activity
20112025
most citedThe Baryon Oscillation Spectroscopic Survey of SDSS-III

2.1k citations · 5.1k across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.IM2025

Semantic search for 100M+ galaxy images using AI-generated captions

Nolan Koblischke, Liam Parker, Francois Lanusse +3

Finding scientifically interesting phenomena through slow manual labeling campaigns severely limits our ability to explore the billions of galaxy images produced by telescopes. In…

astro-ph.GA2023★ 1 cited

Leaving No Branches Behind: Predicting Baryonic Properties of Galaxies from Merger Trees

Chen-Yu Chuang, Christian Kragh Jespersen, Yen-Ting Lin +2

Galaxies play a key role in our endeavor to understand how structure formation proceeds in the Universe. For any precision study of cosmology or galaxy formation, there is a strong…

astro-ph.CO2016★ 197 cited

The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in configuration space

Yuting Wang, Gong-Bo Zhao, Chia-Hsun Chuang +20

We perform a tomographic baryon acoustic oscillations analysis using the two-point galaxy correlation function measured from the combined sample of BOSS DR12, which covers the reds…

astro-ph.CO2015★ 219 cited

The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies

Héctor Gil-Marín, Will J. Percival, Joel R. Brownstein +13

We measure and analyse the clustering of the Baryon Oscillation Spectroscopic Survey (BOSS) relative to the line-of-sight (LOS), for LOWZ and CMASS galaxy samples drawn from the fi…

astro-ph.CO2015★ 16 cited

The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Effect of smoothing of density field on reconstruction and anisotropic BAO analysis

M. Vargas-Magaña, S. Ho, S. Fromenteau +1

The reconstruction algorithm introduced by \cite{Eis07}, which is widely used in clustering analysis, is based on the inference of the first order Lagrangian displacement field fro…

astro-ph.CO2013★ 97 cited

Spectroscopic Needs for Imaging Dark Energy Experiments: Photometric Redshift Training and Calibration

J. Newman, A. Abate, F. Abdalla +58

Large sets of objects with spectroscopic redshift measurements will be needed for imaging dark energy experiments to achieve their full potential, serving two goals:_training_, i.e…