most citedThe Sloan Digital Sky Survey-II Supernova Survey: Technical Summary

471 citations · 471 across the 1 of their papers we have counts for

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astro-ph20081.9k cited

The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies

Charlie Conroy, James E. Gunn, Martin White

The stellar masses, mean ages, metallicities, and star formation histories of galaxies are now commonly estimated via stellar population synthesis (SPS) techniques. SPS relies on s…

astro-ph2008573 cited

The Milky Way Tomography with SDSS: II. Stellar Metallicity

Zeljko Ivezic, Branimir Sesar, Mario Juric +50

Using effective temperature and metallicity derived from SDSS spectra for ~60,000 F and G type main sequence stars (0.2<g-r<0.6), we develop polynomial models for estimating these…

astro-ph200814 cited

The SDSS Discovery of a Strongly Lensed Post-Starburst Galaxy at z=0.766

Min-Su Shin, Michael A. Strauss, Masamune Oguri +4

We present the first result of a survey for strong galaxy-galaxy lenses in Sloan Digital Sky Survey (SDSS) images. SDSS J082728.70+223256.4 was selected as a lensing candidate usin…

astro-ph200744 cited

Optical Cluster-Finding with An Adaptive Matched-Filter Technique: Algorithm and Comparison with Simulations

Feng Dong, Elena Pierpaoli, James E. Gunn +1

We present a modified adaptive matched filter algorithm designed to identify clusters of galaxies in wide-field imaging surveys such as the Sloan Digital Sky Survey. The cluster-fi…

astro-ph2007471 cited

The Sloan Digital Sky Survey-II Supernova Survey: Technical Summary

Joshua A. Frieman, B. Bassett, A. Becker +98

The Sloan Digital Sky Survey-II (SDSS-II) has embarked on a multi-year project to identify and measure light curves for intermediate-redshift (0.05 < z < 0.35) Type Ia supernovae (…

astro-ph20061.4k cited

Cosmological Constraints from the SDSS Luminous Red Galaxies

M Tegmark, D Eisenstein, M Strauss +64

We measure the large-scale real-space power spectrum P(k) using luminous red galaxies (LRGs) in the Sloan Digital Sky Survey (SDSS) and use this measurement to sharpen constraints…