output
19932026
most citedMeasurements of Omega and Lambda from 42 High-Redshift Supernovae

18.1k citations

Showing 2017 · astro-ph.HEShow all

6 papers · 2 filters

astro-ph.HE2017★ 41 cited

Studying the Ultraviolet Spectrum of the First Spectroscopically Confirmed Supernova at redshift two

M. Smith, M. Sullivan, R. C. Nichol +87

We present observations of DES16C2nm, the first spectroscopically confirmed hydrogen-free superluminous supernova (SLSN-I) at redshift z~2. DES16C2nm was discovered by the Dark Ene…

astro-ph.HE2017★ 193 cited

Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory

A. Albert, M. Andre, M. Anghinolfi +1931

The Advanced LIGO and Advanced Virgo observatories recently discovered gravitational waves from a binary neutron star inspiral. A short gamma-ray burst (GRB) that followed the merg…

astro-ph.HE2017★ 253 cited

Science with e-ASTROGAM (A space mission for MeV-GeV gamma-ray astrophysics)

A. De Angelis, V. Tatischeff, I. A. Grenier +248

e-ASTROGAM (enhanced ASTROGAM) is a breakthrough Observatory space mission, with a detector composed by a Silicon tracker, a calorimeter, and an anticoincidence system, dedicated t…

astro-ph.HE2017★ 241 cited

Evidence for a maximum mass cut-off in the neutron star mass distribution and constraints on the equation of state

Justin Alsing, Hector O. Silva, Emanuele Berti

We infer the mass distribution of neutron stars in binary systems using a flexible Gaussian mixture model and use Bayesian model selection to explore evidence for multi-modality an…

astro-ph.HE2017★ 97 cited

Explaining LIGO's observations via isolated binary evolution with natal kicks

D. Wysocki, D. Gerosa, R. O'Shaughnessy +5

We compare binary evolution models with different assumptions about black-hole natal kicks to the first gravitational-wave observations performed by the LIGO detectors. Our compari…

astro-ph.HE2017★ 55 cited

Geodesic models of quasi-periodic-oscillations as probes of quadratic gravity

Andrea Maselli, Paolo Pani, Roberto Cotesta +3

Future very-large-area X-ray instruments (for which the effective area is larger than m) will be able to measure the frequencies of quasi-periodic oscillations~(QPOs) obser…