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19942026
most citedThe Baryon Oscillation Spectroscopic Survey of SDSS-III

2.1k citations · 66.4k across the 576 of their papers we have counts for

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Showing 2003Show all

12 papers · 1 filter

astro-ph2003★ 120 cited

The Abundance of Low-luminosity Lyman alpha Emitters at High Redshift

Michael R. Santos, Richard S. Ellis, Jean-Paul Kneib +2

We derive the luminosity function of high-redshift Lyman alpha emitting sources from a deep, blind, spectroscopic survey that utilized strong-lensing magnification by intermediate-…

astro-ph2003★ 37 cited

An ISOCAM survey through gravitationally lensing galaxy clusters. IV. Luminous infrared galaxies in Cl 0024+1654 and the dynamical status of clusters

D. Coia, B. McBreen, L. Metcalfe +9

Observations of the core of the massive cluster Cl 0024+1654, at a redshift z=0.39, were obtained with the Infrared Space Observatory using ISOCAM at 6.7 mum and 14.3 mum (hereafte…

astro-ph2003★ 125 cited

Weak lensing mass distributions for 24 X-Ray Abell Clusters

Eduardo S. Cypriano, Laerte Sodré, Jean-Paul Kneib +1

We use the weak gravitational lensing effect to study the mass distribution and dynamical state of a sample of 24 X-ray luminous clusters of galaxies () observed with…

astro-ph2003

Measuring the matter distribution within z=0.2 cluster lenses with XMM-Newton

P. B. Marty, J. -P. Kneib, R. Sadat +4

We present an analysis of 7 clusters observed by XMM as part of our survey of 17 most X-ray luminous clusters of galaxies at z=0.2 selected for a comprehensive and unbiased study o…

astro-ph2003★ 12 cited

Discovery of a faint R-band drop-out: a strongly reddened lensed star forming galaxy at z=1.68

J. Richard, D. Schaerer, R. Pello +2

We report the discovery of an unusual emission line galaxy at redshift z=1.68 found from near-IR imaging and spectroscopic observations with ISAAC/VLT of a faint gravitationally le…

astro-ph2003★ 1 cited

Searches for high redshift galaxies using gravitational lensing

J. Richard, R. Pello, J. -P. Kneib +3

We present different methods used to identify high redshift (z>5) objects in the high-magnification regions of lensing galaxy clusters, taking advantage of very well constrained le…