most citedResults of WEBT, VLBA and RXTE monitoring of 3C 279 during 2006-2007

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astro-ph2008136 cited

Results of WEBT, VLBA and RXTE monitoring of 3C 279 during 2006-2007

V. M. Larionov, S. G. Jorstad, A. P. Marscher +2

We present radio-to-optical data taken by the WEBT, supplemented by VLBA and RXTE observations, of 3C 279. Our goal is to use this extensive database to draw inferences regarding t…

astro-ph2008101 cited

A new activity phase of the blazar 3C 454.3. Multifrequency observations by the WEBT and XMM-Newton in 2007-2008

C. M. Raiteri, M. Villata, V. M. Larionov +2

We present and analyse the WEBT multifrequency observations of 3C 454.3 in the 2007-2008 observing season, including XMM-Newton observations and near-IR spectroscopic monitoring, a…

astro-ph200819 cited

Radio continuum properties of young planetary nebulae

L. Cerrigone, G. Umana, C. Trigilio +3

We have selected a small sample of post-AGB stars in transition towards the planetary nebula and present new Very Large Array multi-frequency high-angular resolution radio observat…

astro-ph2008125 cited

Multifrequency monitoring of the blazar 0716+714 during the GASP-WEBT-AGILE campaign of 2007

M. Villata, C. M. Raiteri, V. M. Larionov +5

Since the CGRO operation in 1991-2000, one of the primary unresolved questions about the blazar gamma-ray emission has been its possible correlation with the low-energy (in particu…

astro-ph200859 cited

Radio-to-UV monitoring of AO 0235+164 by the WEBT and Swift during the 2006--2007 outburst

C. M. Raiteri, M. Villata, V. M. Larionov +2

The blazar AO 0235+164 was claimed to show a quasi-periodic behaviour in the radio and optical bands. Moreover, an extra emission component contributing to the UV and soft X-ray fl…

astro-ph200712 cited

Millimeter observations of Planetary Nebulae: a contribution to the Planck pre-launch catalogue

G. Umana, P. Leto, C. Trigilio +5

We present new millimetre 43 GHz observations of a sample of radio-bright Planetary Nebulae. Such observations were carried out to have a good determination of the high-frequency r…