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20012011
most citedGalaxy Number Counts from the Sloan Digital Sky Survey Commissioning Data

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

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6 papers

astro-ph.CO2011★ 110 cited

Super-solar Metal Abundances in Two Galaxies at z ~ 3.57 revealed by the GRB 090323 Afterglow Spectrum

S. Savaglio, A. Rau, J. Greiner +12

We report on the surprisingly high metallicity measured in two absorption systems at high redshift, detected in the Very Large Telescope spectrum of the afterglow of the gamma-ray…

astro-ph2008★ 20 cited

A photometric redshift of for the \agile GRB 080514B

A. Rossi, A. de Ugarte Postigo, P. Ferrero +26

Aims: The AGILE gamma-ray burst GRB 080514B is the first burst with detected emission above 30 MeV and an optical afterglow. However, no spectroscopic redshift for this burst is kn…

astro-ph2008★ 226 cited

The 2175 A dust feature in a Gamma Ray Burst afterglow at redshift 2.45

T. Krühler, A. Küpcü Yoldaş, J. Greiner +6

We present optical and near-infrared photometry of the afterglow of the long Gamma-Ray Burst GRB 070802 at redshift 2.45 obtained with the ESO/MPI 2.2 m telescope equipped with the…

astro-ph2002★ 210 cited

XMM-Newton observation of the Lockman Hole II. Spectral analysis

V. Mainieri, J. Bergeron, G. Hasinger +5

We present the results of the X-ray spectral analysis of the first deep X-ray survey with the XMM-Newton observatory during Performance Verification. We restrict the analysis to th…

astro-ph2001★ 269 cited

Galaxy Number Counts from the Sloan Digital Sky Survey Commissioning Data

Naoki Yasuda, Masataka Fukugita, Vijay K. Narayanan +10

We present bright galaxy number counts in five broad bands () from imaging data taken during the commissioning phase of the Sloan Digital Sky Survey (SDSS). The…

astro-ph2001★ 201 cited

New Results from the X-ray and Optical Survey of the Chandra Deep Field South: The 300ks Exposure

P. Tozzi, P. Rosati, M. Nonino +15

We present results from 300 ks of X-ray observations of the Chandra Deep Field South. The field of the four combined exposures is now 0.1035 deg^2 and we reach a flux limit of 10^{…