! Hubble Space Telescope Cycle 5 (1995) Phase II Proposal Template
! $Id: 5808,v 1.1 1994/12/14 19:28:26 pepsa Exp $
!
!   Refer to the HST Phase II Proposal Instructions to fill this out
!
!   Anything after a "!" is ignored, and may be deleted
!
!   All keywords with multiple entries are comma delimited except the
!   Visit_Requirements and Special_Requirements keywords which can be
!   delimited with carriage returns or semi-colons, but not commas
!
! For help call your Program Coordinator: n/a
!             Phone: n/a             , E-mail: n/a
!
! This partially completed template was generated from a Phase I proposal.
! Name of Phase I Proposal: plavec-042.prop
! Date generated: Wed Dec 14 14:28:19 EST 1994
!

Proposal_Information                           ! Section 4
              Title:  Symbiotic Binaries: Nature of the Hot
                      Components
  Proposal_Category:  AR
Scientific_Category:  Hot Stars
             Cycle:    5

Investigators
     PI_name:         Mirek Plavec
     PI_Institution:  University of California, Los Angeles

          CoI_Name:   Charles Keyes
   CoI_Institution:   Space Telescope Science Institute
           Contact:             ! Y or N (designate at most one contact)

          CoI_Name:   Ivan Hubeny
   CoI_Institution:   USRA, NASA Goddard Space Flight Center,
                      Greenbelt
           Contact:             ! Y or N (designate at most one contact)


Abstract:                                ! Free format text (please update)
    We propose to rediscuss the existing HST observations of two
    symbiotic binaries, namely AG Pegasi and CI Cygni. These
    spectra were obviously taken for the purpose of studying the
    emission lines, typical for such systems; also, many spectra
    of AG Pegasi were obtained for calibration purposes. We
    propose to use this material primarily for an investigation of
    the continuous and absorption-line spectra, which should
    enable us to decide upon the nature of the hot components in
    these two binaries. This project parallels our own observing
    proposal, originally submitted for Cycle 3 and accepted by the
    TAC as supplemental (but not realized), and re-submitted now
    for Cycle 5 under the title ``Nature of the Hot Components of
    Symbiotic Binaries''. The spectra of AG Pegasi, taken for
    wavelength calibration, are of very good quality, and are
    usable for the study of the continuum and probably also of the
    absorption lines. We will attempt to extract as much
    information from all the existing spectra as we can for our
    modeling of the hot components. These can be either accreting
    white degenerate dwarfs, subdwarfs akin to the nuclei of
    planetary nebulae, or accretion disks surrounding non-
    degenerate low-mass stars. In the past, only indirect or
    insufficient clues have been used to resolve this question. We
    also plan to study the emission line profiles in order to
    understand their origin. We possess state-of-the-art modeling
    techniques for stellar atmospheres, accretion disks, and
    emission lines.

Questions                       ! Free format text (please update)

     Observing_Description:

   Real_Time_Justification:



Calibration_Justification:              ! Move appropriate text from Real_Time_Justification

      Additional_Comments:


Fixed_Targets                           ! Section 5.1
  Target_Number:
    Target_Name:
Alternate_Names:
    Description:
       Position:                        ! Most common specification format is
                                        ! RA=0H 0M 0.00S +/- 0S,
                                        ! DEC=0D 0' 0.0" +/- 0",
                                        ! PLATE-ID=0000
        Equinox:
        RV_or_Z:
          RA_PM:                        ! Units are seconds of time per year
         Dec_PM:                        ! Units are seconds of arc per year
          Epoch:
Annual_Parallax:
           Flux:                        ! Include at least V and B-V
       Comments:


Solar_System_Targets                    ! Section 5.2
  Target_Number:
    Target_Name:
    Description:
        Level_1:                        ! Satellite of Sun
        Level_2:                        ! Satellite of Level_1
        Level_3:                        ! Satellite of Level_2
         Window:
           Flux:                        ! Include at least V and B-V
       Comments:


Generic_Targets                         ! Section 5.3
  Target_Number:
    Target_Name:
    Description:
       Criteria:
           Flux:
       Comments:


Scan_Data                               ! Appendix B
    Scan_Number:
       FGS_Scan:
  Cont_or_Dwell:
   Dwell_Points:
     Dwell_Secs:
     Scan_Width:
    Scan_Length:
    Sides_Angle:
   Number_Lines:
      Scan_Rate:
  First_Line_PA:
     Scan_Frame:
  Length_Offset:
   Width_Offset:


! This is a template for a single visit containing a single exposure
! Repeat exposure and visit blocks as needed

Visits                                  ! Section 6
      Visit_Number:
Visit_Requirements:                     ! Section 7.1

! Uncomment or copy visit level special requirements needed
! Most of these requirements (including ORIENT) will limit scheduling

        ! PCS MODE [Fine | Gyro]
        ! GUIDing TOLerance <angle>
        ! ORIENTation <angle1> TO <angle2>
        ! ORIENTation <angle1> TO <angle2> FROM <visit>
        ! ORIENTation <angle1> TO <angle2> FROM NOMINAL
        ! SAME ORIENTation AS <visit>
        ! CVZ
        ! PARallel
        ! AFTER <visit> [BY <time1> [TO <time2>]]
        ! AFTER <date>
        ! BEFORE <date>
        ! BETWEEN <date1> AND <date2>
        ! GROUP <visit-list> WITHIN <time>
        ! PERIOD <time> AND ZERO-PHASE <date>
        ! SEQ <visit-list> WITHIN <time>
        ! ON HOLD [FOR <visit>]

  On_Hold_Comments:
    Visit_Comments:

     Exposure_Number:                   ! Section 6.5
         Target_Name:
              Config:
              Opmode:
            Aperture:
          Sp_Element:
          Wavelength:
 Optional_Parameters:
Number_of_Iterations:
   Time_Per_Exposure:
Special_Requirements:                   ! Section 7.2

! Uncomment or copy exposure level special requirements needed

        ! INTeractive ACQuisition FOR <exp-list>
        ! ONBOARD ACQuisition FOR <exp-list>
        ! POSition TARGet <x-value>,<y-value>
        ! SAME POSition AS <exp>
        ! DO FOR TARGets <targ-list>    ! FGS only
        ! PARallel WITH <exp>
        ! GROUP-FGS <exp-list> WITHIN <time>
        ! SPATIAL SCAN <#> [<exp-list> | SINGLE-EXP ]
        ! RT ANALYSIS [FOR <exp-list>]
        ! REQuires UPLINK
        ! DARK TIME
        ! END ORBIT
        ! EXPAND
        ! MAXimum DURation [<time> | <%>]
        ! MINimum DURation [<time> | <%>]
        ! NO SPLIT
        ! PHASE <number1[0,1]> TO <number2[0,1]>
        ! SEQuence <exp-list> NON-INTerruptible

            Comments:

Data_Distribution                       ! Defaults indicated; change if desired

         Medium:        8MM             ! 8MM or 6250BPI or 1600BPI
Blocking_Factor:        10              ! 10 or 1
                                        ! Only astronomers with very old 9-
                                        ! track tape drives should consider
                                        ! a blocking factor of 1

        Ship_To:        PI_Address      ! STSCI or PI_Address or <free-text>
                                        ! PI Address from Phase I is:
                                        !
                                                 !  Los Angeles, CA 90024-1562
                                        !
                                        !
       Ship_Via:        UPS             ! UPS (2-day) or OVERNIGHT
                                        ! Overnight shipping done at PI expense

Recipient_Email:                        ! Needed if Ship_To: is not PI_Address
                                        ! <free-text>

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! Please send a list of your likes and dislikes to your Program Coordinator