activity
19972026
most citedDiscovery of the peculiar supernova 1998bw in the error box of GRB980425

1.9k citations · 3k across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.HE2026★ 1 cited

GRB 210704A: A Luminous Fast Blue Transient in a GRB Afterglow at

Daniëlle L. A. Pieterse, Andrew J. Levan, Maria E. Ravasio +27

We present detailed, multi-wavelength analysis of GRB 210704A: a Fermi Gamma-ray Burst Monitor discovered and Fermi Large Area Telescope (LAT) detected gamma-ray burst (GRB). The b…

astro-ph.HE2026★ 1 cited

Milliarcsecond-scale spectrum of the persistent radio source associated with FRB 20190417A and constraints for FRB 20181030A

G. Bruni, L. Piro, Y. -P. Yang +6

We aim to confirm the compact nature and constrain the radio spectra of candidate persistent radio sources (PRSs) associated with repeating fast radio bursts (FRBs). We performed E…

astro-ph.HE2026

The Ep-Liso correlation: A new diagnostic tool for kilonova transients

Ruben Farinelli, Fabrizio Cogato, Mattia Bulla +10

The AT2017gfo kilonova transient remains a unique multi-messenger event thanks to its proximity (z=0.00987) and the possibility to investigate time-resolved spectra, providing evid…

astro-ph.HE2026★ 2 cited

GRB 180728A and SN 2018fip: the nearest high-energy cosmological gamma-ray burst with an associated supernova

A. Rossi, L. Izzo, K. Maeda +29

The long GRB 180728A, at a redshift of , stands out due to its high isotropic energy of erg, in contrast with most events at redshif…

astro-ph.HE2025★ 12 cited

The puzzling long GRB 191019A: Evidence for Kilonova Light

G. Stratta, A. M. Nicuesa Guelbenzu, S. Klose +11

GRB 191019A was a long Gamma-ray burst (GRB) lasting about 65 s and, as such, originally thought to be linked to a core-collapse supernova. However, even though follow-up observati…

astro-ph.HE2024★ 27 cited

Discovery of a PRS associated with FRB 20240114A

G. Bruni, L. Piro, Y. -P. Yang +6

We present the discovery of the fourth persistent radio source (PRS) associated with a fast radio burst (FRB). Following previous indications of a candidate PRS associated with FRB…

astro-ph.HE2018★ 27 cited

The optical afterglow of the short gamma-ray burst associated with GW170817

J. D. Lyman, G. P. Lamb, A. J. Levan +33

The binary neutron star merger GW170817 was the first multi-messenger event observed in both gravitational and electromagnetic waves. The electromagnetic signal began approximately…

astro-ph.HE2014★ 11 cited

Another short-burst host galaxy with an optically obscured high star formation rate: The case of GRB 071227

A. Nicuesa Guelbenzu, S. Klose, M. J. Michalowski +9

We report on radio continuum observations of the host galaxy of the short gamma-ray burst 071227 (z=0.381) with the Australia Telescope Compact Array (ATCA). We detect the galaxy i…

astro-ph.CO2009★ 368 cited

Low-Resolution Spectroscopy of Gamma-ray Burst Optical Afterglows: Biases in the Swift Sample and Characterization of the Absorbers

J. P. U. Fynbo, P. Jakobsson, J. X. Prochaska +39

(Abridged). We present a sample of 77 optical afterglows (OAs) of Swift detected GRBs for which spectroscopic follow-up observations have been secured. We provide linelists and equ…

astro-ph2000★ 120 cited

VLT spectroscopy of GRB 990510 and GRB 990712; probing the faint and bright end of the GRB host galaxy population

P. M. Vreeswijk, A. Fruchter, L. Kaper +15

We present time-resolved optical spectroscopy of the afterglows of the gamma-ray bursts GRB 990510 and GRB 990712. Through the identification of several absorption lines in the fir…

astro-ph2000★ 65 cited

GRB990712: First Indication of Polarization Variability in a Gamma-ray Burst Afterglow

E. Rol, R. A. M. J. Wijers, P. M. Vreeswijk +9

We report the detection of significant polarization in the optical afterglow of GRB990712 on three instances 0.44, 0.70 and 1.45 days after the gamma-ray burst, with (P, theta) bei…

astro-ph2000★ 49 cited

Discovery of the optical counterpart and early optical observations of GRB990712

Kailash C. Sahu

We present the discovery observations of the optical counterpart of the gamma-ray burster GRB990712 taken 4.16 hours after the outburst and discuss its light curve observed in the…

astro-ph2000★ 35 cited

Prompt and afterglow emission from the X-ray rich GRB981226 observed with BeppoSAX

F. Frontera, L. A. Antonelli, L. Amati +20

We discuss observations of the prompt X and gamma-ray emission and X-ray afterglow from GRB981226. This event has the weakest gamma-ray peak flux detected with the Gamma-Ray Burst…

astro-ph1999★ 183 cited

Prompt and delayed emission properties of Gamma-Ray Bursts observed with BeppoSAX

F. Frontera, L. Amati, E. Costa +14

We investigated the spectral evolution in the 2--700 keV energy band of Gamma-Ray Bursts (GRBs) detected by the Gamma-Ray Burst Monitor (GRBM) and localized with the Wide Field Cam…

astro-ph1999★ 77 cited

The X-ray, Optical and Infrared Counterpart to GRB 980703

P. M. Vreeswijk, T. J. Galama, A. Owens +36

We report on X-ray, optical and infrared follow-up observations of GRB 980703. We detect a previously unknown X-ray source in the GRB error box; assuming a power law decline we fin…

astro-ph1998★ 1.9k cited

Discovery of the peculiar supernova 1998bw in the error box of GRB980425

T. J. Galama, P. M. Vreeswijk, J. van Paradijs +42

The discovery of X-ray, optical and radio afterglows of gamma-ray bursts (GRBs) and the measurements of the distances to some of them have established that these events come from G…

astro-ph1997★ 60 cited

Spectral Properties of the Prompt X-ray emission and Afterglow from the Gamma-Ray Burst of 28 February 1997

F. Frontera, E. Costa, L. Piro +18

We report high-energy spectral data of the prompt emission of GRB970228 and its X-ray afterglow. We establish that the nature of the X-ray afterglow emission is non-thermal and sim…

astro-ph1997★ 20 cited

Radio Monitoring of the January 11, 1997 Gamma-Ray Burst

D. A. Frail, S. R. Kulkarni, E. Costa +8

We report on a comprehensive radio monitoring program of the bright gamma-ray burster GRB970111. These VLA observations were made at a frequency of 1.4 GHz and span a range of post…