BVRcIc photometry of GRB 980703 and GRB 990123 host galaxies

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dc.creatorSokolov, V. V.
dc.creatorFatkhullin, T. A.
dc.creatorKomarova, V. N.
dc.date2000-01-20
dc.date2000-04-27
dc.date.accessioned2026-07-07T01:51:49Z
dc.date.available2026-07-07T01:51:49Z
dc.descriptionWe present a photometry of GRB 980703 and GRB 990123 host galaxies which was performed about 20 days and a half year after gamma-ray bursts occured, respectively. The contributions of the optical transiets (OT) were negligible in both cases. We derived broad band BVR_cI_c spectra of the host galaxies and compared them to continuum spectra of different Hubble-type galaxies and averaged spectra of starburst galaxies. For H_0=60 km s^{-1} Mpc^{-1} and three Friedmann cosmological models with matter density and cosmological constant parameters (Omega_m,Omega_Lambda) = (1,0),(0,0),(0,1) we estimated M_Brest and star-forming rates (SFRs) using the fluxes in photometric bands for the host galaxies. Within the range of cosmological parameters our estimates of the absolute magnitudes are: M_Brest = -20.60 .. -21.73 for the GRB 980703 host galaxy and M_Brest = -20.20 .. -21.82 for the GRB 990123 host galaxy. We obtained estimates of K-correction values and absolute magnitudes of the host galaxies using SEDs for star-forming galaxies.
dc.description7 pages, 3 encapsulated postscript figures, to appear in Bulletin of the Special Astrophysical Observatory of Russian AS
dc.identifierhttps://arxiv.org/abs/astro-ph/0001357
dc.identifierhttp://arxiv.org/abs/astro-ph/0001357
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/421
dc.subjectAstrophysics
dc.titleBVRcIc photometry of GRB 980703 and GRB 990123 host galaxies
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