Astronomical Data Center

ADCADC/CDS Standard Document for Catalog:
/catalogs/6/6104/

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


VI/104              The Ultraviolet Imaging Telescope (UIT)   (1990, 1995)
================================================================================
The Ultraviolet Imaging Telescope (UIT), ASTRO 1 and ASTRO 2 shuttle missions 
 (1990, 1995)
    Stecher T.P., et al.
    <Astophysical Journal 395, L1 (1992)>
    =1992ApJ...395L...1S
Correcting the distortion of images taken with the Ultraviolet Imaging Telescope
    Greason M.R., Offenberg J.D., Cornett R.H., Hill R.S., Stecher T.P.
    <Publ. Astron. Soc. Pac. 106, 1151 (1994)>
    =1994PASP..106.1151G
The Ultraviolet Imaging Telescope: instrument and data characteristics.
    Stecher T.P., et al.
    <Publ. Astron. Soc. Pac. 109, 584 (1997)>
    =1997PASP..109..584S
================================================================================
ADC_Keywords: Observatory log ; Ultraviolet
Mission_Name: UIT

Description:
    UIT was one of three ultraviolet telescopes on the ASTRO-1 mission
    flown on  the space shuttle Columbia during 2-10 December 1990.
    The same three instruments were later flown on the space
    shuttle Endeavour during 3-17 March 1995, as part of the ASTRO-2
    mission. Exposures were obtained on 70-mm photographic film
    in the 1200-3300 Angstrom range using broadband filters and later
    digitized using a Perkin-Elmer microdensitometer. Image resolution
    was 3 arcseconds over a 40 minute field of view. Overall, UIT-1
    obtained 821 exposures of 66 targets, and UIT-2 obtained 758 images
    of 193 targets.


File Summary:
--------------------------------------------------------------------------------
 FileName    Lrecl    Records    Explanations
--------------------------------------------------------------------------------
ReadMe          80      .        This file
uitlist.dat    121      1481     UIT Observation Log
--------------------------------------------------------------------------------

See also:
    http://archive.stsci.edu/uit/ : UIT in MAST at STScI.
    http://archive.stsci.edu/astro/index.html  : ASTRO MISSION
    VI/103 : The Hopkins Ultraviolet Telescope (HUT)
    VI/105 : Wisconsin Ultraviolet Photo-Polarimeter Experiment (WUPPE)

Byte-by-byte Description of file: uitlist.dat
--------------------------------------------------------------------------------
   Bytes Format  Units   Label    Explanations
--------------------------------------------------------------------------------
  1-  8  A8      ---     Target   Target name specified by UIT mission
 10- 19  F10.6   deg     RAdeg    RA in J2000 decimal degrees
 21- 30  F10.6   deg     DEdeg    DEC in J2000 decimal degrees
 32- 38  A7      ---     PointID  ASTRO Pointid (1)
 40- 43  A4      ---     Jotfid   The first 4 digits of the PointID
 45- 79  A35     ---     Category Translation of the the jotfid
 82- 85  I4      yr      Start.Y  [1990-1995] Start time (year)
     86  A1      ---     ---      [-]
 87- 88  I2      "month" Start.M  [1-12] Start time      (month)
     89  A1      ---     ---      [-]
 90- 91  I2      d       Start.D  [1-31] Start time      (day)
     92  A1      ---     ---      [T]
 93- 94  I2      h       Start.h  [0-24] Start time      (hour)
     95  A1      ---     ---      [:]
 96- 97  I2      min     Start.m  [0-60] Start time      (minute)
     98  A1      ---     ---      [:]
 99-100  I2      s       Start.s  [0-60] Start time      (second)
102-108  F7.1    s       ExpTime  The total exposure time in seconds.
110-111  A2      ---     Filter   Filter ID (2)
    113  I1      ---     ASTRO    [1,2] Astro mission number
115-121  A7      ---     DataID   Dataset identification (3)
--------------------------------------------------------------------------------
Note (1):  All three ASTRO missions assigned a unique pointing ID
           for each target:
      Digit one  - see the "Science Class" section below
      Digit two  - Science Subclass  See Bottom
      Digits 3/4 - Target Numbers within Subclass
      Digit 5    - N => Nth pointing at target with different roll or offset
      Digit 6    - 0 => only one pointing for target
                   N => Nth pointing
      Digits 5 and 6 often not available

Note (2): The UIT instrument included two six-position filter wheels.
     The "A" filters were sensitive in the near-UV while the "B"
     filters were sensitive in the Far-UV.

Note (3): Dataset identification as used by preview page generator etc.
--------------------------------------------------------------------------------

Science Classes: the hierarchy of the classification is the following:

   0       Calibration
   0.0             HUT Camera Sensitivity Targets
   0.1             HUT Spectrometer Focus Targets
   0.2             HUT
   0.3             UIT Flat Field Sources
   0.4             UIT
   0.5             WUPPE Aperture Position Calibrators
   0.6             WUPPE Unpolarized & Polarized Standards
   0.7             BBXRT Calibration Sources
   0.8             BBXRT
   0.9             Joint Focus and Alignment Targets

   1       Solar System Objects
   1.1             Comets
   1.2             Planets
   1.3             Asteroids, etc.

   2       Individual Stars
   2.1             Supergiants
   2.2             Oe/Be Stars
   2.3             Wolf-Rayet Stars
   2.4             Rapid Rotators
   2.5             Normal White Dwarfs
   2.6             Magnetic/Pulsating W.D.'s
   2.7             Planetary Nebula Nuclei
   2.8             Normal Stars A0 & Later

   3       Variable and Binary Stars
   3.1             Pre-Main Sequence Stars
   3.2             Cataclysmic Variables
   3.3             Interacting Binaries
   3.4             Symbiotic Stars
   3.5             Active Chromospheres
   3.6             Pulsating Variables
   3.7             Low Mass X-Ray Binaries
   3.8             High Mass X-Ray Binaries
   3.9             X-Ray Transients

   4       ISM & Nebulae
   4.1             Planetary Nebulae
   4.2             Reflection Nebulae
   4.3             H II Regions
   4.4             Super Nova Remnants
   4.5             I.S. Polarization Probes
   4.6             I.S. Absorption Probes (Nearby & Hot)
   4.7             Herbig-Haro Objects
   4.8             Dark Clouds
   4.9             Diffuse Galactic X-Ray Emission Regions

   5       Star Clusters
   5.1             Metal Poor Globulars
   5.2             Metal Rich Globulars
   5.3             Open (Galactic) Clusters
   5.4             O/B Associations

   6       Normal Galaxies
   6.1             Nearby Galaxies
   6.2             Spirals
   6.3             Ellipticals
   6.4             Irregulars
   6.5             Dwarfs
   6.6             Edge On Systems

   7       Abnormal Galaxies
   7.1             Interacting Galaxies
   7.2             Amorphous Galaxies
   7.3             Rapid Star Formation
   7.4             W/Circumgalactic Matter
   7.5             E/S0 with I.S. Matter

   7       X-Ray Miscellany
   7.6             X-Ray Background
   7.7             Unidentified X-Ray Sources

   8       Active Extragalactic
   8.1             Seyfert I Galaxies
   8.2             Seyfert II Galaxies
   8.3             Radio Galaxies
   8.4             Radio Loud Quasistellar Objects
   8.5             Radio Quiet Quasistellar Objects
   8.6             BL Lacertae Objects
   8.7             LINERs
   8.8             Optically Violent Variable (OVV) Quasars

   9       Clusters of Galaxies
   9.1             Spiral Poor Clusters
   9.2             Spiral Rich Clusters
   9.3             X-Ray Selected Clusters
   9.4             Deep Survey Fields
   9.5             Cooling Flow Clusters

   9       Spacecraft Specific
   9.7             TAPS Tests
   9.8             Gyros/IMC/IPS
   9.9             Waterdumps/Handovers

Acknowledgements:
    Karen Levay <klevay@stsci.edu>
    Randall Thompson <rthomp@stsci.edu>
================================================================================
(End)                                            Mark Allen [CDS]    04-Feb-2002

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