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Institut d'Astrophysique et
de Géophysique (Bât. B5c)

Quartier Agora
Allée du 6 août, 19C
B-4000 Liège 1 (Sart-Tilman)
Belgique

Tel.: 04.366.9779
Fax: 04.366.9729

Seminars

Seminars are regularly held to enable department's researchers as well as external scientists to present the latest findings in their fields. You are most welcome to join us:

16/05/2024 :
16h00  
A multimessenger GW-GRB study of the sGRB population and its future developments
Matteo Pracchia
23/05/2024 :
16h00  
TBA
Dixeena Lopez
26/06/2024 :
16h00  
TBA
Victoria Bonidie
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Next seminar Thursday 16 may, 16h00 (8th Seminar 2024 - poster)
A multimessenger GW-GRB study of the sGRB population and its future developments
Matteo Pracchia (Université de Liège)

Salle de réunion AGO (local -1/14), Institut d'Astrophysique et de Géophysique
Bâtiment B5c, Quartier Agora, Allée du 6 Août, 19C, B-4000 Liège 1 (Sart-Tilman)


The unambiguous joint detection of GRB 170817A and GW170817 has been the long-awaited smoking gun for the association between short gamma-ray bursts (sGRBs) and the merger of binary neutron stars (BNS) systems. The aforementioned sGRB, however, was extremely close and had an unexpectedly low measured luminosity when compared to the other observed sGRBs, suggesting that there is a sub-luminous fraction of the GRB population which is undetected at the usually measured distances.

This work aims to characterize the low-luminosity part of the sGRB population through a multi-messenger GW-GRB Bayesian study. The sGRB population is described via its luminosity probability distribution, modelled through an extension of a broken power law whose parameters have already been constrained through mid-high luminosity sGRB observations. The parameters of this power-law extension, i.e. the low luminosity power index and the low-luminosity cutoff, are constrained through a Bayesian analysis which exploits the results from the modelled GW follow-up analysis of the short GRBs detected during the first three observing runs of the International Gravitational-Wave observatory Network (IGWN).

The results obtained allow us to define the luminosity distribution at lower values for the sGRB population and to give an estimate of the value found for the astrophysical sGRB rate and the joint GW-GRB detection rate for the next IGWN observing runs. There are, nonetheless, some upgrades to the method used for this study that could give a more precise and complete outline of the astrophysical sGRB population.
Previous seminar Next seminar Thursday 23 may, 16h00 (9th Seminar 2024 - poster)
TBA
Dixeena Lopez (Université de Liège)

Le lieu où se tiendra cet évènement n'est pas encore déterminé...
Previous seminar Wednesday 26 june, 16h00 (10th Seminar 2024 - poster) 
TBA
Victoria Bonidie (Pittsburgh University)

Salle de réunion AGO (local -1/14), Institut d'Astrophysique et de Géophysique
Bâtiment B5c, Quartier Agora, Allée du 6 Août, 19C, B-4000 Liège 1 (Sart-Tilman)
University of Liège > Faculty of Sciences > Department of Astrophysics, Geophysics and Oceanography : CoWebAGO, June 2009.