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19952020
most citedNew Insight on Galaxy Formation and Evolution from Keck Spectroscopy of the Hawaii Deep Fields

1.6k citations · 13.9k across the 136 of their papers we have counts for

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Showing 1998Show all

7 papers · 1 filter

astro-ph1998★ 105 cited

B2045+265: A New Four-Image Gravitational Lens from CLASS

C. D. Fassnacht, R. D. Blandford, J. G. Cohen +14

We have discovered a new gravitational lens in the Cosmic Lens All-Sky Survey (CLASS). B2045+265 is a four-image system with a maximum separation of 1.9 arcsec. A fifth radio compo…

astro-ph1998★ 45 cited

Caltech Faint Galaxy Redshift Survey VIII: Analysis for the Field J0053+1234

Judith G. Cohen, Roger Blandford, David W. Hogg +2

The results of a spectroscopic investigation of a complete sample of objects with mag in a 2 by 7.3 arcmin field at J005325+1234 are reported. Redshifts were successfully…

astro-ph1998★ 44 cited

Caltech Faint Galaxy Redshift Survey VII: Data Analysis Techniques and Redshifts in the Field J0053+1234

Judith G. Cohen, David W. Hogg, Michael A. Pahre +3

We present the techniques used to determine redshifts and to characterize the spectra of objects in the Caltech Faint Galaxy Redshift Survey in terms of spectral classes and redshi…

astro-ph1998

The Extremely Red Objects Found Thus Far in the Caltech Faint Galaxy Redshift Survey

Judith G. Cohen, David W. Hogg, Roger Blandford +2

We discuss the very red objects found in the first field of the Caltech Faint Galaxy Redshift Survey, for which the observations and analysis are now complete. In this field, which…

astro-ph1998★ 176 cited

The oxygen-II luminosity density of the Universe

David W. Hogg, Judith G. Cohen, Roger Blandford +1

Equivalent widths of [OII] 3727 A lines are measured in 375 faint galaxy spectra taken as part of the Caltech Faint Galaxy Redshift Survey centered on the Hubble Deep Field. The se…

astro-ph1998★ 27 cited

An Old Cluster in NGC 6822

Judith G. Cohen, John P. Blakeslee

We present spectroscopy of two clusters in the dwarf irregular galaxy NGC 6822. From these we deduce an age for Cluster VII of 11 Gyr and [Fe/H] = -1.95 +/- 0.15 dex. Cluster VII a…