THE ASTRONOMICAL JOURNAL    VOLUME 112, NUMBER 2, PAGE 359          AUGUST 1996

         A MORPHOLOGICAL CATALOG OF GALAXIES IN THE HUBBLE DEEP FIELD

                             SIDNEY VAN DEN BERGH

   Dominion Astrophysical Observatory, National Research Council of Canada,
                    5071 West Saanich Road, V8X 4M6, Canada
                    Electronic mail: vandenbergh@dao.nrc.ca

             ROBERTO G. ABRAHAM, RICHARD S. ELLIS, NIAL R. TANVIR,
                            AND BASILO X. SANTIAGO

  Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA, United Kingdom
          Electronic mail: abraham, rse, nrt & santiago@ast.cam.ac.uk

                              KARL G. GLAZEBROOK

    Anglo-Australian Observatory, P.O. Box 296, Epping, NSW 2121, Australia
                        Electronic mail: kgb@aao.gov.au


                                   ABSTRACT

    We present a catalog of morphological and color data for galaxies with
    21 < I_814 < 25 mag in the Hubble Deep Field (Williams et al. 1996).
    Galaxies have been inspected and (when possible) independently visually
    classified on the MDS and DDO systems.  Measurements of central
    concentration and asymmetry are also included in the catalog.  The
    fraction of interacting and merging objects is seen to be significantly
    higher in the Hubble Deep Field than it is among nearby galaxies.
    Barred spirals are essentially absent from the deep sample.  The
    fraction of early-type galaxies in the Hubble Deep Field is similar to
    the fraction of early-types in the Shapley-Ames Catalog, but the
    fraction of galaxies resembling archetypal grand-design late-type
    spiral galaxies is dramatically lower in the distant HDF sample.