Zobrazeno 1 - 10
of 44
pro vyhledávání: '"J. Michael Burgess"'
Autor:
J. Michael Burgess, Jochen Greiner, Damien Bégué, Dimitrios Giannios, Francesco Berlato, Vladimir M. Lipunov
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 7 (2020)
The detection of a faint, short gamma-ray burst (GRB 170817A) in coincidence with the gravitational wave (GW 170817) detection by LIGO/Virgo is at odds with the expected known luminosity and redshift distribution of short GRBs (sGRB). Examining the o
Externí odkaz:
https://doaj.org/article/997d6e7d973c4a92aeef8149835b2bde
Several tentative associations between high-energy neutrinos and astrophysical sources have been recently reported, but a conclusive identification of these putative neutrino emitters remains challenging. We investigate the context of proposed indivi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7afed326357a79744b95c867d448fc42
Autor:
J. Michael Burgess
Publikováno v:
Journal of Open Source Software. 8:4969
`ronswanson` provides a simple-to-use framework for building so-called table or template models for `astromodels`the modeling package for multi-messenger astrophysical data-analysis framework, `3ML`. With `astromodels` and `3ML` one can build the int
INTEGRAL/SPI is a coded mask instrument observing since 2002 in the keV to MeV energy range, which covers the peak of the $\nu F\nu$ spectrum of most Gamma-Ray Bursts (GRBs). Since its launch in 2008, Fermi/GBM has been the primary instrument for ana
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2175576077ce111dc65fca193b8020b2
Autor:
J. Michael Burgess, Francesca Capel
Publikováno v:
Journal of Open Source Software. 6:3257
Simulating a survey of fluxes and redshifts (distances) from an astrophysical population is a routine task. \texttt{popsynth} provides a generic, object-oriented framework to produce synthetic surveys from various distributions and luminosity functio
Publikováno v:
Nature Astronomy. 4:132-133
The localizations of gamma-ray bursts (GRBs) detected with the Gamma-ray Burst Monitor (GBM) onboard the Fermi satellite are known to be affected by significant systematic errors of 3-15 degrees. This is primarily due to mismatch of the employed Band
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e9417fe70ab88213ff002b02cc340584
Publikováno v:
Astronomy & Astrophysics. 640:A8
We present the first physically motivated background model for the Gamma-Ray Burst Monitor (GBM) onboard the Fermi satellite. Such a physically motivated background model has the potential to significantly improve the scientific output of Fermi/GBM,
Inspired by the confirmed detection of a short gamma-ray burst (GRB) in association with a gravitational wave signal, we present the first Bayesian Fermi-Gamma-ray Burst Monitor (GBM) short GRB spectral catalogue. Both peak flux and time-resolved spe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5c4d4b242342ee0445695bd12368d80c
https://mediatum.ub.tum.de/1539730
https://mediatum.ub.tum.de/1539730
Gamma-ray bursts are the most energetic electromagnetic sources in the Universe. Their prompt gamma-ray radiation corresponds to an energy release of 1E42-1E47J. Fifty years after their discovery and several dedicated space-based instruments, the phy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::564820a902aebaddc981a24f9d37d9a1
http://arxiv.org/abs/1810.06965
http://arxiv.org/abs/1810.06965