Physics and astrophysics with a ground-based gamma-ray telescope of low energy threshold

J. Albert I Fort; A. Armada; C. Baixeras; H. Bartko; D. Bastieri; W. Bednarek; C. Bigongiari; A. Biland; E. Bisesi; O. Blanch; R. K. Bock; T. Bretz; A. Chilingarian; S. Ciprini; S. Commichau; J. L. Contreras; J. Cortina; V. Danielyan; F. Dazzi; A. De Angelis; B. De Lotto; Carlos Domingo Miralles; E. Domingo; D. Dorner; M. Doro; O. Epler; D. Ferenc; E. Fernández; R. Firpo; J. Flix; M. V. Fonseca; L. Font; N. Galante; M. Garczarczyk; M. Gaug; J. Gebauer; R. Giannitrapani; M. Giller; F. Goebel; T. Hengstebeck; P. Jacon; O. C. De Jager; O. Kalekin; D. Kranich; A. Laille; T. Lenisa; E. Lindfors; F. Longo; M. López; J. López; E. Lorenz; F. Lucarelli; K. Mannheim; M. Mariotti; M. Martinez; K. Mase; D. Mazin; C. Merck; M. Merck; M. Meucci; M. Meyer; R. Mirzoyan; S. Mizobuchi; A. Moralejo; E. Oña-Wilhelmi; R. Orduña; N. Otte; D. Paneque; R. Paoletti; M. Pasanen; D. Pascoli; F. Pauss; N. Pavel; R. Pegna; L. Peruzzo; A. Piccioli; M. Pin; R. De Los Reyes; J. Rico; D. Renker; A. Robert; G. Rossato; A. Saggion; A. Sánchez; P. Sartori; V. Scalzotto; T. Schweizer; M. Shayduk; K. Shinozaki; A. Sillanpää; D. Sobczynska; A. Stamerra; L. Stark; L. Takalo; M. Teshima; N. Tonello; A. Torres; N. Turini; G. Viertel; V. Vitale; S. Volkov

doi:10.1016/j.astropartphys.2005.03.005

Physics and astrophysics with a ground-based gamma-ray telescope of low energy threshold

J. Albert I Fort, A. Armada, C. Baixeras, H. Bartko, D. Bastieri, W. Bednarek, C. Bigongiari, A. Biland, E. Bisesi, O. Blanch, R. K. Bock, T. Bretz, A. Chilingarian, S. Ciprini, S. Commichau, J. L. Contreras, J. Cortina, V. Danielyan, F. Dazzi, A. De AngelisB. De Lotto, Carlos Domingo Miralles, E. Domingo, D. Dorner, M. Doro, O. Epler, D. Ferenc, E. Fernández, R. Firpo, J. Flix, M. V. Fonseca, L. Font, N. Galante, M. Garczarczyk, M. Gaug, J. Gebauer, R. Giannitrapani, M. Giller, F. Goebel, T. Hengstebeck, P. Jacon, O. C. De Jager, O. Kalekin, D. Kranich, A. Laille, T. Lenisa, E. Lindfors, F. Longo, M. López, J. López, E. Lorenz, F. Lucarelli, K. Mannheim, M. Mariotti, M. Martinez, K. Mase, D. Mazin, C. Merck, M. Merck, M. Meucci, M. Meyer, R. Mirzoyan, S. Mizobuchi, A. Moralejo, E. Oña-Wilhelmi, R. Orduña, N. Otte, D. Paneque, R. Paoletti, M. Pasanen, D. Pascoli, F. Pauss, N. Pavel, R. Pegna, L. Peruzzo, A. Piccioli, M. Pin, R. De Los Reyes, J. Rico, D. Renker, A. Robert, G. Rossato, A. Saggion, A. Sánchez, P. Sartori, V. Scalzotto, T. Schweizer, M. Shayduk, K. Shinozaki, A. Sillanpää, D. Sobczynska, A. Stamerra, L. Stark, L. Takalo, M. Teshima, N. Tonello, A. Torres, N. Turini, G. Viertel, V. Vitale, S. Volkov

Producció científica: Contribució a revista › Article › Recerca › Avaluat per experts

15 Cites (Scopus)

Resum

© 2005 Elsevier B.V. All rights reserved. Ground-based Cherenkov telescopes have made in recent years important contributions to high energy gamma-ray astronomy. A lower energy threshold, considerably below 100 GeV, and improved sensitivity will be key parameters to extend their role. A lower threshold will permit these instruments to cover wavelengths with good overlap with satellite experiments, thus providing essential complementary information. The latest generation of Imaging Air Cherenkov Telescopes was built with this criterion in mind. Preliminary studies concerning further progress in the same direction have started. We discuss in this contribution the astrophysics and physics arguments for lowering the observable energy threshold as far as the Cherenkov technique permits, and the ensuing complementarity to results obtained with a GLAST-like satellite.

Idioma original	Anglès
Pàgines (de-a)	493-509
Revista	Astroparticle Physics
Volum	23
Número	5
DOIs	https://doi.org/10.1016/j.astropartphys.2005.03.005
Estat de la publicació	Publicada - 1 de juny 2005

Accés al document

10.1016/j.astropartphys.2005.03.005

Altres arxius i enllaços

https://www.scopus.com/pages/publications/21144452812

Com citar-ho

Albert I Fort, J., Armada, A., Baixeras, C., Bartko, H., Bastieri, D., Bednarek, W., Bigongiari, C., Biland, A., Bisesi, E., Blanch, O., Bock, R. K., Bretz, T., Chilingarian, A., Ciprini, S., Commichau, S., Contreras, J. L., Cortina, J., Danielyan, V., Dazzi, F., ... Volkov, S. (2005). Physics and astrophysics with a ground-based gamma-ray telescope of low energy threshold. Astroparticle Physics, 23(5), 493-509. https://doi.org/10.1016/j.astropartphys.2005.03.005

@article{f0fd623ef12e4a25a212c0a06198041e,

title = "Physics and astrophysics with a ground-based gamma-ray telescope of low energy threshold",

abstract = "{\textcopyright} 2005 Elsevier B.V. All rights reserved. Ground-based Cherenkov telescopes have made in recent years important contributions to high energy gamma-ray astronomy. A lower energy threshold, considerably below 100 GeV, and improved sensitivity will be key parameters to extend their role. A lower threshold will permit these instruments to cover wavelengths with good overlap with satellite experiments, thus providing essential complementary information. The latest generation of Imaging Air Cherenkov Telescopes was built with this criterion in mind. Preliminary studies concerning further progress in the same direction have started. We discuss in this contribution the astrophysics and physics arguments for lowering the observable energy threshold as far as the Cherenkov technique permits, and the ensuing complementarity to results obtained with a GLAST-like satellite.",

keywords = "Astrophysics, Cherenkov telescope, Cosmology, Low-energy gamma-ray",

author = "\{Albert I Fort\}, J. and A. Armada and C. Baixeras and H. Bartko and D. Bastieri and W. Bednarek and C. Bigongiari and A. Biland and E. Bisesi and O. Blanch and Bock, \{R. K.\} and T. Bretz and A. Chilingarian and S. Ciprini and S. Commichau and Contreras, \{J. L.\} and J. Cortina and V. Danielyan and F. Dazzi and \{De Angelis\}, A. and \{De Lotto\}, B. and \{Domingo Miralles\}, Carlos and E. Domingo and D. Dorner and M. Doro and O. Epler and D. Ferenc and E. Fern{\'a}ndez and R. Firpo and J. Flix and Fonseca, \{M. V.\} and L. Font and N. Galante and M. Garczarczyk and M. Gaug and J. Gebauer and R. Giannitrapani and M. Giller and F. Goebel and T. Hengstebeck and P. Jacon and \{De Jager\}, \{O. C.\} and O. Kalekin and D. Kranich and A. Laille and T. Lenisa and E. Lindfors and F. Longo and M. L{\'o}pez and J. L{\'o}pez and E. Lorenz and F. Lucarelli and K. Mannheim and M. Mariotti and M. Martinez and K. Mase and D. Mazin and C. Merck and M. Merck and M. Meucci and M. Meyer and R. Mirzoyan and S. Mizobuchi and A. Moralejo and E. O{\~n}a-Wilhelmi and R. Ordu{\~n}a and N. Otte and D. Paneque and R. Paoletti and M. Pasanen and D. Pascoli and F. Pauss and N. Pavel and R. Pegna and L. Peruzzo and A. Piccioli and M. Pin and \{De Los Reyes\}, R. and J. Rico and D. Renker and A. Robert and G. Rossato and A. Saggion and A. S{\'a}nchez and P. Sartori and V. Scalzotto and T. Schweizer and M. Shayduk and K. Shinozaki and A. Sillanp{\"a}{\"a} and D. Sobczynska and A. Stamerra and L. Stark and L. Takalo and M. Teshima and N. Tonello and A. Torres and N. Turini and G. Viertel and V. Vitale and S. Volkov",

year = "2005",

month = jun,

day = "1",

doi = "10.1016/j.astropartphys.2005.03.005",

language = "English",

volume = "23",

pages = "493--509",

journal = "Astroparticle Physics",

issn = "0927-6505",

publisher = "Elsevier",

number = "5",

}

Albert I Fort, J, Armada, A, Baixeras, C, Bartko, H, Bastieri, D, Bednarek, W, Bigongiari, C, Biland, A, Bisesi, E, Blanch, O, Bock, RK, Bretz, T, Chilingarian, A, Ciprini, S, Commichau, S, Contreras, JL, Cortina, J, Danielyan, V, Dazzi, F, De Angelis, A, De Lotto, B, Domingo Miralles, C, Domingo, E, Dorner, D, Doro, M, Epler, O, Ferenc, D, Fernández, E, Firpo, R, Flix, J, Fonseca, MV, Font, L, Galante, N, Garczarczyk, M, Gaug, M, Gebauer, J, Giannitrapani, R, Giller, M, Goebel, F, Hengstebeck, T, Jacon, P, De Jager, OC, Kalekin, O, Kranich, D, Laille, A, Lenisa, T, Lindfors, E, Longo, F, López, M, López, J, Lorenz, E, Lucarelli, F, Mannheim, K, Mariotti, M, Martinez, M, Mase, K, Mazin, D, Merck, C, Merck, M, Meucci, M, Meyer, M, Mirzoyan, R, Mizobuchi, S, Moralejo, A, Oña-Wilhelmi, E, Orduña, R, Otte, N, Paneque, D, Paoletti, R, Pasanen, M, Pascoli, D, Pauss, F, Pavel, N, Pegna, R, Peruzzo, L, Piccioli, A, Pin, M, De Los Reyes, R, Rico, J, Renker, D, Robert, A, Rossato, G, Saggion, A, Sánchez, A, Sartori, P, Scalzotto, V, Schweizer, T, Shayduk, M, Shinozaki, K, Sillanpää, A, Sobczynska, D, Stamerra, A, Stark, L, Takalo, L, Teshima, M, Tonello, N, Torres, A, Turini, N, Viertel, G, Vitale, V & Volkov, S 2005, 'Physics and astrophysics with a ground-based gamma-ray telescope of low energy threshold', Astroparticle Physics, vol. 23, núm. 5, pàg. 493-509. https://doi.org/10.1016/j.astropartphys.2005.03.005

TY - JOUR

T1 - Physics and astrophysics with a ground-based gamma-ray telescope of low energy threshold

AU - Albert I Fort, J.

AU - Armada, A.

AU - Baixeras, C.

AU - Bartko, H.

AU - Bastieri, D.

AU - Bednarek, W.

AU - Bigongiari, C.

AU - Biland, A.

AU - Bisesi, E.

AU - Blanch, O.

AU - Bock, R. K.

AU - Bretz, T.

AU - Chilingarian, A.

AU - Ciprini, S.

AU - Commichau, S.

AU - Contreras, J. L.

AU - Cortina, J.

AU - Danielyan, V.

AU - Dazzi, F.

AU - De Angelis, A.

AU - De Lotto, B.

AU - Domingo Miralles, Carlos

AU - Domingo, E.

AU - Dorner, D.

AU - Doro, M.

AU - Epler, O.

AU - Ferenc, D.

AU - Fernández, E.

AU - Firpo, R.

AU - Flix, J.

AU - Fonseca, M. V.

AU - Font, L.

AU - Galante, N.

AU - Garczarczyk, M.

AU - Gaug, M.

AU - Gebauer, J.

AU - Giannitrapani, R.

AU - Giller, M.

AU - Goebel, F.

AU - Hengstebeck, T.

AU - Jacon, P.

AU - De Jager, O. C.

AU - Kalekin, O.

AU - Kranich, D.

AU - Laille, A.

AU - Lenisa, T.

AU - Lindfors, E.

AU - Longo, F.

AU - López, M.

AU - López, J.

AU - Lorenz, E.

AU - Lucarelli, F.

AU - Mannheim, K.

AU - Mariotti, M.

AU - Martinez, M.

AU - Mase, K.

AU - Mazin, D.

AU - Merck, C.

AU - Merck, M.

AU - Meucci, M.

AU - Meyer, M.

AU - Mirzoyan, R.

AU - Mizobuchi, S.

AU - Moralejo, A.

AU - Oña-Wilhelmi, E.

AU - Orduña, R.

AU - Otte, N.

AU - Paneque, D.

AU - Paoletti, R.

AU - Pasanen, M.

AU - Pascoli, D.

AU - Pauss, F.

AU - Pavel, N.

AU - Pegna, R.

AU - Peruzzo, L.

AU - Piccioli, A.

AU - Pin, M.

AU - De Los Reyes, R.

AU - Rico, J.

AU - Renker, D.

AU - Robert, A.

AU - Rossato, G.

AU - Saggion, A.

AU - Sánchez, A.

AU - Sartori, P.

AU - Scalzotto, V.

AU - Schweizer, T.

AU - Shayduk, M.

AU - Shinozaki, K.

AU - Sillanpää, A.

AU - Sobczynska, D.

AU - Stamerra, A.

AU - Stark, L.

AU - Takalo, L.

AU - Teshima, M.

AU - Tonello, N.

AU - Torres, A.

AU - Turini, N.

AU - Viertel, G.

AU - Vitale, V.

AU - Volkov, S.

PY - 2005/6/1

Y1 - 2005/6/1

N2 - © 2005 Elsevier B.V. All rights reserved. Ground-based Cherenkov telescopes have made in recent years important contributions to high energy gamma-ray astronomy. A lower energy threshold, considerably below 100 GeV, and improved sensitivity will be key parameters to extend their role. A lower threshold will permit these instruments to cover wavelengths with good overlap with satellite experiments, thus providing essential complementary information. The latest generation of Imaging Air Cherenkov Telescopes was built with this criterion in mind. Preliminary studies concerning further progress in the same direction have started. We discuss in this contribution the astrophysics and physics arguments for lowering the observable energy threshold as far as the Cherenkov technique permits, and the ensuing complementarity to results obtained with a GLAST-like satellite.

AB - © 2005 Elsevier B.V. All rights reserved. Ground-based Cherenkov telescopes have made in recent years important contributions to high energy gamma-ray astronomy. A lower energy threshold, considerably below 100 GeV, and improved sensitivity will be key parameters to extend their role. A lower threshold will permit these instruments to cover wavelengths with good overlap with satellite experiments, thus providing essential complementary information. The latest generation of Imaging Air Cherenkov Telescopes was built with this criterion in mind. Preliminary studies concerning further progress in the same direction have started. We discuss in this contribution the astrophysics and physics arguments for lowering the observable energy threshold as far as the Cherenkov technique permits, and the ensuing complementarity to results obtained with a GLAST-like satellite.

KW - Astrophysics

KW - Cherenkov telescope

KW - Cosmology

KW - Low-energy gamma-ray

UR - https://www.scopus.com/pages/publications/21144452812

U2 - 10.1016/j.astropartphys.2005.03.005

DO - 10.1016/j.astropartphys.2005.03.005

M3 - Article

SN - 0927-6505

VL - 23

SP - 493

EP - 509

JO - Astroparticle Physics

JF - Astroparticle Physics

IS - 5

ER -

Physics and astrophysics with a ground-based gamma-ray telescope of low energy threshold

Resum

Accés al document

Altres arxius i enllaços

Fingerprint

Com citar-ho