output
19922026
most citedThe Sloan Digital Sky Survey: Technical Summary

10.4k citations

Showing 2018 · astro-ph.HEShow all

34 papers · 2 filters

astro-ph.HE2018★ 9 cited

Relativistic X-ray jets at high redshift

Daniel A Schwartz, Aneta Siemiginowska, Diana M Worrall +6

Powerful radio sources and quasars emit relativistic jets of plasma and magnetic fields that travel hundreds of kilo-parsecs, ultimately depositing energy into the intra- or inter-…

astro-ph.HE2018★ 21 cited

Detection of a gamma-ray flare from the high-redshift blazar DA 193

Vaidehi S. Paliya, M. Ajello, R. Ojha +10

High-redshift () blazars are the most powerful members of the blazar family. Yet, only a handful of them have both X-ray and -ray detection, thereby making it difficult to…

astro-ph.HE2018★ 29 cited

The Megaparsec-scale Gas-sloshing Spiral in the Remnant Cool Core Cluster Abell 1763

E. M. Douglass, E. L. Blanton, S. W. Randall +4

We present a multiwavelength study of the massive galaxy cluster Abell 1763 at redshift z = 0.231. Image analysis of a 19.6 ks Chandra archival observation reveals a cluster-wide s…

astro-ph.HE2018★ 173 cited

A -ray determination of the Universe's star-formation history

LAT Collaboration, M. Ajello, K. Helgason +4

The light emitted by all galaxies over the history of the Universe produces the extragalactic background light (EBL) at ultraviolet, optical, and infrared wavelengths. The EBL is a…

astro-ph.HE2018★ 65 cited

Searching a Thousand Radio Pulsars for Gamma-ray Emission

David A. Smith, Philippe Bruel, Ismaël Cognard +15

Identifying as many gamma-ray pulsars as possible in the Fermi Large Area Telescope (LAT) data helps test pulsar emission models by comparing predicted and observed properties for…

astro-ph.HE2018★ 8 cited

Theoretically motivated search and detection of non-thermal pulsations from PSRs J1747-2958, J2021+3651, and J1826-1256

Jian Li, Diego F. Torres, Francesco Coti Zelati +3

Based on a theoretical selection of pulsars as candidates for detection at X-ray energies, we present an analysis of archival X-ray observations done with Chandra and XMM-Newton of…