activity
20022025
most citedBlazar spectral variability as explained by a twisting inhomogeneous jet

199 citations · 1.8k across the 86 of their papers we have counts for

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astro-ph2008★ 101 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-ph2008★ 2 cited

Spectroscopy of bright quasars: emission lines and internal extinction

R. Bachev, A. Strigachev, E. Semkov +1

The main purpose of this work is to improve the existing knowledge about the most powerful engines in the Universe - quasars. Although a lot is already known, we still have only a…

astro-ph2008★ 59 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-ph2007★ 31 cited

Recent photometry of symbiotic stars - XII

A. Skopal, M. Vanko, T. Pribulla +4

We present new photometric observations of 15 symbiotic stars (EG And, Z And, AE Ara, BF Cyg, CH Cyg, CI Cyg, V1329 Cyg, TX CVn, AG Dra, Draco C-1, RW Hya, SY Mus, AR Pav, AG Peg,…

astro-ph2007★ 3 cited

Photometric monitoring of the blazar 3C 345 for the period 1996 - 2006

B. Mihov, R. Bachev, L. Slavcheva-Mihova +3

We present the results of the blazar 3C 345 monitoring in Johnson-Cousins BVRI bands for the period 1996 - 2006. We have collected 29 V and 43 R data points for this period; the BI…

astro-ph2006★ 8 cited

The Recurrent Eclipse of an Unusual Pre--Main-Sequence Star in IC 348

S. Nordhagen, W. Herbst, E. C. Williams +1

The recurrence of a previously documented eclipse of a solar-like pre--main-sequence star in the young cluster IC 348 has been observed. The recurrence interval is 4.7 yr…