CERN Accelerating science

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1.
The On-Site Analysis of the Cherenkov Telescope Array / Bulgarelli, Andrea (IASF, Bologna) ; Fioretti, Valentina (Bologna Observ.) ; Zoli, Andrea (Bologna Observ.) ; Aboudan, Alessio (Bologna Observ. ; Padua U., CISAS) ; Rodríguez-Vázquez, Juan José ; De Cesare, Giovanni (Bologna Observ.) ; De Rosa, Adriano (Bologna Observ.) ; Maier, Gernot (DESY, Zeuthen) ; Lyard, Etienne (Geneva Observ.) ; Bastieri, Denis (INFN, Padua ; Padua U.) et al.
The Cherenkov Telescope Array (CTA) observatory will be one of the largest ground-based very high-energy gamma-ray observatories. [...]
arXiv:1509.01963.
- 2015.
Preprint
2.
First detection of the Crab Nebula at TeV energies with a Cherenkov telescope in dual-mirror Schwarzschild-Couder configuration: the ASTRI-Horn telescope / Lombardi, S. (Rome Observ. ; ASDC, Frascati) ; Catalano, O. (IASF, Palermo) ; Scuderi, S. (IASF, Milan) ; Antonelli, L.A. (Rome Observ. ; ASDC, Frascati) ; Pareschi, G. (Brera Observ.) ; Antolini, E. (Bologna Observ.) ; Arrabito, L. (U. Montpellier 2, LUPM) ; Bellassai, G. (Catania Astrophys. Observ.) ; Bernlöhr, K. (Heidelberg, Max Planck Inst.) ; Bigongiari, C. (Rome Observ.) et al.
We report on the first detection of very high-energy (VHE) gamma-ray emission from the Crab Nebula by a Cherenkov telescope in dual-mirror Schwarzschild-Couder (SC) configuration. The result has been achieved by means of the 4 m size ASTRI-Horn telescope, operated on Mt. [...]
arXiv:1909.12149.- 2020-02-01 - 6 p. - Published in : Astron. Astrophys. 634 (2020) A22 Fulltext: PDF;
3.
Science with the Cherenkov Telescope Array / Cherenkov Telescope Array Consortium Collaboration
The Cherenkov Telescope Array, CTA, will be the major global observatory for very high energy gamma-ray astronomy over the next decade and beyond. [...]
arXiv:1709.07997.
- 2017. - 211 p.
Preprint
4.
The AGILE Mission / AGILE Collaboration
AGILE is an Italian Space Agency mission dedicated to the observation of the gamma-ray Universe. The AGILE very innovative instrumentation combines for the first time a gamma-ray imager (sensitive in the energy range 30 MeV - 50 GeV), a hard X-ray imager (sensitive in the range 18-60 keV) together with a Calorimeter (sensitive in the range 300 keV - 100 MeV) and an anticoincidence system. [...]
arXiv:0807.4254.- 2008 - 20 p. - Published in : Astron. Astrophys. 502 (2009) 995-1013 Preprint: PDF; External link: Preprint
5.
On-site observations with the STACEE Cherenkov detector Prototype / Covault, C E
1997
In : 25th International Conference on Cosmic Rays, v.1-7, Durban, South Africa, 28 Jul - 8 Aug 1997, pp.161-164 (v.5)
6.
ORIGIN: Metal Creation and Evolution from the Cosmic Dawn / Herder, Jan-Willem den (SRON, Utrecht) ; Piro, Luigi (IASF, Bologna) ; Ohashi, Takaya (Tokyo Metropolitan U.) ; Kouveliotou, Chryssa (NASA, Marshall) ; Hartmann, Dieter H. (Stanford U., Phys. Dept.) ; Kaastra, Jelle S. (SRON, Utrecht) ; Amati, L. (IASF, Bologna) ; Andersen, M.I. (DARK Cosmology Ctr.) ; Arnaud, M. (Saclay) ; Attéia, J.-L. (Midi-Pyrenees Observ.) et al.
ORIGIN is a proposal for the M3 mission call of ESA aimed at the study of metal creation from the epoch of cosmic dawn. Using high-spectral resolution in the soft X-ray band, ORIGIN will be able to identify the physical conditions of all abundant elements between C and Ni to red-shifts of z=10, and beyond. [...]
arXiv:1104.2048.- 2011 - 34 p. - Published in : Exper.Astron. 34 (2012) 519-549 Fulltext: PDF; External link: Preprint
7.
An accurate solar axions ray-tracing response of BabyIAXO / IAXO collaboration
BabyIAXO is the intermediate stage of the International Axion Observatory (IAXO) to be hosted at DESY. [...]
arXiv:2411.13915.
- 39.
Fulltext
8.
Euclid preparation. Sensitivity to non-standard particle dark matter model / Euclid Collaboration
The Euclid mission of the European Space Agency will provide weak gravitational lensing and galaxy clustering surveys that can be used to constrain the standard cosmological model and its extensions, with an opportunity to test the properties of dark matter beyond the minimal cold dark matter paradigm. [...]
arXiv:2406.18274 ; TTK-24-26.
- 31.
Fulltext
9.
The lstMCpipe library / Garcia, Enrique (CERN ; Annecy, LAPP) ; Vuillaume, Thomas (Annecy, LAPP) ; Nickel, Lukas (Tech. U., Dortmund (main))
The Cherenkov Telescope Array (CTA) is the next generation of ground-based gamma-ray astronomy observatory that will improve the sensitivity of current generation instruments by one order of magnitude. [...]
arXiv:2212.00120.
- 5 p.
Fulltext
10.
The Cherenkov Telescope Array production system for Monte Carlo simulations and analysis / Arrabito, L (U. Montpellier 2, LUPM) ; Bernloehr, K (Heidelberg, Max Planck Inst.) ; Bregeon, J (U. Montpellier 2, LUPM) ; Cumani, P (Barcelona, IFAE) ; Hassan, T (Barcelona, IFAE) ; Haupt, A (DESY, Zeuthen) ; Maier, G (DESY, Zeuthen) ; Moralejo, A (Barcelona, IFAE) ; Neyroud, N (Annecy, LAPP) ; Stagni, F (CERN) et al. /CTA Consortium ; DIRAC Consortium
The Cherenkov Telescope Array (CTA), an array of many tens of Imaging Atmospheric Cherenkov Telescopes deployed on an unprecedented scale, is the next-generation instrument in the field of very high energy gamma-ray astronomy. An average data stream of about 0.9 GB/s for about 1300 hours of observation per year is expected, therefore resulting in 4 PB of raw data per year and a total of 27 PB/year, including archive and data processing. [...]
2017 - 8 p. - Published in : J. Phys.: Conf. Ser. 898 (2017) 052013 Fulltext: PDF;
In : 22nd International Conference on Computing in High Energy and Nuclear Physics, CHEP 2016, San Francisco, Usa, 10 - 14 Oct 2016, pp.052013

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