Particle Physics Division

 

 

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Cherenkov Imaging Telescopes

Left : A CTA telescope prototype – (c) Consortium CTA.

Right : The Atmospheric Cherenkov detection principle. A gamma ray interacts in the atmosphere at an altitude of about 15 km. It creates a shower of particles propagating at nearly the speed of light, thus leading to the emission of a thin bluish conic light beam, known as Cherenkov light. The light propagates to the ground where it illuminates a telescope mirror reflecting the photons to a camera consisting of a grid of photomultiplier pixels.

 

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Observing the entire Sky

 

CTA is in the process of being deployed on two sites in order to cover the entire sky. In the Southern Hemisphere, the site will be situated near the Paranal Observatory in the Atacama Desert north of Chile, which also hosts the VLT.  It will be composed of about a hundred telescopes and will provide a view of the interior regions of the Galactic Plane.  In the Northern Hemisphere, the Roque de los Muchachos Observatory on the Canary Island of La Palma will host around 20 telescopes and will have the principal goal of exploring the extra-galactic universe.

 

On the right : Top image, view of the southern CTA site, Paranal, Chile (c)ESO; Bottom image, View of the northern CTA site, La Palma, Spain (c) Miguel Claro.   

 

The DAp team

 

The SAp group comprises a dozen researchers from LEPCHE and LISIS who already use or will use data from other telescopes like HESS, satellites like Fermi, Integral, XMM-Newton, and the neutrino telescope Antares.  The scientific themes covered by the group range from galactic astrophysics (supernova remnants, X-ray binaries, pulsars, and diffuse flux…) to gamma-ray bursts, in collaboration with the SVOM group in DAp.

The group is involved in the preparatory work in data analysis, in particular with the development of innovative tools for the reconstruction of atmospheric showers and the analysis of sky images, as well as adapting them for real-time operation for the detection of gamma-ray bursts or other transient sources. The group is developing its scientific program by participating in the definition of future observations by the consortium. 

The DAp group is coordinating the development of the data processing software, the data pipeline, which will reconstruct gamma-ray-like photon lists from the raw data of the cameras.  It has also coordinated comparative studies of the infrastructure of 13 site candidates, starting with a generic specification and technical visits contracted out to a public works company (Ingérop)

_{Traduction: Karl Kosack, contact : Thierry Stolarczyk}

 

 

The CTA team at DPhP

 

The CTA team at DPhP is composed of physicists also participating in the astroparticle experiments H.E.S.S. (very high energy photons) and ANTARES (very high energy neutrinos). The group has activities related to hardware (cameras, mirrors for telescopes of the new observatory), but also to the preparation of the exploitation of physics (Galactic Center, dark matter, axions, Lorentz invariance tests, counterparts optical events gravitational waves and more generally physical multi-wavelength, etc.) with their colleagues from DAp.

The physics of CTA is described in detail on the page: https://www.cta-observatory.org/science/and in the publication https://arxiv.org/abs/1709.07997 

The group of the DPhP is composed in 2018 of 7 physicists, 1 postdoctoral fellow and 3 PhD students.

Some recent publications of members of the group (2016-2018) related to the construction and the prospective of physics with CTA and

• dark matter detection:

http://cdsads.u-strasbg.fr/abs/2016JCAP...09..043L

http://cdsads.ustrasbg.fr/abs/2016PhRvD..94j3005B

• assessment of CTA sensitivity:

http://cdsads.u-strasbg.fr/abs/2016SPIE.9906E..3OF 

• transient events and multiwavelength physics:

http://cdsads.u-strasbg.fr/abs/2017ICRC...35.1106S 

• -NectarCAM camera:

 http://cdsads.u-strasbg.fr/abs/2017AIPC.1792h0009G

 

The group (which includes the scientific leader of the NectarCAM camera) is involved in verifying the performance of the NectarCAM camera and preparing the data collection on the CTA site. He works closely with IRFU's technical departments who are responsible for camera management (including the NectarCAM project manager) and integration. He also works in close collaboration with CNRS, DESY-Zeuthen, CIEMAT and UCM GAE (Madrid), ICC-UB and IFAE (Barcelone) groups.

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The group is responsible for providing lightweight mirrors for CTA's MST telescopes. He works in close collaboration with the technical departments of the IRFU.

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Contact: Jean-François Glicenstein