!  File:  4026C.PROP
!  Database:  PEPDB
!  Date:  20-FEB-1994:04:15:03

coverpage:

  title_1:         STUDY OF OPTICAL EMISSION ASSOCIATED WITH RADIO JETS
    title_2:       AND HOT SPOTS -- REPEAT FOR HOPR#0013
    sci_cat:       QUASARS & AGN
    sci_subcat:    JETS
    proposal_for:  RPT/FOC
    cont_id:       1228
    pi_fname:      F. DUCCIO
    pi_lname:      MACCHETTO
    pi_inst:       ESA, SPACE TELESCOPE SCIENCE INSTITUTE
    pi_country:    USA
    pi_phone:      301-338-4790
    keywords_1:    AGN, RADIOEMISSION, JETS
    hours_pri:     1.00
    num_pri:       3
    foc:           X
    pi_position:   DIVISION HEAD, SPD
    off_fname:     F
    off_lname:     MACCHETTO
! end of coverpage

abstract:

    line_1:        ST is uniquely equipped to detect optical emission from synchroton jets and to
    line_2:        study the interaction of jets with their environment. Here we outline a
    line_3:        program of broad and narrow band imaging and limited slit spectroscopy on
    line_4:        carefully selected samples of objects designed to exploit ST for these
    line_5:        purposes. The aims are to study the following:
    line_7:        -morphological relations between radio and optical emission.
    line_8:        -optical and UV counterparts of radio jets and hot spots to derive information
    line_9:        on particle acceleration mechanisms.
    line_10:       -interactions between synchroton jets and in the ambient gas, to use each as a
    line_11:       unique probe of the physical conditions within the other.
    line_12:       -possible relationship between the propagation of radio jets and star
    line_13:       formation.

!
! end of abstract

general_form_proposers:

  lname:           MILEY
    fname:         GEORGE
    mi:            K.
    inst:          SPACE TELESCOPE SCIENCE INSTITUTE
    country:       USA
    esa:           X

!

  lname:           CRANE
    fname:         PHILIPPE
    inst:          EUROPEAN SOUTHERN OBSERVATORY
    country:       GERMANY, WEST
    esa:           X

!

  lname:           MACCHETTO
    fname:         F. DUCCIO
    inst:          ESA, SPACE TELESCOPE SCIENCE INSTITUTE
    country:       USA
    esa:           X

!
! end of general_form_proposers block

general_form_text:

  question:        3
    section:       1
    line_1:        Observations for Cycle 0 are those in Exposure Logsheet Nos:
    line_2:        11,15,20,21,25,26,29,30,39,41,42,51,55,56,58,59,60,62,64,77,79,80,81,85,88,102,
    line_4:        103,104.105,108,109,111,115,117,118,120,121,123,127,129,131,133,134,135,150,
    line_6:        157,158,165
    line_8:        The total duration of these observations shall be 6.5 hours.
    line_9:        All other observations will be done in subsequent cycles.

!

  question:        12
    section:       1
    line_1:        1) Exposure times and filters may be changed after initial observations and
    line_2:        SV experience.
    line_4:        2) PA is only an indication of the radio-orientation of greatest interest.
    line_5:        It should not constrain scheduling.
    line_7:        3) 21.2% of the time for this program is to be charged to P. Crane's CTO
    line_8:        allocation.
    line_10:       78.8% of the time for this program is to be charged to the FOC-IDT GTO
    line_11:       allocation.

!

  question:        13
    section:       1
    line_1:        ST is uniquely equipped to detect optical emission from synchrotron jets and to
    line_2:        study the interaction of jets with their environment. Here we outline a
    line_3:        program of broad and narrow band imaging and limited slit spectroscopy on
    line_4:        carefully selected sample of objects designed to exploit ST for these purposes.
    line_5:        The aims are to study the following:
    line_6:        - morphological relations between radio and optical emission
    line_7:        - optical and UV counterparts of radio jets and hot spots to derive
    line_8:        information on particle acceleration mechanisms
    line_9:        - interactions between synchrotron jets and the ambient gas, to use each
    line_10:       as a unique probe of the physical conditions within the other
    line_11:       - possible relationship between the propagation of radio jets and star
    line_12:       formation

!
!end of general form text

general_form_address:

  lname:           MACCHETTO
    fname:         F. DUCCIO
    category:      PI
    inst:          ESA, SPACE TELESCOPE SCIENCE INSTITUTE
    addr_1:        3700 SAN MARTIN DRIVE
    city:          BALTIMORE
    state:         MD
    zip:           21218
    country:       USA
    phone:         301-338-4790

!
! end of general_form_address records

fixed_targets:

    targnum:       39
    name_1:        M87N
    name_2:        VIRGOA
    name_3:        3C274
    descr_1:       RADIO JET (NUCLEUS)
    pos_1:         RA = 12H 28M 17.55S +/- 0.1S,
    pos_2:         DEC = +12D 40' 01.80" +/- 1"
    equinox:       1950
    pm_or_par:     NO
    rv_or_z:       Z=0.0043
    acqpr_1:       EXT
    plate_req:     N
    comment_1:     PA=-70D
    fluxval_1:     V = 8.74

!
! end of fixed targets

! No solar system records found

! No generic target records found

exposure_logsheet:

    linenum:       114.200
    targname:      M87N
    config:        FOC/96
    opmode:        IMAGE
    aperture:      512X512
    sp_element:    F550M
    num_exp:       2
    time_per_exp:  20M
    priority:      1
    req_1:         CYCLE 1

!

    linenum:       114.300
    targname:      M87N
    config:        FOC/96
    opmode:        IMAGE
    aperture:      512X512
    sp_element:    F502M
    num_exp:       2
    time_per_exp:  20M
    priority:      1
    req_1:         CYCLE 1

!

    linenum:       117.000
    targname:      M87N
    config:        FOC/96
    opmode:        IMAGE
    aperture:      512X512
    sp_element:    F501N
    num_exp:       2
    time_per_exp:  20M
    priority:      1
    req_1:         CYCLE 1

!
! end of exposure logsheet

! No scan data records found