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20112026
most citedObservation of inverse Compton emission from a long -ray burst

226 citations · 2.4k across the 58 of their papers we have counts for

collaborators

58 papers

astro-ph.SR2026

SN 2024afyu interpreted as a Pair Instability Supernova

P. J. Pessi, S. Barmentloo, Ł. Wyrzykowski +63

Pair-instability supernovae (PISNe) are the predicted explosions of very massive stars triggered by electron-positron pair production. Numerous transients have been proposed as PIS…

astro-ph.SR2025

Is the Symbiotic Recurrent Nova T CrB Late? Recent Photometric Evolution and Comparison with Past Pre-Outburst Behaviour

Jaroslav Merc, Łukasz Wyrzykowski, Paul G. Beck +46

T CrB is a symbiotic recurrent nova that last erupted in 1946. Given its recurrence timescale of approximately 80 years, the next outburst is eagerly anticipated by the astronomica…

astro-ph.HE2024★ 1 cited

Rapid Response Mode observations of GRB 160203A: Looking for fine-structure line variability at z=3.52

G. Pugliese, A. Saccardi, V. D Elia +26

Gamma-ray bursts are the most energetic known explosions. Despite fading rapidly, they allow to measure redshift and important properties of their host-galaxies. We report the phot…

astro-ph.HE2021★ 24 cited

The supernova of the MAGIC GRB190114C

A. Melandri, L. Izzo, E. Pian +42

We observed GRB190114C (redshift z = 0.4245), the first GRB ever detected at TeV energies, at optical and near-infrared wavelengths with several ground-based telescopes and the Hub…

astro-ph.IM2021★ 134 cited

Gaia Photometric Science Alerts

S. T. Hodgkin, D. L. Harrison, E. Breedt +108

Since July 2014, the Gaia mission has been engaged in a high-spatial-resolution, time-resolved, precise, accurate astrometric, and photometric survey of the entire sky. Aims: We pr…

astro-ph.GA2021

Gamma-ray bursts as probes of high-redshift Lyman-alpha emitters and radiative transfer models

J. -B. Vielfaure, S. D. Vergani, M. Gronke +7

We present the updated census and statistics of Lyman- emitting long gamma-ray bursts host galaxies (LAE-LGRBs). We investigate the properties of a sub-sample of LAE-LGRBs and t…

astro-ph.HE2020★ 226 cited

Observation of inverse Compton emission from a long -ray burst

V. A. Acciari, S. Ansoldi, L. A. Antonelli +301

Long-duration gamma-ray bursts (GRBs) originate from ultra-relativistic jets launched from the collapsing cores of dying massive stars. They are characterised by an initial phase o…

astro-ph.GA2020★ 19 cited

Lyman continuum leakage in faint star-forming galaxies at redshift z=3-3.5 probed by gamma-ray bursts

J. -B. Vielfaure, S. D. Vergani, J. Japelj +23

We present the observations of Lyman continuum (LyC) emission in the afterglow spectra of GRB 191004B at , together with those of the other two previously known LyC-emitt…

astro-ph.SR2020★ 10 cited

VLT/X-shooter spectroscopy of massive young stellar objects in the 30 Doradus region of the Large Magellanic Cloud

M. L. van Gelder, L. Kaper, J. Japelj +13

The process of massive star () formation is still poorly understood. Observations of massive young stellar objects (MYSOs) are challenging due to their rarity, shor…

astro-ph.SR2020★ 88 cited

Observational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger S190814bv

K. Ackley, L. Amati, C. Barbieri +151

On 2019 August 14, the LIGO and Virgo interferometers detected a high-significance event labelled S190814bv. Preliminary analysis of the GW data suggests that the event was likely…

astro-ph.HE2019★ 4 cited

GRB 190114C in the nuclear region of an interacting galaxy -- A detailed host analysis using ALMA, HST and VLT

A. de Ugarte Postigo, C. C. Thöne, S. Martın +28

GRB 190114C is the first GRB for which the detection of very-high energy emission up to the TeV range has been reported. It is still unclear whether environmental properties might…

astro-ph.GA2019★ 22 cited

Simulating MOS science on the ELT: Ly forest tomography

J. Japelj, C. Laigle, M. Puech +14

Mapping of the large-scale structure through cosmic time has numerous applications in the studies of cosmology and galaxy evolution. At , the structure can be traced by the…

astro-ph.HE2019★ 38 cited

GRB171010A / SN2017htp: a GRB-SN at z=0.33

A. Melandri, D. B. Malesani, L. Izzo +41

The number of supernovae known to be connected with long-duration gamma-ray bursts is increasing and the link between these events is no longer exclusively found at low redshift ($…

astro-ph.GA2019★ 16 cited

New constraints on the physical conditions in H-bearing GRB-host damped Lyman- absorbers

K. E. Heintz, J. Bolmer, C. Ledoux +25

We report the detections of molecular hydrogen (H), vibrationally-excited H (H), and neutral atomic carbon (CI), in two new afterglow spectra of GRBs\,181020A ($z=2.9…

astro-ph.GA2019★ 12 cited

On the dust properties of high redshift molecular clouds and the connection to the 2175 Å extinction bump

K. E. Heintz, T. Zafar, A. De Cia +9

We present a study of the extinction and depletion-derived dust properties of gamma-ray burst (GRB) absorbers at showing the presence of neutral carbon (\ion{C}{I}). By mod…

astro-ph.HE2019★ 93 cited

Are LGRBs biased tracers of star formation? Clues from the host galaxies of the /BAT6 complete sample of bright LGRBs III: Stellar masses, star formation rates and metallicities at

J. T. Palmerio, S. D. Vergani, R. Salvaterra +11

(Abridged) Long gamma-ray bursts (LGRB) have been suggested as promising tracers of star formation owing to their association with the core-collapse of massive stars. The goal of t…

astro-ph.HE2019★ 151 cited

Signatures of a jet cocoon in early spectra of a supernova associated with a -ray burst

L. Izzo, A. de Ugarte Postigo, K. Maeda +39

Long gamma-ray bursts mark the death of massive stars, as revealed by their association with energetic broad-lined stripped-envelope supernovae. The scarcity of nearby events and t…

astro-ph.GA2018★ 23 cited

Cold gas in the early Universe. Survey for neutral atomic-carbon in GRB host galaxies at 1 < z < 6 from optical afterglow spectroscopy

K. E. Heintz, C. Ledoux, J. P. U. Fynbo +14

We present a survey for neutral atomic-carbon (CI) along gamma-ray burst (GRB) sightlines, which probes the shielded neutral gas-phase in the interstellar medium (ISM) of GRB host…

astro-ph.GA2018★ 58 cited

Evidence for diffuse molecular gas and dust in the hearts of gamma-ray burst host galaxies

J. Bolmer, C. Ledoux, P. Wiseman +17

Here we built up a sample of 22 GRBs at redshifts observed with X-shooter to determine the abundances of hydrogen, metals, dust, and molecular species. This allows us to st…

astro-ph.GA2018★ 28 cited

X-shooting GRBs at high redshift: probing dust production history

T. Zafar, P. Møller, D. Watson +16

Evolved asymptotic giant branch (AGB) stars and Type Ia supernovae (SNe) are important contributors to the elements that form dust in the interstellar medium of galaxies, in partic…

astro-ph.GA2018★ 31 cited

Investigation of dust attenuation and star formation activity in galaxies hosting GRBs

D. Corre, V. Buat, S. Basa +6

The gamma-ray bursts hosts (GRBHs) are excellent targets to study the extinction properties of dust and its effects on the global emission of distant galaxies. The dust extinction…

astro-ph.IM2018

Revisiting the science case for near-UV spectroscopy with the VLT

C. J. Evans, B. Barbuy, B. Castilho +8

In the era of Extremely Large Telescopes, the current generation of 8-10m facilities are likely to remain competitive at far-blue visible wavelengths for the foreseeable future. Hi…

astro-ph.HE2018★ 42 cited

Host galaxies of SNe Ic-BL with and without long gamma-ray bursts

J. Japelj, S. D. Vergani, R. Salvaterra +5

Broad-line Ic supernovae (SNe Ic-BL) are a very rare class of core-collapse supernovae exhibiting high ejecta velocities and high kinetic energies. They are the only type of SNe th…

astro-ph.GA2018★ 24 cited

The 2175 Å extinction feature in the optical afterglow spectrum of GRB 180325A at z=2.25

T. Zafar, K. E. Heintz, J. P. U. Fynbo +26

The UV extinction feature at 2175 Å is ubiquitously observed in the Galaxy but is rarely detected at high redshifts. Here we report the spectroscopic detection of the 2175 Å bump o…