output
19922026
most citedObservation of Gravitational Waves from a Binary Black Hole Merger

14.2k citations

Showing 2017Show all

346 papers · 1 filter

astro-ph.SR2017★ 8 cited

An application of the weighted horizontal magnetic gradient to solar compact and eruptive events

M. B. Korsos, Michael S. Ruderman, R. Erdelyi

We propose to apply the weighted horizontal magnetic gradient (), introduced in Korsos et al (2015), for analysing the pre-flare and pre-CME behaviour and evolution of Acti…

physics.app-ph2017

Bright polariton OLEDs operating in the ultra-strong coupling regime

Armando Genco, Alessandro Ridolfo, Salvatore Savasta +3

The generation and control of exotic phenomena in organic electroluminescent microcavities, such as polariton lasing and non-linear optical effects, operating in strong and ultra-s…

astro-ph.SR2017★ 36 cited

Accretion signatures in the X-shooter spectrum of the substellar companion to SR12

Alejandro Santamaría-Miranda, Claudio Cáceres, Matthias R. Schreiber +5

About a dozen substellar companions orbiting young stellar objects or pre-main sequence stars at several hundred au have been identified in the last decade. These objects are inter…

cond-mat.mes-hall2017★ 35 cited

LO-phonon emission rate of hot electrons from an on-demand single-electron source in a GaAs/AlGaAs heterostructure

N. Johnson, C. Emary, S. Ryu +10

Using a recently-developed time-of-flight measurement technique with 1 ps time resolution and electron-energy spectroscopy, we developed a method to measure the longitudinal-optica…

astro-ph.SR2017★ 46 cited

Evidence for eccentric, precessing gaseous debris in the circumstellar absorption towards WD 1145+017

P. Wilson Cauley, Jay Farihi, Seth Redfield +3

We present time-series spectra revealing changes in the circumstellar line profiles for the white dwarf WD 1145+017. Over the course of 2.2 years, the spectra show complete velocit…

astro-ph.SR2017★ 55 cited

The very young resolved stellar populations around stripped-envelope supernovae

Justyn R. Maund

The massive star origins for Type IIP supernovae (SNe) have been established through direct detection of their red supergiants progenitors in pre-explosion observations; however, t…