Bruno Khélifi


Gamma-ray astrophysicist at the Astroparticles & Cosmology laboratory, APC (Paris, France)
CNRS/IN2P3 - Université Paris Cité
My research focuses on the observational study of the acceleration processes of charged particles into galactic astrophysical objects, such as pulsar wind nebulae or PeVatrons.
With the development of the Open Science and the multi-messenger astrophysics, I am involved in projects on open software and open data format in order to realise multi-instrument data analyses.
All my publications can be found on my ORCID profile.



TeV astronomy

The H.E.S.S. experiment

Gamma-ray observations of the Southern sky (10GeV-100TeV)
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The High Energy Stereoscopic System array is located in Namibia and is operated by an european collaboration. Operational since 2002, this instrument permits to observe the TeV sky of the Southern hemisphere. Thanks to its performance, the first catalog of TeV gamma-ray sources has been released in 2018 (A&A 2018 612 A1).

Member of H.E.S.S. since 2002, I contributed to the construction of some equipment (funnels, camera mechanics) and I am responsible for one of the three official data analysis pipelines (HAP-Fr). My research activities are focused on the system pulsar/pulsar wind nebula and on the search for PeVatrons.

The CTA Observatory

The first TeV gamma-ray observatory (10GeV-300TeV)
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The Cherenkov Telescope Array observatory is the next generation for gamma-ray astronomy at very high energy (arXiv:2305.12888). It will have one site per hemisphere. The Northern site is located in the La Palma island (Spain) and will host 13 telescopes to observe gamma rays from 10GeV to 10TeV. The Southern site (illustrated in the above picture) is located in the Atacama desert (Chili) nearby to the ESO Paranal observatory. It will consist on more than 50 telescopes, permitting to detect gamma rays on the full energy range of CTA.

I am participating to CTA since its birth's meeting in 2006 and I am actively contributing to its construction: optics, mechanics and instrumentation of one type of cameras, concepts of calibration and science user support systems, optimisation of telescope layouts, R&D for low-level data reconstruction, data modeling, requirements, science analysis tool for the high-level data, proposal handling website, etc.


Open Science

Data: GADF format, VODF format, H.E.S.S. | Software: Gammapy | Community: Open Science groups

GADF

Data formats for gamma-ray astronomy

Active member of the open initiative Gamma Astro Data Format (GADF) that is about to be ended.

First common open data format for the high-level very-high-energy gamma-ray data, that has became a standard for the community (.

VODF

Open data format for Very-High-Energy gamma-ray and neutrino astronomy

Initiator and convener of the open initiative Very-high-energy Open Data Format (VODF)

Aims:

H.E.S.S. first public data release

First public data from TeV gamma-ray astronomy

Active member of the group that has created the dataset and curated the data under the GADF format (ee arXiv:1810.04516 and DOI 10.5281/zenodo.1421098).

Gammapy

A Python package for gamma-ray astronomy

Project manager of the open research software permitting joint analyses of multi-instrument VHE data (see e.g. A&A 667 A36 (2022)), aiming to respect the FAIR4RS principles. Full description: A&A 678 A157 (2023)

Granted by the jury prize in 2022 of the first Open Research Software awards organised by the French ministry of Research (Gammapy award). Selected as core library of the CTAO Science Analysis Tool (see the CTAO press release).

Open Science Community

Towards an open very-high-energy astrophysics

Member of various groups on data and software, two pillars of the Open Science:

  • ambassador of SoftwareHeritage, the universal archive of open software,
  • member of the international organisations IVOA (International Virtual Open Association), RDA (Research Data Alliance),
  • member of the national organisations ASOV (Action Spécifique Observatoires Virtuels), IN2P3 advisory committee DOP2I (Données Ouvertes Pour les 2 infinis),
  • internal Open Science referent in APC and APC representative of the Open Science group of Université Paris Cité.

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Positions

APC, Paris (France)

Staff Researcher (CNRS)
Gamma-ray astronomy with H.E.S.S. and CTA
Since October 2013

LLR, Palaiseau (France)

Staff Researcher (CNRS)
Gamma-ray astronomy with H.E.S.S. and CTA
November 2002 - September 2013

MPIK, Heidelberg (Germany)

Post-doctorate
Gamma-ray astronomy with H.E.S.S.

Supervised by W. Hofmann

December 2002 - September 2005

Education

Université Paris Cité (France)

Accreditation to supervise research - HDR
The TeV astrophysics towards Open Science

To be soon published

April 2024

Université de Caen - Basse Normandie (France)

PhD
Speciality: Subatomic particles - Gamma-ray astronomy


Gamma sources search with a Maximum Likelihood method: Application to AGN and galactic sources observed by the CAT telescope
Supervised by P. Espigat (PCC-Collège de France, Paris)

Link to manuscript (in French)

November 2002

Skills

Programming Languages & Tools
Data Curation
  • Data modeling for high-level TeV data (with CTAO)
  • Data formating for high-level TeV data (GADF, VODF)

Workflow
  • Low-level analysis of TeV Cherenkov data (calibration, reconstruction, discrimination)
  • Massive production of TeV Cherenkov calibrated data (DL1 in ROOT)
  • Massive production of science-ready data (DL3 in FITS)
  • High-level analysis of TeV gamma-ray data
  • Big data processing on clusters
  • Agile Development & Scrum, Documentation
  • Cross Functional Teams