output
19932026
most citedThe Seventh Data Release of the Sloan Digital Sky Survey

5.4k citations

Showing 2013 · astro-ph.HEShow all

14 papers · 2 filters

astro-ph.HE2013★ 14 cited

Deep GMRT radio observations and a multi-wavelength study of the region around HESS J1858+020

J. M. Paredes, C. H. Ishwara-Chandra, V. Bosch-Ramon +3

There are a number of very high energy sources in the Galaxy that remain unidentified. Multi-wavelength and variability studies, and catalogue searches, are powerful tools to ident…

astro-ph.HE2013★ 18 cited

The optical rebrightening of GRB100814A: an interplay of forward and reverse shocks?

Massimiliano De Pasquale, N. P. M. Kuin, S. Oates +36

We present a wide dataset of gamma-ray, X-ray, UVOIR, and radio observations of the Swift GRB100814A. At the end of the slow decline phase of the X-ray and optical afterglow, this…

astro-ph.HE2013★ 24 cited

Electron Cooling in a Young Radio Supernova: SN 2012aw

Naveen Yadav, Alak Ray, Sayan Chakraborti +8

We present the radio observations and modeling of an optically bright Type II-P supernova (SN), SN 2012aw which exploded in the nearby galaxy Messier 95 (M95) at a distance of $10\…

astro-ph.HE2013★ 20 cited

Radio observations of GRB 100418a: Test of an energy injection model explaining long-lasting GRB afterglows

A. Moin, P. Chandra, J. C. A. Miller-Jones +6

We present the results of our radio observational campaign on GRB 100418a, for which we used the Australia Telescope Compact Array (ATCA), Very Large Array (VLA) and the Very Long…

astro-ph.HE2013★ 16 cited

A hadronic scenario for HESS J1818-154

G. Castelletti, L. Supan, G. Dubner +2

Aims: G15.4+0.1 is a faint supernova remnant (SNR) that has recently been associated with the gamma-ray source HESS J1818-154. We investigate a hadronic scenario for the production…

astro-ph.HE2013★ 1 cited

A combined GMRT/CLFST image of IC443 at 150 MHz

D. Mitra, D. A. Green, A. Pramesh Rao

IC443 is a relatively large Galactic (~45 arcmin) SNR with a high radio surface brightness. It has fine scale structure down to arcsec scales, and so is difficult to image on all a…