VSOP Observations of the Blazar S5 2007+77

A. Kraus; A. Witzel; J.A. Zensus; K. E. Gabanyi; T. P. Krichbaum

arxiv: 0802.0540 · v1 · pith:PNDUVLXZnew · submitted 2008-02-05 · 🌌 astro-ph

VSOP Observations of the Blazar S5 2007+77

K. E. Gabanyi , T. P. Krichbaum , A. Kraus , A. Witzel , J.A. Zensus This is my paper

classification 🌌 astro-ph

keywords blazarepochsobservationsvariabilityvsopwavelengthsachievableanalysed

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The blazar, S5 2007+77 shows intraday variability in cm wavelengths. Seven epochs of VSOP observations were carried out in 1998 and 1999 at 5 GHz to look for the origin of the variability with the highest achievable angular resolution at cm wavelengths. Here the results of four epochs are analysed, which revealed ~10% variations in polarized flux density.

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VSOP Observations of the Blazar S5 2007+77

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