Presented at the 89th Spring Meeting of the AAVSO,
April 15, 2000
Abstract
The
world’s leading neutrino and gravitational wave detectors have come together in
a collaboration with the aim of providing traditional optical astronomers an
early warning of an impending Galactic supernova. It is expected that a robust
alert can be issued within 15 minutes of the neutrino and gravitational wave
detection, leading to an early warning of between 15 minutes and eight hours of
the optical signal’s arrival, depending on the progenitor. Additionally, the
direction of the supernova can be determined to around 5°. Such an alert will
provide invaluable warning, allowing the more precise location necessary for
the world’s premier telescopes to be determined more quickly, through both
all-sky monitors and amateurs ready to start observing upon issuance of an
alert. This talk describes the motivation and implementation of SNEWS, the
current status, and the planned methods for distribution of an alert to
astronomers.