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20022024
most citedGW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

9.8k citations

Showing 2013Show all

21 papers · 1 filter

astro-ph.IM201392 cited

On-Orbit Degradation of Solar Instruments

A. BenMoussa, S. Gissot, U. Schühle +38

We present the lessons learned about the degradation observed in several space solar missions, based on contributions at the Workshop about On-Orbit Degradation of Solar and Space…

astro-ph.CO2013609 cited

A Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34

Dominik A. Riechers, C. M. Bradford, D. L. Clements +61

Massive present-day early-type (elliptical and lenticular) galaxies probably gained the bulk of their stellar mass and heavy elements through intense, dust-enshrouded starbursts -…

astro-ph.CO201329 cited

On inferring extinction laws in z~6 quasars as signatures of supernova dust

Jens Hjorth, Paul M. Vreeswijk, Christa Gall +1

Unusual extinction curves of high-redshift QSOs have been taken as evidence that dust is primarily produced by supernovae at high redshift. In particular, the 3000 A Todini-Ferrara…

astro-ph.SR201310 cited

Topical Issue in Solar Physics: Flux-rope Structure of Coronal Mass Ejections Preface

N. Gopalswamy, T. Nieves-Chinchilla, M. Hidalgo +4

This Topical Issue of Solar Physics, devoted to the study of flux-rope structure in coronal mass ejections (CMEs), is based on two Coordinated Data Analysis Workshops (CDAWs) held…

astro-ph.SR201326 cited

The relationship between hard X-ray pulse timings and the locations of footpoint sources during solar flares

A. R. Inglis, B. R. Dennis

The cause of quasi-periodic pulsations (QPP) in solar flares remains the subject of debate. Recently, Nakariakov & Zimovets (2011) proposed a new model suggesting that, in two-ribb…

astro-ph.SR201343 cited

Diagnosing the time-dependence of active region core heating from the emission measure: II. Nanoflare trains

Jeffrey W. Reep, Stephen J. Bradshaw, James A. Klimchuk

The time-dependence of heating in solar active regions can be studied by analyzing the slope of the emission measure distribution cool-ward of the peak. In a previous study we show…