activity
20082020
most citedMeasurement of the Cosmic Ray e+ plus e- spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope

911 citations · 3.1k across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.CO2020★ 70 cited

Dark Energy Survey Year 3 Results: Measuring the Survey Transfer Function with Balrog

S. Everett, B. Yanny, N. Kuropatkin +97

We describe an updated calibration and diagnostic framework, Balrog, used to directly sample the selection and photometric biases of the Dark Energy Survey's (DES) Year 3 (Y3) data…

astro-ph.CO2020★ 209 cited

Dark Energy Survey Year 3 Results: Photometric Data Set for Cosmology

I. Sevilla-Noarbe, K. Bechtol, M. Carrasco Kind +111

We describe the Dark Energy Survey (DES) photometric data set assembled from the first three years of science operations to support DES Year 3 cosmology analyses, and provide usage…

astro-ph.GA2018★ 134 cited

Discovery of two neighboring satellites in the Carina constellation with MagLiteS

G. Torrealba, V. Belokurov, S. E. Koposov +23

We report the discovery of two ultra-faint satellites in the vicinity of the Large Magellanic Cloud (LMC) in data from the Magellanic Satellites Survey (MagLiteS). Situated 18$^{\c…

astro-ph.IM2018★ 497 cited

The Dark Energy Survey Data Release 1

T. M. C. Abbott, F. B. Abdalla, S. Allam +199

We describe the first public data release of the Dark Energy Survey, DES DR1, consisting of reduced single epoch images, coadded images, coadded source catalogs, and associated pro…

astro-ph.HE2013★ 840 cited

Detection of the Characteristic Pion-Decay Signature in Supernova Remnants

LAT collaboration, M. Ackermann, M. Ajello +167

Cosmic rays are particles (mostly protons) accelerated to relativistic speeds. Despite wide agreement that supernova remnants (SNRs) are the sources of galactic cosmic rays, unequi…

astro-ph.HE2010★ 87 cited

Fermi-LAT Search for Pulsar Wind Nebulae around gamma-ray Pulsars

The Fermi LAT Collaboration, Pulsar Timing Consortium

The high sensitivity of the Fermi-LAT (Large Area Telescope) offers the first opportunity to study faint and extended GeV sources such as pulsar wind nebulae (PWNe). After one year…