output
19922026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2017 · astro-ph.HEShow all

33 papers · 2 filters

astro-ph.HE2017★ 33 cited

SNe 2013K and 2013am: observed and physical properties of two slow, normal Type IIP events

L. Tomasella, E. Cappellaro, M. L. Pumo +28

We present one year of optical and near-infrared photometry and spectroscopy of the Type IIP SNe 2013K and 2013am. Both objects are affected by significant extinction, due to their…

astro-ph.HE2017★ 23 cited

OGLE-2014-SN-073 as a fallback accretion powered supernova

Takashi J. Moriya, Giacomo Terreran, Sergei I. Blinnikov

We investigate the possibility that the energetic Type II supernova OGLE-2014-SN-073 is powered by a fallback accretion following the failed explosion of a massive star. Taking mas…

astro-ph.HE2017★ 87 cited

THESEUS: a key space mission concept for Multi-Messenger Astrophysics

G. Stratta, R. Ciolfi, L. Amati +55

The recent discovery of the electromagnetic counterpart of the gravitational wave source GW170817, has demonstrated the huge informative power of multi-messenger observations. Duri…

astro-ph.HE2017★ 377 cited

Late time afterglow observations reveal a collimated relativistic jet in the ejecta of the binary neutron star merger GW170817

Davide Lazzati, Rosalba Perna, Brian J. Morsony +5

The binary neutron star (BNS) merger GW170817 was the first astrophysical source detected in gravitational waves and multi-wavelength electromagnetic radiation. The almost simultan…

astro-ph.HE2017★ 112 cited

On the Progenitor of Binary Neutron Star Merger GW170817

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1095

On 2017 August 17 the merger of two compact objects with masses consistent with two neutron stars was discovered through gravitational-wave (GW170817), gamma-ray (GRB 170817A), and…

astro-ph.HE2017★ 8 cited

Overdensity of galaxies in the environment of quasar pairs

Angela Sandrinelli, Renato Falomo, Aldo Treves +2

We report on a study of the galaxy environments of low redshift physical quasars pairs. We selected 20 pairs having projected separation 0.5 Mpc and difference of systemic velo…