Catalogues and tables

• Groth Survey Strip

  
  
  • Koo et al. 1996, ApJ 469, 535
    
    • Table 1

  • Simard et al., 2002, ApJS, 142, 1 :
    • Catalogue of structural parameters using separate fits in V606 and I814 for galaxies in the Groth Survey Strip.
    • Catalogue of structural parameters using simultaneous fit in V606 and I814 for galaxies in the Groth Survey Strip.
    • Catalogue of simulations for separate fits of structural parameters.
    • Catalogue of simulations for simultaneous fits of structural parameters

  • Im et al., 2002, ApJ, 571, 136
    • Catalogue of Elliptical galaxies in the Groth Survey Strip
    • Equatorial coordinates of the Elliptical galaxies in the Groth Survey Strip

  • Weiner et al. 2005, ApJ, accepted
    • Redshift catalogue

  • Vogt et al. 2005, ApJS, submitted
    • GSS Source catalogue

• Hubble Deep Field North and Flanking Fields

  • Lowenthal et al. 1997, ApJ 481, 673
    
    • Table 1
      
    • Table 2
      
    • Table 3
      

  • Phillips et al. 1997, ApJ 489, 543
    
    • Table 1
    • Table 2

  • Guzmán et al. 1997, ApJ 489, 559
    
    • Table 1

  • Mendez & Guzmán 1998, A&A, 333, 106
    
    • Table 1
    • Table 2

  • Unpublished Catalogue of Galaxies identified by the DEEP Team in the Flanking Fields. This is the source catalogue that Vogt et al. (1997), Phillips et al. (1997), Guzmán et al. (1997), and Mendez & Guzmán (1998) used to select objects. The column description file is also available.
    

    The photometry in this catalogue was carried out using circular apertures of 3 arc sec diameter, as described by Phillips et al. (1997). These will present small differences ( ~ 0.12 mag, rms) relative to published values for the sample of 51 compact galaxies that were analysed by Phillips et al. (1997) and Guzmán et al. (1997). This is because for the papers, the I814 magnitudes were recalculated using elliptical apertures to 8 arc sec . The differences should only be significant in the case of galaxies with larger apparent sizes or with elongated shapes.
    

    The notes explain how the V-I colours in the catalogue were calculated. See also the web page describing the astrometric solution which was written by Lowenthal, Guzmán and Gallego.
    In the downloadable table, the 103 DEEP team redshifts in the Flanking Fields have been included. Stars that were spectroscopically confirmed by our own observations have z = 0, while unmeasured quantities have been assigned INDEF values.
    

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