activity
19932023
most citedThe Sloan Digital Sky Survey: Technical Summary

10.4k citations · 99.4k across the 342 of their papers we have counts for

collaborators
Showing 2016Show all

12 papers · 1 filter

astro-ph.IM2016★ 236 cited

The DESI Experiment Part II: Instrument Design

DESI Collaboration, Amir Aghamousa, Jessica Aguilar +290

DESI (Dark Energy Spectropic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations and the growth of structure through redshift…

astro-ph.IM2016★ 1.3k cited

The DESI Experiment Part I: Science,Targeting, and Survey Design

DESI Collaboration, Amir Aghamousa, Jessica Aguilar +290

DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations (BAO) and the growth of structure through…

astro-ph.CO2016★ 49 cited

Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: application to the SDSS-III BOSS DR12 galaxies

Xiao-Dong Li, Changbom Park, Cristiano G. Sabiu +5

We apply the methodology developed in \cite{Li2014,Li2015} to BOSS DR12 galaxies and derive cosmological constraints from the redshift dependence of the Alcock-Paczynski (AP) effec…

astro-ph.GA2016★ 445 cited

The Sloan Digital Sky Survey Quasar Catalog: twelfth data release

Isabelle Pâris, Patrick Petitjean, Nicholas P. Ross +43

We present the Data Release 12 Quasar catalog (DR12Q) from the Baryon Oscillation Spectroscopic Survey (BOSS) of the SDSS-III. This catalog includes all SDSS-III/BOSS objects that…

astro-ph.GA2016★ 10 cited

The Chemical Abundance Structure of the Inner Milky Way: A Signature of "Upside-Down" Disk Formation?

Jenna K. C. Freudenburg, David H. Weinberg, Michael R. Hayden +1

We present a model for the [alpha/Fe]-[Fe/H] distribution of stars in the inner Galaxy, R=3-5 kpc, measured as a function of vertical distance |z| from the midplane by Hayden et al…

astro-ph.CO2016★ 15 cited

Galaxy Three-Point Correlation Functions and Halo/Subhalo Models

Hong Guo, Zheng Zheng, Peter S. Behroozi +9

We present the measurements of the luminosity-dependent redshift-space three-point correlation functions (3PCFs) for the Sloan Digital Sky Survey (SDSS) DR7 Main galaxy sample. We…

astro-ph.CO2016★ 3.1k cited

The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample

Shadab Alam, Metin Ata, Stephen Bailey +69

We present cosmological results from the final galaxy clustering data set of the Baryon Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III. Our combined gal…

astro-ph.GA2016★ 115 cited

Equilibrium and Sudden Events in Chemical Evolution

David H. Weinberg, Brett H. Andrews, Jenna Freudenburg

We present new analytic solutions for one-zone (fully mixed) chemical evolution models and explore their implications. In contrast to existing analytic models, we incorporate a rea…

astro-ph.GA2016★ 171 cited

Inflow, Outflow, Yields, and Stellar Population Mixing in Chemical Evolution Models

Brett H. Andrews, David H. Weinberg, Ralph Schönrich +1

Chemical evolution models are powerful tools for interpreting stellar abundance surveys and understanding galaxy evolution. However, their predictions depend heavily on the treatme…

astro-ph.GA2016★ 49 cited

On the Deuterium-to-Hydrogen Ratio of the Interstellar Medium

David H. Weinberg

Observations show that the global deuterium-to-hydrogen ratio (D/H) in the local interstellar medium (ISM) is about 90% of the primordial ratio predicted by big bang nucleosynthesi…

astro-ph.GA2016★ 263 cited

Selection bias in dynamically-measured super-massive black hole samples: its consequences and the quest for the most fundamental relation

Francesco Shankar, Mariangela Bernardi, Ravi K. Sheth +7

We compare the set of local galaxies having dynamically measured black holes with a large, unbiased sample of galaxies extracted from the Sloan Digital Sky Survey. We confirm earli…

astro-ph.CO2016★ 44 cited

The effects of assembly bias on cosmological inference from galaxy-galaxy lensing and galaxy clusters

Joseph E. McEwen, David H. Weinberg

The combination of galaxy-galaxy lensing (GGL) and galaxy clustering is a promising route to measuring the amplitude of matter clustering and testing modified gravity theories of c…