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A search for Fermi bursts associated with supernovae and their frequency of occurrence

Kovacevic, M. (författare)
Izzo, L. (författare)
Wang, Y. (författare)
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Muccino, M. (författare)
Della Valle, M. (författare)
Amati, L. (författare)
Barbarino, C. (författare)
Enderli, M. (författare)
Pisani, G. B. (författare)
Li, L. (författare)
Stockholms universitet,KTH,Fysik,Stockholm University, Sweden,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC),KTH Royal Institute of Technology, Sweden
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 (creator_code:org_t)
2014-09-30
2014
Engelska.
Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 569, s. A108-
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
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  • Context. Observations suggest that most long duration gamma-ray bursts (GRBs) are connected with broad-line supernovae Ib/c, (SNe-Ibc). The presence of GRB-SNe is revealed by rebrightenings emerging from the optical GRB afterglow 10-15 days, in the rest-frame of the source, after the prompt GRB emission. Aims. Fermi/GBM has a field of view (FoV) about 6.5 times larger than the FoV of Swift, therefore we expect that a number of GRB-SN connections have been missed because of lack of optical and X-ray instruments on board of Fermi, which are essential for revealing SNe associated with GRBs. This has motivated our search in the Fermi catalog for possible GRB-SN events. Methods. The search for possible GRB-SN associations follows two requirements: (1) SNe should fall inside the Fermi/GBM error box of the considered long GRB, and (2) this GRB should occur within 20 days before the SN event. Results. We have found five cases within z < 0.2 fulfilling the above reported requirements. One of them, GRB130702A-SN 2013dx, was already known to have a GRB-SN association. We have analyzed the remaining four cases and we have concluded that three of them are, very likely, just random coincidences due to the Fermi/GBM large error box associated with each GRB detection. We found one GRB possibly associated with a SN 1998bw-like source, GRB 120121B/SN 2012ba. Conclusions. The very low redshift of GRB 120121B/SN 2012ba (z = 0 : 017) implies a low isotropic energy of this burst (E-iso = 1 : 39 x 10(48)) erg. We then compute the rate of Fermi low-luminosity GRBs connected with SNe to be rho(0,b) <= 770 Gpc(-3) yr(-1). We estimate that Fermi/GBM could detect 1-4 GRBs-SNe within z <= 0.2 in the next 4 years.

Ämnesord

NATURVETENSKAP  -- Fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Nyckelord

gamma-ray burst: general
supernovae: general

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