activity
19992025
most citedThe fourth data release of the Kilo-Degree Survey: ugri imaging and nine-band optical-IR photometry over 1000 square degrees

322 citations · 3.4k across the 103 of their papers we have counts for

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Showing 2018Show all

19 papers · 1 filter

astro-ph.SR2018

Burst occurrence in young massive stellar objects

Meyer D. M. -A., Vorobyov E. I., Elbakyan V. G. +3

Episodic accretion-driven outbursts are an extreme manifestation of accretion variability. It has been proposed that the development of gravitational instabilities in the proto-cir…

physics.ins-det2018

A new beamline for laser spin-polarization at ISOLDE

W. Gins, R. D. Harding, M. Baranowski +11

A beamline dedicated to the production of laser-polarized radioactive beams has been constructed at ISOLDE, CERN. We present here different simulations leading to the design and co…

astro-ph.SR2018

Solar flares and Kelvin-Helmholtz instabilities: A parameter survey

Wenzhi Ruan, Chun Xia, Rony Keppens

Hard X-ray (HXR) sources are frequently observed near the top of solar flare loops, and the emission is widely ascribed to bremsstrahlung. We here revisit an alternative scenario w…

astro-ph.HE2018

LOFAR discovery of a 23.5-second radio pulsar

C. M. Tan, C. G. Bassa, S. Cooper +16

We present the discovery of PSR J0250+5854, a radio pulsar with a spin period of 23.5 s. This is the slowest-spinning radio pulsar known. PSR J0250+5854 was discovered by the LOFAR…

astro-ph.HE2018

The 1989 and 2015 outbursts of V404 Cygni: a global study of wind-related optical features

D. Mata Sánchez, T. Muñoz-Darias, J. Casares +19

The black hole transient V404 Cygni exhibited a bright outburst in June 2015 that was intensively followed over a wide range of wavelengths. Our team obtained high time resolution…

astro-ph.HE2018

Measurement of Cosmic-ray Electrons at TeV Energies by VERITAS

VERITAS Collaboration, A. Archer, W. Benbow +58

Cosmic-ray electrons and positrons (CREs) at GeV-TeV energies are a unique probe of our local Galactic neighborhood. CREs lose energy rapidly via synchrotron radiation and inverse-…