Astronomical Data Center

ADCADC/CDS Standard Document for Catalog:
/journal_tables/AJ/109/1352/

The following is the "ReadMe" document that describes this ADC catalog. You can access the files described here in three ways:

1. Use the ADC Data Viewer Suite to visualize the data. [preview
2. Get the data files via anonymous FTP. (See Note.) [ftp


J/AJ/109/1352       Stellar occultation candidates    (McDonald+ 1995)
================================================================================
Triton stellar occultation candidates: 1995-1999
     McDonald S.W., Elliot J.L.
    <Astron. J. 109, 1352 (1995)>
    =1995AJ....109.1352M      (SIMBAD/NED BibCode)
================================================================================
ADC_Keywords: Occultations ; Positional data

Abstract:
    We have completed a search for candidates for stellar occultations by
    Triton over the years 1995-1999 CCD strip scan images provided star
    positions in the relevant sky area to a depth of about 17.5Rmag. Over
    this time period, we find that Triton passes within 1.0arcsec of 75
    stars. Appulses with geocentric minimum separations of less than
    0.35arcsec will result in stellar occultations, but further astrometry
    and photometry is necessary to refine individual predictions for
    identification of actual occultations. Finder charts are included to
    aid in further studies and prediction refinement. The two most
    promising potential occultations, Tr176 and Tr180, occur in 1997.

File Summary:
--------------------------------------------------------------------------------
  FileName      Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe             80        .   This file
table2             95       75   Possible occultations by Triton
--------------------------------------------------------------------------------

See also:
  J/AJ/104/862 : Stellar occultation candidates (McDonald+ 1992)

Byte-by-byte Description of file: table2
--------------------------------------------------------------------------------
   Bytes Format   Units    Label   Explanations
--------------------------------------------------------------------------------
   1-  5  A5      ---      ID      Star name
   7- 14  A8   "DD/MM/YY"  AppDate Date of the closest approach
  16- 17  I2      h        Apph    UT time of the closest approach
  19- 20  I2      min      Appm    UT time of the closest approach
  22- 25  F4.2    arcsec   SepMin  Minimum separation of the closest approach
  27- 29  I3      deg      PA      Position angle of Triton relative to the 
                                    star at the time of the closest approach 
                                    (North to East)
  31- 34  F4.1    mag      Rmag    CCD magnitude
  36- 39  F4.1    km/s     Vel     Velocity of the occultation shadow
      41  A1      ---    l_S/N     Limit flag on S/N
  42- 44  I3      ---      S/N     Signal to noise ratio (1)
  46- 48  I3      deg      Dist    Angular distance between Triton and the Sun
  50- 51  I2      h        RAh     Right ascension (J2000) of the star
  53- 54  I2      min      RAm     Right ascension (J2000) of the star
  56- 61  F6.3    s        RAs     Right ascension (J2000) of the star
      63  A1      ---      DE-     Declination sign
  64- 65  I2      deg      DEd     Declination (J2000) of the star
  67- 68  I2      arcmin   DEm     Declination (J2000) of the star
  70- 74  F5.2    arcsec   DEs     Declination (J2000) of the star
  76- 79  I4      deg      Elon    [-179/155] Sub_Earth longitude of the star 
                                    at the mid-time of the event
  81- 95  A15     ---      Strip   Strip numbers on which an image of the 
                                    candidate star was measured
--------------------------------------------------------------------------------
Note (1): The S/N for the light curve has been calculated for an averaging
           interval of 20km (the approximate scale height of Triton's
           atmosphere), based on the S/N of 30.3 achieved for Tr60 by Elliot
           et al. (1993BAAS...25.1106E) with the 0.9m KAO telescope with a CCD
           photometer (no filter). Background limited performance has been
           assumed, which may lead to an overestimate of S/N for the brightest
           sources. Potential observers should evaluate the S/N for their own
           photometric equipment.
--------------------------------------------------------------------------------

History: Prepared via OCR at CDS.
================================================================================
(End)                           James Marcout, Patricia Bauer [CDS]  01-Apr-1997

Go to ADC Home Page