The optical/near-IR spectral energy distribution of the GRB 000210 host galaxy

Simple item page
dc.creatorGorosabel, J.
dc.creatorChristensen, L.
dc.creatorHjorth, J.
dc.creatorFynbo, J. U.
dc.creatorPedersen, H.
dc.creatorJensen, B. L.
dc.creatorAndersen, M. I.
dc.creatorLund, N.
dc.creatorJaunsen, A. O.
dc.creatorCerón, J. M. Castro
dc.creatorTirado, A. J. Castro
dc.creatorFruchter, A.
dc.creatorGreiner, J.
dc.creatorPian, E.
dc.creatorVreeswijk, P. M.
dc.creatorBurud, I.
dc.creatorFrontera, F.
dc.creatorKaper, L.
dc.creatorKlose, S.
dc.creatorKouveliotou, C.
dc.creatorMasetti, N.
dc.creatorPalazzi, E.
dc.creatorRhoads, J.
dc.creatorRol, E.
dc.creatorSalamanca, I.
dc.creatorTanvir
dc.creatorWijers, R. A. M. J.
dc.creatorHeuvel, E. P. J. van den
dc.date2003-01-29
dc.date.accessioned2026-07-07T02:07:21Z
dc.date.available2026-07-07T02:07:21Z
dc.descriptionWe report on UBVRIZJsHKs-band photometry of the dark GRB 000210 host galaxy. Fitting a grid of spectral templates to its Spectral Energy Distribution (SED), we derived a photometric redshift (z=0.842\+0.0540.042) which is in excellent agreement with the spectroscopic one (z=0.8463+/-0.0002; Piro et al. 2002). The best fit to the SED is obtained with a blue starburst template with an age of 0.181\+0.0370.026 Gyr. We discuss the implications of the inferred low value of Av and the age of the dominant stellar population for the non detection of the GRB 000210 optical afterglow.
dc.description4 pages, 1 figure, contribution to the Rome 2002 GRB workshop
dc.identifierhttps://arxiv.org/abs/astro-ph/0301564
dc.identifierhttp://arxiv.org/abs/astro-ph/0301564
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5667
dc.subjectAstrophysics
dc.titleThe optical/near-IR spectral energy distribution of the GRB 000210 host galaxy
dc.typetext

Files

Collections

arXiv