activity
20132018
most citedGRB hosts through cosmic time - VLT/X-Shooter emission-line spectroscopy of 96 GRB-selected galaxies at 0.1 < z < 3.6

102 citations · 407 across the 10 of their papers we have counts for

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Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2018★ 56 cited

Accretion geometry of the black-hole binary Cygnus X-1 from X-ray polarimetry

M. Chauvin, H. -G. Florén, M. Friis +13

Black-hole binary (BHB) systems comprise a stellar-mass black hole and a closely orbiting companion star. Matter is transferred from the companion to the black hole, forming an acc…

astro-ph.HE2018★ 18 cited

The PoGO+ view on Crab off-pulse hard X-ray polarisation

M. Chauvin, H. -G. Florén, M. Friis +11

The linear polarisation fraction and angle of the hard X-ray emission from the Crab provide unique insight into high energy radiation mechanisms, complementing the usual imaging, t…

astro-ph.HE2017★ 2 cited

Shedding new light on the Crab with polarized X-rays

M. Chauvin, H. -G. Florén, M. Friis +13

Strong magnetic fields, synchrotron emission, and Compton scattering are omnipresent in compact celestial X-ray sources. Emissions in the X-ray energy band are consequently expecte…

astro-ph.HE2015

Exploring Gamma-Ray Bursts, Their Immediate Environment and Host Galaxies

Mette Friis

Lasting anywhere from a few milliseconds to several minutes, GRBs shine hundreds of times brighter than a typical supernova, making them briefly the brightest source of cosmic gamm…

astro-ph.HE2015★ 39 cited

GRB 140606B / iPTF14bfu: Detection of shock-breakout emission from a cosmological gamma-ray burst?

Z. Cano, A. de Ugarte Postigo, D. Perley +13

We present optical and near-infrared photometry of GRB~140606B (), and optical photometry and spectroscopy of its associated supernova (SN). The results of our modelling i…

astro-ph.HE2013★ 29 cited

Thermal emission in the early X-ray afterglows of GRBs: following the prompt phase to the late times

Mette Friis, Darach Watson

Thermal radiation, peaking in soft X-rays, has now been detected in a handful of GRB afterglows and has to date been interpreted as shock break-out of the GRB's progenitor star. We…