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IX/51 GRB list (1990-2014) (Ruggeri+, 2016)
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Beginning of ReadMe :IX/51 GRB list (1990-2014) (Ruggeri+, 2016)
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Possible Gamma-Ray Burst radio detections by the Square Kilometre Array.
New perspectives.
Ruggeri A.C., Capozziello S.
<Thesis, Universita degli Studi di Napoli Federico II, (2016)>
=2016Ap&SS.361..279R
=2017yCat.9051....0R
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ADC_Keywords: Gamma rays
Keywords: gamma-rays: bursts - cosmology: cosmological parameters - radio band -
SKA radio-telescope
Abstract:
The next generation interferometric radio telescope, the Square
Kilometre Array (SKA), which will be the most sensitive and largest
radio telescope ever constructed, could greatly contribute to the
detection, survey and characterization of Gamma Ray Bursts (GRBs). By
the SKA, it will be possible to perform the follow up of GRBs even for
several months. This approach would be extremely useful to extend the
Spectrum Energetic Distribution (SED) from the gamma to the to radio
band and would increase the number of radio detectable GRBs. In
principle, the SKA could help to understand the physics of GRBs by
setting constraints on theoretical models. This goal could be achieved
by taking into account multiple observations at different wavelengths
in order to obtain a deeper insight of the sources. Here, we present
an estimation of GRB radio detections, showing that the GRBs can
really be observed by the SKA. The approach that we present consists
in determining blind detection rates derived by a very large sample
consisting of merging several GRB catalogues observed by current
missions as Swift, Fermi, Agile and INTEGRAL and by previous missions
as BeppoSAX, CGRO, GRANAT, HETE-2, Ulysses and Wind. The final
catalogue counts 7516 distinct sources. We compute the fraction of
GRBs that could be observed by the SKA at high and low frequencies,
above its observable sky. Considering the planned SKA sensitivity and
through an extrapolation based on previous works and observations, we
deduce the minimum fluence in the range 15-150keV. This is the
energy interval where a GRB should emit to be detectable in the radio
band by the SKA. Results seem consistent with observational
capabilities.
Description:
To investigate the potentialities of the SKA related to the GRB
detections in radio band, we need a good instrumental probability, so
that we present here a useful repository of all GRBs taken by several
catalogues.
The thesis is available at:
http://www.fedoa.unina.it/10538/1/Ruggeri_Alan_Cosimo_27.pdf
The paper is available at:
http://adsabs.harvard.edu/abs/2016Ap%26SS.361..279R