Gamma ray sources observation with the ARGO-YBJ detector
- Autori: B. Bartoli; BERNARDINI, Paolo; X. J. Bi; C. Bleve; I. Bolognino; P. Branchini; A. Budano; A. K. Calabrese Melcarne; P. Camarri; Z. Cao; A. Cappa; R. Cardarelli; S. Catalanotti; C. Cattaneo; P. Celio; S. Z. Chen; T. L. Chen; Y. Chen; P. Creti; S. W. Cui; B. Z. Dai; G. D’Alì Staiti; Danzengluobu; M. Dattoli; DE MITRI, Ivan; B. D’Ettorre Piazzoli; T. Di Girolamo; X. H. Ding; G. Di Sciascio; C. F. Feng; Zhaoyang Feng; Zhenyong Feng; F. Galeazzi; P. Galeotti; E. Giroletti; Q. B. Gou; Y. Q. Guo; H. H. He; Haibing Huo; Hongbo Hue; Q. Huang; M. Iacovacci; R. Iuppa; I. James; H. Y. Jia; Labaciren; H. J. Li; J. Y. Li; X. X. Li; G. Liguori; C. Liu; C. Q. Liu; J. Liu; M. Y. Liu; H. Lu; X. H. Ma; MANCARELLA, Giovanni; S. M. Mari; MARSELLA, GIOVANNI; MARTELLO, Daniele; S. Mastroianni; P. Montini; C. C. Ning; A. Pagliaro; PANAREO, Marco; B. Panico; PERRONE, Lorenzo; P. Pistilli; X. B. Qu; E. Rossi; F. Ruggieri; P. Salvini; R. Santonico; P. R. Shen; X. D. Sheng; F. Shi; C. Stanescu; A. Surdo; Y. H. Tan; P. Vallania; S. Vernetto; C. Vigorito; B. Wang; H. Wang; C. Y. Wu; H. R. Wu; B. Xu; L. Xue; Y. X. Yan; Q. Y. Yang; X. C. Yang; Z. G. Yao; A. F. Yuan; M. Zha; H. M. Zhang; JilongZhang, JianliZhang; L. Zhang; P. Zhang; X. Y. Zhang; Y. Zhang; Zhaxiciren, Zhaxisangzhu; X. X. Zhou; F. R. Zhu; Q. Q. Zhu; G. Zizzi
- Anno di pubblicazione: 2011
- Tipologia: Articolo in rivista
- Parole Chiave: Gamma Astronomy; Array Detector
- OA Link: http://hdl.handle.net/10447/466523
Abstract
In this paper we report on the observations of TeV gamma ray sources performed by the air shower detector ARGO-YBJ. The objects studied in this work are the blazar Markarian 421 and the extended galactic source MGROJ1908+06, monitored during 2 years of operation. Mrk421 has been detected by ARGO-YBJ with a statistical significance of 11 standard deviations. The observed TeV emission was highly variable, showing large enhancements of the flux during active periods. The study of the spectral behaviour during flares revealed a positive correlation of the hardness with the flux, as already reported in the past by the Whipple telescope, suggesting that this is a long term property of the source. ARGO-YBJ observed a strong correlation between TeV gamma rays and the X-ray flux measured by RXTM/ASM and SWIFT/BAT during the whole period, with a time lag compatible with zero, supporting the one-zone SSC model to describe the emission mechanism. MGROJ1908+06 has been detected by ARGO-YBJ with 5 standard deviation of significance. From our data the source appears extended and the measured extension is ext=0.48+0.26−0.28, in agreement with a previous HESS observation. The average flux is in marginal agreement with that reported by MILAGRO, but significantly higher than that obtained by HESS, suggesting a possible flux variability.