output
20012026
most citedThe Seventh Data Release of the Sloan Digital Sky Survey

5.4k citations

Showing 2019 · astro-ph.HEShow all

17 papers · 2 filters

astro-ph.HE2019★ 33 cited

The Nucleosynthetic Yields of Core-Collapse Supernovae, prospects for the Next Generation of Gamma-Ray Astronomy

Sydney Andrews, Chris L. Fryer, Samuel W. Jones +2

Though the neutrino-driven convection model for the core-collapse explosion mechanism has received strong support in recent years, there are still many uncertainties in the explosi…

astro-ph.HE2019★ 8 cited

Gamma-rays from kilonovae and the cosmic gamma-ray background

Pilar Ruiz-Lapuente, Oleg Korobkin

The recent detection of the gravitational wave event GW170817, produced by the coalescence of two neutron stars, and of its optical-infrared counterpart, powered by the radioactive…

astro-ph.HE2019★ 64 cited

Constraining properties of the next nearby core-collapse supernova with multi-messenger signals

MacKenzie L. Warren, Sean M. Couch, Evan P. O'Connor +1

With the advent of modern neutrino and gravitational wave detectors, the promise of multi-messenger detections of the next galactic core-collapse supernova has become very real. Su…

astro-ph.HE2019★ 46 cited

Co-production of light and heavy -process elements via fission deposition

Nicole Vassh, Matthew R. Mumpower, Gail C. McLaughlin +2

We apply for the first time fission yields determined across the chart of nuclides from the macroscopic-microscopic theory of the Finite Range Liquid Drop Model to simulations of r…

astro-ph.HE2019★ 11 cited

Chandra Observations of the Spectacular A3411-12 Merger Event

Felipe Andrade-Santos, Reinout J. van Weeren, Gabriella Di Gennaro +17

We present deep Chandra observations of A3411-12, a remarkable merging cluster that hosts the most compelling evidence for electron re-acceleration at cluster shocks to date. Using…

astro-ph.HE2019★ 389 cited

Stringent constraints on neutron-star radii from multimessenger observations and nuclear theory

Collin D. Capano, Ingo Tews, Stephanie M. Brown +6

The properties of neutron stars are determined by the nature of the matter that they contain. These properties can be constrained by measurements of the star's size. We obtain stri…