activity
19922026
most citedThe Sloan Digital Sky Survey: Technical Summary

10.4k citations · 104.3k across the 663 of their papers we have counts for

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10 papers · 1 filter

astro-ph2008★ 5.4k cited

The Seventh Data Release of the Sloan Digital Sky Survey

K. Abazajian

This paper describes the Seventh Data Release of the Sloan Digital Sky Survey (SDSS), marking the completion of the original goals of the SDSS and the end of the phase known as SDS…

astro-ph2008★ 150 cited

Estimating the Redshift Distribution of Photometric Galaxy Samples II. Applications and Tests of a New Method

Carlos E. Cunha, Marcos Lima, Hiroaki Oyaizu +2

In Lima et al. 2008 we presented a new method for estimating the redshift distribution, N(z), of a photometric galaxy sample, using photometric observables and weighted sampling fr…

astro-ph2008★ 57 cited

Discovery of A Very Bright, Strongly-Lensed z=2 Galaxy in the SDSS DR5

Huan Lin, Elizabeth Buckley-Geer, Sahar S. Allam +8

We report on the discovery of a very bright z = 2.00 star-forming galaxy that is strongly lensed by a foreground z=0.422 luminous red galaxy (LRG). This system was found in a syste…

astro-ph2008★ 158 cited

Constraining the Scatter in the Mass-Richness Relation of maxBCG Clusters With Weak Lensing and X-ray Data

Eduardo Rozo, Eli S. Rykoff, August Evrard +10

We measure the logarithmic scatter in mass at fixed richness for clusters in the maxBCG cluster catalog, an optically selected cluster sample drawn from SDSS imaging data. Our meas…

astro-ph2008★ 1.9k cited

Dark Energy and the Accelerating Universe

Joshua Frieman, Michael Turner, Dragan Huterer

The discovery ten years ago that the expansion of the Universe is accelerating put in place the last major building block of the present cosmological model, in which the Universe i…

astro-ph2008★ 31 cited

Two More Candidate AM Canum Venaticorum (AM CVn) Binaries from the Sloan Digital Sky Survey

S. F. Anderson, A. C. Becker, D. Haggard +18

AM CVn systems are a select group of ultracompact binaries with the shortest orbital periods of any known binary subclass; mass-transfer is likely from a low-mass (partially-)degen…

astro-ph2008★ 43 cited

Average Properties of a Large Sample of z_abs ~ z_em associated Mg II Absorption Line Systems

D. Vanden Berk, P. Khare, D. G. York +16

We have studied a sample of 415 associated (z_ab z_em; relative velocity with respect to QSO <3000km/s) Mg II absorption systems with 1.0<=z_ab<=1.86, in the spectra of SDSS DR3 QS…

astro-ph2008★ 207 cited

Estimating the Redshift Distribution of Faint Galaxy Samples

Marcos Lima, Carlos E. Cunha, Hiroaki Oyaizu +3

We present an empirical method for estimating the underlying redshift distribution N(z) of galaxy photometric samples from photometric observables. The method does not rely on phot…

astro-ph2008★ 95 cited

The Correlation Function of Optically Selected Galaxy Clusters in the Sloan Digital Sky Survey

Juan Estrada, Emiliano Sefusatti, Joshua A. Frieman

We measure the two-point spatial correlation function for clusters selected from the photometric MaxBCG galaxy cluster catalog for the Sloan Digital Sky Survey (SDSS). We evaluate…

astro-ph2008★ 128 cited

A Measurement of the Rate of type-Ia Supernovae at Redshift 0.1 from the First Season of the SDSS-II Supernova Survey

Benjamin Dilday, R. Kessler, J. A. Frieman +50

We present a measurement of the rate of type Ia supernovae (SNe Ia) from the first of three seasons of data from the SDSS-II Supernova Survey. For this measurement, we include 17 S…