Zobrazeno 1 - 10
of 45
pro vyhledávání: '"Eric Delagnes"'
Autor:
S. Karkar, Barbara Biasuzzi, J. Bolmont, F. Toussenel, S. Caroff, Pierre Jean, Gerard Fontaine, NectarCAM, T. Ravel, David Gascon, Andreu Sanuy, T. Suomijärvi, C. Marty, Jürgen Knödlseder, Pankaj Sharma, J. F. Glicenstein, J.-P. Lenain, P.-O. Petrucci, Jean-François Olive, Adellain Tsiahina, C. Jarnot, S. Rivoire, Dieter Hoffmann, Eric Delagnes, Marc Ribó, Luis Ángel Tejedor, Francois Brun, S. J. Fegan, J. M. Paredes, J. Prast
Publikováno v:
Nucl.Instrum.Meth.A
Nucl.Instrum.Meth.A, 2021, 1007, pp.165413. ⟨10.1016/j.nima.2021.165413⟩
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Elsevier, 2021, 1007, pp.165413. ⟨10.1016/j.nima.2021.165413⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Nucl.Instrum.Meth.A, 2021, 1007, pp.165413. ⟨10.1016/j.nima.2021.165413⟩
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Elsevier, 2021, 1007, pp.165413. ⟨10.1016/j.nima.2021.165413⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
NectarCAM is a camera for the medium-sized telescopes of the Cherenkov Telescope Array (CTA), which covers the energy range of 100 GeV to 30 TeV. The camera is equipped with 265 focal plane modules (FPMs). Each FPM comprises 7 pixels, each consisting
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::939738a48aef2e1b2f590307b4de2348
https://hal.science/hal-03238822/file/S0168900221003971.pdf
https://hal.science/hal-03238822/file/S0168900221003971.pdf
Autor:
Eric Delagnes, Y. Geerebaert, Nathalie Michel, F. Gebreyohannes, S. Elidrissi-Moubtassim, O. Thiam, F. Haddad, N. Audouin, Noël Servagent, Thomas Sounalet, B. Boyer, Charbel Koumeir, F. Poirier, O. Gevin, P. Manigot, M. Verderi, C. Thiebaux, Frédéric Magniette, G. Blain
Publikováno v:
Nucl.Instrum.Meth.B
Nucl.Instrum.Meth.B, 2020, 466, pp.8-11. ⟨10.1016/j.nimb.2020.01.003⟩
Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms, Elsevier, 2020, 466, pp.8-11. ⟨10.1016/j.nimb.2020.01.003⟩
Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms, 2020, 466, pp.8-11. ⟨10.1016/j.nimb.2020.01.003⟩
Nucl.Instrum.Meth.B, 2020, 466, pp.8-11. ⟨10.1016/j.nimb.2020.01.003⟩
Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms, Elsevier, 2020, 466, pp.8-11. ⟨10.1016/j.nimb.2020.01.003⟩
Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms, 2020, 466, pp.8-11. ⟨10.1016/j.nimb.2020.01.003⟩
International audience; PEPITES is a new type of transparent beam profiler (
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::29dab2dfa42ee9c9eb4287d13120d667
https://hal.archives-ouvertes.fr/hal-02467213
https://hal.archives-ouvertes.fr/hal-02467213
Publikováno v:
IEEE Transactions on Nuclear Science. 64:1071-1079
This paper presents a 13-b, 2.56- $\mu \text{s}$ conversion time, 2 V input range, 32-channel single slope analog-to-digital converter (ADC) called OWB-1 and implemented in a 0.35- $\mu \text{m}$ CMOS commercial technology. It is based on an improved
Autor:
P. Baron, P. Sizun, J. Pancin, J. Pibernat, S. Anvar, T. Roger, A. Rebii, G. F. Grinyer, E. C. Pollacco, T. Goigoux, Eric Delagnes, J. Giovinazzo, J. L. Pedroza, B. Blank
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Elsevier, 2016, 840, pp.15-27. ⟨10.1016/j.nima.2016.09.018⟩
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2016, 840, pp.15-27. ⟨10.1016/j.nima.2016.09.018⟩
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Elsevier, 2016, 840, pp.15-27. ⟨10.1016/j.nima.2016.09.018⟩
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2016, 840, pp.15-27. ⟨10.1016/j.nima.2016.09.018⟩
International audience; The General Electronics for TPCs (GET) has been developed to equip a generation of time projection chamber detectors for nuclear physics, and may also be used for a wider range of detector types. The goal of this paper is to p
Measurements of timing resolution of ultra-fast silicon detectors with the SAMPIC waveform digitizer
Autor:
Christophe Royon, V. De Cacqueray, Matthias Saimpert, J. Maalmi, D. Breton, N. Minafra, Eric Delagnes, H. M. X. Grabas
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Elsevier, 2016, 835, pp.51-60. ⟨10.1016/j.nima.2016.08.019⟩
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2016, 835, pp.51-60. ⟨10.1016/j.nima.2016.08.019⟩
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Elsevier, 2016, 835, pp.51-60. ⟨10.1016/j.nima.2016.08.019⟩
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2016, 835, pp.51-60. ⟨10.1016/j.nima.2016.08.019⟩
The SAMpler for PICosecond time (SAMPIC) chip has been designed by a collaboration including CEA/IRFU/SEDI, Saclay and CNRS/LAL/SERDI, Orsay. It benefits from both the quick response of a time to digital converter and the versatility of a waveform di
Autor:
H. Leich, Thomas Murach, T. Schwab, Marko Kossatz, P. Nayman, Albert Jahnke, Francois Brun, P. Vincent, J.-P. Lenain, Jim Hinton, Christian Stegmann, A. Balzer, J. Bolmont, J. F. Glicenstein, P. Manigot, M. Füßling, Eric Delagnes, Michael Backes, Gianluca Giavitto, Marek Penno, T. Chaminade, F. Toussenel, Terry Ashton, M. de Naurois, David Salek, E. Moulin, D. Berge, Gerard Fontaine, J.-P. Tavernet, Kleopas Shiningayamwe, S. Ohm, V. Lefranc, A. Kretzschmann, J. Thornhill, H. Lüdecke, V. Marandon, Markus Schade, Stefan Klepser, B. Giebels, Iryna Lypova, D. Ross, Tobias Gräber, S. Bonnefoy, Constantin Steppa
Publikováno v:
Astroparticle Physics
Astroparticle Physics, 2020, 118, pp.102425. ⟨10.1016/j.astropartphys.2019.102425⟩
Astropart.Phys.
Astropart.Phys., 2020, 118, pp.102425. ⟨10.1016/j.astropartphys.2019.102425⟩
Astroparticle physics 118, 102425-(2020). doi:10.1016/j.astropartphys.2019.102425
Astroparticle Physics, Elsevier, 2020, 118, pp.102425. ⟨10.1016/j.astropartphys.2019.102425⟩
Astroparticle Physics, 2020, 118, pp.102425. ⟨10.1016/j.astropartphys.2019.102425⟩
Astropart.Phys.
Astropart.Phys., 2020, 118, pp.102425. ⟨10.1016/j.astropartphys.2019.102425⟩
Astroparticle physics 118, 102425-(2020). doi:10.1016/j.astropartphys.2019.102425
Astroparticle Physics, Elsevier, 2020, 118, pp.102425. ⟨10.1016/j.astropartphys.2019.102425⟩
The High Energy Stereoscopic System (H.E.S.S.) is one of the three arrays of imaging atmospheric Cherenkov telescopes (IACTs) currently in operation. It is composed of four 12-meter telescopes and a 28-meter one, and is sensitive to gamma rays in the
Autor:
M. Verderi, Noël Servagent, F. Poirier, B. Boyer, C. Thiebaux, Frédéric Magniette, C. Koumeir, R. Cornat, M. Rubio Roy, Ferid Haddad, O. Gevin, Y. Geerebaert, Eric Delagnes, P. Manigot
Publikováno v:
Nucl.Instrum.Meth.A
14th Pisa Meeting on Advanced Detectors
14th Pisa Meeting on Advanced Detectors, May 2018, La Biodola-Isola d'Elba, Italy. pp.29-30, ⟨10.1016/j.nima.2018.09.134⟩
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
14th Pisa Meeting on Advanced Detectors
14th Pisa Meeting on Advanced Detectors, May 2018, La Biodola-Isola d'Elba, Italy. pp.29-30, ⟨10.1016/j.nima.2018.09.134⟩
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Beam profiling during patient treatment in protontherapy requires ultra-thin monitors to preserve the high beam quality. For detectors upstream in the line, a material budget as low as ∼ 15 μ m water-equivalent is needed. In addition, the current
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b360c3b592068357280505616cd45042
https://hal.archives-ouvertes.fr/hal-02475944
https://hal.archives-ouvertes.fr/hal-02475944
Autor:
Francois Brun, A. Kretzschmann, P. Manigot, Mathieu de Naurois, Jean-Philippe Lenain, Kleopas Shiningayamwe, David Salek, Eric Delagnes, Marek Penno, G. Fontaine, A. Balzer, S. Bonnefoy, Thomas Schwab, Berrie Giebels, Stefan Klepser, Marko Kossatz, Thomas Chaminade, V. Lefranc, Emmanuel Moulin, Terry Ashton, Iryna Lypova, David Berge, Stefan Ohm, J. Thornhill, Jean-Francois Glicenstein, Albert Jahnke, Jim Hinton, D. Ross, Michael Backes, Constantin Steppa, Markus Schade, Vincent Marandon, Tobias Gräber, H. Leich, Gianluca Giavitto, Francois Toussnel, P. Nayman, H. Lüdecke, C. Stegmann, Matthias Fuessling
Publikováno v:
PoS
35th International Cosmic Ray Conference
35th International Cosmic Ray Conference, Jul 2017, Busan, South Korea. pp.834, ⟨10.22323/1.301.0834⟩
Scopus-Elsevier
NASA Astrophysics Data System
35th International Cosmic Ray Conference
35th International Cosmic Ray Conference, Jul 2017, Busan, South Korea. pp.834, ⟨10.22323/1.301.0834⟩
Scopus-Elsevier
NASA Astrophysics Data System
In 2015/16, the photomultiplier cameras of the H.E.S.S. Cherenkov telescopes CT1-4 have undergone a major upgrade. The entire electronics has been replaced, using NECTAr chips for the front-end readout. A new ventilation system has been installed and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ca370c613c4bf7ac69a99a0246b67dcd
https://hal.archives-ouvertes.fr/hal-01891227
https://hal.archives-ouvertes.fr/hal-01891227
Autor:
P. Manigot, Constantin Steppa, Vincent Marandon, V. Lefranc, Marek Penno, Mathieu de Naurois, Terry Ashton, Francois Toussnel, Rachel Simoni, David Salek, P. Nayman, Thomas Chaminade, Albert Jahnke, Iryna Lypova, H. Lüdecke, C. Stegmann, Markus Schade, Stefan Ohm, H. Leich, M. Füßling, D. Ross, S. Klepser, Eric Delagnes, A. Kretzschmann, Thomas Schwab, B. Giebels, Jim Hinton, Marko Kossatz, J. Thornhill, Jean-Francois Glicenstein, Gianluca Giavitto, Emmanuel Moulin, Tobias Gräber, Francois Brun, G. Fontaine, A. Balzer, David Berge
Publikováno v:
EPJ Web of Conferences, Vol 136, p 03002 (2017)
EPJ Web Conf.
6th Roma International Workshop on Astroparticle Physics
6th Roma International Workshop on Astroparticle Physics, Jun 2016, Rome, Italy. pp.03002, ⟨10.1051/epjconf/201713603002⟩
EPJ Web Conf.
6th Roma International Workshop on Astroparticle Physics
6th Roma International Workshop on Astroparticle Physics, Jun 2016, Rome, Italy. pp.03002, ⟨10.1051/epjconf/201713603002⟩
International audience; The High Energy Stereoscopic System (H.E.S.S.) is an array of imaging atmospheric Cherenkov telescopes (IACTs) located in Namibia. It was built to detect Very High Energy (VHE, >100 GeV) cosmic gamma rays, and consists of four
Autor:
Marko Kossatz, Berrie Giebels, Vincent Marandon, Francois Brun, Mathieu de Naurois, Stefan Klepser, Stefan Ohm, P. Manigot, J. Thornhill, H. Leich, Jean-Philippe Lenain, Terry Ashton, Albert Jahnke, Emmanuel Moulin, Iryna Lypova, David Berge, Markus Schade, Gianluca Giavitto, D. Ross, Marek Penno, Jean-Francois Glicenstein, Michael Backes, Kleopas Shiningayamwe, Thomas Chaminade, Thomas Schwab, A. Kretzschmann, Jim Hinton, S. Bonnefoy, V. Lefranc, C. Stegmann, Constantin Steppa, Tobias Gräber, Eric Delagnes, Francois Toussnel, P. Nayman, H. Lüdecke, Matthias Fuessling, David Salek, G. Fontaine, A. Balzer
Publikováno v:
NASA Astrophysics Data System
PoS
35th International Cosmic Ray Conference
35th International Cosmic Ray Conference, Jul 2017, Busan, South Korea. pp.805, ⟨10.22323/1.301.0805⟩
PoS
35th International Cosmic Ray Conference
35th International Cosmic Ray Conference, Jul 2017, Busan, South Korea. pp.805, ⟨10.22323/1.301.0805⟩
International audience; The 14 years old cameras of the H.E.S.S. 12-m telescopes have been upgraded in 2015/2016, with the goals of reducing the system failure rate, reducing the dead time and improving the overall performance of the array. This conf
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c390484481492a3f8fb09082a9da10b5