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J/ApJS/111/143      Virgo cluster ultraviolet sources (Brosch+ 1997)
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Faust observations of ultraviolet sources toward the Virgo cluster
      Brosch N., Formiggini L., Almoznino E., Sasseen T., Lampton M., Bowyer S.
     <Astrophys. J. Suppl. Ser. 111, 143 (1997)>
     =1997ApJS..111..143B      (SIMBAD/NED BibCode)
================================================================================
ADC_Keywords: Clusters, galaxy ; Photometry, ultraviolet ; Photometry, UBV
Mission_Name: FAUST
Keywords: galaxies: clusters: individual (Virgo) -
          galaxies: fundamental parameters - ultraviolet: galaxies -
          ultraviolet: stars

Abstract:
    We analyze three UV images covering a ~100 square degree field toward
    the Virgo cluster, obtained by the FAUST space experiment. We detect
    191 sources to a signal-to-noise ratio of 4.4 and identify 94% of
    them. Most sources have optical counterparts in existing catalogs, and
    about half are identified as galaxies. Some sources with no listed
    counterpart were observed at the Wise Observatory. We present the
    results of low-resolution visible spectrophotometry and discuss the
    foreground 101 stellar sources and the 76 detected galaxies, both in
    the cluster and in the foreground or background. We derive conclusions
    on star formation properties of galaxies and on the total UV flux from
    discrete and diffuse sources in the cluster. We test for the presence
    of intracluster dust, determine the clustering properties of UV
    emitting galaxies, and derive the UV luminosity function of Virgo
    galaxies.

File Summary:
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  FileName  Lrecl  Records  Explanations
--------------------------------------------------------------------------------
ReadMe         80        .  This file
table1         76      191  Detected FAUST sources in the Virgo images
table2         73      101  Stars toward the Virgo cluster
table4         80       76  Galaxies toward the Virgo cluster-ultraviolet data
table5         80       76  Galaxies toward the Virgo cluster-multispectral data
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See also:
          VII/48 : Catalogue of middle UV photometry of Virgo cluster galaxies
   J/ApJS/96/461 : Far-UV Point Sources (Bowyer+ 1995)

Byte-by-byte Description of file: table1
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   Bytes Format Units   Label     Explanations
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   1-  3  I3    ---     ID        Identification number
       5  A1    ---   n_RAh       [*] Note (1)
   6-  7  I2    h       RAh       Right ascension (1950)
   9- 10  I2    min     RAm       Right ascension (1950)
  12- 15  F4.1  s       RAs       Right ascension (1950)
      16  A1    ---     DE-       Declination sign
  17- 18  I2    deg     DEd       Declination (1950)
  20- 21  I2    arcmin  DEm       Declination (1950)
  23- 24  I2    arcsec  DEs       Declination (1950)
  26- 30  F5.2  mag     UVmag     Adopted FAUST UV magnitude (2)
  32- 36  F5.3  mag   e_UVmag     ? rms uncertainty on UVmag
  37- 38  A2    ---   u_UVmag     [: ] Uncertainty flag on UVmag (3)
      40  I1    ---     Nobs      Number of observations (4)
  42- 60  A19   ---     Ident     Proposed identification
      61  A1    ---   n_Ident     [?] Note (5)
  63- 66  I4    ---     FAUST     ? Entry in FAUST catalog
      67  A1    ---     ---       [/]
  68- 71  I4    ---     FAUST2    ? Second entry in FAUST catalog
      72  A1    ---     ---       [/]
  73- 76  I4    ---     FAUST3    ? Third entry in FAUST catalog
--------------------------------------------------------------------------------
Note (1): An * indicates objects for which the coordinates were calculated from
           an astrometric solution based in bright, well-identified stellar
           images.
Note (2): The adopted UV magnitude is the average of the different FAUST
           measurements. The error is the root mean square of the individual
           errors.
Note (3): A colon (:) indicates a very large measurement error.
Note (4): Nobs is the number of times a source was observed, i.e., the number
           of FAUST images in which it appears.
Note (5): The question mark (?) at ID 44, ID 57, and ID 69 indicates that the
           proposed identification is a bit off the FAUST source.
          ID  52: The UV source may be a blend of the emission from the galaxy
                    and the HD 108285 (A2) star.
          ID 155: The three stars near the FAUST source have been observed
                   spectroscopically and identified with late G or K star.
                   The proposed identification is the faint KARA 68181 galaxy
                   marked on the overlays of the PSS. Note that there is a dE
                   galaxy (VCC 1866) a bit far from the FAUST source.
          ID 164: This source is near the TD-1 26442 from the Extended TD-1
                   catalog (preprint). On the PSS there is a faint V>15 blue
                   looking candidate 123945+163743 not observed.
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Byte-by-byte Description of file: table2
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   Bytes Format Units   Label   Explanations
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   1-  3  I3    ---     Source  Source number
   5- 22  A18   ---     Name    Identification name
  24- 28  A5    ---     SpType  Spectral classification (1)
      30  A1    ---   l_Vmag    Limit flag on Vmag
  31- 35  F5.2  mag     Vmag    ? V or B magnitude (2)
      37  A1    ---   n_Vmag    [B] B: B magnitude in Vmag, else V magnitude
  39- 43  F5.2  mag     B-V     ? B-V colour index (2)
  45- 49  F5.2  mag     U-B     ? U-B colour index (2)
  51- 55  F5.2  mag     UVmag   FAUST UV magnitude
  56- 57  A2    ---   u_UVmag   [: ] Uncertainty flag on UVmag
  58- 61  F4.2  mag   e_UVmag   ? rms uncertainty on UVmag
  64- 73  A10   ---     Other   Other Identifications
--------------------------------------------------------------------------------
Note (1): The spectral classification is mainly from HIC (Cat. <I/196>), in
            which case the HIC number is marked in Other
           The stars classified from WiseObs spectra have the note (e) early,
           or (l) late, according to the appearance or absence of spectral
           features in our low-resolution spectra.
Note (2): The V, B-V and U-B data are from HIC (Cat. <I/196>), or from
           SAO (Cat. <I/111>) when the star is an SAO object but not a HIC
           object or from the HD (Cat. <III/135>) catalog if not in either of
           the two. Seven PG objects have spectral and photometric data from
           Green et al. (1986, Cat. <II/207>).
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Byte-by-byte Description of file: table4
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   Bytes Format Units   Label     Explanations
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   1-  3  I3    ---     Source    Source number
   5- 15  A11   ---     Name      Name
  18- 38  A21   ----    MType     Morphological type
  40- 44  F5.2  mag     4*E(B-V)  Reddening
  47- 51  F5.2  mag     UVmag     FAUST UV magnitude
  53- 56  F4.2  mag   e_UVmag     rms uncertainty on FAUST UV magnitude
      58  A1    ---   l_GUV       Limit flag on GUV
  59- 63  F5.2  mag     GUV       ? GUV UV magnitude (Kodaira et al.,
                                     1990ApJ...363..422K) (1)
  65- 68  F4.2  mag   e_GUV       ? rms uncertainty on GUV
  70- 73  F4.1  mag     SCAP      ? SCAP UV magnitude (Donas et al.,
                                      1987A&A...180...12D) (1)
      75  A1    ---   l_S+C       Limit flag on S+C
  76- 80  F5.2  mag     S+C       ? S+C UV magnitude (Smith & Cornett, 1982,
                                     Cat. <VII/48>) (1)
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Note (1): All GUV measurements were transformed into monochromatic magnitudes.
           Note that each experiment measured at different spectral segment:
           GUV measured effectively at 1560{AA} with a bandwidth of FWHM=230{AA}
           SCAP measured at ~2000{AA} and the passband was ~200{AA}, and the
           Goddar imager (S+C) had a 1150{AA} wide passband centered
           near 2421{AA}
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Byte-by-byte Description of file: table5
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   Bytes Format Units     Label     Explanations
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   1-  3  I3    ---       Source    Source number
   5- 18  A14   ---       Name      Name
  20- 24  A5    ---       TType     T Type (1)
  26- 30  F5.2  mag       UVmag     FAUST UV magnitude
  32- 35  F4.2  mag     e_UVmag     rms uncertainty on UVmag
  37- 38  A2    ---     l_FI(HI)    [=< ] Limit flag on FI(HI)
  39- 47  F9.5  Jy.km/s   FI(HI)    ? H I flux integral (from the sources
                                       given in section 4.2)
  49- 51  F3.1  Jy.km/s   FI(HI)2   ? Second value of FI(HI) for N=171
  52- 56  F5.2  Jy        S60um     ? FIR flux densities at 60{mu}m (2)
  58- 62  F5.2  Jy        S100um    ? FIR flux densities at 100{mu}m (2)
  64- 68  I5    km/s      HRV       ? Heliocentric radial velocity (3)
  70- 74  F5.2  mag       Btot      ? Total B magnitude (3) (4)
      75  A1    ---       ---       [+]
  76- 80  F5.2  mag       Btot+     ? Additional Btot for sources 126 and 171
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Note (1): The T type is the translation of the morphological type(s) given in
           table 4, using the prescription from Table A of Tully 1988
            (Cat. <VII/145>).
Note (2): From IRAS Faint Source Catalogue (Cat. <II/156>)
Note (3): Data originate from BST (Binggelli et al., 1985AJ.....90.1681B),
           RC3 (Cat. <VII/155>, or UGC (Cat. <VII/26>).
Note (4):  Btot has been corrected for Galactic extinction, as explained in
           the text.
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History: Prepared via OCR at CDS.
================================================================================
(End)                           James Marcout, Patricia Bauer [CDS]  13-Oct-1997

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