Caltech Faint Galaxy Redshift Survey X: A Redshift Survey in the Region of the Hubble Deep Field North

Abstract

A redshift survey has been carried out in the region of the Hubble Deep Field North using the Low Resolution Imaging Spectrograph at the Keck Observatory. The resulting redshift catalog, which contains 671 entries, is a compendium of our own data together with published LRIS/Keck data. It is more than 92% complete for objects, irrespective of morphology, to $R=24$ mag in the HDF itself and to $R=23$ mag in the Flanking Fields within a diameter of 8 arcmin centered on the HDF, an unusually high completion for a magnitude limited survey performed with a large telescope. A median redshift $z=1.0$ is reached at $R\sim 23.8$. Strong peaks in the redshift distribution, which arise when a group or poor cluster of galaxies intersect the area surveyed, can be identified to $z\sim 1.2$ in this dataset. More than 68% of the galaxies are members of these redshift peaks. In a few cases, closely spaced peaks in $z$ can be resolved into separate groups of galaxies that can be distinguished in both velocity and location on the sky. The radial separation of these peaks in the pencil-beam survey is consistent with a characteristic length scale for the their separation of $\approx$70 Mpc in our adopted cosmology ($h=0.6,{\Omega }_M=0.3$, $\Lambda =0$). Strong galaxy clustering is in evidence at all epochs back to $z\le 1.1$. (abstract abridged)

Accepted to the ApJ. This version contains all the figures and tables. 2 minor typos in table 2b corrected

References in corpus (3)

• Optically Faint Microjansky Radio Sources
• The Merger Rate to Redshift One from Kinematic Pairs: Caltech Faint Galaxy Redshift Survey XI
• NICMOS Imaging of the Dusty Microjansky Radio Source VLA J123642+621331 at z = 4.424

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