activity
19972018
most citedDust Depletion and Extinction in a Gamma-Ray Burst Afterglow

107 citations · 375 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2018★ 98 cited

The X-shooter GRB afterglow legacy sample (XS-GRB)

J. Selsing, D. Malesani, P. Goldoni +53

In this work we present spectra of all -ray burst (GRB) afterglows that have been promptly observed with the X-shooter spectrograph until 31-03-2017. In total, we obtained spect…

astro-ph.HE2015

GRB host galaxies with VLT/X-Shooter: properties at 0.8 < z < 1.3

S. Piranomonte, J. Japelj, S. D. Vergani +19

Long gamma-ray bursts (LGRBs) are associated with the death of massive stars. Their host galaxies therefore represent a unique class of objects tracing star formation across the ob…

astro-ph.GA2014★ 31 cited

Herschel observations of gamma-ray burst host galaxies: implications for the topology of the dusty interstellar medium

P. Schady, S. Savaglio, T. Mueller +11

Long-duration gamma-ray bursts (GRBs) are indisputably related to star formation, and their vast luminosity in gamma rays pin-points regions of star formation independent of galaxy…

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-ph2004★ 107 cited

Dust Depletion and Extinction in a Gamma-Ray Burst Afterglow

Sandra Savaglio, S. Michael Fall

We put stringent constraints for the first time on the dust properties in the circumburst medium of a gamma-ray burst (GRB) afterglow. This is based on the optical spectrum of GRB…

astro-ph2003★ 73 cited

Abundances in the Neutral Interstellar Medium of I Zw 18 from FUSE Observations

A. Aloisi, S. Savaglio, T. M. Heckman +3

We report on new FUSE far-UV spectroscopy of the most metal-poor blue compact dwarf galaxy I Zw 18. The new data represent an improvement over previous FUSE spectra by a factor of…