activity
19962005
most citedSpectroscopic Studies of z~5.7 and z~6.5 Galaxies: Implications for Reionization

6 citations · 6 across the 1 of their papers we have counts for

collaborators

8 papers

astro-ph20056 cited

Spectroscopic Studies of z~5.7 and z~6.5 Galaxies: Implications for Reionization

Esther M. Hu, Lennox L. Cowie, Peter Capak +1

The recent development of large, complete samples which identify high-redshift galaxies at z~5.7 and z~6.5 from deep, wide-field surveys provides detailed information on the earlie…

astro-ph2002

The Nature of the faint far-infrared extragalactic source population: Optical/NIR and radio follow-up observations of ISOPHOT deep-field sources using Keck, Subaru, and VLA telescopes

Yuko Kakazu, D. B. Sanders, R. D. Joseph +11

We report on optical and near-infrared (NIR) follow-up spectroscopy of faint far-infrared (FIR) sources found in our deep FIR survey by Kawara et al.

astro-ph2000

ISO deep far-infrared survey in the "Lockman Hole" II. Power spectrum analysis: evidence of a strong evolution in number counts

H. Matsuhara, K. Kawara, Y. Sato +8

We investigate the characteristics of FIR brightness fluctuations at 90 micron and 170 micron in the Lockman Hole, which were surveyed with ISOPHOT aboard the Infrared Space Observ…

astro-ph1999

Galaxies at z>5: The View from Hawaii

Esther M. Hu, Lennox L. Cowie, Richard G. McMahon

We review the properties of z>5 galaxies studied with HST and with the Keck telescopes, and discuss the detectability of Lyman alpha emission-line galaxies out to z~6.5 based on th…

astro-ph1999

High Resolution Radio Imaging of Distant Submillimeter Galaxies

E. A. Richards, F. E. Bauer, A. J. Barger +1

Using a combination of radio and optical imaging at 0.1\arcs to 0.2\arcs resolution with the VLA/MERLIN and HST has led to a breakthrough in our understanding of radio emission fro…

astro-ph1999

The view of galaxy formation from Hawaii: Seeing the dark side of the universe

L. L. Cowie, A. J. Barger

The strength of the submillimeter background light shows directly that much of the energy radiated by star formation and AGN is moved to far infrared wavelengths. However, it is on…