activity
20042026
most citedThe Emergence of a Lanthanide-Rich Kilonova Following the Merger of Two Neutron Stars

765 citations · 11.8k across the 178 of their papers we have counts for

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Showing astro-ph.COShow all

10 papers · 1 filter

astro-ph.CO2013★ 93 cited

Molecular Hydrogen in the Damped Lyman-alpha System towards GRB 120815A at z=2.36

T. Krühler, C. Ledoux, J. P. U. Fynbo +32

We present the discovery of molecular hydrogen (H_2), including the presence of vibrationally-excited H_2^* in the optical spectrum of the afterglow of GRB 120815A at z=2.36 obtain…

astro-ph.CO2013★ 4 cited

Clustering of galaxies around GRB sight-lines

Vladimir Sudilovsky, Jochen Greiner, Arne Rau +11

There is evidence of an overdensity of strong intervening MgII absorption line systems distributed along the lines of sight towards GRB afterglows relative to quasar sight-lines. I…

astro-ph.CO2012★ 66 cited

A deep search for the host galaxies of GRBs with no detected optical afterglow

A. Rossi, S. Klose, P. Ferrero +28

Gamma-Ray Bursts can provide information about star formation at high redshifts. Even in the absence of a optical/near-infrared/radio afterglow, the high detection rate of X-ray af…

astro-ph.CO2011★ 97 cited

BL Lacertae objects beyond redshift 1.3 - UV-to-NIR photometry and photometric redshift for Fermi/LAT blazars

Arne Rau, P. Schady, J. Greiner +17

Observations of the gamma-ray sky with Fermi led to significant advances towards understanding blazars, the most extreme class of Active Galactic Nuclei. A large fraction of the po…

astro-ph.CO2011★ 184 cited

The SEDs and Host Galaxies of the dustiest GRB afterglows

T. Krühler, J. Greiner, P. Schady +18

(Abridged) Until recently the information inferred from gamma-ray burst follow-up observations was mostly limited to optically bright afterglows, biasing all demographic studies ag…

astro-ph.CO2011★ 72 cited

GRB 090426: Discovery of a jet break in a short burst afterglow

A. Nicuesa Guelbenzu, S. Klose, A. Rossi +14

Context: The link between the duration of GRBs and the nature of their progenitors remains disputed. Short bursts (with durations of less than ~2 s) are less frequently observed, t…