Hostname: page-component-89b8bd64d-ksp62 Total loading time: 0 Render date: 2026-05-08T19:57:05.302Z Has data issue: false hasContentIssue false
  • English
  • Français

Localisation of gamma-ray bursts from the combined SpIRIT+HERMES-TP/SP nano-satellite constellation – CORRIGENDUM

Published online by Cambridge University Press:  01 April 2024

M. Thomas ,
M. Trenti ,
A. Sanna ,
R. Campana ,
G. Ghirlanda ,
J. Rípa ,
L. Burderi ,
F. Fiore ,
Y. Evangelista  and
L. Amati
...Show all authors
Rights & Permissions [Opens in a new window]

Abstract

An abstract is not available for this content. As you have access to this content, full HTML content is provided on this page. A PDF of this content is also available in through the ‘Save PDF’ action button.

Information

Type
Corrigendum
Information
Publications of the Astronomical Society of Australia , Volume 41 , 2024 , e017
Check for updates
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of Astronomical Society of Australia

The authors regret the inclusion of an error in the above article. In Thomas et al. (Reference Thomas2023), in Section 4.4 and 4.5.2 we incorrectly report that we are using the Flnc_Band_Phtfluxb data from the Fermi GBM Burst catalog, when in reality we are using the Pflx_Band_Phtfluxb data to generate GRB fluxes.

References

Thomas, M. et al. (2023) ‘Localisation of gamma-ray bursts from the combined SpIRIT+HERMES-TP/SP nano-satellite constellation’, Publications of the Astronomical Society of Australia, 40, p. e008. doi: 10.1017/pasa.2023.4.CrossRefGoogle Scholar