First Results from the Wide Angle Camera of the ROSETTA Mission (Articolo in rivista)

Type
Label
  • First Results from the Wide Angle Camera of the ROSETTA Mission (Articolo in rivista) (literal)
Anno
  • 2005-01-01T00:00:00+01:00 (literal)
Alternative label
  • C. Barbieri, S. Fornasier, I. Bertini, F. Angrilli, G.A. Bianchini, S. Debei, M. De Cecco, G. Parzianello, M. Zaccariotto, V. Da Deppo, G. Naletto, (2005)
    First Results from the Wide Angle Camera of the ROSETTA Mission
    in Memorie della Società astronomica italiana supplementi
    (literal)
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  • C. Barbieri, S. Fornasier, I. Bertini, F. Angrilli, G.A. Bianchini, S. Debei, M. De Cecco, G. Parzianello, M. Zaccariotto, V. Da Deppo, G. Naletto, (literal)
Pagina inizio
  • 28 (literal)
Pagina fine
  • 33 (literal)
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  • 6 (literal)
Rivista
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  • Department of Astronomy, University of Padova - Vicolo dell'Osservatorio, 2 I-35122 Padova Department of Mechanical Engineering, University of Padova - Via Venezia, 1 I-35122 Padova Department of Informatics Engineering, University of Padova - Via Gradenigo, 6A I-35122 Padova CNR-IFN UOS Padova (literal)
Titolo
  • First Results from the Wide Angle Camera of the ROSETTA Mission (literal)
Abstract
  • This paper gives a brief description of the Wide Angle Camera (WAC), built by the Center of Studies and Activities for Space (CISAS) of the University of Padova for the ESA ROSETTA Mission, of data we have obtained about the new mission targets, and of the first results achieved after the launch in March 2004. The WAC is part of the OSIRIS imaging system, built under the PI-ship of Dr. U. Keller (Max-Planck-Institute for Solar System Studies) which comprises also a Narrow Angle Camera (NAC) built by the Laboratoire d'Astrophysique Spatiale (LAS) of Marseille. CISAS had also the responsibility to build the shutter and the front door mechanism for the NAC. The images show the excellent optical quality of the WAC, exceeding the specifications both in term of encircled energy (80% in one pixel over a FoV of 12×12 sq degree), limiting magnitude (fainter than the 13th in 30s exposure time through a wideband red filter) and amount of distortions. (literal)
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