activity
19972025
most citedThe discovery of polarization in the afterglow of GRB 990510 with the ESO Very Large Telescope

132 citations · 395 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.IM2025★ 4 cited

Ground calibration plan for the Athena/X-IFU microcalorimeter spectrometer

Alexeï Molin, François Pajot, Marc Audard +24

The X-ray Integral Field Unit is the X-ray imaging spectrometer on-board one of ESA's next large missions, Athena. Athena is set to investigate the theme of the Hot and Energetic U…

astro-ph.HE2015★ 46 cited

Accessing the population of high redshift Gamma Ray Bursts

G. Ghirlanda, R. Salvaterra, G. Ghisellini +19

Gamma Ray Bursts (GRBs) are a powerful probe of the high redshift Universe. We present a tool to estimate the detection rate of high-z GRBs by a generic detector with defined energ…

astro-ph2005★ 24 cited

Long term flaring activity of XRF 011030 observed with BeppoSAX

A. Galli, L. Piro

We present the spectral and temporal analysis of the X-ray flash XRF011030 observed with BeppoSAX. This event is characterized by a very long X-ray bursting activity that lasts abo…

astro-ph2005★ 30 cited

X-ray continuum properties of GRB afterglows observed by XMM-Newton and Chandra

B. Gendre, A. Corsi, L. Piro

We present a catalog of XMM-Newton and Chandra observations of gamma-ray burst (GRB) afterglows, reduced in a common way using the most up-to-date calibration files and software. W…

astro-ph2001★ 28 cited

GRB 990704: the most X-ray rich BeppoSAX gamma-ray burst

M. Feroci, L. A. Antonelli, P. Soffitta +8

We present the X- and -ray detection of GRB 990704 and the discovery and study of its X-ray afterglow, 1SAX J1219.5-0350. Two pointed BeppoSAX observations with the narrow field…

astro-ph2001★ 7 cited

On the Origin of the FeK Line in the Seyfert 2 Galaxy NGC 7172

M. Dadina, L. Bassani, M. Cappi +6

The Seyfert 2 Galaxy NGC 7172 was observed twice by BeppoSAX narrow field instruments approximately one year apart. As found in previous observations, the source is variable on sho…