447 citations · 974 across the 16 of their papers we have counts for
16 papers
The Star Formation Rate Intensity Distribution Function--Implications for the Cosmic Star Formation Rate History of the Universe
Kenneth M. Lanzetta, Noriaki Yahata, Sebastian Pascarelle +2
We address the effects of cosmological surface brightness dimming on observations of faint galaxies by examining the distribution of "unobscured" star formation rate intensities ve…
Discovery of the Galaxy Proximity Effect and Implications for Measurements of the Ionizing Background Radiation at Low Redshifts
Sebastian M. Pascarelle, Kenneth M. Lanzetta, Hsiao-Wen Chen +1
We present an analysis of galaxy and QSO absorption line pairs toward 24 QSOs at redshifts between z~0.2 and 1 in an effort to establish the relationship between galaxies and absor…
The Unusual Spectral Energy Distribution of a Galaxy Previously Reported to be at Redshift 6.68
Hsiao-Wen Chen, Kenneth M. Lanzetta, Sebastian Pascarelle +1
Observations of distant galaxies are important both for understanding how galaxies form and for probing the physical conditions of the universe at the earliest epochs. It is, howev…
On the compared accuracy and reliability of spectroscopic and photometric redshift measurements
Alberto Fernandez-Soto, Kenneth M. Lanzetta, Hsiao-Wen Chen +2
We present a comparison between the spectroscopic catalog of the HDF recently published by Cohen et al and the redshifts measured by our group for those objects using photometric t…
Photometry and Photometric Redshifts of Faint Galaxies in the Hubble Deep Field South NICMOS Field
Noriaki Yahata, Kenneth M. Lanzetta, Hsiao-Wen Chen +4
We present a catalog of photometry and photometric redshifts of 335 faint objects in the HDF-S NICMOS field. The analysis is based on (1) infrared images obtained with the Hubble S…
Galaxies of Redshift z > 5: The View from Stony Brook
Kenneth M. Lanzetta, Hsiao-Wen Chen, Alberto Fernandez-Soto +3
We report on some aspects of our efforts to establish properties of the extremely faint galaxy population by applying our photometric redshift technique to the HDF and HDF-S WFPC2…