activity
20142026
most citedDark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

1.2k citations · 27.1k across the 411 of their papers we have counts for

collaborators
Showing 2016Show all

34 papers · 1 filter

astro-ph.GA2016

A stellar over-density associated with the Small Magellanic Cloud

A. Pieres, B. X. Santiago, A. Drlica-Wagner +64

We report the discovery of a stellar over-density 8 north of the center of the Small Magellanic Cloud (Small Magellanic Cloud Northern Over-Density; SMCNOD) using data fr…

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.CO2016★ 53 cited

Imprint of DES super-structures on the Cosmic Microwave Background

A. Kovács, C. Sánchez, J. García-Bellido +58

Small temperature anisotropies in the Cosmic Microwave Background can be sourced by density perturbations via the late-time integrated Sachs-Wolfe effect. Large voids and superclus…

astro-ph.HE2016★ 500 cited

Searching for Dark Matter Annihilation in Recently Discovered Milky Way Satellites with Fermi-LAT

The Fermi-LAT, DES Collaborations, A. Albert +70

We search for excess gamma-ray emission coincident with the positions of confirmed and candidate Milky Way satellite galaxies using 6 years of data from the Fermi Large Area Telesc…

astro-ph.CO2016★ 33 cited

Weak lensing magnification in the Dark Energy Survey Science Verification Data

M. Garcia-Fernandez, E. Sánchez, I. Sevilla-Noarbe +68

In this paper the effect of weak lensing magnification on galaxy number counts is studied by cross-correlating the positions of two galaxy samples, separated by redshift, using dat…

astro-ph.HE2016★ 46 cited

A Search for Kilonovae in the Dark Energy Survey

Z. Doctor, R. Kessler, H. Y. Chen +68

The coalescence of a binary neutron star (BNS) pair is expected to produce gravitational waves (GW) and electromagnetic (EM) radiation, both of which may be detectable with current…

astro-ph.GA2016★ 160 cited

Farthest Neighbor: The Distant Milky Way Satellite Eridanus II

T. S. Li, J. D. Simon, A. Drlica-Wagner +56

We present Magellan/IMACS spectroscopy of the recently-discovered Milky Way satellite Eridanus II (Eri II). We identify 28 member stars in Eri II, from which we measure a systemic…

astro-ph.GA2016★ 115 cited

Nearest Neighbor: The Low-Mass Milky Way Satellite Tucana III

J. D. Simon, T. S. Li, A. Drlica-Wagner +56

We present Magellan/IMACS spectroscopy of the recently discovered Milky Way satellite Tucana III (Tuc III). We identify 26 member stars in Tuc III, from which we measure a mean rad…

astro-ph.CO2016★ 131 cited

Weak-lensing mass calibration of redMaPPer galaxy clusters in Dark Energy Survey Science Verification data

P. Melchior, D. Gruen, T. McClintock +78

We use weak-lensing shear measurements to determine the mean mass of optically selected galaxy clusters in Dark Energy Survey Science Verification data. In a blinded analysis, we s…

astro-ph.CO2016★ 16 cited

Galaxy bias from galaxy-galaxy lensing in the DES Science Verification Data

J. Prat, C. Sánchez, R. Miquel +68

We present a measurement of galaxy-galaxy lensing around a magnitude-limited () sample of galaxies from the Dark Energy Survey Science Verification (DES-SV) data. We…

astro-ph.CO2016★ 24 cited

Inference from the small scales of cosmic shear with current and future Dark Energy Survey data

N. MacCrann, J. Aleksić, A. Amara +61

Cosmic shear is sensitive to fluctuations in the cosmological matter density field, including on small physical scales, where matter clustering is affected by baryonic physics in g…

astro-ph.GA2016★ 2 cited

The Dark Energy Survey view of the Sagittarius stream: discovery of two faint stellar system candidates

E. Luque, A. Pieres, B. Santiago +63

We report the discovery of two new candidate stellar systems in the constellation of Cetus using the data from the first two years of the Dark Energy Survey (DES). The objects, DES…

astro-ph.GA2016★ 76 cited

VDES J2325-5229 a z=2.7 gravitationally lensed quasar discovered using morphology independent supervised machine learning

Fernanda Ostrovski, Richard G. McMahon, Andrew J. Connolly +56

We present the discovery and preliminary characterization of a gravitationally lensed quasar with a source redshift and image separation of lensed by a foregrou…

astro-ph.GA2016★ 4 cited

Discovery of a z=0.65 Post-Starburst BAL Quasar in the DES Supernova Fields

Dale Mudd, Paul Martini, Suk Sien Tie +55

We present the discovery of a z=0.65 low-ionization broad absorption line (LoBAL) quasar in a post-starburst galaxy in data from the Dark Energy Survey (DES) and spectroscopy from…

astro-ph.HE2016★ 47 cited

The Evolution of Active Galactic Nuclei in Clusters of Galaxies from the Dark Energy Survey

E. Bufanda, D. Hollowood, T. E. Jeltema +53

The correlation between active galactic nuclei (AGN) and environment provides important clues to AGN fueling and the relationship of black hole growth to galaxy evolution. In this…

astro-ph.HE2016★ 57 cited

A DECam Search for an Optical Counterpart to the LIGO Gravitational Wave Event GW151226

P. S. Cowperthwaite, E. Berger, M. Soares-Santos +97

We report the results of a Dark Energy Camera (DECam) optical follow-up of the gravitational wave (GW) event GW151226, discovered by the Advanced LIGO detectors. Our observations c…

astro-ph.CO2016★ 22 cited

Optical-SZE Scaling Relations for DES Optically Selected Clusters within the SPT-SZ Survey

A. Saro, S. Bocquet, J. Mohr +68

We study the Sunyaev-Zel'dovich effect (SZE) signature in South Pole Telescope (SPT) data for an ensemble of 719 optically identified galaxy clusters selected from 124.6 deg of…

astro-ph.CO2016★ 71 cited

Testing the lognormality of the galaxy and weak lensing convergence distributions from Dark Energy Survey maps

L. Clerkin, D. Kirk, M. Manera +57

It is well known that the probability distribution function (PDF) of galaxy density contrast is approximately lognormal; whether the PDF of mass fluctuations derived from weak lens…

astro-ph.CO2016★ 118 cited

Cosmic Voids and Void Lensing in the Dark Energy Survey Science Verification Data

C. Sánchez, J. Clampitt, A. Kovacs +69

Galaxies and their dark matter halos populate a complicated filamentary network around large, nearly empty regions known as cosmic voids. Cosmic voids are usually identified in spe…

astro-ph.GA2016★ 56 cited

Galaxy Populations in Massive Galaxy Clusters to z=1.1: Color Distribution, Concentration, Halo Occupation Number and Red Sequence Fraction

C. Hennig, J. J. Mohr, A. Zenteno +70

We study the galaxy populations in 74 Sunyaev Zeldovich Effect (SZE) selected clusters from the South Pole Telescope (SPT) survey that have been imaged in the science verification…

astro-ph.CO2016★ 105 cited

Host Galaxy Identification for Supernova Surveys

Ravi R. Gupta, Steve Kuhlmann, Eve Kovacs +57

Host galaxy identification is a crucial step for modern supernova (SN) surveys such as the Dark Energy Survey (DES) and the Large Synoptic Survey Telescope (LSST), which will disco…

astro-ph.CO2016★ 156 cited

Cosmology constraints from shear peak statistics in Dark Energy Survey Science Verification data

T. Kacprzak, D. Kirk, O. Friedrich +81

Shear peak statistics has gained a lot of attention recently as a practical alternative to the two point statistics for constraining cosmological parameters. We perform a shear pea…

astro-ph.CO2016★ 61 cited

Galaxy-Galaxy Lensing in the DES Science Verification Data

J. Clampitt, C. Sánchez, J. Kwan +73

We present galaxy-galaxy lensing results from 139 square degrees of Dark Energy Survey (DES) Science Verification (SV) data. Our lens sample consists of red galaxies, known as redM…

astro-ph.CO2016★ 124 cited

Detection of the kinematic Sunyaev-Zel'dovich effect with DES Year 1 and SPT

B. Soergel, S. Flender, K. T. Story +80

We detect the kinematic Sunyaev-Zel'dovich (kSZ) effect with a statistical significance of by combining a cluster catalogue derived from the first year data of the Dark Ene…