!  File:  4830C.PROP
!  Database:  PEPDB
!  Date:  23-FEB-1994:05:18:10

coverpage:

  title_1:         STELLAR AND GAS DYNAMICS IN NORMAL GALAXIES AUGMENTATION:
    title_2:       -CYC3HIGH
    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:     10.90
    num_pri:       10
    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_1:         RA=00H 42M 44.3303S +/- 0.3",
    pos_2:         DEC=+41D 16' 08.972" +/- 0.3",
    pos_3:         PLATE-ID=01JV
    equinox:       J2000
    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",
    pos_2:         PA=45D,
    pos_3:         FROM 1
    equinox:       J2000
    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",
    pos_2:         PA=45D,
    pos_3:         FROM 1
    equinox:       J2000
    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",
    pos_2:         PA=45D,
    pos_3:         FROM 1
    equinox:       J2000
    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",
    pos_2:         PA=45D,
    pos_3:         FROM 1
    equinox:       J2000
    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",
    pos_2:         PA=225D,
    pos_3:         FROM 1
    equinox:       J2000
    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",
    pos_2:         PA=225D,
    pos_3:         FROM 1
    equinox:       J2000
    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",
    pos_2:         PA=225D,
    pos_3:         FROM 1
    equinox:       J2000
    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",
    pos_2:         PA=225D,
    pos_3:         FROM 1
    equinox:       J2000
    fluxnum_1:     1
    fluxval_1:     F(5470)=7.7E-16

!

    targnum:       10
    name_1:        NGC224-OFFSET
    descr_1:       A,140
    pos_1:         RA-OFF=4.4547S +/- 0.0018S,
    pos_2:         DEC-OFF=-55.392" +/- 0.02",
    pos_3:         FROM 1
    equinox:       J2000
    fluxnum_1:     1
    fluxval_1:     V=14.58 +/- 0.02
    fluxnum_2:     2
    fluxval_2:     B-V=0.93

!

    targnum:       11
    name_1:        F193
    descr_1:       A,140
    pos_1:         RA=08H 51M 35.80S+/-0.2",
    pos_2:         DEC=+11D 53' 34.7"+/-0.2",
    pos_3:         PLATE-ID=028I
    equinox:       J2000
    comment_1:     GSC 0081400741
    fluxnum_1:     1
    fluxval_1:     V=12.28
    fluxnum_2:     2
    fluxval_2:     B-V=1.0

!

    targnum:       12
    name_1:        F193-N
    descr_1:       A,140
    pos_1:         R=0.125",
    pos_2:         PA=0D,
    pos_3:         FROM 11
    equinox:       J2000

!

    targnum:       13
    name_1:        F193-S
    descr_1:       A,140
    pos_1:         R=0.125",
    pos_2:         PA=180D,
    pos_3:         FROM 11
    equinox:       J2000

!

    targnum:       14
    name_1:        F193-E
    descr_1:       A,140
    pos_1:         R=0.125",
    pos_2:         PA=90D,
    pos_3:         FROM 11
    equinox:       J2000

!

    targnum:       15
    name_1:        F193-W
    descr_1:       A,140
    pos_1:         R=0.125",
    pos_2:         PA=270D,
    pos_3:         FROM 11
    equinox:       J2000

!

    targnum:       16
    name_1:        M67-I17
    descr_1:       A,140
    pos_1:         RA=08H 51M 08.39S+/-0.1",
    pos_2:         DEC=+11D 47' 21.1"+/-0.1",
    pos_3:         PLATE-ID=028I
    equinox:       J2000
    comment_1:     GSC0081401657
    fluxnum_1:     1
    fluxval_1:     V=12.4 +/- 0.4
    fluxnum_2:     2
    fluxval_2:     B-V=1.0

!

    targnum:       17
    name_1:        M67-I17-N
    descr_1:       A,140
    pos_1:         R=0.125",
    pos_2:         PA=0D,
    pos_3:         FROM 16
    equinox:       J2000

!

    targnum:       18
    name_1:        M67-I17-S
    descr_1:       A,140
    pos_1:         R=0.125",
    pos_2:         PA=180D,
    pos_3:         FROM 16
    equinox:       J2000

!

    targnum:       19
    name_1:        M67-I17-E
    descr_1:       A,140
    pos_1:         R=0.125",
    pos_2:         PA=90D,
    pos_3:         FROM 16
    equinox:       J2000

!

    targnum:       20
    name_1:        M67-I17-W
    descr_1:       A,140
    pos_1:         R=0.125",
    pos_2:         PA=270D,
    pos_3:         FROM 16
    equinox:       J2000

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       301.000
    sequence_1:    DEFINE
    sequence_2:    VDSP
    targname:      #
    config:        FOS/RD
    opmode:        ACCUM
    aperture:      #
    sp_element:    G570H
    num_exp:       1
    time_per_exp:  345S
    priority:      1
    param_1:       STEP-PATT=SINGLE

!

    linenum:       302.000
    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:       303.000
    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:       304.000
    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_1:         GROUP 304-353 WITHIN 60D;
    req_2:         GROUP 304-325 NO GAP;
    req_3:         ONBOARD ACQ FOR 305;
    req_4:         CYCLE 3 / 304-353
    comment_1:     LINES 304-325 DEFINE A GRID ON
    comment_2:     THE SKY.  DO NOT SPLIT "NO GAP"
    comment_3:     GROUPS FURTHER (IE. DO NOT ADD
    comment_4:     NEW GSACQS).

!

    linenum:       305.000
    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-X=3,
    param_2:       SCAN-STEP-X=0.25,
    param_3:       SEARCH-SIZE-Y=3,
    param_4:       SCAN-STEP-Y=0.25
    req_1:         ONBOARD ACQ FOR 306;

!

    linenum:       306.000
    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-X=3,
    param_2:       SCAN-STEP-X=0.1,
    param_3:       SEARCH-SIZE-Y=3,
    param_4:       SCAN-STEP-Y=0.1
    req_1:         ONBOARD ACQ FOR 307-325

!

    linenum:       307.000
    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:       308.000
    sequence_1:    USE VDSP
    targname:      NGC224
    aperture:      0.3
    time_per_exp:  X4.0
    req_1:         SEQ 308-309 NO GAP

!

    linenum:       309.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 308

!

    linenum:       310.000
    sequence_1:    USE VDSP
    targname:      NGC224-NE1
    aperture:      0.3
    time_per_exp:  X4.0
    req_1:         SEQ 310-311 NO GAP

!

    linenum:       311.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 310

!

    linenum:       312.000
    sequence_1:    USE VDSP
    targname:      NGC224-NE2
    aperture:      0.3
    time_per_exp:  X4.334
    req_1:         SEQ 312-313 NO GAP

!

    linenum:       313.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 312

!

    linenum:       314.000
    sequence_1:    USE VDSP
    targname:      NGC224-NE3
    aperture:      0.3
    time_per_exp:  X5.0
    req_1:         SEQ 314-315 NO GAP

!

    linenum:       315.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 314

!

    linenum:       316.000
    sequence_1:    USE VDSP
    targname:      NGC224-NE4
    aperture:      0.5
    time_per_exp:  X3.0
    req_1:         SEQ 316-317 NO GAP

!

    linenum:       317.000
    sequence_1:    USE CAL-VD
    aperture:      0.5
    req_1:         CALIB FOR 316

!

    linenum:       318.000
    sequence_1:    USE VDSP
    targname:      NGC224-SW1
    aperture:      0.3
    time_per_exp:  X4.0
    req_1:         SEQ 318-319 NO GAP

!

    linenum:       319.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 318

!

    linenum:       320.000
    sequence_1:    USE VDSP
    targname:      NGC224-SW2
    aperture:      0.3
    time_per_exp:  X4.334
    req_1:         SEQ 320-321 NO GAP

!

    linenum:       321.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 320

!

    linenum:       322.000
    sequence_1:    USE VDSP
    targname:      NGC224-SW3
    aperture:      0.3
    time_per_exp:  X5.0
    req_1:         SEQ 322-323 NO GAP

!

    linenum:       323.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 322

!

    linenum:       324.000
    sequence_1:    USE VDSP
    targname:      NGC224-SW4
    aperture:      0.5
    time_per_exp:  X3.0
    req_1:         SEQ 324-325 NO GAP

!

    linenum:       325.000
    sequence_1:    USE CAL-VD
    aperture:      0.5
    req_1:         CALIB FOR 324

!

    linenum:       326.000
    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 326-339 NO GAP;
    req_2:         ONBOARD ACQ FOR 327

!

    linenum:       327.000
    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-X=3,
    param_2:       SCAN-STEP-X=0.1,
    param_3:       SEARCH-SIZE-Y=3,
    param_4:       SCAN-STEP-Y=0.1
    req_1:         ONBOARD ACQ FOR 328-339

!

    linenum:       328.000
    sequence_1:    USE STAR
    targname:      F193
    aperture:      0.3
    time_per_exp:  X5.0
    req_1:         SEQ 328-329 NO GAP;
    req_2:         CALIB FOR 304-325

!

    linenum:       329.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 328

!

    linenum:       330.000
    sequence_1:    USE STAR
    targname:      F193
    aperture:      0.5
    time_per_exp:  X1.5
    req_1:         SEQ 330-331 NO GAP;
    req_2:         CALIB FOR 304-325

!

    linenum:       331.000
    sequence_1:    USE CAL-VD
    aperture:      0.5
    req_1:         CALIB FOR 330

!

    linenum:       332.000
    sequence_1:    USE STAR
    targname:      F193-N
    aperture:      0.5
    time_per_exp:  X1.5
    req_1:         SEQ 332-333 NO GAP;
    req_2:         CALIB FOR 304-325

!

    linenum:       333.000
    sequence_1:    USE CAL-VD
    aperture:      0.5
    req_1:         CALIB FOR 332

!

    linenum:       334.000
    sequence_1:    USE STAR
    targname:      F193-S
    aperture:      0.5
    time_per_exp:  X1.5
    req_1:         SEQ 334-335 NO GAP;
    req_2:         CALIB FOR 304-325

!

    linenum:       335.000
    sequence_1:    USE CAL-VD
    aperture:      0.5
    req_1:         CALIB FOR 334

!

    linenum:       336.000
    sequence_1:    USE STAR
    targname:      F193-E
    aperture:      0.5
    time_per_exp:  X1.5
    req_1:         SEQ 336-337 NO GAP;
    req_2:         CALIB FOR 304-325

!

    linenum:       337.000
    sequence_1:    USE CAL-VD
    aperture:      0.5
    req_1:         CALIB FOR 336

!

    linenum:       338.000
    sequence_1:    USE STAR
    targname:      F193-W
    aperture:      0.5
    time_per_exp:  X1.5
    req_1:         SEQ 338-339 NO GAP;
    req_2:         CALIB FOR 304-325

!

    linenum:       339.000
    sequence_1:    USE CAL-VD
    aperture:      0.5
    req_1:         CALIB FOR 338

!

    linenum:       340.000
    targname:      M67-I17
    config:        FOS/RD
    opmode:        ACQ/BINARY
    aperture:      4.3
    sp_element:    MIRROR
    num_exp:       1
    time_per_exp:  0.82S
    priority:      1
    req_1:         GROUP 340-353 NO GAP;
    req_2:         ONBOARD ACQ FOR 341

!

    linenum:       341.000
    targname:      M67-I17
    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-X=3,
    param_2:       SCAN-STEP-X=0.1,
    param_3:       SEARCH-SIZE-Y=3,
    param_4:       SCAN-STEP-Y=0.1
    req_1:         ONBOARD ACQ FOR 342-353

!

    linenum:       342.000
    sequence_1:    USE STAR
    targname:      M67-I17
    aperture:      0.3
    time_per_exp:  X5.0
    req_1:         SEQ 342-343 NO GAP;
    req_2:         CALIB FOR 304-325

!

    linenum:       343.000
    sequence_1:    USE CAL-VD
    aperture:      0.3
    req_1:         CALIB FOR 342

!

    linenum:       344.000
    sequence_1:    USE STAR
    targname:      M67-I17
    aperture:      0.5
    time_per_exp:  X1.5
    req_1:         SEQ 344-345 NO GAP;
    req_2:         CALIB FOR 304-325

!

    linenum:       345.000
    sequence_1:    USE CAL-VD
    aperture:      0.5
    req_1:         CALIB FOR 344

!

    linenum:       346.000
    sequence_1:    USE STAR
    targname:      M67-I17-N
    aperture:      0.5
    time_per_exp:  X1.5
    req_1:         SEQ 346-347 NO GAP;
    req_2:         CALIB FOR 304-325

!

    linenum:       347.000
    sequence_1:    USE CAL-VD
    aperture:      0.5
    req_1:         CALIB FOR 346

!

    linenum:       348.000
    sequence_1:    USE STAR
    targname:      M67-I17-S
    aperture:      0.5
    time_per_exp:  X1.5
    req_1:         SEQ 348-349 NO GAP;
    req_2:         CALIB FOR 304-325

!

    linenum:       349.000
    sequence_1:    USE CAL-VD
    aperture:      0.5
    req_1:         CALIB FOR 348

!

    linenum:       350.000
    sequence_1:    USE STAR
    targname:      M67-I17-E
    aperture:      0.5
    time_per_exp:  X1.5
    req_1:         SEQ 350-351 NO GAP;
    req_2:         CALIB FOR 304-325

!

    linenum:       351.000
    sequence_1:    USE CAL-VD
    aperture:      0.5
    req_1:         CALIB FOR 350

!

    linenum:       352.000
    sequence_1:    USE STAR
    targname:      M67-I17-W
    aperture:      0.5
    time_per_exp:  X1.5
    req_1:         SEQ 352-353 NO GAP;
    req_2:         CALIB FOR 304-325

!

    linenum:       353.000
    sequence_1:    USE CAL-VD
    aperture:      0.5
    req_1:         CALIB FOR 352

!
! end of exposure logsheet

! No scan data records found