!  File:  1149C.PROP
!  Database:  PEPDB
!  Date:  16-FEB-1994:03:39:38

coverpage:

  title_1:         HR DEL PHASE DEPENDENT WIND
    sci_cat:       STELLAR ASTROPHYSICS
    sci_subcat:    SUBLUMINOUS STARS
    proposal_for:  GTO/HRS
    pi_title:      PROF.
    pi_fname:      JOHN
    pi_mi:         B.
    pi_lname:      HUTCHINGS
    pi_inst:       DOMINION ASTROPHYSICAL OBSERVATORY
    pi_country:    CANADA
    pi_phone:      (604) 363-0018
    keywords_1:    CATACLYSMIC VARIABLE, MASS-LOSS, STELLAR WIND, OLD
    keywords_2:    NOVA, UV SPECTROSCOPY
    hours_pri:     0.75
    num_pri:       1
    pi_position:   PROFESSOR
! end of coverpage

abstract:

    line_1:        The CIV lambda1550 resonance line will be observed at medium HRS resolution,
    line_2:        at 5 orbital phases, to study the phase dependence of the wind from the system.
    line_3:        Low resolution IUE data have shown that a wind is seen in the star, with
    line_4:        apparent but unresolved changes in an orbit. The data will be used in
    line_5:        understanding mass flows in a CV binary system viewed at a known angle.

!
! end of abstract

general_form_proposers:

  lname:           HUTCHINGS
    fname:         JOHN
    mi:            B.
    inst:          DOMINION ASTROPHYSICAL OBSERVATORY
    country:       CANADA

!
! end of general_form_proposers block

general_form_text:

  question:        3
    section:       1
    line_1:        A series of four-minute integrations is requested on HR Del at lambda1550.
    line_2:        These exposures should all occur within as few orbital cycles as possible to
    line_3:        avoid confusion by changes which are not phase related. We request as even as
    line_4:        possible spacing in phase of ~0.25, with one overlap phase monitor
    line_5:        non-phase-dependent changes.
    line_7:        One 5 minute WFC camera image will be taken, presumably adjacent to one of the
    line_8:        spectroscopic exposures, with the F492M filter.
    line_10:       Observations to be made in Cycle 2.

!

  question:        4
    section:       1
    line_1:        ST with HRS is the only way to obtain UV spectra with derived spectral and
    line_2:        time resolution. WFC will provide unprecedented spatial reolution of the
    line_3:        nebula.

!

  question:        5
    section:       1
    line_1:        Target orbital phasing is an essential part of the spectroscopic program.
    line_2:        Image timing is not important.

!

  question:        7
    section:       1
    line_1:        All data will be reduced with DAO equipment and software. Analysis will
    line_2:        include some modelling of the CIV line profiles.

!

  question:        10
    section:       1
    line_1:        All software, computing and personnel support.

!

  question:        13
    section:       1
    line_1:        5 observations will be made of CIV lambda1550 at E+4 resolution of HR Del. The
    line_2:        data will cover intervals of ~0.25 in orbital phase, with one repeat, to
    line_3:        monitor non-phase related profile changes. Data will be obtained within a few
    line_4:        orbital cycles.

!
!end of general form text

general_form_address:

  lname:           HUTCHINGS
    fname:         JOHN
    mi:            B.
    title:         PROF.
    category:      PI
    inst:          DOMINION ASTROPHYSICAL OBSERVATORY
    addr_1:        5071 W. SAANICH RD.
    addr_2:        V8X 4M6
    city:          VICTORIA
    state:         BC
    country:       CANADA
    phone:         (604) 363-0018
    telex:         049-7295

!
! end of general_form_address records

fixed_targets:

    targnum:       1
    name_1:        HR-DEL
    descr_1:       CATACLYSMIC VARIABLE (OLD NOVA)
    pos_1:         RA = 20H 40M 04.2S +/- 1",
    pos_2:         DEC = +18D 58'51" +/- 1"
    equinox:       1950
    comment_1:     UV FLUX KNOWN FROM IUE DATA

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       1.000
    targname:      HR-DEL
    config:        HRS
    opmode:        ACQ
    aperture:      2.0
    sp_element:    MIRROR-A2
    num_exp:       1
    time_per_exp:  1.8S
    priority:      2
    req_1:         ONBOARD ACQ FOR 2-6; CYCLE 2 /1-7

!

    linenum:       2.000
    targname:      ^
    config:        ^
    opmode:        ACCUM
    aperture:      2.0
    sp_element:    G160M
    wavelength:    1545
    num_exp:       ^
    time_per_exp:  4M
    priority:      ^
    req_1:         PERIOD 0.214167D +/- 0.000001D;
    req_2:         ZERO-PHASE JD2443322.3 +/- 1.0D;
    req_3:         PHASE 0.0 +/- 0.05

!

    linenum:       3.000
    targname:      ^
    config:        ^
    opmode:        ^
    aperture:      ^
    sp_element:    ^
    wavelength:    ^
    num_exp:       ^
    time_per_exp:  ^
    priority:      ^
    req_1:         PERIOD 0.214167D +/- 0.000001D;
    req_2:         ZERO-PHASE JD2443322.3 +/- 1.0D;
    req_3:         PHASE 0.25 +/- 0.05

!

    linenum:       4.000
    targname:      ^
    config:        ^
    opmode:        ^
    aperture:      ^
    sp_element:    ^
    wavelength:    ^
    num_exp:       ^
    time_per_exp:  ^
    priority:      ^
    req_1:         PERIOD 0.214167D +/- 0.000001D;
    req_2:         ZERO-PHASE JD2443322.3 +/- 1.0D;
    req_3:         PHASE 0.50 +/- 0.05

!

    linenum:       5.000
    targname:      ^
    config:        ^
    opmode:        ^
    aperture:      ^
    sp_element:    ^
    wavelength:    ^
    num_exp:       ^
    time_per_exp:  ^
    priority:      ^
    req_1:         PERIOD 0.214167D +/- 0.000001D;
    req_2:         ZERO-PHASE JD2443322.3 +/- 1.0D;
    req_3:         PHASE 0.75 +/- 0.05

!

    linenum:       6.000
    targname:      ^
    config:        ^
    opmode:        ^
    aperture:      ^
    sp_element:    ^
    wavelength:    ^
    num_exp:       ^
    time_per_exp:  ^
    priority:      ^
    req_1:         PERIOD 0.214167D +/- 0.000001D;
    req_2:         ZERO-PHASE JD2443322.3 +/- 1.0D;
    req_3:         PHASE 0.0 +/- 0.05;
    req_4:         GROUP 2-6 WITHIN 4D

!

    linenum:       7.000
    targname:      ^
    config:        WFC
    opmode:        IMAGE
    aperture:      ALL
    sp_element:    F492M
    num_exp:       ^
    time_per_exp:  5M
    priority:      ^
    comment_1:     ZERO-PHASE IS ARBITRARY. 6 AND 2 AT
    comment_2:     SAME PHASE, BUT DIFFERENT CYCLES.

!
! end of exposure logsheet

! No scan data records found