Astronomical Data Center

ADCADC/CDS Standard Document for Catalog:
/journal_tables/MNRAS/317/55/

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


VII/221                     PSCz catalog                       (Saunders+, 2000)
================================================================================
The PSCz catalogue
    Saunders W., Sutherland W.J., Maddox S.J., Keeble O., Oliver S.J.,
    Rowan-Robinson M., McMahon R.G., Efstathiou G.P., Tadros H., White S.D.M.,
    Frenk C.S., Carraminana A., Hawkins M.R.S.
    <Mon. Not. R. Astron. Soc. 317, 55 (2000)>
    =2000MNRAS.317...55S
================================================================================
ADC_Keywords: Infrared sources ; Photometry, infrared ; Galaxies, optical;
              Redshifts ; Surveys
Keywords: catalogues - surveys - galaxies: distances and redshifts, clustering -
          large-scale structure of the Universe

Description:
    The PSCz survey consists of redshifts, infra-red and optical
    photometry, and assorted other information for 18351 IRAS sources,
    mostly selected from the Point Source Catalog. The survey was designed
    to select almost all galaxies with flux brighter than 0.595Jy at 60
    microns, over the 84% of the sky with extinction small enough
    that reliable and complete optical identification and spectroscopy was
    possible. Some of the sources are not galaxies and some are multiple
    entries for the same galaxy as described below. There are in total
    15411 galaxies or possible galaxies, for which redshifts are available
    for 14677. The galaxies without redshift are mostly distant or at low
    latitude, as described below. Many of these galaxies have now been
    observed as part of the BTP project (Saunders et al 1999,
    astro-ph/9909174 "The Behind the Plane Survey"), and their redshifts
    will be included in future revisions of the catalogue.

    The main catalogue is "pscz.dat". There is also a short version
    of the catalogue, "psczvs.dat", containing sufficient information
    for most studies. They correspond to the version 2.2.

File Summary:
--------------------------------------------------------------------------------
 FileName   Lrecl Records  Explanations
--------------------------------------------------------------------------------
ReadMe         80       .  This file
notes.txt      79     468  Explanatory notes
pscz.dat      533   18351  Main catalogue
psczvs.dat    100   18411  Short version of main catalogue
psczcg.dat    533      60  Sources close to coverage gap
psczcgvs.dat  100      60  Short version of psczcg.dat
psczcat3.tex  836     849  Text for the accompanying paper
psczcat3.ps   132  203058  Postscript version
pscz2_2.dat   141   73404  Original version of pscz.dat with 4 lines/source,
                            explained in "notes.txt"
psczmask.dat  78      506 *Default mask defining the areas with inadequate
                            or confused IRAS coverage (10.56sr)
himask.dat    78      883 *More conservative mask for higher completeness
                            (9.06sr)
qcd.f          80    1112  Routines for using mask, coordinate transforms etc
g2bin.f        45       9  (l,b) to bin number
psi.f          76      18  Estimated selection function
igalrefs.txt   61      48  Redshift references
ilg.dat       124      11  Local Group galaxies deliberately excluded
--------------------------------------------------------------------------------
Note on psczmask.dat, himask.dat: list of excluded 'lune bins' and are read
    in by the fortran77 routine rdmask in "qcd.f" (see file "notes.txt")
--------------------------------------------------------------------------------

See also:
   II/125 : IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986)
   II/174 : IRAS 2Jy Redshift Survey Data File  (Strauss+ 1992)
  VII/185 : IRAS 1.2 Jy IRAS Redshift Survey (Strauss+ 1990,92,95)
  J/MNRAS/253/485 : QMW IRAS galaxy catalogue (QIGC) (Rowan-Robinson+, 1991)
  J/MNRAS/308/897 : QDOT all-sky IRAS galaxy redshift survey (Lawrence+, 1999)


Byte-by-byte Description of file: psczcg.dat pscz.dat
--------------------------------------------------------------------------------
   Bytes Format Units       Label    Explanations
--------------------------------------------------------------------------------
   2- 12  A11   ---         CNAME   *Name e.g. Q12345+4856
  14- 15  I2    h           RAh      Right ascension B1950
  16- 17  I2    min         RAm      Right ascension B1950
  18- 20  I3    0.1s        RAds     Right ascension B1950
      22  A1    ---         DE-      Declination sign B1950
  23- 24  I2    deg         DEd      Declination B1950
  25- 26  I2    arcmin      DEm      Declination B1950
  27- 28  I2    arcsec      DEs      Declination B1950
  29- 36  F8.2  Jy          S12      Flux at 12um
  37- 44  F8.2  Jy          S25      Flux at 25um
  45- 52  F8.2  Jy          S60      Flux at 60um
  53- 60  F8.2  Jy          S100     Flux at 100um
      62  I1    ---       q_S12     *[1,9] Flux origin and quality flag at 12um
      63  I1    ---       q_S25     *[1,9] Flux origin and quality flag at 25um
      64  I1    ---       q_S60     *[1,9] Flux origin and quality flag at 60um
      65  I1    ---       q_S100    *[1,9] Flux origin and quality flag at 100um
      67  I1    ---         SES12    [0,8] Small Extended Source flag at 12um
      68  I1    ---         SES25    [0,8] Small Extended Source flag at 25um
      69  I1    ---         SES60    [0,8] Small Extended Source flag at 60um
      70  I1    ---         SES100   [0,8] Small Extended Source flag at 100um
  72- 74  I3    %         e_S12      Flux uncertainty at 12um
  75- 77  I3    %         e_S25      Flux uncertainty at 25um
  78- 80  I3    %         e_S60      Flux uncertainty at 60um
  81- 83  I3    %         e_S100     Flux uncertainty at 100um
  85- 87  I3    arcsec      PosMin   Minor axis of 2{sigma} error ellipse
  88- 90  I3    arcsec      PosMax   Major axis of 2{sigma} error ellipse
  91- 93  I3    deg         PosPA    Position angle E of N of major axis
                                      of error ellipse
      95  I1    ---         Cirr1   *Cirrus flag
      96  I1    ---         Cirr2   *Cirrus flag
  97- 99  I3    MJy/sr      Cirr3   *Cirrus flag
     101  A1    ---         CC1      [A-N X] Correlation Coefficient at 12um
     102  A1    ---         CC2      [A-N X] Correlation Coefficient at 25um
     103  A1    ---         CC3      [A-M X1] Correlation Coefficient at 60um
     104  A1    ---         CC4      [A-N X1] Correlation Coefficient at 100um
     106  A1    ---         CONF     [0-9 ACDEF] Confusion flag, hex encoded
     107  A1    ---         DISC     [0-9 A-D] Discrepant flux flag, hex encoded
     108  A1    ---         HSD      [0-8] High Source Density flag, hex encoded
     110  I1    ---         PNEARH   [0-9] Nearby hours-confirmed sources
     111  I1    ---         PNEARW   [0-5] Nearby weeks-confirmed sources
     113  I1    ---         CES12   *Nearby seconds confirmed extended sources
                                      at 12um
     114  I1    ---         CES25   *Nearby seconds confirmed extended sources
                                      at 25um
     115  I1    ---         CES60   *Nearby seconds confirmed extended sources
                                      at 60um
     116  I1    ---         CES100  *Nearby seconds confirmed extended sources
                                      at 100um
 117-121  I5    ---         SNR60    10 x signal/noise of weakest detection
                                      at 60um
 122-123  I2    ---         NHCON    Number of hours-confirmed source detections
 124-125  I2    ---         MHCON    Potential number of hours-confirmed source
                                      detections
 127-130  I4    ---         FCOR60  *1000*flux correction factor applied at 60um
 132-136  A5    ---         PLATE    Plate number (POSS or SRC)
 138-144  A7    ---         NOM      Nominal plate centre in RA,dec
 146-148  I3    ---         NUM      Identifier for source on this plate
 150-151  I2    h           RAoh     ? Optical right ascension B1950
 152-153  I2    min         RAom     ? Optical right ascension B1950
 154-158  F5.2  s           RAos     ? Optical right ascension B1950
     160  A1    ---         DEo-     ? Optical declination sign B1950
 161-162  I2    deg         DEod     ? Optical declination B1950
 163-164  I2    arcmin      DEom     ? Optical declination B1950
 165-168  F4.1  arcsec      DEos     ? Optical declination B1950
 170-172  I3    arcsec      ADX      ? North/South Delta Optical/IRAS position
 173-175  I3    arcsec      ADY      ? East/West Delta Optical/IRAS position
 176-179  F4.1  ---         ALK      ? log_10 likelihood for optical
                                      identification
 180-182  I3    %           REL      ? Prob. correct optical identification
     183  A1    ---         CAND     ? Optical candidate A,B etc
     184  I1    ---         IOPT    *? Schmidt plate material used
 185-190  F6.2  mag         Bmag     ? Estimated optical B magnitude
 191-193  I3    arcsec      MajAxiO  ? Optical major axis
 194-196  I3    arcsec      MinAxiO  ? Optical minor axis
 197-199  I3    deg         PAO      ? Optical major axis position angle E of N
 200-206  F7.3 mag/arcsec+2 SuBr     ? Average optical surface brightness
 207-208  I2    ---         IDTYPE   Cross-identification type from PSC
 209-220  A12   ---         Oname    Optical name
 221-226  F6.2  mag         mag      Zwicky/RC3 magnitude
 227-231  F5.1  arcmin      D1X     *RC3/UGC/MCG/ESO D25 diameter from CATX
 232-234  I3    %           AR      *Axial ratio d25/D25 from CATX
 235-240  I6    km/s        Hvel     Best available heliocentric velocity (cz)
 241-244  I4    km/s      e_Hvel     Error on heliocentric velocity
 245-247  I3    ---       r_Hvel    *Reference for heliocentric velocity
 248-253  I6    km/s        Hvel2    Heliocentric velocity (cz)
                                      measured as part of PSCz survey
 254-257  I4    km/s      e_Hvel2    Error on PSCz heliocentric velocity
 258-260  I3    ---       r_Hvel2   *Reference for PSCz heliocentric velocity
 261-262  I2    ---         TType    De Vaucouleurs Type, 99 = unknown
 264-271  A8    ---         PGC      Catalogue of Principal Galaxies
                                      (PGC, Cat. <VII/119>) name
 273-280  F8.4  deg         RAdeg    Right ascension B1950 (IRAS source)
 282-289  F8.4  deg         DEdeg    Declination B1950 (IRAS source)
 291-298  F8.4  deg         GLON     Galactic longitude
 300-307  F8.4  deg         GLAT     Galactic latitude
 308-313  I6    km/s        cz       Velocity cz in Local Group frame
 314-318  F5.1  Mpc         Dist     Distance  from Rowan-Robinson 1988
 319-322  I4    ---         IDclus   Cluster identification from
                                      Rowan-Robinson 1988
 324-328  F5.2  [MJy/sr]    ALI100  *log10(100um background in MJy/sr)
 329-333  F5.2  [MJy/sr]    ALI100B *log10(100um background in MJy/sr
                                        for lune bin)
 334-339  I6    ---         NLBIN    Lune bin number
 341-342  A2    ---         CLASS   *Optical classification code
 344-348  A5    ---         CSEC     PSCz sector, e.g. A/123
 349-352  I4    mm          Xpos     X position from nominal bottom left corner
                                      of Schmidt plate
 353-356  I4    mm          Ypos     Y position from nominal bottom left corner
                                      of Schmidt plate
     358  A1    ---         CSTAT    [JORXPCELS?0] Optical material used
     359  A1    ---         CAREA    h=high|b|, p=other PSCz,
                                     l=BTP, c=in coverage gaps
     360  A1    ---         CZSTAT  *[#-1234lpxq] Redshift status
     362  A1    ---         C12CLAS  Classification in 1.2Jy survey
 363-370  F8.2  Jy          F3PSC    PSC flux at 60um
 371-378  F8.2  Jy          F4PSC    PSC flux at 100um
 379-383  F5.2  mag         ABB     *Estimated average B extinction in lune bin
                                      derived from 100 micron background
     385  A1    ---         CPSCZ   *[^&=-+] Source category
 386-387  I2    ---         MHCONB  * 2 or >=3 hours-confirmed coverages
                                      for this lune bin
     389  A1    ---         CQDOT    [q] q = in QDOT 1-in-6 sample
 390-393  I4    km/s        W20     *HI (21cm) 20% velocity width or flag
 394-395  I2    km/s      e_W20      Error on W20
 396-399  I4    km/s        W50     *HI (21cm) 50% velocity width or flag
 400-401  I2    km/s      e_W50      Error on W50
 402-403  I2    ---       r_W20     *HI reference
 404-410  F7.3  Jy          FP12     Addscan flux at 12um using point
                                      source template
 411-419  F9.3  Jy          FP25     Addscan flux at 25um using point
                                      source template
 420-428  F9.3  Jy          FP60     Addscan flux at 60um using point
                                      source template
 429-437  F9.3  Jy          FP100    Addscan flux at 100um using point
                                      source template
 439-442  I4    mJy       e_FP12     Statistical error in FP12
 443-446  I4    mJy       e_FP25     Statistical error in FP25
 447-450  I4    mJy       e_FP60     Statistical error in FP60
 451-454  I4    mJy       e_FP100    Statistical error in FP100
     456  I1    ---         BP12     Background fit subtracted or not at 12um
     457  I1    ---         BP25     Background fit subtracted or not at 25um
     458  I1    ---         BP60     Background fit subtracted or not at 60um
     459  I1    ---         BP100    Background fit subtracted or not at 100um
 460-468  F9.3  Jy          FE12     Coadded or extended addscan flux at 12um
 469-477  F9.3  Jy          FE25     Coadded or extended addscan flux at 25um
 478-486  F9.3  Jy          FE60     Coadded or extended addscan flux at 60um
 487-495  F9.3  Jy          FE100    Coadded or extended addscan flux at 100um
 497-500  I4    mJy       e_FE12     Statistical error in FE12
 501-504  I4    mJy       e_FE25     Statistical error in FE25
 505-508  I4    mJy       e_FE60     Statistical error in FE60
 509-512  I4    mJy       e_FE100    Statistical error in FE100
     514  I1    ---         BE12    *[0-2] Background fit at 12un
     515  I1    ---         BE25    *[0-2] Background fit at 25um
     516  I1    ---         BE60    *[0-2] Background fit at 60um
     517  I1    ---         BE100   *[0-2] Background fit at 100um
 518-525  F8.4 arcmin+2     WIDTH2   Addscan width squared at 60um
 526-533  F8.4 arcmin+2   e_WIDTH2   Error on WIDTH2
--------------------------------------------------------------------------------
Note on CPSCZ: source category:
   = PSC (or PSC reject file) source, and not a large-diameter optical galaxy.
   + addscanned large optical galaxy added to PSCz.
   - PSC source associated with a "+" addscan object (normally excluded).
   & high latitude PSCz source, but in a bin excluded by psczmask.dat .
   ^ high latitude optical galaxy, in a bin excluded by psczmask.dat .

Note on CZSTAT: redshift status:
   1 PSCz redshift, excellent quality
   2 PSCz redshift, good quality
   3 PSCz redshift, low s/n but secure
   4 PSCz redshift, marginal detection, unreliable
   l literature redshift, see r_Hvel for details.
   p private communication, see r_Hvel for details.
   q redshift from QDOT (J/MNRAS/308/897) or QCCOD
   # redshift wanted for PSCz, but still unknown
   x Give up, too optically faint (B or b_J > 19.5 mag)
   - Don't need it: galactic source, duplicate, part of larger galaxy etc.

Note on CNAME: IRAS Names.
  Digits hhmmm+ddmm as in PSC. The initial letter means:
    Q: from QIGC (Cat. J/MNRAS/253/485)
    P: from PSC  (Cat. II/215)
    R: from PSC reject file
    O: from optical catalogue

Note on q_S12, q_S25, q_S60, q_S100:
    1 = upper limit, 2 = moderate, 3 = OK, 4 = new HCON merged flux,
    5 = addscanned flux/1.1, 6 = coadded flux,
    7 = addscanned flux with point source template, 9 = single HCON.

Note on CES12, CES25, CES60, CES100:
    1 = flagged as confirmed extended source,
    2 = in SSS (Small Scale Structure) catalog (Cat. <VII/73>)
    3 = in Large Galaxy Catalog,
    4 = addscan flux,
    5 = addscan flux, source is double,
    6 = coadd flux,
    7 = coadd flux, source is double,
    8 = addscanned flux, Yahil software used,
    9 = addscanned point source flux, Yahil software used.
   2-8 data from QIGC, there should be none in here except class='ds' sources.

Note on Cirr1, Cirr2, Cirr3:
    The cirrus flag measures the number of sources detected only at
    100{mu}m in a 1-{deg}^2^ area around the source

Note on FCOR60: FCOR60 = NINT(FCOR(3) *1000)
    FCOR = correction factors applied to correct for overestimated faint
    fluxes as in Explanatory Supp. For the supplementary single-HCON
    sources, we have applied a factor of 1.121, as used in the PSC for 2
    out of possible 4 HCON detections. For merged single-HCON sources,
    unmerged in PSC due to software errors, we have corrected the
    correction factors accordingly.

Note on IOPT: Source of Schmidt plate material.
    1 = POSS-O/APM,        2 = SRC-bJ/APM,
    3,4,5 = SRC-bJ/Cosmos, 6 = SR/Cosmos,
    7 = POSS-E/APM,        9 = RC3 diameters .
    The optical information from plate scans is for the candidate with the
    best likelihood, not necessarily that for which the redshift is taken.
    The probability that these are the same depends strongly on latitude;
    at high latitude they are very reliable.

    The optical material is heterogeneous and except for IOPT=2 is
    uncalibrated. IOPT=6 magnitudes are estimated red mags, otherwise B or
    b_J. Due to saturation, magnitudes brighter than about 16 mag are very
    unreliable. Where a correct bright galaxy has been misclassified by
    the source-finding software as a star, the magnitude will be
    meaningless.

Note on D1X, AR:
    CATX is the all-sky optical galaxy compilation based on the CGCG, UGC,
    MGC and the ESO catalogues

Note on r_Hvel, r_Hvel2: Velocity references
  (negative reference numbers are PSCz or private communication)
   -99 INT/FOS or AAT/FORS
   -98 NOT
   -97 CTIO 60"
   -96 Fairall for PSCz
   -95 Nancay measurements for PSCz
   -94 AAT service data
   -93 INT/IDS500
   -92 Cananea
   -91 Parkes
   -90 WHT/FOSII
   -32 Juraszek
   -31 Visnanathan
   -30 Kraan-Kortweg
   -29 Lu, Pantoja
   -28 Nancay
   -27 Chamaraux, Yamada, Takata, Nakanishi
   -25 WHT Ultraluminous
   -24 QCCOD pole extension
   -23 QCCOD
   -21 Giovanelli + Haynes
   -20 DaCosta
   -10 - 70  as in Huchra 1991, See Cat. <VII/193>
    83  QDOT, Lawrence et al., Cat. <J/MNRAS/308/897>
    84  Leech et al., 1988MNRAS.231..977L
    85  NED, see http://nedwww.ipac.caltech.edu/
    86  PGC (Cat. <VII/119>), LEDA
    87  1.2Jy, Cat. <VII/185>
    88  Allen et al., 1990ApJ...355..130A
    89  Seeberger
    90  RC3 HI, Cat. <VII/155>
    91  RC3 optical, Cat. <VII/155>
    92  Fairall
    97  Tully 1987ApJ...321..280T
    98  Lonsdale and Hacking 1989ApJ...339..712L,
        Lonsdale 1986 (see Eales et al., 1988ApJ...328..530E)

Note on ALI100, ALI100B, ABB:
  100um backgrounds from Rowan-Robinson et al., 1991MNRAS.249..729R
   ALI4 is the background in a 0.5 degree beam centered on the source,
        corrected for that point source only.
  ALI4B is the background averaged over lune bin, and is corrected for
        all IGAL sources.
    ABB is based on ALI4B, and has been crudely corrected for
        temperature variation of dust across the galaxy.

Note on MHCONB:
    MHCONB is the number of HCON coverages, crudely estimated from
    Explanatory Supp Fig I.C.1, for comparing source counts, fluxes etc.

Note on W20, W50:
    The HI data is extremely heterogeneous in quality, reduction and
    linewidth definition.
    -999 = private,
    -997 = not reduced,
    -996 = to be observed,
    -995 = s/n < 5
    -994 = detected OK but not measured,
      -1 = non-detection,
      -2 = confused,

Note on r_W20: HI references:
      -5  Parkes (Cat. <VIII/15>)
      -4  Nancay for PSCz
      -3  Lu
      -2  Bottinelli
      -1  Giovanelli and Haynes
       1  LEDA
       2  Pantoja 1997, Cat. <J/AJ/113/905>
       3  Seeberger 1994, Cat. <J/A+A/286/17>

Note on BE12, BE25, BE60, BE100:
      0=no   1=yes   2=coadded flux

Note on CLASS: object classification from optical data etc.
     g : galaxy or galaxies
    gf: faint galaxy, B or b_j > 19.5 mag.
    go: optical galaxy with 1D addscanned flux
    gr: Rice et al galaxy with 2D coadded photometry
    ss: Star, confirmed spectroscopically (by us, 1.2 Jansky or de Grijp)
    bs: Bright star from plate or telescope TV, no spectrum
    is: Star from IRAS colours and plate/TV appearance
    c : Cirrus
    pn: Planetary Nebula
    rn: Reflection Nebula
    h2: HII region
    zz: Other galactic source
    lm: in Large Magellanic Cloud
    sm: in Small Magellanic Cloud
    vb: Visually blank on sky survey plates, no non-stellar id
    kb: K' image blank, no non-stellar id
    rb: Radio blank, no 6 or 20cm id
    de: delete from catalogue, part of extended galaxy
    d1: delete from catalogue, broken up 1HCON source already listed elsewhere
    du: deleted optical galaxy, part of multiple system unresolved by IRAS
    dr: deleted optical galaxy, already in as Rice etal galaxy
    ao: PSC source associated with addscanned optical galaxy
    ar: PSC source associated with Rice etal optical galaxy

    The divisions above between Galactic classifications 'pn','rn' etc are
    not rigorous.

    The CLASS='go' and 'gr' sources were optically selected (see
    accompanying paper) and their IRAS fluxes determined by addscanning or
    coadding. Their fluxes (F12 to F100) are addscan or coadded fluxes,
    reduced by a factor 1.1 to bring them statistically into line with PSC
    fluxes. Where the resulting flux F(3) is 0.6 Jy or greater, they are
    added to the catalogue and flagged with CPSCZ='+'. There are 1467 such
    sources representing 1402 individual galaxies resolved by IRAS. The
    associated PSC source is retained in the catalogue, but is flagged as
    CPSCZ='-' and will normally be excluded (1290 sources).
--------------------------------------------------------------------------------

Byte-by-byte Description of file: psczvs.dat psczcgvs.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  9  A9    ---     CPNAME    PSCz name eg A/123/456
      11  A1    ---     CPSCZ     Source category
      12  A1    ---     CZSTAT    Redshift status
  13- 14  A2    ---     CLASS     Optical classification code
  16- 17  I2    h       RAh       Rigth ascension B1950
  18- 19  I2    min     RAm       Rigth ascension B1950
  20- 22  I3    0.1s    RAds      Rigth ascension B1950
      24  A1    ---     DE-       Declination sign B1950
  25- 26  I2    deg     DEd       Declination B1950
  27- 28  I2    arcmin  DEm       Declination B1950
  29- 30  I2    arcsec  DEs       Declination B1950
  31- 36  F6.1  deg     GLON      Galactic longitude
  37- 42  F6.1  deg     GLAT      Galactic latitude
  43- 50  F8.2  Jy      F60       Flux at 60um
  51- 56  I6    km/s    Vhel      Best available heliocentric velocity (cz)
  57- 60  I4    km/s  e_Vhel      Error on heliocentric velocity
  61- 63  I3    ---   r_Vhel      Reference for heliocentric velocity
  64- 75  A12   ---     Oname     Optical name
  76- 79  I4    MJy/sr  I100B     100 micron background for that lune bin
  80- 84  F5.2  mag     ABB       Estimated average B extinction for that
                                   lune bin
      86  A1    ---     CHSD      High Source Density flag, hex encoded
      88  A1    ---     MHCONB    2 or >=3 hours-confirmed coverages for
                                   this lune bin
  89- 94  F6.2  ---     F100/F60  Ratio of 100micron/60micron flux,
                                   (negative means upper limit at 100um)
  95-100  I6    ---     NLBIN     Lune bin
--------------------------------------------------------------------------------

General Notes:
    Many fields are taken directly from Point Source Catalogue (II/125).
    See IRAS Explanatory Supplement (Beichman et al., 1988NASAR1190....1B)
    for more information.

    If there are problems that cannot be resolved by careful reading of
    these notes or the accompanying paper, please contact Will Saunders
    (will@roe.ac.uk) or Will Sutherland (W.Sutherland1@physics.ox.ac.uk).

Acknowledgements: Will Saunders <will@roe.ac.uk>
================================================================================
(End)              Will Saunders [ROE], Patricia Bauer [CDS]         19-May-2000

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