Two other teams, one lead by Derek Fox of Caltech and the other lead by Jens Hjorth of the University of Copenhagen, detected x-ray and
optical afterglows from the burst.
(B) The burst leaves
an optical afterglow.
Its optical afterglow was detected 84 hours after burst detection.
Another small proportion of GRBs exhibit comparatively short - duration bursts that average only 0.3 seconds and very little x-ray and
optical afterglow (Gehrels et al, 2002).
Not exact matches
These telescopes, along with Swift's own UV /
Optical Telescope and other robotic telescopes alerted by the satellites, monitored the six - week
afterglow of visible light following the burst.
As the wave expands and the fire fades, the
afterglow changes «color» from x-ray to
optical light to radio waves.
Related sites Gamma ray burst
afterglows Optical Observations of GRBs An explanation of microlensing Joining the GRB Network as an amateur
Using radio telescopes in Australia and
optical telescopes in Hawaii, Keane and his colleagues detected an FRB and linked its fading
afterglow to a host galaxy some six billion light - years from Earth.
Its three onboard instruments will observe GRBs and their
afterglows in four different wavebands: gamma ray, X-ray, ultraviolet and
optical.
«In particular, we will work on the developments of RTP molecules and polymers with potential of finding high - tech applications in bioimaging,
optical recording, anti-counterfeiting, and
afterglow organic LEDs.»
They also discovered that a monthlong
afterglow followed the event that could be observed with instruments used to detect
optical frequencies, x-rays or radio waves.
Quick follow - up observations undertaken with the 8.2 - m Antu instrument at European Southern Observatory's Very Large Telescope in the Paranal and the 1.5 - meter Danish telescope at La Silla identified a faint, point - like object in visible light that was fading rapidly, the
optical counterpart of the gamma - ray burst called the «
afterglow» (Pedersen et al, 2000).
However, X-ray,
optical and radio emission continues in an «
afterglow.»
While the burst's
afterglow showed a steady decline in brightness at both
optical and X-ray wavelengths, that was not the case at radio wavelengths.