output
20042019
most citedA new activity phase of the blazar 3C 454.3. Multifrequency observations by the WEBT and XMM-Newton in 2007-2008

101 citations

7 papers

astro-ph.SR2019★ 1 cited

V348 And and V572 Per: Bright Triple Systems with Eccentric Eclipsing Binaries

P. Zasche, R. Uhlar, P. Svoboda +5

The eclipsing binaries are still important objects for our understanding of the universe. Especially these ones located within the more complex multiple systems can help us solving…

astro-ph.SR2012★ 3 cited

GK Boo and AE For: Two low-mass eclipsing binaries with dwarf companions

P. Zasche, P. Svoboda, R. Uhlar

A study of late-type low-mass eclipsing binaries provides us with important information about the most common stars in the Universe. We obtain the first light curves and perform pe…

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-ph2007★ 3 cited

Eclipsing Binaries with Possible Light-Time Effect

Zasche Petr, Zejda Miloslav, Brat Lubos

The period changes of six eclipsing binaries have been studied with focus on the light-time effect. With the least squares method we also calculated parameters of such an effect an…

astro-ph2005★ 10 cited

The possible orbital period of the nova V1493 Aquilae

Andrej Dobrotka, Michael Friedjung, Alon Retter +2

Period analysis of CCD photometry of V1493 Aql (Nova Aql 1999 no. 1) performed during 12 nights through I and R filters a few weeks after maximum is presented. The PDM method for p…

astro-ph2005★ 1 cited

Light Variations of the Anomalous Central Star of Planetary Nebula Sh 2-71

Zdenek Mikulasek, Augustin Skopal, Miloslav Zejda +5

We present an analysis of light variations in UBVRI of the anomalous object in the center of planetary nebula Sh 2-71. We refined the linear ephemeris of the light maxima to JD{max…