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Table · dataset · 2008

R-band photometry of GRB 060206

Listed in IVOA Registry (Virtual Observatory)

The Rapid Telescopes for Optical Response (RAPTOR) system at Los Alamos National Laboratory observed GRB 060206 starting 48.1min after gamma-ray emission triggered the Burst Alert Telescope on board the Swift satellite.

Description

The afterglow light curve measured by RAPTOR shows a spectacular rebrightening by ~1mag about 1hr after the trigger and peaks at R~16.4mag. Shortly after the onset of the explosive rebrightening, the optical transient doubled its flux on a timescale of about 4min.

The total R-band fluence received from GRB 060206 during this episode is 2.3x10^9^ergs/cm^2^. In the rest frame of the burst (z=4.045), this yields an isotropic equivalent energy release of E_iso_~0.7x10^50^ergs in just a narrow UV band, {lambda}~130{+/-}22nm. We discuss the implications of RAPTOR observations for untriggered searches for fast optical transients and studies of GRB environments at high redshift.

Links

Where it is published

Documentation and papers

Catalogue records · 2

Topics

Stated by source
Gamma-Ray · Optical
Provenance · 1 source records, 9 field assertions
SourceKeyLast seenRaw
IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/apj/642/l9915 d agoJSON v1
FieldAssertionExtractorEvidence
access_levelsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:gamma-raysource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:opticalsource · IVOA Registryconnector:ivoa_registry@1.0.0
descriptionsource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_description
license_textsource · IVOA Registryconnector:ivoa_registry@1.0.0
publication_datesource · IVOA Registryconnector:ivoa_registry@1.0.0
titlesource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_title
updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0