activity
19982015
most citedDetection of the optical afterglow of GRB 000630: Implications for dark bursts

141 citations · 436 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2015★ 55 cited

The Needle in the 100 deg2 Haystack: Uncovering Afterglows of Fermi GRBs with the Palomar Transient Factory

Leo P. Singer, Mansi M. Kasliwal, S. Bradley Cenko +32

The Fermi Gamma-ray Space Telescope has greatly expanded the number and energy window of observations of gamma-ray bursts (GRBs). However, the coarse localizations of tens to a hun…

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-ph.CO2011★ 55 cited

GRB091127/SN2009nz and the VLT/X-shooter spectroscopy of its host galaxy: probing the faint end of the mass-metallicity relation

S. D. Vergani, H. Flores, S. Covino +36

We perform a detailed study of the gamma-ray burst GRB091127/SN2009nz host galaxy at z=0.490 using the VLT/X-shooter spectrograph in slit and integral-field unit (IFU). From the an…

astro-ph2008★ 20 cited

A photometric redshift of for the \agile GRB 080514B

A. Rossi, A. de Ugarte Postigo, P. Ferrero +26

Aims: The AGILE gamma-ray burst GRB 080514B is the first burst with detected emission above 30 MeV and an optical afterglow. However, no spectroscopic redshift for this burst is kn…

astro-ph2007★ 66 cited

Detection of GRB 060927 at z = 5.47: Implications for the Use of Gamma-Ray Bursts as Probes of the End of the Dark Ages

A. E. Ruiz-Velasco, H. Swan, E. Troja +54

We report on follow-up observations of the GRB 060927 using the ROTSE-IIIa telescope and a suite of larger aperture ground-based telescopes. An optical afterglow was detected 20 s…

astro-ph2003★ 33 cited

GRB 020813: polarization in the case of a smooth optical decay

J. Gorosabel, E. Rol, S. Covino +35

We present the results of a VLT polarimetric monitoring campaign of the GRB 020813 optical afterglow carried out in three nights, from 0.88 to 4.20 days after the gamma-ray event.…