activity
20022026
most citedCIV 1549 as an Eigenvector 1 Parameter for Active Galactic Nuclei

237 citations · 3.8k across the 103 of their papers we have counts for

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astro-ph2008★ 16 cited

Quasar optical variability: searching for interband time delays

Rumen S. Bachev

Aims. The main purpose of this paper is to study time delays between the light variations in different wavebands for a sample of quasars. Measuring a reliable time delay for a larg…

astro-ph2008★ 45 cited

The WEBT Campaign on the Intermediate BL Lac Object 3C66A in 2007-2008

M. Boettcher, K. Fultz

Prompted by a high optical state in September 2007, the Whole Earth Blazar Telescope (WEBT) consortium organized an intensive optical, near-IR (JHK) and radio observing campaign on…

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★ 27 cited

Rotational velocities of the giants in symbiotic stars: III. Evidence of fast rotation in S-type symbiotics

R. K. Zamanov, M. F. Bode, C. H. F. Melo +5

We have measured the projected rotational velocities (vsini) in a number of symbiotic stars and M giants using high resolution spectroscopic observations. On the basis of our measu…

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…