Astronomical Data Center

ADCADC/CDS Standard Document for Catalog:
/catalogs/5/5090/

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

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V/90           Catalogue of X-Ray Binaries                   (van Paradijs 1995)
================================================================================
A Catalogue of X-Ray Binaries
    van Paradijs J.
    <in 'X-ray Binaries', Lewin W.H.G., van Paradijs J.,  
      van den Heuvel E.P.J., Eds., Cambridge University Press, 
      Chapter 14, p. 536-577, ISBN 0 521 41684 1 (1995)> 
      =1995xrb..book.....L
================================================================================
ADC_Keywords: Binaries, X-ray; X-ray sources
Mission_Name: Ariel-5, CGRO, Exosat, Ginga, Granat, HEAO-1, HEAO-2, Hakucho 
          OSO-7, OAO, Rosat, SAS-3, Tenma, Uhuru, Vela-5, Vela-6

Description:
  The objects described in this catalog are X-Ray binaries, i.e., 
  semi-detached binary stars in which matter is transferred from 
  a usually more or less normal star to a neutron star or black hole. 
  Thus, cataclysmic variables are not included.  The tables provide 
  basic information of the systems as well as selected references. 
  The tables contain 124 low-mass and 69 high mass X-ray binaries.


File Summary:
--------------------------------------------------------------------------------
 FileName    Lrecl    Records    Explanations
--------------------------------------------------------------------------------
ReadMe          80          .     This file
table1.dat     269        124     low mass X-ray binaries (LMXB)
tab1ref.dat    108        681     notes and references to table1.dat
table2.dat     269         69     high mass X-ray binaries (HMXB)
tab2ref.dat     95        445     notes and references to table2.dat
table3.dat      29        141     cross references from often used nomenclature
refs.dat        80       1339     references
--------------------------------------------------------------------------------

See also: 
  5082: Cataclysmic Variables (Ritter)

Byte-by-byte Description of file: table1.dat, table2.dat
--------------------------------------------------------------------------------
   Bytes  Format   Units  Label       Explanations
--------------------------------------------------------------------------------
   1- 12   A12     ---    ID         *source name (as hhmm+/-ddd)
  13- 25   A13     ---    alt         alternate source name
  26- 37   A12     ---    opt_src1   *Opt. counterpart name or location in
                                      finding chart
  38- 48   A11     ---    opt_src2   *Opt. counterpart name or location in
                                      finding chart
  49- 50   I2      h      RAh         Right Ascension -hours (B1950)
  53- 54   I2      min    RAm         Right Ascension -minutes
  55- 58   F4.1    s      RAs         ?Right Ascension - seconds
                                      (accurate to 0.1s)
      59   A1      ---    DE-         Declination sign (B1950)
  60- 61   I2      deg    DEd         Declination degrees
  62- 63   I2      arcmin DEm         ?Declination arc minutes 
  64- 65   I2      arcsec DEs         ?Declination arc seconds
                                      (accurate to 1arcsec)
  66- 72   F7.2    deg    GLON        Galactic Longitude (accurate to 0.1 deg)
  73- 78   F6.2    deg    GLAT        Galactic Latitude
  79- 84   A6      ---    src_info   *combination of src_pos and acc_pos, where
                                      src_pos = spectral region for
                                      positional data
                                      acc_pos = positional accuracy indication
  85- 89   A5      ---    type       *[ABDGPTUZ ] source type code 
  90- 98   A9      ---    origin     *[ACExoGrHaKMORSLTUV ]
                                      catalogs/experiments 
                                      listing/detecting source
      99   A1      ---    LMX_HMXB    [LH]! L = LMXB ; H = HMXB
 100-114   A15     ---    r_chart     reference code to finding chart
 115-123   A9      mag    Vmag        visual magnitude optical counterpart
 124-132   A9      mag    B-V         (B-V) color index optical counterpart
 133-137   A5      mag    U-B         (U-B) color index optical counterpart
 138-141   A4      mag    Other_mag   Other magnitude value
 142-157   A16     ---    ID_Othr_mag identification of the Other_mag
 158-168   A11     ---    Sp          Spectral type optical counterpart
                                      (HMXB only)
 169-176   A8      mag    E(B-V)      Estimate for interstellar reddening
 177-187   A11     uJy    F(X)       *X-ray flux 
 188-192   A5      uJy    F(X)lo     *X-ray flux lower limit range
 193-196   A4      uJy    F(X)hi     *X-ray flux upper limit range
 197-203   A7      ---    P           Orbital period (unit in unit_P field)
     204   A1      ---    unit_P     *unit of Orbital period
 205-224   A20     s      Ppulse      Pulse period for pulsars
 225-242   A18     ---    r_photomtry reference codes for the photometry
 243-256   A14     ---    r_F(X)      reference codes for the X-ray fluxes
 257-271   A15     ---    r_P         reference codes for Orbital and
                                      Pulse periods
--------------------------------------------------------------------------------
Note on ID:
  The source name gives rough information on its B1950 position 
  using the convention hhmm+ddd where hh and mm are the hours and 
  minutes of right ascention, ddd the declanation in units of 0.1
  degree. In some cases more or less accurate positions were given. 
  A prefix J indicated that the name was based on J2000 coordinates.
Note on origin:
  The following codes were used [with reference codes]:
  A:   Ariel V sky survey [795,1255]
  C:   Compton gamma-ray Observatory
  E:   Einstein Observatory
  Exo: Exosat
  G:   Ginga
  Gr:  Granat
  H:   HEAO 1 A-1 sky survey [1305]
  Ha:  Hakucho
  K:   Kvant
  M:   MIT OSO-7 sky survey [754]
  OAO: Orbiting Astronomical Observatory
  R:   Rosat
  S:   SAS-3
  SL:  Space Lab
  T:   Tenma
  U:   Uhuru sky survey [333]
  V:   Vela-5 and -6 satellites.
Note on type:
  Codes for source type:
  A:   atoll source (11 LMXBs) [437]
  B:   X-ray burst source (42 LMXBs)
  D:   'dipping' LMXBs (9) 
  G:   globular cluster X-ray source (12 LMXBs)
  P:   X-ray pulsar (3 LMXBs, 29 HMXBs)
  T:   transient X-ray source (41 LMXBs, 30 HMXBs)
  U:   ultrasoft X-ray spectrum (17 LMXBs, 3 HMXBs). These sources
       include black-hole candidates; some extreme ultra-soft (EUS) 
       source may be white dwarfs on whose surface steady nuclear burning
       takes place [1184]
  Z:   Z-type (6 LMXBs)
Note on src_info:
  src_pos:
  Spectral region that observations were taken for position determination:
  o:   optical
  x:   X-ray
  r:   radio
  IR:  infrared
  A reference on the source position is given in tab1ref.dat after the 
  key 'pos'. Also included is an indication of the accuracy of that 
  position, in the form of an equivalent (90% confidence level) error 
  radius which can only be considered and approximation (e.g. when the 
  error box is not circular). When no accuracy is quoted it is about 
  one arcsec or better.
Note on opt_src1, opt_src2: 
  Names of optical counterpart, or an asterisk followed by a star number 
  which refers to the star numbers used in the finding chart; the word
  'star' refers to a star in the finding chart that has not been given a
  number or letter.  The r_chart column contains the reference to the 
  finding chart. Many optical counterparts have been indicated with a 
  variable-star name, as given in the 'General Catalogue of Variable 
  Stars' (ADC ID's: 2139B, 2172B, 2195) and in recent name lists of
  variable stars as published in the 'IAU Information Bulletin on 
  Variable Stars', or a number in a well-known catalogue (e.g., HD, 
  SAO). For X-ray sources in globular clusters, the cluster name is 
  given, in addition to the name of a stellar counterpart.
Note on F(X), F(X)hi, F(X)lo:
  The flux is given in units of 1 micro Jansky , which is
    10**(-29) erg cm**(-2) s**(-1) Hz**(-1) 
    = 2.4 x 10**(-12) erg cm-**(2) s-**(1) keV**(-1)
Note on unit_P:  
  The orbital period for LMXBs (table1.dat) is given in hours, and
  for HMXBs (table2.dat) in days.
--------------------------------------------------------------------------------
 
Byte-by-byte Description of file: tab*ref.dat
--------------------------------------------------------------------------------
   Bytes  Format   Units Label     Explanations
--------------------------------------------------------------------------------
   1- 12   A12     ---   ID        Source identification 
  17-108   A92     ---   note      notes to the table for the source
--------------------------------------------------------------------------------

Byte-by-byte Description of file: table3.dat
--------------------------------------------------------------------------------
   Bytes  Format   Units Label   Explanations
--------------------------------------------------------------------------------
   1- 13   A13     ---   alt     Variable star, GX number, Globular Cluster or
                                  constellation
  15- 26   A12     ---   ID      Source identification
      28   A1      ---   table   table number
--------------------------------------------------------------------------------

Byte-by-byte Description of file: refs.dat
--------------------------------------------------------------------------------
   Bytes  Format   Units Label     Explanations
--------------------------------------------------------------------------------
   1-  4   I4      ---   refcode   code number for reference
   7- 80   A74     ---   reftext   text of reference
--------------------------------------------------------------------------------

History:
  The catalog was received by the ADC in the form of the original tables.
  All formatting characters were removed, the notes were placed in a 
  separate file and the data fields were reorganized. The RA and DEC in the 
  tables were reformatted to conform to the same format by expanding 
  decimals where necessary into minutes or seconds. In this process some
  indication of the positional accuracy has been lost. The tables were 
  checked for consistency with the data format tables. Please report any 
  data that differ from the published tables in any other respects. 

================================================================================
(End)                N. Paul Kuin [NASA/ADC]                 9-Jan-1997

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