ÚTEFČVUT Ústav technické a experimentální fyziky ČVUT v PrazeInstitute of Experimental and Applied Physics, CTU in Prague

Fitting GRB afterglow broadband data to hydrodynamical simulations

NázevTitle
Fitting GRB afterglow broadband data to hydrodynamical simulationsFitting GRB afterglow broadband data to hydrodynamical simulations
Druh výsledkuResult type
Příspěvek ve sborníkuProceedings paper
AutořiAuthors
F. Knust, H.-J. van Eerten, J. Greiner, R. Filgas
Klíčová slovaKeywords
GRB
KonferenceConference
Swift: 10 Years of Dicovery (Rome, Italy, 2014-12-02)
Časopis / citaceJournal / citation
In: Proceedings of Science, SISSA/ISAS, 2014 · ISSN 1824-8039
RokYear
2014
JazykLanguage
eng
ZáznamyRecords
ProjektProject
Porovnání syntetických světelných křivek optických dosvitů gama záblesků s pozorovanými daty z detektoru GRONDComparing synthetic lightcurves of GRB afterglows with observational data from GROND.
Citace ke staženíDownload citation
TXT · BibTeX

AbstraktAbstract

The Gamma-Ray burst Optical Near-infrared Detector (GROND) offers early time data of Gamma Ray Burst (GRB) afterglows in 4 optical and 3 near-infrared (NIR) bands simultaneously. We extended the SCALEFIT package to allow for joint fits of GROND and Swift/XRT data. Using GRB 140512A, we demonstrate the improvements over fitting X-ray data only. We are able to constrain some of the parameters of the fireball model, for others we derive limits.

The Gamma-Ray burst Optical Near-infrared Detector (GROND) offers early time data of Gamma Ray Burst (GRB) afterglows in 4 optical and 3 near-infrared (NIR) bands simultaneously. We extended the SCALEFIT package to allow for joint fits of GROND and Swift/XRT data. Using GRB 140512A, we demonstrate the improvements over fitting X-ray data only. We are able to constrain some of the parameters of the fireball model, for others we derive limits.

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