output
19952026
most citedObservational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

19.6k citations

Showing 2016Show all

78 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★ 23 cited

Velocity Segregation and Systematic Biases In Velocity Dispersion Estimates With the SPT-GMOS Spectroscopic Survey

Matthew. B. Bayliss, Kyle Zengo, Jonathan Ruel +15

The velocity distribution of galaxies in clusters is not universal; rather, galaxies are segregated according to their spectral type and relative luminosity. We examine the velocit…

astro-ph.SR2016★ 178 cited

The Gould's Belt Distances Survey (GOBELINS) I. Trigonometric parallax distances and depth of the Ophiuchus complex

Gisela N. Ortiz-León, Laurent Loinard, Marina A. Kounkel +14

We present the first results of the Gould's Belt Distances Survey (GOBELINS), a project aimed at measuring the proper motion and trigonometric parallax of a large sample of young s…

astro-ph.GA2016★ 28 cited

A Study of Quasar Selection in the Dark Energy Survey Supernova fields

S. S. Tie, P. Martini, D. Mudd +75

We present a study of quasar selection using the DES supernova fields. We used a quasar catalog from an overlapping portion of the SDSS Stripe 82 region to quantify the completenes…

astro-ph.GA2016★ 13 cited

Stellar Populations of Shell Galaxies

S. Carlsten, G. K. T. Hau, A. Zenteno

We present a study of the inner (out to 1 R) stellar populations of 9 shell galaxies. We derive stellar population parameters from long slit spectra by both…