Optical Observations and Multiband Modelling of the Afterglow of GRB 041006: Evidence of A Hard Electron Energy Spectrum

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dc.creatorMisra, Kuntal
dc.creatorResmi, L.
dc.creatorPandey, S. B.
dc.creatorBhattacharya, D.
dc.creatorSagar, R.
dc.date2005-11-11
dc.date.accessioned2026-07-07T06:45:01Z
dc.date.available2026-07-07T06:45:01Z
dc.descriptionWe present the CCD Cousins R band photometric observations of the afterglow of GRB 041006. The multiband afterglow evolution is modelled using an underlying `hard' electron energy spectrum with a $p_1 \sim 1.3$. The burst appears to be of very low energy ($E \sim 10^{48}$ ergs) confined to a narrow cone of opening angle $θ\sim 2.3^{\circ}$. The associated supernova is compared with SN1998bw and is found to be brighter.
dc.descriptionAccepted for publication in Bull. Astr. Soc. India (BASI)
dc.identifierhttps://arxiv.org/abs/astro-ph/0511352
dc.identifierhttp://arxiv.org/abs/astro-ph/0511352
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/102944
dc.subjectAstrophysics
dc.titleOptical Observations and Multiband Modelling of the Afterglow of GRB 041006: Evidence of A Hard Electron Energy Spectrum
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