C
C. Leto
Researcher at Agenzia Spaziale Italiana
Publications - 1
Citations - 222
C. Leto is an academic researcher from Agenzia Spaziale Italiana. The author has contributed to research in topics: Blazar & Quasar. The author has an hindex of 1, co-authored 1 publications receiving 211 citations.
Papers
More filters
Journal ArticleDOI
Simultaneous Planck, Swift, and Fermi observations of X-ray and γ-ray selected blazars
Paolo Giommi,G. Polenta,G. Polenta,Anne Lähteenmäki,Anne Lähteenmäki,D. J. Thompson,M. Capalbi,S. Cutini,Dario Gasparrini,J. González-Nuevo,Jonathan León-Tavares,M. López-Caniego,Mn Mazziotta,C. Monte,C. Monte,M. Perri,S. Rainò,S. Rainò,G. Tosti,G. Tosti,Andrea Tramacere,F. Verrecchia,Hugh D. Aller,M. F. Aller,E. Angelakis,Denis Bastieri,Denis Bastieri,Andrei Berdyugin,Anna Bonaldi,Laura Bonavera,Laura Bonavera,Carlo Burigana,David N. Burrows,S. Buson,E. Cavazzuti,G. Chincarini,Sergio Colafrancesco,L. Costamante,F. Cuttaia,Filippo D'Ammando,G. de Zotti,G. de Zotti,M. Frailis,Lars Fuhrmann,S. Galeotta,F. Gargano,N. Gehrels,Nicola Giglietto,Nicola Giglietto,Francesco Giordano,Marcello Giroletti,E. Keihänen,O. King,Thomas P. Krichbaum,Anthony Lasenby,N. Lavonen,Charles R. Lawrence,C. Leto,Elina Lindfors,Nazzareno Mandolesi,Marcella Massardi,Walter Max-Moerbeck,Peter F. Michelson,M. G. Mingaliev,Paolo Natoli,Paolo Natoli,Paolo Natoli,I. Nestoras,E. Nieppola,E. Nieppola,Kari Nilsson,B. Partridge,Vasiliki Pavlidou,T. J. Pearson,Pietro Procopio,Jörg P. Rachen,Anthony C. S. Readhead,R. Reeves,A. Reimer,R. Reinthal,S. Ricciardi,Joseph L. Richards,D. Riquelme,Jari Saarinen,Anna Sajina,M. Sandri,P. Savolainen,A. Sievers,A. Sillanpää,Yu. V. Sotnikova,Mark Stevenson,G. Tagliaferri,L. O. Takalo,Joni Tammi,D. Tavagnacco,Luca Terenzi,L. Toffolatti,Merja Tornikoski,Corrado Trigilio,M. Turunen,G. Umana,H. Ungerechts,F. Villa,Jingwen Wu,Andrea Zacchei,J. A. Zensus,Xu Zhou +106 more
TL;DR: In this paper, simultaneous Planck, Swift, Fermi, and ground-based data for 105 blazars belonging to three samples with flux limits in the soft X-ray, hard Xray, and gamma-ray bands, with additional 5 GHz flux-density limits to ensure a good probability of a Planck detection.