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=== Structure of the unit === | === Structure of the unit === | ||
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This unit is an [[https:// | This unit is an [[https:// | ||
|“International Research Laboratory” (IRL) of CNRS]], e.g. a long lasting joint research structure created outside of the French territory. IRLs exist to bring together teams of researchers, | |“International Research Laboratory” (IRL) of CNRS]], e.g. a long lasting joint research structure created outside of the French territory. IRLs exist to bring together teams of researchers, | ||
IRLs are international schemes in which research work is jointly conducted around a shared scientific focus. These structure, within an identified location, the significant and lasting presence of scientists from a limited number of French and foreign research institutions. | IRLs are international schemes in which research work is jointly conducted around a shared scientific focus. These structure, within an identified location, the significant and lasting presence of scientists from a limited number of French and foreign research institutions. | ||
- | The IRL2009 FSLAC administrative location is at c/o IAC Via Lactea, ES38205 La Laguna, Island of Tene-rife, Spain. The staff may work at 3 possible locations, either the Teide Observatory (Tenerife, for the Themis team), or the Roque de los Muchachos Observatory (La Palma, for the Haute Energie | + | The IRL2009 FSLAC administrative location is at c/o IAC Via Lactea, ES38205 La Laguna, Island of Tenerife, Spain. The staff may work at 3 possible locations, either the Teide Observatory (Tenerife, for the Themis team), or the Roque de los Muchachos Observatory (La Palma, for the high-energy |
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- | The main reasons to exist of our IRL 2009 FSLAC are to strengthen and facilitate the scientific and tech-nological French activities in the Canary Islands (Spain) and to strengthen and formalize a long lasting | + | |
- | 1. in the field of gamma-ray astronomy at very high energies around the Cherenkov Telescope Ar-ray (CTA, ESFRI roadmap 2016) facilities development in the Canary Islands, namely the CTA North Observatory in La Palma | + | |
- | 2. in the field of solar physics, where both Parties have been jointly engaged since many years in the building and exploitation of the French telescope THEMIS, that is sited in Tenerife since 1994, and also the forthcoming next generation of solar telescopes, EST (ESFRI roadmap 2016) | + | |
- | 3. in the field the Cosmic Microwave Background (CMB) observations with the development of the KISS spectrometer | + | |
- | Teams, platforms, shared services, etc.: | + | |
- | The IRL 2009 is currently structured in two teams, one involved in the development of the CTA northern observatory (team “Haute Energie”), | + | |
- | Platforms (CNRS terminology): | + | |
- | - The THEMIS team maintains, operates and makes available to the whole of the French, Spanish and European communities the platform ‘THEMIS Solar Telescope’, | + | |
- | - The Haute Energie team currently participates to the building of the platform “CTA northern ar-ray”, a gamma-ray Cherenkov observatory which, when completed, will become the foremost global observatory for very high-energy gamma-ray astronomy over the next decade and be-yond. The scientific potential of CTA is extremely broad: from understanding the role of relativ-istic cosmic particles to the search for dark matter. | + | |
- | The IRL is self-hosted in a rented “chalet adosado” located at Avenida Menceyes | + | |
+ | The base offices are located at Avenida Menceyes | ||
=== Scientific objectives === | === Scientific objectives === | ||
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These collaborations are concentrated in three instrumentation projects of the French and Spanish communities, | These collaborations are concentrated in three instrumentation projects of the French and Spanish communities, | ||
- | * 1. in the field of gamma-ray astronomy at very high energies around the [[https:// | + | * 1. in the field of **gamma-ray astronomy at very high energies** around the [[https:// |
- | * 2. in the field of solar physics, where both Parties | + | * 2. in the field of **solar physics**, where both parties |
- | * 3. in the field the Cosmic Microwave Background (CMB) observations with the development of the KISS spectrometer and the NIKA2 cameras to be installed on the QUIJOTE telescope at the Teide Observatory | + | * 3. in the field the **Cosmic Microwave Background (CMB)** observations with the development of the KISS spectrometer and the NIKA2 cameras to be installed on the QUIJOTE telescope at the Teide Observatory |
- | Teams, platforms, shared services, etc.: | + | |
- | The IRL 2009 is currently structured in two teams, one involved in the development of the CTA northern observatory (team “Haute Energie”), | + | === FSLAC Teams === |
- | Platforms (CNRS terminology): | + | |
- | - The THEMIS team maintains, operates and makes available to the whole of the French, Spanish and European communities the platform ‘THEMIS Solar Telescope’, | + | |
- | - The Haute Energie team currently participates to the building of the platform “CTA northern ar-ray”, a gamma-ray Cherenkov observatory which, when completed, will become the foremost global observatory for very high-energy gamma-ray astronomy over the next decade and be-yond. The scientific potential of CTA is extremely broad: from understanding the role of relativ-istic cosmic particles to the search for dark matter. | + | |
- | The IRL is self-hosted in a rented “chalet adosado” located at Avenida Menceyes | + | |
+ | FSLAC is currently structured in two teams, one involved in the development of the CTA northern observatory (team “Haute Energie”), | ||
+ | * The THEMIS team maintains, operates and makes available to the whole of the French, Spanish and European communities the platform ‘THEMIS Solar Telescope’, | ||
+ | * The high-energy team currently participates to the building of the platform “CTA northern array”, a gamma-ray Cherenkov observatory which, when completed, will become the foremost global observatory for very high-energy gamma-ray astronomy over the next decade and be-yond. The scientific potential of CTA is extremely broad: from understanding the role of relativistic cosmic particles to the search for dark matter. | ||
- | === Current FSLAC Team === | + | == Current FSLAC staff == |
Ramon Garcia Lopez, FSLAC director, high-energy astrophysicist \\ | Ramon Garcia Lopez, FSLAC director, high-energy astrophysicist \\ | ||
Bernard Gelly, FSLAC deputy-director, | Bernard Gelly, FSLAC deputy-director, | ||
- | Richard Drouet, Optomechanics engineer \\ | + | Richard Drouet, Optomechanics |
- | Didier Laforgue, Software & command-control engineer \\ | + | Didier Laforgue, Software & command-control |
Fabia Acero, high-energy astrophysicist \\ | Fabia Acero, high-energy astrophysicist \\ | ||
Etienne Pariat, solar physicist \\ | Etienne Pariat, solar physicist \\ | ||
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=== FSLAC news and scientific highlights === | === FSLAC news and scientific highlights === | ||
+ | * [[science: | ||
* [[https:// | * [[https:// | ||
- | * [[Results: | + | * [[science: |