X-ray spectral evolution of TeV BL Lacertae objects: eleven years of observations with BeppoSAX, XMM-Newton and Swift satellites (Corrigendum)

F. Massaro; A. Tramacere; A. Cavaliere; M. Perri; P. Giommi

doi:10.1051/0004-6361/20078639e

Free Access

Erratum

This article is an erratum for: [this article]

Issue		A&A Volume 528, April 2011


Article Number		C1
Number of page(s)		2
Section		Extragalactic astronomy
DOI		https://doi.org/10.1051/0004-6361/20078639e
Published online		16 March 2011

A&A 528, C1 (2011)

X-ray spectral evolution of TeV BL Lacertae objects: eleven years of observations with BeppoSAX, XMM-Newton and Swift satellites (Corrigendum)

F. Massaro¹, A. Tramacere², A. Cavaliere¹, M. Perri³ and P. Giommi³

¹ Dipartimento di Fisica, Università di Roma Tor Vergata via della Ricerca scientifica 1, 00133 Roma, Italy
e-mail: fmassaro@cfa.harvard.edu
² Dipartimento di Fisica, Università di Roma La Sapienza, Piazzale A. Moro 2, 00185 Roma, Italy
³ ASI Science Data Center, ESRIN, 00044 Frascati, Italy

This article has no abstract.

Key words: galaxies: active / BL Lacertae objects: general / X-rays: galaxies / radiation mechanisms: non-thermal / errata, addenda

Erratum to: A&A 478, 395-401 (2008), DOI: 10.1051/0004-6361:20078639

© ESO, 2011

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