activity
20172022
most citedFalse outliers of the Ep,i - Eiso correlation?

11 citations · 28 across the 5 of their papers we have counts for

collaborators

9 papers

astro-ph.IM20207 cited

Methods for detection and analysis of weak radio sources with single-dish radio telescopes

M. Marongiu, A. Pellizzoni, E. Egron +13

The detection of mJy/sub-mJy point sources is a significant challenge for single-dish radio telescopes. Detection or upper limits on the faint afterglow from GRBs or other sources…

astro-ph.HE2020

A search for prompt gamma-ray counterparts to fast radio bursts in the Insight-HXMT data

C. Guidorzi, M. Marongiu, R. Martone +118

No robust detection of prompt electromagnetic counterparts to fast radio bursts (FRBs) has yet been obtained, in spite of several multi-wavelength searches carried out so far. Spec…

astro-ph.HE2019

Lowly polarized light from a highly magnetized jet of GRB 190114C

N. Jordana-Mitjans, C. G. Mundell, S. Kobayashi +12

We report multi-color optical imaging and polarimetry observations of the afterglow of the first TeV- detected gamma-ray burst, GRB 190114C, using RINGO3 and MASTER II polarimeters…

astro-ph.HE2019

A cumulative search for hard X/-Ray emission associated with fast radio bursts in Fermi/GBM data

R. Martone, C. Guidorzi, R. Margutti +6

Context. Fast Radio Bursts (FRBs) are millisecond-long bursts uniquely detected at radio frequencies. FRB 131104 is the only case for which a -ray transient positionally and tem…

astro-ph.HE2019

A search for gamma-ray prompt emission associated with the Lorimer Burst FRB010724

C. Guidorzi, M. Marongiu, R. Martone +6

No transient electromagnetic emission has yet been found in association to fast radio bursts (FRBs), the only possible exception (3sigma confidence) being the putative gamma-ray si…

astro-ph.IM20192 cited

A robotic pipeline for fast GRB followup with the Las Cumbres observatory network

R. Martone, C. Guidorzi, C. G. Mundell +9

In the era of multi-messenger astronomy the exploration of the early emission from transients is key for understanding the encoded physics. At the same time, current generation net…