The optical afterglow and host galaxy of GRB 000926

J.U. Fynbo, J. Gorosabel, T.H. Dall, H. Pedersen, M.I. Andersen, P. Møller, S. Holland, I. Smail, N. Kobayashi, Niels Lund

Research output: Chapter in Book/Report/Conference proceedingArticle in proceedingsResearchpeer-review


In this paper we illustrate with the case of GRB 000926 how Gamma Ray Bursts (GRBs) can be used as cosmological lighthouses to identify and study star forming galaxies at high redshifts. The optical afterglow of the burst was located with optical imaging at the Nordic Optical Telescope 20.7 hours after the burst. Rapid follow-up spectroscopy allowed the determination of the redshift of the burst and a measurement of the host galaxy HI-column density in front of the burst. With late-time narrow band Lyalpha as well as broad band imaging, we have studied the emission from the host galaxy and found that it is a strong Lyalpha emitter in a state of active star formation.
Original languageEnglish
Title of host publicationLighthouses of the universe : The most luminous celestial objects and their use for cosmology
Publication date2002
ISBN (Print)3-540-43769-X, 978-3-540-43769-7
ISBN (Electronic)978-3-540-48014-3
Publication statusPublished - 2002
EventMPA/ESO/MPE/USM Joint Astronomy Conference on Lighthouses of the Universe - Garching, Germany
Duration: 6 Aug 200110 Aug 2001


ConferenceMPA/ESO/MPE/USM Joint Astronomy Conference on Lighthouses of the Universe
SeriesE S O Astrophysics Symposia


Dive into the research topics of 'The optical afterglow and host galaxy of GRB 000926'. Together they form a unique fingerprint.

Cite this