First detection of gamma rays from the crab nebula with the CELESTE "solar farm" Cherenkov detector

D. A. Smith; R. Bazer-Bachi; H. Bergeret; P. Bruel; A. Cordier; G. Debiais; M. De Naurois; J. P. Dezalay; D. Dumor; P. Eschstruth; P. Espigat; B. Fabre; P. Fleury; B. Giebels; N. Hérault; J. Holder; M. Hrabovsky; R. Legallou; I. Malet; B. Merkel; F. Münz; A. Musquère; J. F. Olive; E. Paré; J. Québert; T. Reposeur; L. Rob; T. Sako; P. Schovanek; A. Volte

doi:10.1016/S0920-5632(99)00838-5

First detection of gamma rays from the crab nebula with the CELESTE "solar farm" Cherenkov detector

D. A. Smith
, R. Bazer-Bachi
, H. Bergeret
, P. Bruel
, A. Cordier
, G. Debiais
, M. De Naurois
, J. P. Dezalay
, D. Dumor
, P. Eschstruth
, P. Espigat
, B. Fabre
, P. Fleury
, B. Giebels
, N. Hérault
, J. Holder
, M. Hrabovsky
, R. Legallou
, I. Malet
, B. Merkel

F. Münz, A. Musquère, J. F. Olive, E. Paré, J. Québert, T. Reposeur, L. Rob, T. Sako, P. Schovanek, A. Volte

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

Résumé

We have converted the THEMIS solar array (French Pyrenees) into an atmospheric Cherenkov telescope, called CELESTE, sensitive to astrophysical gamma rays above 30 GeV (7x10²⁴ Hz). In early 1998 the Crab nebula was detected at 80 GeV with a preliminary 18 heliostat setup. The full 40 heliostat array has since been commissioned. The STACEE experiment using the same technique in New Mexico is also analysing their first data. Thus, the window between the EGRET instrument and the Cherenkov imagers has been opened. We describe the CELESTE detector and the data analysis, and discuss the prospects for studying AGN (specifically, blazars) and galactic sources in this energy range.

langue originale	Anglais
Pages (de - à)	163-172
Nombre de pages	10
journal	Nuclear Physics B - Proceedings Supplements
Volume	80
Numéro de publication	1-3
Les DOIs	https://doi.org/10.1016/S0920-5632(99)00838-5
état	Publié - 1 janv. 2000

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10.1016/S0920-5632(99)00838-5

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Smith, D. A., Bazer-Bachi, R., Bergeret, H., Bruel, P., Cordier, A., Debiais, G., De Naurois, M., Dezalay, J. P., Dumor, D., Eschstruth, P., Espigat, P., Fabre, B., Fleury, P., Giebels, B., Hérault, N., Holder, J., Hrabovsky, M., Legallou, R., Malet, I., ... Volte, A. (2000). First detection of gamma rays from the crab nebula with the CELESTE "solar farm" Cherenkov detector. Nuclear Physics B - Proceedings Supplements, 80(1-3), 163-172. https://doi.org/10.1016/S0920-5632(99)00838-5

@article{4d90da2afcc94799bd3e87a461b1fe9a,

title = "First detection of gamma rays from the crab nebula with the CELESTE {"}solar farm{"} Cherenkov detector",

abstract = "We have converted the THEMIS solar array (French Pyrenees) into an atmospheric Cherenkov telescope, called CELESTE, sensitive to astrophysical gamma rays above 30 GeV (7x1024 Hz). In early 1998 the Crab nebula was detected at 80 GeV with a preliminary 18 heliostat setup. The full 40 heliostat array has since been commissioned. The STACEE experiment using the same technique in New Mexico is also analysing their first data. Thus, the window between the EGRET instrument and the Cherenkov imagers has been opened. We describe the CELESTE detector and the data analysis, and discuss the prospects for studying AGN (specifically, blazars) and galactic sources in this energy range.",

author = "Smith, \{D. A.\} and R. Bazer-Bachi and H. Bergeret and P. Bruel and A. Cordier and G. Debiais and \{De Naurois\}, M. and Dezalay, \{J. P.\} and D. Dumor and P. Eschstruth and P. Espigat and B. Fabre and P. Fleury and B. Giebels and N. H{\'e}rault and J. Holder and M. Hrabovsky and R. Legallou and I. Malet and B. Merkel and F. M{\"u}nz and A. Musqu{\`e}re and Olive, \{J. F.\} and E. Par{\'e} and J. Qu{\'e}bert and T. Reposeur and L. Rob and T. Sako and P. Schovanek and A. Volte",

year = "2000",

month = jan,

day = "1",

doi = "10.1016/S0920-5632(99)00838-5",

language = "English",

volume = "80",

pages = "163--172",

journal = "Nuclear Physics B - Proceedings Supplements",

issn = "0920-5632",

number = "1-3",

}

Smith, DA, Bazer-Bachi, R, Bergeret, H, Bruel, P, Cordier, A, Debiais, G, De Naurois, M, Dezalay, JP, Dumor, D, Eschstruth, P, Espigat, P, Fabre, B, Fleury, P, Giebels, B, Hérault, N, Holder, J, Hrabovsky, M, Legallou, R, Malet, I, Merkel, B, Münz, F, Musquère, A, Olive, JF, Paré, E, Québert, J, Reposeur, T, Rob, L, Sako, T, Schovanek, P & Volte, A 2000, 'First detection of gamma rays from the crab nebula with the CELESTE "solar farm" Cherenkov detector', Nuclear Physics B - Proceedings Supplements, VOL. 80, Numéro 1-3, p. 163-172. https://doi.org/10.1016/S0920-5632(99)00838-5

TY - JOUR

T1 - First detection of gamma rays from the crab nebula with the CELESTE "solar farm" Cherenkov detector

AU - Smith, D. A.

AU - Bazer-Bachi, R.

AU - Bergeret, H.

AU - Bruel, P.

AU - Cordier, A.

AU - Debiais, G.

AU - De Naurois, M.

AU - Dezalay, J. P.

AU - Dumor, D.

AU - Eschstruth, P.

AU - Espigat, P.

AU - Fabre, B.

AU - Fleury, P.

AU - Giebels, B.

AU - Hérault, N.

AU - Holder, J.

AU - Hrabovsky, M.

AU - Legallou, R.

AU - Malet, I.

AU - Merkel, B.

AU - Münz, F.

AU - Musquère, A.

AU - Olive, J. F.

AU - Paré, E.

AU - Québert, J.

AU - Reposeur, T.

AU - Rob, L.

AU - Sako, T.

AU - Schovanek, P.

AU - Volte, A.

PY - 2000/1/1

Y1 - 2000/1/1

N2 - We have converted the THEMIS solar array (French Pyrenees) into an atmospheric Cherenkov telescope, called CELESTE, sensitive to astrophysical gamma rays above 30 GeV (7x1024 Hz). In early 1998 the Crab nebula was detected at 80 GeV with a preliminary 18 heliostat setup. The full 40 heliostat array has since been commissioned. The STACEE experiment using the same technique in New Mexico is also analysing their first data. Thus, the window between the EGRET instrument and the Cherenkov imagers has been opened. We describe the CELESTE detector and the data analysis, and discuss the prospects for studying AGN (specifically, blazars) and galactic sources in this energy range.

AB - We have converted the THEMIS solar array (French Pyrenees) into an atmospheric Cherenkov telescope, called CELESTE, sensitive to astrophysical gamma rays above 30 GeV (7x1024 Hz). In early 1998 the Crab nebula was detected at 80 GeV with a preliminary 18 heliostat setup. The full 40 heliostat array has since been commissioned. The STACEE experiment using the same technique in New Mexico is also analysing their first data. Thus, the window between the EGRET instrument and the Cherenkov imagers has been opened. We describe the CELESTE detector and the data analysis, and discuss the prospects for studying AGN (specifically, blazars) and galactic sources in this energy range.

UR - https://www.scopus.com/pages/publications/0033634068

U2 - 10.1016/S0920-5632(99)00838-5

DO - 10.1016/S0920-5632(99)00838-5

M3 - Article

AN - SCOPUS:0033634068

SN - 0920-5632

VL - 80

SP - 163

EP - 172

JO - Nuclear Physics B - Proceedings Supplements

JF - Nuclear Physics B - Proceedings Supplements

IS - 1-3

ER -

First detection of gamma rays from the crab nebula with the CELESTE "solar farm" Cherenkov detector

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