output
20032026
most citedGW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

9.8k citations

Showing 2020 · astro-ph.HEShow all

11 papers · 2 filters

astro-ph.HE2020★ 57 cited

Evidence of 200 TeV photons from HAWC J1825-134

A. Albert, R. Alfaro, C. Alvarez +81

The Earth is bombarded by ultra-relativistic particles, known as cosmic rays (CRs). CRs with energies up to a few PeV (=10 eV), the knee in the particle spectrum, are believ…

astro-ph.HE2020★ 16 cited

Multiwavelength Characterization of the High Mass X-ray Binary Population of M31

Margaret Lazzarini, Benjamin F. Williams, Meredith Durbin +7

We present our analysis of high quality high mass X-ray binary (HMXB) candidates in M31 selected from point-source optical-counterpart candidates from the Chandra-PHAT survey catal…

astro-ph.HE2020★ 15 cited

A deep Chandra survey for faint X-ray sources in the Galactic globular cluster M30, and searches for optical and radio counterparts

Yue Zhao, Craig O. Heinke, Haldan N. Cohn +11

We present a deep () {\it Chandra} survey of the Galactic globular cluster M30 (NGC 7099). Combining the new Cycle 18 with the previous Cycle 3 observations w…

astro-ph.HE2020★ 4 cited

Swift/XRT, Chandra and XMM-Newton observations of IGR J17091-3624 as it returns into quiescence

Pereyra, Margarita, Altamirano +11

IGR J17091-3624 is a low mass X-ray binary (LMXB) which received wide attention from the community thanks to its similarities with the bright black hole system GRS 1915+105. Both s…

astro-ph.HE2020★ 40 cited

The MAVERIC Survey: Chandra/ACIS Catalog of Faint X-ray sources in 38 Galactic globular clusters

Arash Bahramian, Jay Strader, James C. A. Miller-Jones +11

Globular clusters host a variety of lower-luminosity ( erg s) X-ray sources, including accreting neutron stars and black holes, millisecond pulsars, cataclysmic…

astro-ph.HE2020★ 18 cited

The stringent upper limit on jet power in the persistent soft state source 4U~1957+11

Thomas J. Maccarone, Arlo Osler, James C. A. Miller-Jones +5

We present extremely deep upper limits on the radio emission from 4U~1957+11, an X-ray binary that is generally believed to be a persistently accreting black hole that is almost al…