Photometric Properties of Galaxies on Large Spatial Scales Centered on the Hubble Deep Field

Details Photometric Properties of Galaxies on Large Spatial Scales Centered on the Hubble Deep Field Photometric Properties of Galaxies on Large Spatial Scales Centered on the Hubble Deep Field

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aas...19110508p&link_type=abstract

American Astronomical Society, 191st AAS Meeting, #105.08; Bulletin of the American Astronomical Society, Vol. 29, p.1378

Astronomy and Astrophysics

Astronomy

Scientific paper

We have conducted a two-color survey of galaxies detected on the POSS-I fields covering a 96 square degree region centered on the Hubble Deep Field. We have investigated the photometric properties known to correlate with the Morphology-Density Relation as described by Odewahn and Aldering (1995). By constructing a galaxy surface density map, we can locate any large-scale regions of high or low density. The two-color survey map can also be used to study concentrations of early and late type galaxies.

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