118 have
    line_2:        returned images of a total of 8 galaxy nuclei, all of which have shown
    line_3:        fascinating detail. A major finding so far is the high frequency of nuclear
    line_4:        power-law cusps.

!

  question:        9
    section:       1
    line_1:        Dressler: Carnegie provides ground-based data and workstation.
    line_3:        Faber: WFPC IDT provides workstation.  USCS provides summer salary and student.
    line_5:        Kormendy: CFHT and UH provide ground-based data.  UH provides workstation.
    line_7:        Lauer: KPNO provides workstation and summer salary.
    line_9:        Richstone: U. Michigan cost-shares for 1/2 of workstation and provides student
    line_10:       and Richstone's summer salary.
    line_12:       Tremaine: Canadian citizen covered by Canadian funds.

!
!end of general form text

general_form_address:

  lname:           FABER
    fname:         SANDRA
    mi:            M.
    title:         PROF.
    category:      PI
    inst:          LICK OBSERVATORY
    addr_1:        UNIVERSITY OF CALIFORNIA
    city:          SANTA CRUZ
    state:         CA
    zip:           95064
    country:       USA
    phone:         408-459-2944

!
! end of general_form_address records

fixed_targets:

    targnum:       1
    name_1:        NGC524
    descr_1:       E,302
    pos_1:         RA = 01H 24M 47.753S +/-2",
    pos_2:         DEC = +09D 32' 19.39" +/-2"
    equinox:       2000.0
    rv_or_z:       V = 2470
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 15.82 +/- 2.0

!

    targnum:       5
    name_1:        NGC1172
    descr_1:       E,303
    pos_1:         RA = 03H 01M 36.045S    +/- 2",
    pos_2:         DEC = -14D 50' 13.63"    +/- 2"
    equinox:       2000.0
    rv_or_z:       V = 1669
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 14.86 +/- 2.0

!

    targnum:       6
    name_1:        NGC1331
    descr_1:       E,304
    pos_1:         RA = 03H 26M 28.258S    +/- 2",
    pos_2:         DEC = -21D 21' 18.96"    +/- 2"
    equinox:       2000.0
    rv_or_z:       V = 1326
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 15.00 +/- 2.0

!

    targnum:       8
    name_1:        NGC1400
    descr_1:       E,303
    pos_1:         RA = 03H 39M 30.713S    +/- 2",
    pos_2:         DEC = -18D 41' 16.70"    +/- 2"
    equinox:       2000.0
    rv_or_z:       V = 483
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 14.99 +/- 2.0

!

    targnum:       9
    name_1:        NGC1426
    descr_1:       E,303
    pos_1:         RA = 03H 42M 49.105S    +/- 2",
    pos_2:         DEC = -22D 6' 29.56"    +/- 2"
    equinox:       2000.0
    rv_or_z:       V = 1358
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 14.85 +/- 2.0

!

    targnum:       10
    name_1:        NGC1700
    descr_1:       E,303
    pos_1:         RA = 04H 56M 56.224S    +/- 2",
    pos_2:         DEC = -04D 51' 57.35"    +/- 2"
    equinox:       2000.0
    rv_or_z:       V = 3976
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 14.86 +/- 2.0

!

    targnum:       11
    name_1:        NGC2636
    descr_1:       E,304
    pos_1:         RA = 08H 48M 24.726S    +/- 2",
    pos_2:         DEC = +73D 40' 15.34"    +/- 2"
    equinox:       2000.0
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 15.00 +/- 2.0

!

    targnum:       12
    name_1:        NGC2832
    descr_1:       E,303
    pos_1:         RA = 09H 19M 46.80S    +/- 2",
    pos_2:         DEC = +33D 44' 58.7"    +/- 2"
    equinox:       2000.0
    rv_or_z:       V = 6946
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 16.84 +/- 2.0

!

    targnum:       13
    name_1:        NGC2841
    descr_1:       E,301
    pos_1:         RA = 09H 22M 02.7S    +/- 2",
    pos_2:         DEC = +50D 58' 35"    +/- 2"
    equinox:       2000.0
    rv_or_z:       V = 652
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 14.69 +/- 2.0

!

    targnum:       16
    name_1:        NGC3599
    descr_1:       E,304
    pos_1:         RA = 11H 15M 26.944S    +/- 2",
    pos_2:         DEC = +18D 6' 37.27"    +/- 2"
    equinox:       2000.0
    rv_or_z:       V = 700
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 15.00 +/- 2.0

!

    targnum:       18
    name_1:        NGC3608
    descr_1:       E,303
    pos_1:         RA = 11H 16M 58.859S    +/- 2",
    pos_2:         DEC = +18D 8' 55.59"    +/- 2"
    equinox:       2000.0
    rv_or_z:       V = 1210
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 15.00 +/- 2.0

!

    targnum:       19
    name_1:        NGC4150
    descr_1:       E,302
    pos_1:         RA = 12H 10M 33.7S    +/- 2",
    pos_2:         DEC = +30D 24' 06"    +/- 2"
    equinox:       2000.0
    rv_or_z:       V = 244
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 15.00 +/- 2.0

!

    targnum:       20
    name_1:        NGC4239
    descr_1:       E,304
    pos_1:         RA = 12H 17M 14.963S    +/- 2",
    pos_2:         DEC = +16D 31' 52.74"    +/- 2"
    equinox:       2000.0
    rv_or_z:       V = 946
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 15.00 +/- 2.0

!

    targnum:       27
    name_1:        NGC4486B
    descr_1:       E,304
    pos_1:         RA = 12H 30M 31.986S    +/- 2",
    pos_2:         DEC = +12D 29' 24.56"    +/- 2"
    equinox:       2000.0
    rv_or_z:       V = 1486
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 15.00 +/- 2.0

!

    targnum:       29
    name_1:        NGC4636
    descr_1:       E,303
    pos_1:         RA = 12H 42M 49.801S    +/- 2",
    pos_2:         DEC = +02D 41' 17.29"    +/- 2"
    equinox:       2000.0
    rv_or_z:       V = 979
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 16.84 +/- 2.0

!

    targnum:       30
    name_1:        NGC4697
    descr_1:       E,303
    pos_1:         RA = 12H 48M 35.896S    +/- 2",
    pos_2:         DEC = -05D 47' 57.34"    +/- 2"
    equinox:       2000.0
    rv_or_z:       V = 1308
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 15.40 +/- 2.0

!

    targnum:       33
    name_1:        NGC4874
    descr_1:       E,303
    pos_1:         RA = 12H 59M 35.65S    +/- 2",
    pos_2:         DEC = +27D 57' 33.0"    +/-2"
    equinox:       2000.0
    rv_or_z:       V = 7176
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 18.40 +/- 2.0

!

    targnum:       34
    name_1:        NGC4889
    descr_1:       E,303
    pos_1:         RA = 13H 00M 8.04S    +/- 2",
    pos_2:         DEC = +27D 58' 36.3"    +/- 2"
    equinox:       2000.0
    rv_or_z:       V = 6467
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 17.48 +/- 2.0

!

    targnum:       35
    name_1:        NGC5322
    descr_1:       E,303
    pos_1:         RA = 13H 49M 15.447S    +/- 2",
    pos_2:         DEC = +60D 11' 24.52"    +/- 2"
    equinox:       2000.0
    rv_or_z:       V = 1902
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 15.65 +/- 2.0

!

    targnum:       36
    name_1:        NGC5813
    descr_1:       E,303
    pos_1:         RA = 15H 01M 11.231S    +/- 2",
    pos_2:         DEC = +01D 42' 5.71"    +/- 2"
    equinox:       2000.0
    rv_or_z:       V = 1882
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 15.88 +/- 2.0

!

    targnum:       38
    name_1:        NGC6166
    descr_1:       E,303,315
    pos_1:         RA = 16H 28M 38.45S    +/- 2",
    pos_2:         DEC = +39D 33' 3.0"    +/- 2"
    equinox:       2000.0
    rv_or_z:       V = 8882
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 18.88 +/- 2.0

!

    targnum:       40
    name_1:        ABELL1020
    descr_1:       E,303
    pos_1:         RA = 10H 27M 49.585S    +/- 2",
    pos_2:         DEC = +10D 26' 31.17"    +/- 2"
    equinox:       2000.0
    rv_or_z:       V = 19500
    fluxnum_1:     1
    fluxval_1:     SURF(V) = 16.34 +/- 2.0

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       1.000
    targname:      NGC2841
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  70S
    priority:      1
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES
    req_1:         CYCLE 2 / 1-56;
    req_2:         PCS FINE / 1-56;
    req_3:         GROUP 1-2 NO GAP
    comment_1:     CAN SWITCH TO COARSE
    comment_2:     TRACK IF FINE IS A
    comment_3:     PROBLEM, BUT PREFER
    comment_4:     FINE WHEN POSSIBLE.

!

    linenum:       2.000
    targname:      NGC2841
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  260S
    s_to_n:        100
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       3.000
    targname:      NGC2636
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  80S
    priority:      1
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES
    req_1:         GROUP 3-4 WITHIN 1D;
    req_2:         SAME ORIENT FOR 4 AS 3;
    req_3:         SAME POS FOR 4 AS 3;

!

    linenum:       4.000
    targname:      NGC2636
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  400S
    s_to_n:        100
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       5.000
    targname:      NGC4486B
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  80S
    priority:      1
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES
    req_1:         GROUP 5-6 WITHIN 1D;
    req_2:         SAME ORIENT FOR 6 AS 5;
    req_3:         SAME POS FOR 6 AS 5;

!

    linenum:       6.000
    targname:      NGC4486B
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  400S
    s_to_n:        100
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       7.000
    targname:      NGC1172
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  80S
    priority:      1
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES
    req_1:         GROUP 7-8 WITHIN 1D;
    req_2:         SAME ORIENT FOR 8 AS 7;
    req_3:         SAME POS FOR 8 AS 7;

!

    linenum:       8.000
    targname:      NGC1172
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  300S
    s_to_n:        100
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       9.000
    targname:      NGC4697
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  140S
    priority:      1
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES
    req_1:         GROUP 9-10 WITHIN 1D;
    req_2:         SAME ORIENT FOR 10 AS 9;
    req_3:         SAME POS FOR 10 AS 9;

!

    linenum:       10.000
    targname:      NGC4697
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  500S
    s_to_n:        100
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       11.000
    targname:      NGC1426
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  80S
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES
    req_1:         GROUP 11-12 WITHIN 1D;
    req_2:         SAME ORIENT FOR 12 AS 11;
    req_3:         SAME POS FOR 12 AS 11;

!

    linenum:       12.000
    targname:      NGC1426
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  300S
    s_to_n:        100
    fluxnum_1:     1
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       13.000
    targname:      NGC1331
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  80S
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES
    req_1:         GROUP 13-14 WITHIN 1D;
    req_2:         SAME ORIENT FOR 14 AS 13;
    req_3:         SAME POS FOR 14 AS 13;

!

    linenum:       14.000
    targname:      NGC1331
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  400S
    s_to_n:        100
    fluxnum_1:     1
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       15.000
    targname:      NGC3608
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  100S
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES
    req_1:         GROUP 15-16 WITHIN 1D;
    req_2:         SAME ORIENT FOR 16 AS 15;
    req_3:         SAME POS FOR 16 AS 15;

!

    linenum:       16.000
    targname:      NGC3608
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  400S
    s_to_n:        100
    fluxnum_1:     1
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       17.000
    targname:      NGC1400
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  100S
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES
    req_1:         GROUP 17-18 WITHIN 1D;
    req_2:         SAME ORIENT FOR 18 AS 17;
    req_3:         SAME POS FOR 18 AS 17;

!

    linenum:       18.000
    targname:      NGC1400
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  350S
    s_to_n:        100
    fluxnum_1:     1
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       19.000
    targname:      NGC1700
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  80S
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES
    req_1:         GROUP 19-20 WITHIN 1D;
    req_2:         SAME ORIENT FOR 20 AS 19;
    req_3:         SAME POS FOR 20 AS 19;

!

    linenum:       20.000
    targname:      NGC1700
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  350S
    s_to_n:        100
    fluxnum_1:     1
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       22.000
    targname:      NGC4636
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  700S
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       23.000
    targname:      NGC4889
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  1700S
    s_to_n:        100
    fluxnum_1:     1
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       24.000
    targname:      NGC5322
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  120S
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES
    req_1:         GROUP 24-25 WITHIN 1D;
    req_2:         SAME ORIENT FOR 25 AS 24;
    req_3:         SAME POS FOR 25 AS 24;

!

    linenum:       25.000
    targname:      NGC5322
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  500S
    s_to_n:        100
    fluxnum_1:     1
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       26.000
    targname:      NGC5813
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  120S
    priority:      1
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES
    req_1:         GROUP 26-27 WITHIN 1D;
    req_2:         SAME ORIENT FOR 27 AS 26;
    req_3:         SAME POS FOR 27 AS 26;

!

    linenum:       27.000
    targname:      NGC5813
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  500S
    s_to_n:        100
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       27.100
    targname:      ABELL1020
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       3
    time_per_exp:  700S
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       27.200
    targname:      NGC3599
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  80S
    s_to_n:        100
    fluxnum_1:     1
    priority:      3
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES
    req_1:         GROUP 27.2-27.3 WITHIN 1D;
    req_2:         SAME ORIENT FOR 27.3 AS 27.2;
    req_3:         SAME POS FOR 27.3 AS 27.2;

!

    linenum:       27.300
    targname:      NGC3599
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  400S
    s_to_n:        100
    fluxnum_1:     1
    priority:      3
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       27.600
    targname:      NGC524
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  120S
    s_to_n:        100
    fluxnum_1:     1
    priority:      3
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES
    req_1:         GROUP 27.6-27.7 WITHIN 1D;
    req_2:         SAME ORIENT FOR 27.7 AS 27.6;
    req_3:         SAME POS FOR 27.7 AS 27.6;

!

    linenum:       27.700
    targname:      NGC524
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  500S
    s_to_n:        100
    fluxnum_1:     1
    priority:      3
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       29.000
    targname:      NGC2832
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  700S
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       30.000
    targname:      NGC4874
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  1700S
    s_to_n:        100
    fluxnum_1:     1
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       31.000
    targname:      NGC6166
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       3
    time_per_exp:  1700S
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       33.000
    targname:      NGC4150
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  80S
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES
    req_1:         GROUP 33-34 WITHIN 1D;
    req_2:         SAME ORIENT FOR 34 AS 33;
    req_3:         SAME POS FOR 34 AS 33;

!

    linenum:       34.000
    targname:      NGC4150
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  400S
    s_to_n:        100
    fluxnum_1:     1
    priority:      2
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!

    linenum:       55.000
    targname:      NGC4239
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  80S
    priority:      1
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES
    req_1:         GROUP 55-56 WITHIN 1D;
    req_2:         SAME ORIENT FOR 56 AS 55;
    req_3:         SAME POS FOR 56 AS 55;

!

    linenum:       56.000
    targname:      NGC4239
    config:        PC
    opmode:        IMAGE
    aperture:      PC6
    sp_element:    F555W
    num_exp:       2
    time_per_exp:  400S
    s_to_n:        100
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT = NO,
    param_2:       PRE-FLASH = YES

!
! end of exposure logsheet

! No scan data records found