Astronomical Data Center

ADCADC/CDS Standard Document for Catalog:
/journal_tables/ApJ/565/511/

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/ApJ/565/511       Cataclysmic variables in the 2MASS 2IDR  (Hoard+, 2002)
================================================================================
Infrared properties of cataclysmic variables in the 2 micron All-Sky Survey
Second Incremental Data Release.
    Hoard D.W., Wachter S., Clark L.L., Bowers T.P.
      <Astrophys. J. 565, 511 (2002)>
      =2002ApJ...565..511H      (SIMBAD/NED BibCode)
================================================================================
ADC_Keywords: Stars, variable ; Novae ; Binaries, cataclysmic ;
              Photometry, infrared
Keywords: accretion, accretion disks - infrared: stars -
          novae, cataclysmic variables - stars: dwarf novae -
          stars: fundamental parameters - surveys

Abstract:
    Cataclysmic variables (CVs) have "traditionally" been observed
    primarily at short wavelengths because accretion-generated luminosity,
    which peaks in the optical-ultraviolet, dominates the radiated energy
    of most systems. Hence, relatively little is known about their
    infrared (IR) properties. Investigating CVs in the IR will contribute
    to the understanding of key system components that are expected to
    radiate at these wavelengths, such as the cool outer disk, accretion
    stream, and secondary star. We have compiled the near-IR J, H, and Ks
    band photometry of all cataclysmic variables contained in the sky
    coverage of the Second Incremental Data Release of the 2 Micron All
    Sky Survey (2MASS). This data comprises 251 cataclysmic variables with
    reliably identified near-IR counterparts and S/N>10 photometry in one
    or more of the three near-IR bands. In addition to tables containing
    the 2MASS data, we present a set of near-IR finding charts for
    selected systems.

File Summary:
--------------------------------------------------------------------------------
 FileName      Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe            80        .   This file
table1.dat       114      251   CVs in the 2MASS 2nd Incremental Data Release
table2.dat        32      152   Undetected CVs in the 2MASS 2nd Incremental
                                 Data Release
table3.dat        46      118   Problematic CVs in the 2MASS 2nd Incremental
                                 Data Release
notes.dat         78      230   Individual notes
--------------------------------------------------------------------------------

See also:
   B/2mass : The 2MASS database (IPAC/UMass, 2000)
     V/110 : Catalog of Cataclysmic Variables (Downes+ 2001)

Byte-by-byte Description of file: table1.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label    Explanations
--------------------------------------------------------------------------------
   1-  9  A9    ---     Name     Downes et al. (2001, Cat. <V/110>) cataclysmic
                                  variable name
  11- 12  I2    h       RAh      Hour of Right Ascension (J2000)
  14- 15  I2    min     RAm      Minute of Right Ascension (J2000)
  17- 20  F4.1  s       RAs      Second of Right Ascension (J2000)
      22  A1    ---     DE-      Sign of the Declination (J2000)
  23- 24  I2    deg     DEd      Degree of Declination (J2000)
  26- 27  I2    arcmin  DEm      Arcminute of Declination (J2000)
  29- 30  I2    arcsec  DEs      Arcsecond of Declination (J2000)
  32- 35  F4.2  arcsec  Offset   ? Optical CV and near-IR counterpart offset (1)
  37- 43  A7    ---     Type     Downes et al. (2001, Cat. <V/110>) CV
                                  classification type (2)
  45- 52  F8.6  d       Porb     ? Orbital period (3)
      54  A1    ---   l_Jmag     Indicates 95% confidence upper limit on Jmag
  55- 60  F6.3  mag     Jmag     ? The 2MASS J band magnitude
  62- 66  F5.3  mag   e_Jmag     ? The 1{sigma} uncertainty in Jmag
      68  A1    ---   l_Hmag     Indicates 95% confidence upper limit on Hmag
  69- 74  F6.3  mag     Hmag     ? The 2MASS H band magnitude
  76- 80  F5.3  mag   e_Hmag     ? The 1{sigma} uncertainty in Hmag
      82  A1    ---   l_Ksmag    Indicates 95% confidence upper limit on Ksmag
  83- 88  F6.3  mag     Ksmag    ? The 2MASS K_s_ band magnitude
  90- 94  F5.3  mag   e_Ksmag    ? The 1{sigma} uncertainty in Ksmag
  96-114  A19   ---   n_Name     Short notes on Name (4)
--------------------------------------------------------------------------------
Note (1): The astrometric accuracy of the 2MASS PSC is better than 0.2arcseconds
Note (2): We have defined each of these sub-type categories to include the
           following classification codes given in Downes et al.
          (2001, Cat. <V/110>):
          dwarf novae = ug, ugz, ugss, ugsu, ugwz
          novalikes = nl, ux, vy
          classical novae = n, na, nb, nc
          recurrent novae = nr, nra, nrb
          magnetic CVs = am, dq
          The uncertain/unclassified systems include the general classification
           code of "cv" as well as any targets with uncertain classification
           (denoted with ":" or "?") and/or conflicting classifications
           (e.g., "ug/vy").  In a few cases, to avoid "recounting" the same
           targets, we chose between multiple (but compatible) classifications.
Note (3): Orbital periods inferred from the superhump period relation of
           Stolz & Schoembs (1984A&A...132..187S) are listed here, but periods
           described by Downes et al. (2001, Cat. <V/110>) as
           "uncertain/unreliable" are not listed.
Note (4): An asterisk indicates that additional information about the CV is
           given in notes.dat file.
          The data quality flags are
           rd: read flag, describing the photometry method,
           bl: blend flag, describing the number of profiles fit during the
                photometry
           cc: contamination flag, describing various photometry problems.
          Each flag is followed by a three digit code giving the flag values
            for the Jmag, Hmag, and Kmag columns, respectively.
          Acceptable values for rd are
           0: source not detected, 95% confidence upper limit magnitude is given
           1: aperture photometry magnitude
           2: profile-fitting magnitude
           all other values indicate unusable data.
          Acceptable values for bl are
           0: source not detected, corresponding to rd=0)
           1: single profile fit to isolated source
           values >1 indicate multiple sources detected in a small region.
          Acceptable values for cc are
           0: not contaminated or not detected
           all other values indicate contaminated data (e.g., P, D, and S
            indicate different contamination artifacts caused by a nearby bright
            star, C indicates confusion with a nearby source, B indicates
            confusion during merging of the J, H, and K_s_ band data sets).
--------------------------------------------------------------------------------

Byte-by-byte Description of file: table2.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  9  A9    ---     Name      Cataclysmic variable name from Downes et al.
                                   (2001, Cat. <V/110>)
      11  A1    ---   n_Name      [a] Indicates additional comments available
                                       in notes.dat file
  13- 14  I2    h       RAh       Hour of Right Ascension (J2000)
  16- 17  I2    min     RAm       Minute of Right Ascension (J2000)
  19- 22  F4.1  s       RAs       Second of Right Ascension (J2000)
      24  A1    ---     DE-       Sign of the Declination (J2000)
  25- 26  I2    deg     DEd       Degree of Declination (J2000)
  28- 29  I2    arcmin  DEm       Arcminute of Declination (J2000)
  31- 32  I2    arcsec  DEs       Arcsecond of Declination (J2000)
--------------------------------------------------------------------------------

Byte-by-byte Description of file: table3.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  9  A9    ---     Name      Downes et al. (2001, Cat. <V/110>) cataclysmic
                                   variable name
  11- 12  I2    h       RAh       Hour of Right Ascension (J2000)
  14- 15  I2    min     RAm       Minute of Right Ascension (J2000)
  17- 20  F4.1  s       RAs       Second of Right Ascension (J2000)
      22  A1    ---     DE-       Sign of the Declination (J2000)
  23- 24  I2    deg     DEd       Degree of Declination (J2000)
  26- 27  I2    arcmin  DEm       Arcminute of Declination (J2000)
  29- 30  I2    arcsec  DEs       Arcsecond of Declination (J2000)
  32- 46  A15   ---   n_Name      Notes on Name (1)
--------------------------------------------------------------------------------
Note (1): Notes:
             * = Additional information about the CV is given in notes.dat file
  Uncertain ID = A CV for which there is insufficient or imprecise information
                  pertaining to its optical position and/or identification that
                  precludes identification of the near-IR counterpart.
       Cluster = A CV located in a star cluster that is too crowded to obtain
                  2MASS photometry. The cluster's NGC catalog number is given.
      Artifact = A CV located in the exclusion region defined around diffraction
                  spikes of nearby bright stars.
       Crowded = The near-IR field around the CV is more crowded than the
                  optical field, and conclusive identification of the CV's
                  near-IR counterpart is not possible.
       Blended = The near-IR counterpart of the CV is blended with one or more
                  additional near-IR sources in the 2MASS images.
--------------------------------------------------------------------------------

Byte-by-byte Description of file: notes.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  9  A9    ---     Name      Star name
  11- 80  A70   ---     Note      Text of the note
--------------------------------------------------------------------------------

History:
    From electronic version of the journal

================================================================================
(End)                    Greg Schwarz [AAS], Patricia Bauer [CDS]    22-Mar-2002

Go to ADC Home Page