The Nordic Optical Telescope discovers supernova associated with
monster Gamma-Ray Burst
Release date: 2013/11/28
On April 27 the Fermi and Swift satellites discovered
one of the most luminous gamma-ray bursts ever discovered on Earth.
Last week four papers were published in the prestigious
Science
magazine reporting on the properties of the gamma-ray burst GRB
130427A and its afterglow observed over a very broad range of
frequencies from optical light to high-energy γ-rays. One of the most important discoveries related to this
burst was carried out with the Nordic Optical Telescope in concert
with the Gran Telescopio Canarias, namely the detection of the
supernova associated with the burst, the tell-tale signature that an
exploding star was the origin of the burst.
Gamma-ray bursts (GRBs) are energetic eruptions in gamma-rays that
briefly light up the gamma-ray sky. For decades following their
discovery in the late 1960s, their origin has remained a complete
mystery. In the late 1990s it was established that GRBs originate from
the most distant reaches of the Universe. They are therefore the most
luminous known objects, and they are also extremely rare, occurring in
typical galaxies only once every several million years. Only
occasionally do these extreme explosions occur in the more nearby
galaxies. In these cases, we not only detect extremely bright bursts
here on Earth, but we also have the opportunity to study what exactly
happened in the explosion. In the case of the gamma-ray burst from
April 27 2013, designated GRB 130427A, a team led by Dong Xu from the
Dark Cosmology Centre in Copenhagen used the Nordic Optical Telescope
and the Gran Telescopio Canarias to discover and characterize the
Broad-lined Type Ic supernova
(SN2013cq)
that accompanied this relatively nearby (z=0.34) gamma-ray burst.
A supernova is the light emitted by an exploding star at the end of
its life, and its detection provides a direct clue to the progenitor
of the GRB. The discovery of a SN associated with this GRB is
important, as it establishes clearly that these extremely bright
bursts are formed by the same class of very massive, hydrogen-stripped
stars as other much less extreme gamma-ray bursts that we had
previously studied at similar distances. Given that this GRB is
similar in properties to the bulk of the population of gamma-ray
bursts seen in the more distant Universe, this discovery puts us a
step closer to understanding the GRB phenomenon in general. In
particular, we can now be more confident of the nature and origin of
distant GRBs, and we can exploit them as valuable probes of the most
remote and ancient parts of the Universe.
The evolution in time of the luminosity of the GRB emission, measured
since the GRB explosion. There is excess emission starting a few days
after the GRB, compared to extrapolation of the early emission (black
squares). This extra emission (blue points), peaking about 15 days
after the GRB, is the associated SN, named SN 2013cq (from Xu et al.,
Astrophysical Journal,
776, 98).
This first spectrum, taken with the Nordic Optical Telescope less than
a day after the burst, is dominated by the afterglow of the gamma-ray
bursts. Over the following days and weeks the emission is gradually
dominated by the light from the associated supernova, SN2013cq (from
Xu et al., Astrophysical Journal,
776, 98)