!  File:  4062C.PROP
!  Database:  PEPDB
!  Date:  20-FEB-1994:07:04:43

coverpage:

  title_1:         STELLAR AND GAS DYNAMICS IN NORMAL GALAXIES AUGMENTATION:
    title_2:       CYCLE 2 OBSERVATIONS
    sci_cat:       GALAXIES & CLUSTERS
    proposal_for:  AUG/FOS
    cont_id:       3782
    pi_title:      DR.
    pi_fname:      HOLLAND
    pi_mi:         C.
    pi_lname:      FORD
    pi_inst:       SPACE TELESCOPE SCIENCE INSTITUTE
    pi_country:    USA
    pi_phone:      (410) 338-4803
    keywords_1:    GALAXIES, STELLAR DYNAMICS, IONIZED GAS
    hours_pri:     18.11
    num_pri:       25
    fos:           Y
! end of coverpage

abstract:

    line_1:        The FOS will be used with small apertures to map the stellar
    line_2:        velocity dispersion and rotation in a grid
    line_3:        covering the central 1" of NGC224 (M31).
    line_4:        The velocity disperions and rotation curves will be
    line_5:        used to model the nuclear dynamics and to measure the nuclear
    line_6:        M/L.  Line strengths will be used to measure changes in the
    line_7:        stellar populations in the central 1".  FOS spectra of
    line_8:        emission-line clouds within the nuclear region will be used to
    line_9:        establish their physical characteristics, ionization
    line_10:       mechanisms, and dynamics.

!
! end of abstract

general_form_proposers:

  lname:           BEAVER
    fname:         EDWARD
    inst:          UC, SAN DIEGO
    country:       USA

!

  lname:           BURBIDGE
    fname:         E. MARGARET
    inst:          UC, SAN DIEGO
    country:       USA

!

  lname:           MARGON
    fname:         BRUCE
    inst:          WASHINGTON, UNIVERSITY OF
    country:       USA

!

  lname:           ANGEL
    fname:         J. ROGER
    mi:            P.
    inst:          ARIZONA, UNIVERSITY OF
    country:       USA

!

  lname:           BARTKO
    fname:         FRANK
    inst:          APPLIES RESEARCH CORPORATION
    country:       USA

!

  lname:           DAVIDSEN
    fname:         ARTHUR
    mi:            F.
    inst:          JOHNS HOPKINS UNIVERSITY
    country:       USA

!

  lname:           HARMS
    fname:         RICHARD
    mi:            J.
    inst:          APPLIED RESEARCH CORPORATION
    country:       USA

!

  lname:           BOHLIN
    fname:         RALPH
    inst:          SPACE TELESCOPE SCIENCE INSTITUTE
    country:       USA

!

  lname:           FORD
    fname:         HOLLAND
    mi:            C.
    inst:          SPACE TELESCOPE SCIENCE INSTITUTE
    country:       USA

!
! end of general_form_proposers block

general_form_text:

  question:        3
    section:       1
    line_1:        FOS observations of NGC 224 (M31) will consist of spectra at locations
    line_2:        along the major axis (position angle 45 deg) of 0.0", +/-0.25",
    line_3:        +-0.50", and +/-0.75" using grating G570H and the 0.3" aperture.  Two
    line_4:        additional points at +/-1.0" will be obtained using the 0.5" aperture.
    line_5:        All these major axis positions have been moved from the FOS/GTO
    line_6:        baseline program into this augmented time proposal to unify the target
    line_7:        acquisition and ensure that all positions in the nuclear region are
    line_8:        registered at precisely known positions. Along the minor axis (Position
    line_9:        angle 135 deg) we will obtain spectra at +/-0.25", +-0.50", and
    line_10:       +/-0.75" using grating G570H and the 0.3" aperture.  Additional
    line_11:       spectra at 8 off-axis points parallel to and on either side of the
    line_12:       major axis ((+/-0.25", +/-0.25") and (+/-0.25", +/-0.5")) using the
    line_13:       same grating/aperture combination will also be obtained.
    line_14:       Acquisition will be done using a binary search on a nearby star
    line_15:       identified in a WFC image, followed by two small peak-ups on the
    line_16:       brightest peak in the nucleus of NGC 224.  Since the selected
    line_17:       star is not in the same WFC CCD frame as the nucleus of NGC 224,
    line_18:       we will update the coordinates in the proposal once the geometric
    line_19:       calibration of mosaic WFC frames is complete.  For use as a
    line_20:       template star in Fourier quotient deconvolutions, we will obtain a
    line_21:       spectrum of the K star F193 using the same grating and aperture.
    line_22:       Internal wavelength calibrations will be obtained through the same
    line_23:       grating and aperture on each of the M31 exposures and on F193.

!

  question:        4
    section:       1
    line_1:        NGC 224 (M31) has been observed extensively from the ground
    line_2:        both photometrically and spectroscopically.  In addition, the nucleus
    line_3:        of NGC 224 has been imaged from the balloon-borne Stratoscope
    line_4:        telescope.  Despite the spherical aberration of the HST primary, our
    line_5:        Cycle 0 images resolve more structure in the nucleus of M31 than is
    line_6:        even apparent from the Stratoscope images; structure that can be
    line_7:        resolved with no correction for spherical aberration should yield
    line_8:        unconfused dynamical measurements that are impossible to obtain from
    line_9:        the ground in even the best seeing.

!

  question:        5
    section:       1
    line_1:        The observations of the nuclear region of NGC 224 (M31) are arranged
    line_2:        on a finely spaced (0.25") rectangular grid along the major and minor
    line_3:        axes.  To ensure the precise relative registration of the pointing
    line_4:        positions in the grid, we wish to perform only one target acquisition
    line_5:        and use only small angle maneuvers to obtain the spectra at each of
    line_6:        the 23 ensuing points in the grid.  The requisite observations have
    line_7:        been indicated with GROUP NO GAP in the exposure log sheet.
    line_9:        The observations of the star F193 are for use as a template in the
    line_10:       Fourier quotient analysis of the NGC 224 nuclear spectra.  To avoid
    line_11:       any potential temporal changes in the instrument that might invalidate
    line_12:       the use of these observations as a template, we request that they be
    line_13:       scheduled within 60 days of the NGC 224 observations.

!

  question:        6
    section:       1
    line_1:        Precise wavelength calibrations are required to study the kinematics of
    line_2:        the gas and stars in the nucleus of NGC 224 (M31).  Internal WAVE
    line_3:        calibrations are required for observations using grating G570H as
    line_4:        indicated in the exposure log.  These calibration exposures must be
    line_5:        obtained immediately following the science exposures with no
    line_6:        intervening motion of the FOS filter/grating wheel or apertures.

!

  question:        7
    section:       1
    line_1:        The FOS spectra will be processed using the latest available
    line_2:        calibration data to transform the raw count data into flux-calibrated,
    line_3:        wavelength-calibrated images. Velocities and dispersions for the
    line_4:        NGC 224 spectra will be obtained using Fourier quotient routines
    line_5:        operating in IRAF based on the algorithms outlined by
    line_6:        Sargent et al (1977).  In addition, we will test more complex
    line_7:        dynamical models for NGC 224 by folding spectra of our template star
    line_8:        through the dynamical model and the point response of HST and
    line_9:        integrating the resulting spectra over the FOS apertures
    line_10:       (eg, Dressler & Richstone 1988; Kormendy 1988).  This will allow us to
    line_11:       test the validity of our conclusions in the face of complications due
    line_12:       to the aberrated images produced by the primary mirror.

!

  question:        8
    section:       1
    line_1:        The PC and WFC images of the target galaxies will be measured for
    line_2:        precise target coordinates, so that the FOS observations can be done
    line_3:        as blind offsets from a nearby isolated star.  We have selected an
    line_4:        appropriate star from our WFC images, but we will update the
    line_5:        coordinates in our target list once a final geometric calibration of
    line_6:        the WFC mosaic has been established.
    line_8:        While not officially listed as co-investigators, the following
    line_9:        scientists are actively involved in research with the FOS GTO team and
    line_10:       are expected to contribute significantly to its scientific output:
    line_11:       W. P. Blair, S. Caganoff, G. A. Kriss, A. Uomoto (JHU);
    line_12:       R. Antonucci (UCSB); L. Armus (Cal Tech); I. Evans, A. Kinney (STScI);
    line_13:       L. Dressel (ARC); R. Allen, P. Smith (U. Arizona);
    line_14:       S. Anderson (U. Washington); R. Cohen, R. Hier, V. Junkarrinen,
    line_15:       E. Rosenblatt (UCSD).

!

  question:        9
    section:       1
    line_1:        Since there are 29 separate FOS IDT GTO programs, only those related
    line_2:        to the current proposal are listed here.
    line_4:        1040 - Velocity Dispersions in the Nuclei of Giant Ellipticals
    line_5:        1041, 3191, 3276 - The Nucleus of Normal and Starburst Galaxies
    line_6:        1044, 3193, 3277 - Stellar and Gas Dynamics in Normal Galaxies

!

  question:        10
    section:       1
    line_1:        All resources for these programs are provided by NASA through the
    line_2:        FOS IDT contract NAS 5-29293.

!
!end of general form text

general_form_address:

  lname:           FORD
    fname:         HOLLAND
    mi:            C.
    category:      PI
    inst:          SPACE TELESCOPE SCIENCE INSTITUTE

!
! end of general_form_address records

fixed_targets:

    targnum:       1
    name_1:        NGC224
    name_2:        M31
    descr_1:       E,301,910
    pos_2:         RA=00H 42M 44.3303S +/- 0.3",
    pos_3:         DEC=+41D 16' 08.972" +/- 0.3",
    pos_4:         PLATE-ID=01JV
    equinox:       2000
    rv_or_z:       V=-200
    fluxnum_1:     1
    fluxval_1:     F(5470)=4.4E-16
    fluxnum_2:     2
    fluxval_2:     E(B-V)=0.11

!

    targnum:       2
    name_1:        NGC224-NE1
    descr_1:       E,301,913
    pos_1:         R=0.25" +/- 0.02",
    pos_2:         PA=45D +/- 4.5D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=4.8E-16

!

    targnum:       3
    name_1:        NGC224-NE2
    descr_1:       E,301,913
    pos_1:         R=0.50" +/- 0.02",
    pos_2:         PA=45D +/- 2.3D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=4.0E-16

!

    targnum:       4
    name_1:        NGC224-NE3
    descr_1:       E,301,913
    pos_1:         R=0.75" +/- 0.05",
    pos_2:         PA=45D +/- 2.3D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=3.2E-16

!

    targnum:       5
    name_1:        NGC224-NE4
    descr_1:       E,301,913
    pos_1:         R=1.0" +/- 0.05",
    pos_2:         PA=45D +/- 2.3D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=6.8E-16

!

    targnum:       6
    name_1:        NGC224-SW1
    descr_1:       E,301,913
    pos_1:         R=0.25" +/- 0.02",
    pos_2:         PA=225D +/- 4.5D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=4.3E-16

!

    targnum:       7
    name_1:        NGC224-SW2
    descr_1:       E,301,913
    pos_1:         R=0.50" +/- 0.05",
    pos_2:         PA=225D +/- 2.3D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=4.0E-16

!

    targnum:       8
    name_1:        NGC224-SW3
    descr_1:       E,301,913
    pos_1:         R=0.75" +/- 0.05",
    pos_2:         PA=225D +/- 2.3D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=3.4E-16

!

    targnum:       9
    name_1:        NGC224-SW4
    descr_1:       E,301,913
    pos_1:         R=1.0" +/- 0.05",
    pos_2:         PA=225D +/- 2.3D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=7.7E-16

!

    targnum:       10
    name_1:        NGC224-NW1
    descr_1:       E,301,913
    pos_1:         R=0.25" +/- 0.02",
    pos_2:         PA=315D +/- 4.5D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=4.0E-16

!

    targnum:       11
    name_1:        NGC224-NW2
    descr_1:       E,301,913
    pos_1:         R=0.50" +/- 0.02",
    pos_2:         PA=315D +/- 2.3D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=3.2E-16

!

    targnum:       12
    name_1:        NGC224-NW3
    descr_1:       E,301,913
    pos_1:         R=0.75" +/- 0.05",
    pos_2:         PA=315D +/- 2.3D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=2.7E-16

!

    targnum:       13
    name_1:        NGC224-SE1
    descr_1:       E,301,913
    pos_1:         R=0.25" +/- 0.02",
    pos_2:         PA=135D +/- 4.5D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=4.0E-16

!

    targnum:       14
    name_1:        NGC224-SE2
    descr_1:       E,301,913
    pos_1:         R=0.50" +/- 0.02",
    pos_2:         PA=135D +/- 2.3D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=3.2E-16

!

    targnum:       15
    name_1:        NGC224-SE3
    descr_1:       E,301,913
    pos_1:         R=0.75" +/- 0.05",
    pos_2:         PA=135D +/- 2.3D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=2.7E-16

!

    targnum:       16
    name_1:        NGC224-N1
    descr_1:       E,301,913
    pos_1:         R=0.354" +/- 0.02",
    pos_2:         PA=0D +/- 4.5D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=4.0E-16

!

    targnum:       17
    name_1:        NGC224-N2
    descr_1:       E,301,913
    pos_1:         R=0.433" +/- 0.02",
    pos_2:         PA=26.565D +/- 2.3D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=3.6E-16

!

    targnum:       18
    name_1:        NGC224-E1
    descr_1:       E,301,913
    pos_1:         R=0.354" +/- 0.02",
    pos_2:         PA=90D +/- 4.5D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=4.3E-16

!

    targnum:       19
    name_1:        NGC224-E2
    descr_1:       E,301,913
    pos_1:         R=0.433" +/- 0.02",
    pos_2:         PA=63.435D +/- 2.3D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=3.9E-16

!

    targnum:       20
    name_1:        NGC224-S1
    descr_1:       E,301,913
    pos_1:         R=0.354" +/- 0.02",
    pos_2:         PA=180D +/- 4.5D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=3.7E-16

!

    targnum:       21
    name_1:        NGC224-S2
    descr_1:       E,301,913
    pos_1:         R=0.433" +/- 0.02",
    pos_2:         PA=206.565D +/- 2.3D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=3.5E-16

!

    targnum:       22
    name_1:        NGC224-W1
    descr_1:       E,301,913
    pos_1:         R=0.354" +/- 0.02",
    pos_2:         PA=270D +/- 4.5D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=3.9E-16

!

    targnum:       23
    name_1:        NGC224-W2
    descr_1:       E,301,913
    pos_1:         R=0.433" +/- 0.02",
    pos_2:         PA=243.435D +/- 2.3D,
    pos_3:         FROM 1
    fluxnum_1:     1
    fluxval_1:     F(5470)=3.6E-16

!

    targnum:       24
    name_1:        NGC224-OFFSET
    descr_1:       A,140
    pos_2:         RA-OFF=4.4547S +/- 0.0018S,
    pos_3:         DEC-OFF=-55.392" +/- 0.02",
    pos_4:         FROM 1
    fluxnum_1:     1
    fluxval_1:     V=14.58 +/- 0.02
    fluxnum_2:     2
    fluxval_2:     B-V=0.93

!

    targnum:       25
    name_1:        F193
    descr_1:       A,140
    pos_1:         RA=08H 51M 35.80S+/-0.1",
    pos_2:         DEC=+11D 53' 34.7"+/-0.1",
    pos_3:         PLATE-ID=028I
    equinox:       J2000
    comment_1:     GSC  814  741
    fluxnum_1:     1
    fluxval_1:     V=12.28
    fluxnum_2:     2
    fluxval_2:     B-V=1.0

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       201.000
    sequence_1:    DEFINE
    sequence_2:    VDSP
    targname:      #
    config:        FOS/RD
    opmode:        ACCUM
    aperture:      #
    sp_element:    G570H
    num_exp:       1
    time_per_exp:  300S
    priority:      1
    param_1:       STEP-PATT=SINGLE

!

    linenum:       202.000
    sequence_1:    DEFINE
    sequence_2:    CAL-VD
    targname:      WAVE
    config:        FOS/RD
    opmode:        ACCUM
    aperture:      #
    sp_element:    G570H
    num_exp:       1
    time_per_exp:  DEF
    priority:      1
    param_1:       STEP-PATT=SINGLE

!

    linenum:       203.000
    sequence_1:    DEFINE
    sequence_2:    STAR
    targname:      #
    config:        FOS/RD
    opmode:        ACCUM
    aperture:      #
    sp_element:    G570H
    num_exp:       1
    time_per_exp:  120S
    fluxnum_1:     1
    priority:      1
    param_1:       STEP-PATT=SINGLE

!

    linenum:       204.000
    targname:      NGC224-OFFSET
    config:        FOS/RD
    opmode:        ACQ/BINARY
    aperture:      4.3
    sp_element:    MIRROR
    num_exp:       1
    time_per_exp:  6.0S
    priority:      1
    req_2:         GROUP 204-267 WITHIN 60D;
    req_3:         GROUP 204-261 WITHIN 7D;
    req_4:         GROUP 204-225 NO GAP;
    req_5:         ONBOARD ACQ FOR 205;
    req_6:         CYCLE 2 / 204-267
    comment_1:     LINES 204-261 DEFINE A GRID ON
    comment_2:     THE SKY.  PLEASE SCHEDULE ALL
    comment_3:     OBSERVATIONS AS CLOSE IN TIME
    comment_4:     AS POSSIBLE SO THAT THE SAME
    comment_5:     GUIDE STARS ARE USED FOR ALL
    comment_6:     GSACQS.

!

    linenum:       205.000
    targname:      NGC224-NE1
    config:        FOS/RD
    opmode:        ACQ/PEAK
    aperture:      0.5
    sp_element:    MIRROR
    num_exp:       1
    time_per_exp:  2S
    priority:      1
    param_1:       SEARCH-SIZE = 3,
    param_2:       SCAN-STEP = 0.25
    req_1:         ONBOARD ACQ FOR 206
    comment_1:     DO NOT SPLIT "NO GAP" GROUPS
    comment_2:     FURTHER (IE. DO NOT ADD NEW
    comment_3:     GSACQS).

!

    linenum:       206.000
    targname:      NGC224-NE1
    config:        FOS/RD
    opmode:        ACQ/PEAK
    aperture:      0.3
    sp_element:    MIRROR
    num_exp:       1
    time_per_exp:  5S
    priority:      1
    param_1:       SEARCH-SIZE = 3,
    param_2:       SCAN-STEP = 0.1
    req_1:         ONBOARD ACQ FOR 207-225

!

    linenum:       207.000
    targname:      NGC224-NE1
    config:        FOS/RD
    opmode:        ACQ
    aperture:      4.3
    sp_element:    MIRROR
    num_exp:       1
    time_per_exp:  63S
    priority:      1
    comment_1:     MAKE A PICTURE TO VERIFY
    comment_2:     LOCATION

!

    linenum:       208.000
    sequence_1:    USE VDSP
    targname:      NGC224
    aperture:      0.3
    time_per_exp:  X4.0
    req_1:         SEQ 208-209 NO GAP

!

    linenum:       209.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 208

!

    linenum:       210.000
    sequence_1:    USE VDSP
    targname:      NGC224-NE1
    aperture:      0.3
    time_per_exp:  X4.0
    req_1:         SEQ 210-211 NO GAP

!

    linenum:       211.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 210

!

    linenum:       212.000
    sequence_1:    USE VDSP
    targname:      NGC224-NE2
    aperture:      0.3
    time_per_exp:  X4.334
    req_1:         SEQ 212-213 NO GAP

!

    linenum:       213.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 212

!

    linenum:       214.000
    sequence_1:    USE VDSP
    targname:      NGC224-NE3
    aperture:      0.3
    time_per_exp:  X5.0
    req_1:         SEQ 214-215 NO GAP

!

    linenum:       215.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 214

!

    linenum:       216.000
    sequence_1:    USE VDSP
    targname:      NGC224-NE4
    aperture:      0.5
    time_per_exp:  X3.0
    req_1:         SEQ 216-217 NO GAP

!

    linenum:       217.000
    sequence_1:    USE CAL-VD
    aperture:      0.5
    req_1:         CALIB FOR 216

!

    linenum:       218.000
    sequence_1:    USE VDSP
    targname:      NGC224-SW1
    aperture:      0.3
    time_per_exp:  X4.0
    req_1:         SEQ 218-219 NO GAP

!

    linenum:       219.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 218

!

    linenum:       220.000
    sequence_1:    USE VDSP
    targname:      NGC224-SW2
    aperture:      0.3
    time_per_exp:  X4.334
    req_1:         SEQ 220-221 NO GAP

!

    linenum:       221.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 220

!

    linenum:       222.000
    sequence_1:    USE VDSP
    targname:      NGC224-SW3
    aperture:      0.3
    time_per_exp:  X5.0
    req_1:         SEQ 222-223 NO GAP

!

    linenum:       223.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 222

!

    linenum:       224.000
    sequence_1:    USE VDSP
    targname:      NGC224-SW4
    aperture:      0.5
    time_per_exp:  X3.0
    req_1:         SEQ 224-225 NO GAP

!

    linenum:       225.000
    sequence_1:    USE CAL-VD
    aperture:      0.5
    req_1:         CALIB FOR 224

!

    linenum:       226.000
    targname:      NGC224-OFFSET
    config:        FOS/RD
    opmode:        ACQ/BINARY
    aperture:      4.3
    sp_element:    MIRROR
    num_exp:       1
    time_per_exp:  6.0S
    priority:      1
    req_2:         GROUP 226-243 NO GAP;
    req_3:         ONBOARD ACQ FOR 227

!

    linenum:       227.000
    targname:      NGC224-NE1
    config:        FOS/RD
    opmode:        ACQ/PEAK
    aperture:      0.5
    sp_element:    MIRROR
    num_exp:       1
    time_per_exp:  2S
    priority:      1
    param_1:       SEARCH-SIZE = 3,
    param_2:       SCAN-STEP = 0.25
    req_1:         ONBOARD ACQ FOR 228

!

    linenum:       228.000
    targname:      NGC224-NE1
    config:        FOS/RD
    opmode:        ACQ/PEAK
    aperture:      0.3
    sp_element:    MIRROR
    num_exp:       1
    time_per_exp:  5S
    priority:      1
    param_1:       SEARCH-SIZE = 3,
    param_2:       SCAN-STEP = 0.1
    req_1:         ONBOARD ACQ FOR 229-243

!

    linenum:       229.000
    targname:      NGC224-NE1
    config:        FOS/RD
    opmode:        ACQ
    aperture:      4.3
    sp_element:    MIRROR
    num_exp:       1
    time_per_exp:  63S
    priority:      1
    comment_1:     MAKE A PICTURE TO VERIFY
    comment_2:     LOCATION

!

    linenum:       230.000
    sequence_1:    USE VDSP
    targname:      NGC224-NW1
    aperture:      0.3
    time_per_exp:  X4.334
    req_1:         SEQ 230-231 NO GAP

!

    linenum:       231.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 230

!

    linenum:       232.000
    sequence_1:    USE VDSP
    targname:      NGC224-NW2
    aperture:      0.3
    time_per_exp:  X5.334
    req_1:         SEQ 232-233 NO GAP

!

    linenum:       233.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 232

!

    linenum:       234.000
    sequence_1:    USE VDSP
    targname:      NGC224-NW3
    aperture:      0.3
    time_per_exp:  X6.0
    req_1:         SEQ 234-235 NO GAP

!

    linenum:       235.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 234

!

    linenum:       236.000
    sequence_1:    USE VDSP
    targname:      NGC224-N1
    aperture:      0.3
    time_per_exp:  X4.0
    req_1:         SEQ 236-237 NO GAP

!

    linenum:       237.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 236

!

    linenum:       238.000
    sequence_1:    USE VDSP
    targname:      NGC224-N2
    aperture:      0.3
    time_per_exp:  X4.334
    req_1:         SEQ 238-239 NO GAP

!

    linenum:       239.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 238

!

    linenum:       240.000
    sequence_1:    USE VDSP
    targname:      NGC224-W1
    aperture:      0.3
    time_per_exp:  X4.0
    req_1:         SEQ 240-241 NO GAP

!

    linenum:       241.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 240

!

    linenum:       242.000
    sequence_1:    USE VDSP
    targname:      NGC224-W2
    aperture:      0.3
    time_per_exp:  X4.334
    req_1:         SEQ 242-243 NO GAP

!

    linenum:       243.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 242

!

    linenum:       244.000
    targname:      NGC224-OFFSET
    config:        FOS/RD
    opmode:        ACQ/BINARY
    aperture:      4.3
    sp_element:    MIRROR
    num_exp:       1
    time_per_exp:  6.0S
    priority:      1
    req_2:         GROUP 244-261 NO GAP;
    req_3:         ONBOARD ACQ FOR 245

!

    linenum:       245.000
    targname:      NGC224-NE1
    config:        FOS/RD
    opmode:        ACQ/PEAK
    aperture:      0.5
    sp_element:    MIRROR
    num_exp:       1
    time_per_exp:  2S
    priority:      1
    param_1:       SEARCH-SIZE = 3,
    param_2:       SCAN-STEP = 0.25
    req_1:         ONBOARD ACQ FOR 246

!

    linenum:       246.000
    targname:      NGC224-NE1
    config:        FOS/RD
    opmode:        ACQ/PEAK
    aperture:      0.3
    sp_element:    MIRROR
    num_exp:       1
    time_per_exp:  5S
    priority:      1
    param_1:       SEARCH-SIZE = 3,
    param_2:       SCAN-STEP = 0.1
    req_1:         ONBOARD ACQ FOR 247-261

!

    linenum:       247.000
    targname:      NGC224-NE1
    config:        FOS/RD
    opmode:        ACQ
    aperture:      4.3
    sp_element:    MIRROR
    num_exp:       1
    time_per_exp:  63S
    priority:      1
    comment_1:     MAKE A PICTURE TO VERIFY
    comment_2:     LOCATION

!

    linenum:       248.000
    sequence_1:    USE VDSP
    targname:      NGC224-SE1
    aperture:      0.3
    time_per_exp:  X4.334
    req_1:         SEQ 248-249 NO GAP

!

    linenum:       249.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 248

!

    linenum:       250.000
    sequence_1:    USE VDSP
    targname:      NGC224-SE2
    aperture:      0.3
    time_per_exp:  X5.334
    req_1:         SEQ 250-251 NO GAP

!

    linenum:       251.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 250

!

    linenum:       252.000
    sequence_1:    USE VDSP
    targname:      NGC224-SE3
    aperture:      0.3
    time_per_exp:  X6.0
    req_1:         SEQ 252-253 NO GAP

!

    linenum:       253.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 252

!

    linenum:       254.000
    sequence_1:    USE VDSP
    targname:      NGC224-E1
    aperture:      0.3
    time_per_exp:  X4.0
    req_1:         SEQ 254-255 NO GAP

!

    linenum:       255.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 254

!

    linenum:       256.000
    sequence_1:    USE VDSP
    targname:      NGC224-E2
    aperture:      0.3
    time_per_exp:  X4.334
    req_1:         SEQ 256-257 NO GAP

!

    linenum:       257.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 256

!

    linenum:       258.000
    sequence_1:    USE VDSP
    targname:      NGC224-S1
    aperture:      0.3
    time_per_exp:  X4.0
    req_1:         SEQ 258-259 NO GAP

!

    linenum:       259.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 258

!

    linenum:       260.000
    sequence_1:    USE VDSP
    targname:      NGC224-S2
    aperture:      0.3
    time_per_exp:  X4.334
    req_1:         SEQ 260-261 NO GAP

!

    linenum:       261.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 260

!

    linenum:       262.000
    targname:      F193
    config:        FOS/RD
    opmode:        ACQ/BINARY
    aperture:      4.3
    sp_element:    MIRROR
    num_exp:       1
    time_per_exp:  0.73S
    priority:      1
    req_1:         GROUP 262-267 NO GAP;
    req_2:         ONBOARD ACQ FOR 263

!

    linenum:       263.000
    targname:      F193
    config:        FOS/RD
    opmode:        ACQ/PEAK
    aperture:      0.3
    sp_element:    MIRROR
    num_exp:       1
    time_per_exp:  0.2S
    priority:      1
    param_1:       SEARCH-SIZE = 3,
    param_2:       SCAN-STEP = 0.1
    req_1:         ONBOARD ACQ FOR 264-267

!

    linenum:       264.000
    sequence_1:    USE STAR
    targname:      F193
    aperture:      0.3
    time_per_exp:  X1.0
    req_1:         SEQ 264-265 NO GAP;
    req_2:         CALIB FOR 204-261

!

    linenum:       265.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 264

!

    linenum:       266.000
    sequence_1:    USE STAR
    targname:      F193
    aperture:      0.5
    time_per_exp:  X1.0
    req_1:         SEQ 266-267 NO GAP;
    req_2:         CALIB FOR 204-261

!

    linenum:       267.000
    sequence_1:    USE CAL-VD
    aperture:      0.5
    req_1:         CALIB FOR 266

!
! end of exposure logsheet

! No scan data records found