Zobrazeno 1 - 10
of 139
pro vyhledávání: '"T. Maccacaro"'
Autor:
X. Barcons, F. J. Carrera, M. T. Ceballos, M. J. Page, J. Bussons-Gordo, A. Corral, J. Ebrero, S. Mateos, J. A. Tedds, M. G. Watson, D. Baskill, M. Birkinshaw, T. Boller, N. Borisov, M. Bremer, G. E. Bromage, H. Brunner, A. Caccianiga, C. S. Crawford, M. S. Cropper, R. Della Ceca, P. Derry, A. C. Fabian, P. Guillout, Y. Hashimoto, G. Hasinger, B. J. M. Hassall, G. Lamer, N. S. Loaring, T. Maccacaro, K. O. Mason, R. G. McMahon, L. Mirioni, J. P. D. Mittaz, C. Motch, I. Negueruela, J. P. Osborne, F. Panessa, I. Pérez-Fournon, J. P. Pye, T. P. Roberts, S. Rosen, N. Schartel, N. Schurch, A. Schwope, P. Severgnini, R. Sharp, G. C. Stewart, G. Szokoly, A. Ullán, M. J. Ward, R. S. Warwick, P. J. Wheatley, N. A. Webb, D. Worrall, W. Yuan, H. Ziaeepour
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2007, 476 (3), pp.1191-1203. ⟨10.1051/0004-6361:20077606⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy & astrophysics, 2007, Vol.476(3), pp.1191-1203 [Peer Reviewed Journal]
Astronomy and Astrophysics-A&A, EDP Sciences, 2007, 476 (3), pp.1191-1203. ⟨10.1051/0004-6361:20077606⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy & astrophysics, 2007, Vol.476(3), pp.1191-1203 [Peer Reviewed Journal]
[Aims] X-ray sources at intermediate fluxes (a few x 10-14 erg cm-2 s-1) with a sky density of ~100 deg-2 are responsible for a significant fraction of the cosmic X-ray background at various energies below 10 keV. The aim of this paper is to provide
Autor:
A. Caccianiga, P. Severgnini, V. Braito, R. Della Ceca, T. Maccacaro, A. Wolter, X. Barcons, F. J. Carrera, I. Lehmann, M. J. Page, R. Saxton, N. A. Webb
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
This paper presents the analysis of a statistically complete sample of 28 serendipitous X-ray sources selected in 82 pointed XMM-Newton fields down to a count-rate of 0.002 counts s-1 (4.5-7.5 keV energy band). This is the first sample selected in th
Publikováno v:
Scopus-Elsevier
We present the scientific goals and the strategy of the REX survey, a project which has been recently initiated at the Brera Astronomical Observatory in Milan with the aim of selecting a large and statistically representative sample of BL Lac objects
Autor:
M. J. Page, R. Della Ceca, Michael Freyberg, Yoshihiro Ueda, Jonathan Tedds, Franz E. Bauer, Hermann Brunner, Silvia Mateos, Xavier Barcons, Francisco J. Carrera, J. Ebrero, T. Maccacaro, G. Lamer, Stefan Rosén, A. Corral, María Teresa Ceballos, M. G. Watson
AXIS (An XMM-Newton International Survey) is a survey of 36 high Galactic latitude XMM-Newton observations covering 4.8 deg2 and containing 1433 serendipitous X-ray sources detected with 5-sigma significance. We have studied the X-ray source counts i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b46eac5ee012a783462126861bc941a3
http://arxiv.org/abs/astro-ph/0703451
http://arxiv.org/abs/astro-ph/0703451
Publikováno v:
BL Lac Objects ISBN: 3540513892
BL Lac Objects
BL Lac Objects
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::75ec3f20f8353d4e24af14ae317994d2
https://doi.org/10.1007/bfb0031164
https://doi.org/10.1007/bfb0031164
The XMM-Newton observation of the optically Type 1 AGN AXJ0447-0627 (z=0.214) unambiguously reveals a complex, bright and prominent set of lines in the 4-8 keV rest frame energy range. Although, from a phenomenological point of view, the observed pro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::272c2d941eb4811aae030c6d768068a0
XMM-Newton observations are presented for the z=0.83 cluster of galaxies MS1054-0321, the highest redshift cluster in the Einstein Extended Medium Sensitivity Survey (EMSS). The temperature inferred by the XMM-Newton data, T=7.2 (+0.7, -0.6) keV, is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::842c48c4697534dc8009670d45cbf5ff
Autor:
Alessandro Caccianiga, Paola Severgnini, Volker Beckmann, R. Della Ceca, I. Cagnoni, T. Maccacaro, V. Braito, Anna Wolter, I. M. Gioia
Publikováno v:
403 (2003): 555.
info:cnr-pdr/source/autori:Della Ceca R., V. Braito, V. Beckmann, A. Caccianiga, I. Cagnoni, I.M. Gioia, T. Maccacaro, P. Severgnini, A. Wolter/titolo:A Hard Medium Survey with ASCA. IV: the Radio-Loud Type 2 QSO AXJ0843+294 2/doi:/rivista:/anno:2003/pagina_da:555/pagina_a:/intervallo_pagine:555/volume:403
info:cnr-pdr/source/autori:Della Ceca R., V. Braito, V. Beckmann, A. Caccianiga, I. Cagnoni, I.M. Gioia, T. Maccacaro, P. Severgnini, A. Wolter/titolo:A Hard Medium Survey with ASCA. IV: the Radio-Loud Type 2 QSO AXJ0843+294 2/doi:/rivista:/anno:2003/pagina_da:555/pagina_a:/intervallo_pagine:555/volume:403
We discuss the X-ray, optical and radio properties of AX J0843+2942, a high luminosity Type 2 AGN found in the ASCA Hard Serendipitous Survey. The X-ray spectrum is best described by an absorbed power-law model with photon index of Gamma = 1.72 (+0.3
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f44c8441ebcb600ed465423787567d94
http://arxiv.org/abs/astro-ph/0305505
http://arxiv.org/abs/astro-ph/0305505
Autor:
K. Sekiguchi, Wolfgang Pietsch, R. Della Ceca, Paola Severgnini, Alessandro Caccianiga, Francisco J. Carrera, V. Braito, Anna Wolter, Masayuki Akiyama, Toshiyuki Sasaki, Xavier Barcons, Michitoshi Yoshida, N. A. Webb, M. G. Watson, T. Maccacaro
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Scopus-Elsevier
instname
Scopus-Elsevier
We have performed a detailed analysis of 3 optically normal galaxies extracted from the XMM Bright Serendipitous Source Sample. Thanks to the good statistics of the XMM-Newton data, we have unveiled the presence of an AGN in all of them. In particula
Publikováno v:
AIP Conference Proceedings.
We describe the selection technique adopted to extract from the REX sample (Radio Emitting X-ray sources) a well-defined subsample of 109 Optically Bright REX (OB-REX). Here we present the optical, X-ray and radio properties of the OB-REX sources and