Astronomical Data Center

ADCADC/CDS Standard Document for Catalog:
/catalogs/5/5098/

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


V/98                    MSX Infrared Astrometric Catalog (Egan+ 1996)
================================================================================
The MSX Infrared Astrometric Catalog
       Egan M.P., Price S.D.
      <Astron. J 112, 2862 (1996)>
      =1996AJ....112.2862E
================================================================================
ADC_Keywords: Infrared sources ; Proper motions ; Spectroscopy ;
              Cross identifications
Mission_Name: MSX

Abstract:
    The MSX Infrared Astrometric Catalog has been contructed as a tool for
    improving the pointing accuracy of infrared observations. The catalog
    contains 177,860 astrometric stars, 61,242 which have been identified
    with their infrared counterparts from IRAS catalogs and the Catalog of
    Infrared Observations through position and color matching. Infrared
    flux densities are predicted for 6 wavelength bands between 4 and
    22um. The catalog identifications are complete to within the spatial
    coverage of current surveys for those astrometric stars brightest in
    the infrared. By predicting fluxes of astrometric stars without IR
    identifications we are able to extend the catalog to areas of the sky
    which were incomplete in the IRAS catalogs. Furthermore, by retaining
    stars below the brightness limit of current surveys we are able to
    provide better spatial coverage to help point or position the next
    generation of infrared telescopes.

Description:
    This version of the MSX IR Astrometric Catalog is a truncated version
    of the documentation which exists for the convenience of the user and
    is primarily intended to allow quick access to the file formats and
    other information needed to access the information. The AJ paper
    contains the definitive information about the catalog itself.

    The MSX IR Astrometric Catalog, Version 4.2.1 was constructed from a
    number of visible astrometric catalogs, and contains position
    information accurate to the sub-arcsecond level. The FK5 (1988 Fricke
    Schwan & Lederle, Cat. <I/149>), FK5 Extension (1991 Fricke, Schwan
    & Corbin, Cat. <I/175>), Astrographic Catalog of Reference Stars (1991
    Corbin & Urban, Cat. <I/171>), Position and Proper Motion Catalog
    (1988 Roeser & Bastian, Cat. <I/146>) and PPM South (1991 Bastian et
    al., Cat. <I/193>) were the sources of position and magnitude
    information. The PPM and FK5 catalogs contain 1-D spectral type
    information, and this was supplemented where possible with 2-D MK
    spectral types. The ACRS and PPM quote photographic magnitudes. These
    were transformed to V magnitude using the spectral type and expected
    B-V color.

    Spatial coincidence and color-matching criteria (based on V-[12] color
    and spectral type) were used to identify IR counterparts of the
    astrometric stars. The IRAS Point Source (Cat. <II/125>), Faint Source
    (Cat. <II/156>), Faint Source Reject file, and Serendipitous Survey
    (Cat. <II/126>) catalogs were used to supply IR observations, as was
    the Catalog of Infrared Observations (1993 Gezari et al., Cat
    <II/209>).

    The infrared telescope (SPIRIT III) aboard the Ballistic Missile
    Defense Organization (BMDO) Midcourse Space Experiment (MSX) (Mill et
    al., 1994, J. of Spacecraft & Rockets 31, 900) has detectors which
    allow spatial resolution 30 times better than that achieved by IRAS

    The IR flux in each SPIRIT III band was estimated using the V
    magnitude, spectral type, and IR flux (if available) to determine a
    blackbody spectrum for the star, which was then convolved with the
    system spectral response of each SPIRIT III radiometer band. Stars
    which were brighter than 8th magnitude in band A were retained in the
    final MSX IR astrometric catalog. In MSXv4.2.1, there are 177860
    stars, 61242 of which had IR counterparts.

File Summary:
--------------------------------------------------------------------------------
 FileName    Lrecl    Records   Explanations
--------------------------------------------------------------------------------
ReadMe          80          .   This file
msx.dat        221     177860   MSX Infrared Astrometric Catalog
--------------------------------------------------------------------------------

See also:
   http://www.ipac.caltech.edu/ipac/msx/msx.html : MSX page
   http://www.sdl.usu.edu/programs/spirit3/: SPIRIT III page
    V/107 : MSX5C Infrared Point Source Catalog (Egan+ 1999)
   II/125 : IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986)
   II/126 : IRAS Serendipitous Survey Catalog (Kleinmann+ 1986)
   II/156A : IRAS Faint Source Catalog, |b| > 10, Version 2.0 (Moshir+ 1989)
   II/209 : Catalog of Infrared observations, Edition 3.5 (Gezari+ 1996)

Byte-by-byte Description of file: msx.dat
--------------------------------------------------------------------------------
   Bytes Format Units        Label     Explanations
--------------------------------------------------------------------------------
       1  A1    ---          AsID     *[FfANS] Original astrometric catalog ID
   2-  7  I6    ---          AsName    Astrometric catalog number
       8  A1    ---          IrID     *[PFSBZC] IR catalog ID
   9- 21  A13   ---          IrName    Name of star in IR catalog
  22- 23  I2    h            RAh       Right ascension, J2000
  24- 25  I2    min          RAm       Right ascension, J2000
  26- 31  F6.3  s            RAs       Right ascension, J2000
      32  A1    ---          DE-       Sign of declination
  33- 34  I2    deg          DEd       Declination, J2000
  35- 36  I2    arcmin       DEm       Declination, J2000
  37- 41  F5.2  arcsec       DEs       Declination, J2000
  42- 47  F6.1  ms         e_RAs       Mean R.A. error*cos(dec)
  48- 52  F5.1 0.01arcsec  e_DEs       Mean declination error
  53- 61  F9.3 10-2s/yr      pmRA      Proper motion in right ascension (J2000)
  62- 70  F9.2 10-2arcsec/yr pmDE      Proper motion in declination (J2000)
  71- 76  F6.1 0.1mas/yr   e_pmRA      Mean error of R.A. PM*cos(dec)
  77- 82  F6.1 0.1mas/yr   e_pmDE      Mean error of Dec. PM
  83- 85  A3    ---          Sp       *Spectral type
  86- 87  A2    ---          LRS       IRAS LRS designation
  88- 92  F5.2  mag          Vmag      V visual magnitude
  93-101  E9.3  Jy           F12um     ?=0.000E+00 IRAS 12mu flux
 102-110  E9.3  Jy           F25um     ?=0.000E+00 IRAS 25mu flux
 111-119  E9.3  Jy           F60um     ?=0.000E+00 IRAS 60mu flux
 120-128  E9.3  Jy           F100um    ?=0.000E+00 IRAS 100mu flux
     129  I1    ---        q_F12um     IRAS 12um flux quality flag
     130  I1    ---        q_F25um     IRAS 25um flux quality flag
     131  I1    ---        q_F60um     IRAS 60um flux quality flag
     132  I1    ---        q_F100um    IRAS 100um flux quality flag
 133-141  E9.3  Jy           FSIIIA   *SPIRIT III Band A flux density estimate
 142-150  E9.3  Jy           FSIIIB1  *SPIRIT III Band B1 flux density estimate
 151-159  E9.3  Jy           FSIIIB2  *SPIRIT III Band B2 flux density estimate
 160-168  E9.3  Jy           FSIIIC   *SPIRIT III Band C flux density estimate
 169-177  E9.3  Jy           FSIIID   *SPIRIT III Band D flux density estimate
 178-186  E9.3  Jy           FSIIIE   *SPIRIT III Band E flux density estimate
 187-195  E9.3  Jy           F12umEst  Estimated IRAS 12 micron flux
 196-199  F4.1  um           Lam1     *? Wavelength of CIO observation
 200-208  E9.3  Jy           Flux1    *? Corresponding Flux of CIO observation
 209-212  F4.1  um           Lam2     *? Wavelength of CIO observation
 213-221  E9.3  Jy           Flux2    *? Corresponding Flux of CIO observation
--------------------------------------------------------------------------------
Note on AsID:
  F  FK5, Cat. <I/149>
  f  FK5 Extension, Cat. <I/175>
  A  ACRS, Cat. <I/171>
  N  PPM, Cat. <I/146>
  S  PPM South, Cat. <I/193>
Note on IrID:
  P  IRAS Point Source Catalog, Cat. <II/125>
  F  IRAS Faint Source Catalog, Cat. <II/156>
  B  Combined PSC/FSC data, Cat. <II/125> and Cat. <II/156>
  Z  IRAS Faint Source Reject
  S  IRAS Serendiptious Survey, Cat. <II/126>
  C  Catalog of IR Observations, Cat. <II/209>
Note on Sp:
  Coded spectral type, e.g. G83 = G8 III; G80 = G8
Note on Lam1, Lam2, Flux1, Flux2:
  These values were originally embedded in the IRAS Fxxum columns.
Note on FSIIIA, FSIIIB1, FSIIIB2, FSIIIC, FSIIID, FSIIIE:
  the wavelength domains are specified by the central wavelength 
  (isophotal wavelength) and the FWHM wavelength range (in {mu}m):
  ----------------------------
  Band  Center   FWHM Points
  ----------------------------
  A     8.28     6.8  - 10.8
  B1    4.29     4.22 - 4.36
  B2    4.25     4.24 - 4.45
  C    12.13     11.1 - 13.2
  D    14.65     13.5 - 15.9
  E    21.34     18.2 - 25.1
  ----------------------------
--------------------------------------------------------------------------------

History:
  * 06-Nov-1996: AAS CD-ROM series, Volume 7, 1996, Lee Brotzman [ADS]
  * 04-Dec-1997: Wavelength + fluxes from CIO disentangled from IRAS fluxes
================================================================================
(End)                                   Francois Ochsenbein   [CDS]  04-Dec-1997

Go to ADC Home Page