!   $Id: 5454,v 6.1 1994/07/27 18:10:55 pepsa Exp $

coverpage:

  title_1:         ELLIPTICALS WITH KINEMATICALLY DISTINCT CORES : CYCLE 4 MEDIUM
    sci_cat:       GALAXIES & CLUSTERS
    sci_subcat:    NUCLEI/CORES
    proposal_for:  GO
    pi_fname:      MARIJN
    pi_lname:      FRANX
    pi_inst:       6830
    pi_country:    NETHERLANDS
    pi_phone:      (011) 31 50 634067
    hours_pri:     14.54
    num_pri:       16
    wf_pc:         Y
    off_fname:     PIET
    off_lname:     VAN DER KRUIT
    off_title:     CHAIRMAN
    off_inst:      6830
    off_addr_1:    KAPTEYN ASTRONOMICAL INSTITUTE
    off_addr_2:    P.O. BOX 800
    off_city:      GRONINGEN
    off_zip:       9700 AV
    off_country:   NETHERLANDS
    off_phone:     (31) 50 634053
! end of coverpage

abstract:

    line_1:        The discovery by Franx and Illingworth of a kinematically-distinct
    line_2:        stellar core in the nucleus of the giant radio elliptical IC 1459, and
    line_3:        the confirmation that such components are quite common, has added a
    line_4:        valuable diagnostic tool for understanding the structure and the formation
    line_5:        of ellipticals. These cores are substantial (10**10 solar masses for
    line_6:        IC 1459) and offer a valuable and unique diagnostic of the dynamical state
    line_7:        of the nuclei of ellipticals.  Further study will address their formation
    line_8:        by investigating whether these cores could be the end result of a
    line_9:        `starburst' event, or from the capture of a stellar companion, or even
    line_10:       the merging of primordial subclumps.  Here we propose to take advantage
    line_11:       of the high resolution imaging of the PC to image the 16 galaxies with
    line_12:       known kinematically distinct cores from our magnitude limited sample of
    line_13:       77 ellipticals. The focus of the program is the detection of stellar
    line_14:       disks (as suggested by the spectroscopic line profile analysis) and
    line_15:       color differences between the core region and the rest of the galaxy.
    line_16:       If the cores have been affected by accretion of stars or gas, and star
    line_17:       formation, then such differences are naturally expected. This program
    line_18:       also allows us to identify the color of any jets or shells and map the
    line_19:       dust at small radii. These data are an essential complement to our
    line_20:       extensive ground-based spectroscopic and imaging survey.

!
! end of abstract

general_form_proposers:

  lname:           FRANX
    fname:         MARIJN
    inst:          6830
    country:       NETHERLANDS
    esa:           Y

!

  lname:           ILLINGWORTH
    fname:         GARTH
    inst:          1552
    country:       USA

!

  lname:           FORBES
    fname:         DUNCAN
    inst:          1552
    country:       USA

!
! end of general_form_proposers block

general_form_text:

  question:        3
    section:       1
    line_1:        We propose to observe all 16 ellipticals with known kinematically distinct
    line_2:        cores from our magnitude limited sample of 77 galaxies.  Several of the
    line_3:        galaxies are of special interest. IC 1459 because it is one the most extreme
    line_4:        examples of a galaxy with a kinematically distinct core.  NGC 7626 is
    line_5:        remarkable because it has a very irregular rotation curve(1).  It is very well
    line_6:        possible that the central parts are not fully relaxed.  It will be very
    line_7:        interesting to see whether HST detects any sharp, high contrast features in
    line_8:        this galaxy.  NGC 1439 is the intrinsically faintest galaxy in the sample, with
    line_9:        the lowest velocity dispersion.  NGC 1427 has a rotation curve that is
    line_10:       unresolved even at subarcsecond seeing.  NGC 5982 is the only galaxy which has
    line_11:       a distinct core that has a rotation axis parallel to the major axis. All other
    line_12:       systems rotate around the minor axis.
    line_13:       We propose to obtain sets of images in the F555W and F814W filters.  The F555W
    line_14:       filter is chosen for this study because it provides high throughput and its PSF
    line_15:       will be well monitored. This is important for removing a nuclear point source
    line_16:       prior to further analysis (as was necessary for IC 1459) and if deconvolution
    line_17:       is applied.  The F814W filter provides a long wavelength base for color
    line_18:       analysis (it is less affected by dust), the background sky is fainter (Wright
    line_19:       1985) and better samples the dominant stellar component.  Although we expect
    line_20:       WFPC2 to have an image quality close to specifications (i.e. 70% in 0.1''), we
    line_21:       can still in principle gain through deconvolution techniques with imaging
    line_22:       closer to the diffraction limit of the telescope (i.e. 80% in 0.1'').
    line_23:       1. Jedrzejewski  Schechter 1988, ApJ, 330, L87

!

  question:        4
    section:       1
    line_1:        The use of the imaging capabilities of HST is a logical and important component
    line_2:        of a broadly-based observational program involving ground-based long-slit
    line_3:        spectra and ground-based images of ellipticals with kinematically-distinct
    line_4:        cores.  Both the spectroscopic and the imaging results suggest that these
    line_5:        distinct nuclear subcomponents are unresolved from the ground in typical
    line_6:        1-2'' seeing.  The cores of ellipticals are known to be at best marginally
    line_7:        resolved from the ground, with a few notable exceptions (see e.g., ref. 1).  If
    line_8:        compact star clusters or black-holes are significant in these cores, the small
    line_9:        gains in resolution possible at Hawaii and other sites will not be decisive in
    line_10:       establishing the structure of the nuclei on scales <0.2''.  The results by
    line_11:       Lauer et al (ref. 2,3,4) have shown convincingly that PC imaging can do
    line_12:       significantly better than any ground-based facilities.  The images requested
    line_13:       here will complement the available ground-based multicolor CCD surface
    line_14:       photometry by allowing comparison of the core structure and properties with
    line_15:       those at larger radii.  Furthermore, the early `discovery' spectroscopic
    line_16:       observations have been supplemented by a set of higher S/N long-slit spectra
    line_17:       taken with the highest practical ground-based spatial resolution (1'' with
    line_18:       0.3-0.6'' pixels) at a variety of position angles.  These data have been
    line_19:       acquired both in the Northern and Southern hemispheres, at CTIO and Lick.
    line_20:       The use of the imaging capabilities of HST is a logical and important component
    line_21:       Ideally one would like high spatial resolution spectroscopic observations from
    line_22:       HST.  This is impractical without a good imaging capacity and without a
    line_23:       long-slit spectrograph on HST; the FOS integrations required would be

!

  question:        4
    section:       2
    line_1:        prohibitively long.  The best approach is the compromise one of high resolution
    line_2:        HST images, combined with ground-based kinematical mapping and overlapping with
    line_3:        ground-based images that define the large-scale (r > 5-10'') structure.
    line_4:        1. Kormendy 1985, ApJ, 292, L9
    line_5:        2. Lauer, et al 1991, ApJ, 369, L41
    line_6:        3. Lauer, et al 1992a, AJ, 103, 703
    line_7:        4. Lauer, et al 1992b, AJ, 104, 552

!

  question:        5
    section:       1
    line_1:

!

  question:        6
    section:       1
    line_1:

!


!


!

  question:        8
    section:       1
    line_1:

!

  question:        9
    section:       1
    line_1:        The PI (MF) and Co-I (GDI) have been involved in several previous HST programs.
    line_2:        They include:
    line_4:        2684 (The Medium Deep Survey), GDI.
    line_5:        4664 (Nearby Nuclei Snapshot Survey), GDI.
    line_6:        3551 (Ellipticals with Kinematically Distinct Nuclei), GDI and MF.
    line_7:        2227 and  3905 (The Extra-Galactic Distance Scale), GDI.
    line_9:        The most directly related program is 3551 from cycle 2. This was a single color
    line_10:       (F555W) PC imaging project of seven galaxies with kinematically distinct cores.
    line_11:       In our paper (Illingworth, Forbes Franx 1993, in preparation) we report that IC
    line_12:       1459 reveals an unresolved point source (V 18.5mag), a cusp to the central
    line_13:       starlight profile (with a slope similar to that found for M87) and a small
    line_14:       scale dust lane that appears to reach into the very nucleus and may thus be
    line_15:       associated with material that fuels the nuclear activity. Reduction and
    line_16:       analysis of the other six galaxies are in progress. Although this data contains
    line_17:       much useful information on small scales, it provides no color information which
    line_18:       is the main focus of this proposal. The data requested here will also benefit
    line_19:       from the improved optics allowing more subtle features, than present in IC
    line_20:       1459, to be revealed.
    line_22:       Program 4664 involved short, single color (F555W) exposures of nearby SO and
    line_23:       spiral nuclei. Although it is related in general aim (to probe the nuclear

!

  question:        9
    section:       2
    line_1:        region of galaxies unavailable to ground-based observations) this program can
    line_2:        not address the specific areas that can be tackled with the multi-color data
    line_3:        requested in this proposal.
    line_5:        Publications include:
    line_6:        Illingworth, Forbes  Franx 1993, in preparation (June 93).
    line_7:        Forbes et al. 1993, IAU 158, Very High Angular Resolution Imaging, in press.
    line_8:        Forbes, Illingworth  Franx 1993, in preparation (July 93).
    line_9:        Griffiths et al. 1993, Science with the HST, in press.
    line_11:       There have also been various abstracts published from talks and posters at AAS
    line_12:       meetings.

!

  question:        10
    section:       1
    line_1:        Most of the data reduction will be carried out at Lick Observatory.
    line_2:        Lick Observatory has a strong foundation for image processing of large
    line_3:        HST images (via the Medium Deep Survey key project and WFPC IDT). The
    line_4:        department has a powerful host SUN 4/280 system with high performance
    line_5:        peripherals.  Both GDI and DAF have UCSC-supplied SUN workstations,
    line_6:        which will draw upon the departmental resources.  Several staff are
    line_7:        available to support the systems and system software development.
    line_8:        There is also a pool of ten or more graduate students, some of whom
    line_9:        have University Fellowships, who work intensively with optical imaging
    line_10:       and spectroscopy.  S. Faber, an WFPC IDT team member, is on the Lick
    line_11:       faculty, and will be a source of the IDT team's valuable early
    line_12:       experience in processing WFPC data. GDI also has access to the 3 m and
    line_13:       1 m telescopes on Mt. Hamilton, and to the Keck 10m.
    line_15:       MF, previously a Hubble Fellow, is now a full Professor at the Kapteyn
    line_16:       Astronomical Institute. This position includes summer salary, and some
    line_17:       research funding. The Kapteyn Institute is involved in several HST GO
    line_18:       programs.

!
!end of general form text

general_form_address:

  lname:           FRANX
    fname:         MARIJN
    category:      PI
    inst:          6830
    addr_1:        KAPTEYN ASTRONOMICAL INSTITUTE
    addr_2:        P.O. BOX 800
    city:          GRONINGEN
    zip:           9700 AV
    country:       NETHERLANDS
    phone:         (011) 31 50 634067
    telex:         FRANX@ASTRO.RUG.NL

!

  lname:
    category:      CON

!
! end of general_form_address records

fixed_targets:

    targnum:       1
    name_1:        IC1459
    descr_1:       E,303
    pos_1:         RA=  22H57M10.47S +/- 0.1S,
    pos_2:         DEC=-36D27'45.2 " +/- 1.0",
    pos_3:         PLATE-ID=05XU
    equinox:       J2000
    comment_1:     FLUX IS SURFACE BRIGHTNESS AT 1
    comment_2:     ARCSEC DISTANCE FROM CENTER
    comment_3:     SURFACE BRIGHTNESS (MUCH) HIGHER
    comment_4:     AT CENTER
    fluxnum_1:     1
    fluxval_1:     SURF(R)=15.1 +/- 1

!

    targnum:       2
    name_1:        NGC1427
    descr_1:       E,303
    pos_1:         RA=  03H42M19.50S +/- 0.1S,
    pos_2:         DEC=-35D23'32.7 " +/-  1.0"
    equinox:       J2000
    comment_1:     FLUX IS SURFACE BRIGHTNESS AT 1
    comment_2:     ARCSEC DISTANCE FROM CENTER
    comment_3:     SURFACE BRIGHTNESS (MUCH) HIGHER
    comment_4:     AT CENTER

!

    targnum:       3
    name_1:        NGC1439
    descr_1:       E,303
    pos_1:         RA=  03H44M49.86S +/- 0.1S,
    pos_2:         DEC=-21D55'13.8" +/-  1.0"
    equinox:       J2000
    comment_1:     FLUX IS SURFACE BRIGHTNESS AT 1
    comment_2:     ARCSEC DISTANCE FROM CENTER
    comment_3:     SURFACE BRIGHTNESS (MUCH) HIGHER
    comment_4:     AT CENTER
    fluxnum_1:     1
    fluxval_1:     SURF(R)=16.0 +/- 1

!

    targnum:       4
    name_1:        NGC1700
    descr_1:       E,303
    pos_1:         RA=  04H56M56.21S +/- 0.1S,
    pos_2:         DEC=-04D51'56.5" +/-  1.0",
    pos_3:         PLATE-ID=04MX
    equinox:       J2000
    comment_1:     FLUX IS SURFACE BRIGHTNESS AT 1
    comment_2:     ARCSEC DISTANCE FROM CENTER
    comment_3:     SURFACE BRIGHTNESS (MUCH) HIGHER
    comment_4:     AT CENTER
    fluxnum_1:     1
    fluxval_1:     SURF(R)=15.5 +/- 1

!

    targnum:       5
    name_1:        NGC3608
    descr_1:       E,303
    pos_1:         RA=  11H16M58.95S +/- 0.1S,
    pos_2:         DEC= 18D08'54.9 " +/- 1.0",
    pos_3:         PLATE-ID=01TO
    equinox:       J2000
    comment_1:     FLUX IS SURFACE BRIGHTNESS AT 1
    comment_2:     ARCSEC DISTANCE FROM CENTER
    comment_3:     SURFACE BRIGHTNESS (MUCH) HIGHER
    comment_4:     AT CENTER
    fluxnum_1:     1
    fluxval_1:     SURF(R)=16.2 +/- 1

!

    targnum:       6
    name_1:        NGC4278
    descr_1:       E,303
    pos_1:         RA=  12H20M06.86S +/- 0.1S,
    pos_2:         DEC= 29D16'50.3" +/-  1.0",
    pos_3:         PLATE-ID=00DJ
    equinox:       J2000
    comment_1:     FLUX IS SURFACE BRIGHTNESS AT 1
    comment_2:     ARCSEC DISTANCE FROM CENTER
    comment_3:     SURFACE BRIGHTNESS (MUCH) HIGHER
    comment_4:     AT CENTER
    fluxnum_1:     1
    fluxval_1:     SURF(R)=15.4 +/- 1

!

    targnum:       7
    name_1:        NGC4365
    descr_1:       E,303
    pos_1:         RA=  12H24M28.30S +/- 0.1S,
    pos_2:         DEC=  7D19'03.4" +/-  1.0",
    pos_3:         PLATE-ID=01UQ
    equinox:       J2000
    comment_1:     FLUX IS SURFACE BRIGHTNESS AT 1
    comment_2:     ARCSEC DISTANCE FROM CENTER
    comment_3:     SURFACE BRIGHTNESS (MUCH) HIGHER
    comment_4:     AT CENTER
    fluxnum_1:     1
    fluxval_1:     SURF(R)=15.9 +/- 1

!

    targnum:       8
    name_1:        NGC4406
    descr_1:       E,303
    pos_1:         RA=  12H26M11.78S +/- 0.1S,
    pos_2:         DEC= 12D56'46.3" +/-  1.0",
    pos_3:         PLATE-ID=00IY
    equinox:       J2000
    comment_1:     FLUX IS SURFACE BRIGHTNESS AT 1
    comment_2:     ARCSEC DISTANCE FROM CENTER
    comment_3:     SURFACE BRIGHTNESS (MUCH) HIGHER
    comment_4:     AT CENTER
    fluxnum_1:     1
    fluxval_1:     SURF(R)=15.7 +/- 1

!

    targnum:       10
    name_1:        NGC4494
    descr_1:       E,303
    pos_1:         RA=  12H31M24.09S +/- 0.1S,
    pos_2:         DEC= 25D46'28.9"  +/- 1.0"
    equinox:       J2000
    comment_1:     FLUX IS SURFACE BRIGHTNESS AT 1
    comment_2:     ARCSEC DISTANCE FROM CENTER
    comment_3:     SURFACE BRIGHTNESS (MUCH) HIGHER
    comment_4:     AT CENTER
    fluxnum_1:     1
    fluxval_1:     SURF(R)=15.6 +/- 1

!

    targnum:       11
    name_1:        NGC4552
    descr_1:       E,303
    pos_1:         RA=  12H35M39.83S +/- 0.1S,
    pos_2:         DEC= 12D33'22.8"  +/- 1.0",
    pos_3:         PLATE-ID=00IY
    equinox:       J2000
    comment_1:     FLUX IS SURFACE BRIGHTNESS AT 1
    comment_2:     ARCSEC DISTANCE FROM CENTER
    comment_3:     SURFACE BRIGHTNESS (MUCH) HIGHER
    comment_4:     AT CENTER
    fluxnum_1:     1
    fluxval_1:     SURF(R)=15.0 +/- 1

!

    targnum:       12
    name_1:        NGC4589
    descr_1:       E,303
    pos_1:         RA=  12H37M24.89S +/- 0.1S,
    pos_2:         DEC= 74D11'30.9"  +/- 1.0"
    equinox:       J2000
    comment_1:     FLUX IS SURFACE BRIGHTNESS AT 1
    comment_2:     ARCSEC DISTANCE FROM CENTER
    comment_3:     SURFACE BRIGHTNESS (MUCH) HIGHER
    comment_4:     AT CENTER
    fluxnum_1:     1
    fluxval_1:     SURF(R)=16.3 +/- 1

!

    targnum:       13
    name_1:        NGC5322
    descr_1:       E,303
    pos_1:         RA=  13H49M15.45S +/- 0.1S,
    pos_2:         DEC= 60D11'25.9"  +/- 1.0",
    pos_3:         PLATE-ID=01R0
    equinox:       J2000
    comment_1:     FLUX IS SURFACE BRIGHTNESS AT 1
    comment_2:     ARCSEC DISTANCE FROM CENTER
    comment_3:     SURFACE BRIGHTNESS (MUCH) HIGHER
    comment_4:     AT CENTER
    fluxnum_1:     1
    fluxval_1:     SURF(R)=15.8 +/- 1

!

    targnum:       14
    name_1:        NGC5813
    descr_1:       E,303
    pos_1:         RA=  15H01M11.18S +/- 0.1S,
    pos_2:         DEC= 01D42'07.1"  +/- 1.0"
    equinox:       J2000
    comment_1:     FLUX IS SURFACE BRIGHTNESS AT 1
    comment_2:     ARCSEC DISTANCE FROM CENTER
    comment_3:     SURFACE BRIGHTNESS (MUCH) HIGHER
    comment_4:     AT CENTER
    fluxnum_1:     1
    fluxval_1:     SURF(R)=16.0 +/- 1

!

    targnum:       15
    name_1:        NGC5982
    descr_1:       E,303
    pos_1:         RA=  15H38M39.94S +/- 0.1S,
    pos_2:         DEC= 59D21'21.6" +/-  1.0"
    equinox:       J2000
    comment_1:     FLUX IS SURFACE BRIGHTNESS AT 1
    comment_2:     ARCSEC DISTANCE FROM CENTER
    comment_3:     SURFACE BRIGHTNESS (MUCH) HIGHER
    comment_4:     AT CENTER
    fluxnum_1:     1
    fluxval_1:     SURF(R)=15.9 +/- 1

!

    targnum:       16
    name_1:        NGC7626
    descr_1:       E,303
    pos_1:         RA=  23H20M42.55S +/- 0.1S,
    pos_2:         DEC= 08D13'01.0"  +/-  1.0"
    equinox:       J2000
    comment_1:     FLUX IS SURFACE BRIGHTNESS AT 1
    comment_2:     ARCSEC DISTANCE FROM CENTER
    comment_3:     SURFACE BRIGHTNESS (MUCH) HIGHER
    comment_4:     AT CENTER
    fluxnum_1:     1
    fluxval_1:     SURF(R)=16.6 +/- 1

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       1.000
    targname:      IC1459
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  1000S
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         CYCLE 4 / 1-16.1;
    req_2:         GROUP 1-1.1 NO GAP

!

    linenum:       1.100
    targname:      IC1459
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F814W
    num_exp:       1
    time_per_exp:  500S
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         SAME POS FOR 1.1 AS 1.0
    

!

    linenum:       2.000
    targname:      NGC1427
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  1000S
    fluxnum_1:     1
    priority:      4
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         GROUP 2-2.1 NO GAP

!

    linenum:       2.100
    targname:      NGC1427
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F814W
    num_exp:       1
    time_per_exp:  500S
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         SAME POS FOR 2.1 AS 2.0

!

    linenum:       3.000
    targname:      NGC1439
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  1000S
    fluxnum_1:     1
    priority:      6
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         GROUP 3-3.1 NO GAP

!

    linenum:       3.100
    targname:      NGC1439
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F814W
    num_exp:       1
    time_per_exp:  500S
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         SAME POS FOR 3.1 AS 3.0

!

    linenum:       4.000
    targname:      NGC1700
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  1000S
    fluxnum_1:     1
    priority:      5
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         GROUP 4-4.1 NO GAP

!

    linenum:       4.100
    targname:      NGC1700
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F814W
    num_exp:       1
    time_per_exp:  500S
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         SAME POS FOR 4.1 AS 4.0

!

    linenum:       5.000
    targname:      NGC3608
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  1000S
    fluxnum_1:     1
    priority:      7
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         GROUP 5-5.1 NO GAP

!

    linenum:       5.100
    targname:      NGC3608
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F814W
    num_exp:       1
    time_per_exp:  500S
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         SAME POS FOR 5.1 AS 5.0

!

    linenum:       6.000
    targname:      NGC4278
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  1000S
    fluxnum_1:     1
    priority:      7
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         GROUP 6-6.1 NO GAP

!

    linenum:       6.100
    targname:      NGC4278
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F814W
    num_exp:       1
    time_per_exp:  500S
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         SAME POS FOR 6.1 AS 6.0

!

    linenum:       7.000
    targname:      NGC4365
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  1000S
    fluxnum_1:     1
    priority:      7
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         GROUP 7-7.1 NO GAP

!

    linenum:       7.100
    targname:      NGC4365
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F814W
    num_exp:       1
    time_per_exp:  500S
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         SAME POS FOR 7.1 AS 7.0

!

    linenum:       8.000
    targname:      NGC4406
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  1000S
    fluxnum_1:     1
    priority:      7
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         GROUP 8-8.1 NO GAP

!

    linenum:       8.100
    targname:      NGC4406
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F814W
    num_exp:       1
    time_per_exp:  500S
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         SAME POS FOR 8.1 AS 8.0

!

    linenum:       10.000
    targname:      NGC4494
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  1000S
    fluxnum_1:     1
    priority:      7
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         GROUP 10-10.1 NO GAP

!

    linenum:       10.100
    targname:      NGC4494
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F814W
    num_exp:       1
    time_per_exp:  500S
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         SAME POS FOR 10.1 AS 10.0

!

    linenum:       11.000
    targname:      NGC4552
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  1000S
    fluxnum_1:     1
    priority:      7
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         GROUP 11-11.1 NO GAP

!

    linenum:       11.100
    targname:      NGC4552
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F814W
    num_exp:       1
    time_per_exp:  500S
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         SAME POS FOR 11.1 AS 11.0

!

    linenum:       12.000
    targname:      NGC4589
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  1000S
    fluxnum_1:     1
    priority:      7
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         GROUP 12-12.1 NO GAP

!

    linenum:       12.100
    targname:      NGC4589
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F814W
    num_exp:       1
    time_per_exp:  500S
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         SAME POS FOR 12.1 AS 12.0

!

    linenum:       13.000
    targname:      NGC5322
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  1000S
    fluxnum_1:     1
    priority:      3
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         GROUP 13-13.1 NO GAP

!

    linenum:       13.100
    targname:      NGC5322
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F814W
    num_exp:       1
    time_per_exp:  500S
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         SAME POS FOR 13.1 AS 13.0
!

    linenum:       14.000
    targname:      NGC5813
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  1000S
    fluxnum_1:     1
    priority:      7
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         GROUP 14-14.1 NO GAP

!

    linenum:       14.100
    targname:      NGC5813
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F814W
    num_exp:       1
    time_per_exp:  500S
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         SAME POS FOR 14.1 AS 14.0

!

    linenum:       15.000
    targname:      NGC5982
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  1000S
    fluxnum_1:     1
    priority:      7
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         GROUP 15-15.1 NO GAP

!

    linenum:       15.100
    targname:      NGC5982
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F814W
    num_exp:       1
    time_per_exp:  500S
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         SAME POS FOR 15.1 AS 15.0

!

    linenum:       16.000
    targname:      NGC7626
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F555W
    num_exp:       1
    time_per_exp:  1000S
    fluxnum_1:     1
    priority:      2
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         GROUP 16-16.1 NO GAP 

!

    linenum:       16.100
    targname:      NGC7626
    config:        WFPC2
    opmode:        IMAGE
    aperture:      PC1
    sp_element:    F814W
    num_exp:       1
    time_per_exp:  500S
    fluxnum_1:     1
    priority:      1
    param_1:       CR-SPLIT=0.5
    param_2:       CR-TOLERANCE=0.1
    param_3:       ATD-GAIN=7
    req_1:         SAME POS FOR 16.1 AS 16.0

!
! end of exposure logsheet

! No scan data records found