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MAGIC observations of PG 1553+113 during a multiwavelength campaign in July 2006

Authors :
Albert, J.
Aliu, E.
Anderhub, H.
Antoranz, P.
Baixeras, C.
Barrio, J. A.
Bartko, H.
Bastieri, D.
Becker, J. K.
Bednarek, W.
Berdyugin, A.
Berger, K.
Bigongiari, C.
Biland, A.
Bock, R. K.
Bordas, P.
Bosch Ramon, V.
Bretz, T.
Britvitch, I.
Camara, M.
Carmona, E.
Chilingarian, A.
Commichau, S.
Contreras, J. L.
Cortina, J.
Costado, M. T.
Curtef, V.
Danielyan, V.
Dazzi, F.
Angelis, A. D.
Delgado, C.
Reyes, R. D.
Lotto, B. D.
Dorner, D.
Doro, M.
Errando, M.
Fagiolini, M.
Ferenc, D.
Fernandez, E.
Firpo, R.
Fonseca, M. V.
Font, L.
Fuchs, M.
Galante, N.
Garcia Lopez, R. J.
Garczarczyk, M.
Gaug, M.
Goebel, F.
Hakobyan, D.
Hayashida, M.
Hengstebeck, T.
Herrero, A.
Hohne, D.
Hose, J.
Hsu, C. C.
Huber, S.
Jacon, P.
Jogler, T.
Kosyra, R.
Kranich, D.
Kritzer, R.
Laille, A.
Lindfors, E.
Lombardi, S.
Longo, Francesco
Lopez, M.
Lorenz, E.
Majumdar, P.
Maneva, G.
Mannheim, K.
Mariotti, M.
Martinez, M.
Mazin, D.
Merck, C.
Meucci, M.
Meyer, M.
Miranda, J. M.
Mirzoyan, R.
Mizobuchi, S.
Moralejo, A.
Nieto, D.
Nilsson, K.
Ninkovic, J.
Ona Wilhelmi, E.
Otte, N.
Oya, I.
Panniello, M.
Paoletti, R.
Pasanen, M.
Pascoli, D.
Pauss, F.
Pegna, R.
Persic, M.
Peruzzo, L.
Piccioli, A.
Prandini, E.
Puchades, N.
Raymers, A.
Rico, J.
Rhode, W.
Rissi, M.
Robert, A.
Rugamer, S.
Saggion, A.
Saito, T. Y.
Sanchez, A.
Sartori, P.
Scalzotto, V.
Scapin, V.
Schmitt, R.
Schweizer, T.
Shayduk, M.
Shinozaki, K.
Shore, S. N.
Sidro, N.
Sillanpaa, A.
Sobczynska, D.
Spanier, F.
Stamerra, A.
Stark, L. S.
Takalo, L.
Temnikov, P.
Tescaro, D.
Teshima, M.
Torres, D. F.
Turini, N.
Vankov, H.
Venturini, A.
Vitale, V.
Wagner, R. M.
Wibig, T.
Wittek, W.
Zandanel, F.
Zanin, R.
Zapatero, J.
J., Albert
E., Aliu
H., Anderhub
P., Antoranz
C., Baixera
J. A., Barrio
H., Bartko
D., Bastieri
J. K., Becker
W., Bednarek
A., Berdyugin
K., Berger
C., Bigongiari
A., Biland
R. K., Bock
P., Borda
V., Bosch Ramon
T., Bretz
I., Britvitch
M., Camara
E., Carmona
A., Chilingarian
S., Commichau
J. L., Contrera
J., Cortina
M. T., Costado
V., Curtef
V., Danielyan
F., Dazzi
A. D., Angeli
C., Delgado
R. D., Reye
B. D., Lotto
D., Dorner
M., Doro
M., Errando
M., Fagiolini
D., Ferenc
E., Fernandez
R., Firpo
M. V., Fonseca
L., Font
M., Fuch
N., Galante
R. J., Garcia Lopez
M., Garczarczyk
M., Gaug
F., Goebel
D., Hakobyan
M., Hayashida
T., Hengstebeck
A., Herrero
D., Hohne
J., Hose
C. C., Hsu
S., Huber
P., Jacon
T., Jogler
R., Kosyra
D., Kranich
R., Kritzer
A., Laille
E., Lindfor
S., Lombardi
Longo, Francesco
M., Lopez
E., Lorenz
P., Majumdar
G., Maneva
K., Mannheim
M., Mariotti
M., Martinez
D., Mazin
C., Merck
M., Meucci
M., Meyer
J. M., Miranda
R., Mirzoyan
S., Mizobuchi
A., Moralejo
D., Nieto
K., Nilsson
J., Ninkovic
E., Ona Wilhelmi
N., Otte
I., Oya
M., Panniello
R., Paoletti
M., Pasanen
D., Pascoli
F., Pau
R., Pegna
M., Persic
L., Peruzzo
A., Piccioli
E., Prandini
N., Puchade
A., Raymer
J., Rico
W., Rhode
M., Rissi
A., Robert
S., Rugamer
A., Saggion
T. Y., Saito
A., Sanchez
P., Sartori
V., Scalzotto
V., Scapin
R., Schmitt
T., Schweizer
M., Shayduk
K., Shinozaki
S. N., Shore
N., Sidro
A., Sillanpaa
D., Sobczynska
F., Spanier
A., Stamerra
L. S., Stark
L., Takalo
P., Temnikov
D., Tescaro
M., Teshima
D. F., Torre
N., Turini
H., Vankov
A., Venturini
V., Vitale
R. M., Wagner
T., Wibig
W., Wittek
F., Zandanel
R., Zanin
J., Zapatero
Source :
E-Prints Complutense: Archivo Institucional de la UCM, Universidad Complutense de Madrid, E-Prints Complutense. Archivo Institucional de la UCM, instname
Publication Year :
2008
Publisher :
EDP Sciences, 2008.

Abstract

The active galactic nucleus PG 1553+113 was observed by the MAGIC telescope in July 2006 during a multiwavelength campaign, in which telescopes in the optical, X-ray, and very high energies participated. Although the MAGIC data were affected by strong atmospheric absorption (calima), they were analyzed after applying a correction. In 8.5 hours, a signal was detected with a significance of 5.0 sigma. The integral flux above 150 GeV was (2.6 +/- 0.9)*10^{-7} ph/s/m^2. By fitting the differential energy spectrum with a power law, a spectral index of -4.1 +/- 0.3 was obtained.<br />4 pages, 3 figures, accepted for publication in A&A

Details

ISSN :
14320746 and 00046361
Volume :
493
Database :
OpenAIRE
Journal :
Astronomy & Astrophysics
Accession number :
edsair.doi.dedup.....7d67f62c76bcd71cf652c48ddee7eb3b
Full Text :
https://doi.org/10.1051/0004-6361:20079048