activity
19962008
most citedThe COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background: I. Limits and Detections

695 citations · 1.4k across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph2008★ 26 cited

Obscured and powerful AGN and starburst activities at z~3.5

M. Polletta, A. Omont, S. Berta +9

We report the discovery of two sources at z=3.867 and z=3.427 that exhibit powerful starburst and AGN activities. They benefit from data from radio to X rays from the CFHTLS-D1/SWI…

astro-ph1998★ 278 cited

Cosmic Histories of Stars, Gas, Heavy Elements, and Dust

Yichuan C. Pei, S. Michael Fall, Michael G. Hauser

We present a set of coupled equations that relate the stellar, gaseous, chemical, and radiation constituents of the universe averaged over the whole galaxy population. Using as inp…

astro-ph1998★ 695 cited

The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background: I. Limits and Detections

M. G. Hauser, R. G. Arendt, T. Kelsall +15

The DIRBE on the COBE spacecraft was designed primarily to conduct systematic search for an isotropic CIB in ten photometric bands from 1.25 to 240 microns. The results of that sea…

astro-ph1998★ 237 cited

The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background: IV. Cosmological Implications

E. Dwek, R. G. Arendt, M. G. Hauser +11

In this paper we examine the cosmological constraints of the recent DIRBE and FIRAS detection of the extragalactic background light between 125-5000 microns on the metal and star f…

astro-ph1997★ 45 cited

M87: A Misaligned BL LAC?

Zlatan I. Tsvetanov, George F. Hartig, Holland C. Ford +5

The nuclear region of M87 was observed with the Faint Object Spectrograph (FOS) on the Hubble Space Telescope (HST) at 6 epochs, spanning 18 months, after the HST image quality was…

astro-ph1996★ 72 cited

Cosmic Emissivity and Background Intensity from Damped Lyman-Alpha Galaxies

S. Michael Fall, Stephane Charlot, Yichuan C. Pei

We present a new method to compute the cosmic emissivity $\E_ν$ and background intensity . Our method is based entirely on data from quasar absorption-line studies, namely, th…