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Completed RESEARCH INFRASTRUCTURE Swedish Research Council

Fermi Gamma Ray Space Telescope

22.29M kr SEK

Funder Swedish National Space Agency
Recipient Organization Kth, Royal Institute of Technology
Country Sweden
Start Date Jan 01, 2022
End Date Dec 31, 2024
Duration 1,095 days
Number of Grantees 2
Roles Co-Investigator; Principal Investigator
Data Source Swedish Research Council
Grant ID 2021-00180_SNSB
Grant Description

The Fermi GST has already revolutionised our view of the high-energy universe.

In particular, the exciting results on dark matter (DM), gamma-ray bursts (GRBs), active galactic nuclei (AGNs), and pulsars have shown how splendid the telescope is.

The results of the recent NASA Senior Review confirmed that and recognised Fermi’s continued importance in multi-messenger astronomy.

Though the Swedish community is relatively small we have been active in Fermi since its inception, contributing to hardware, calibration and data analysis.

Most recently we have concentrated our efforts in data monitoring, coordination of transient follow-up and development of analysis techniques.

This participation has been possible thanks to long-term support from the Swedish National Space Agency.This application is aimed at continued funding to allow Sweden to remain a member in the international Fermi collaboration, and projects to maximise the Swedish scientific return. Swedish scientists are mainly involved in studies of gamma-ray bursts, active galactic nuclei and dark matter.

Our projects are therefore focused to support these areas, through development of event selection and data analysis techniques as well as data quality monitoring and improving transient follow-up.In the coming period, Fermi will continue to play a vital role in multi-messenger astronomy, such as the search for electromagnetic counterparts to gravitational waves.

To meet these challenges, we are broadening the Swedish participation to also include the GBM instrument on-board Fermi.

This is the most prolific detector of gamma-ray bursts in orbit, and therefore highly relevant to follow-up studies of gravitational events.

As part of this renewal, we will help improve localization techniques, contribute to burst advocate shifts and develop techniques to perform highly time-resolved spectral analysis.A seperate application outlining our scientific projects, which will make use of this involvement in Fermi, will be submited to SNSA call 2021-R.

All Grantees

Kth, Royal Institute of Technology

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