The variability of 30 PG quasars has been observed in the red band during 3 years. A rest-frame structure function analysis shows an increase of variability with the time interval up to 0.2 mag rms after 2 years. A comparison with the IUE data available for PG quasars shows that the variability increases with the rest-frame frequency at each time interval. Evidence for this effect is supported by the analysis of the average variability of other published quasar samples. The effect can account completely for the increase of variability with redshift found in other studies
We characterize the optical variability properties of eight lobe-dominated radio quasars (QSOs): B2 ...
The long-term variability of a sample of 180 optically selected QSOs in the field of the Selected Ar...
The long-term optical variability of a composite, complete sample of quasars is investigated. While ...
The variability of 30 PG quasars has been observed in the red band during 3 years. A rest-frame stru...
We performed a new analysis of B and R light curves of a sample of PG quasars. We confirm the variab...
In previous studies we have shown that the optical variability of quasars increases, on average, wit...
Aims. The study of the ensemble properties of the UV/optical broadband variability of quasars is ham...
Aims. The study of the ensemble properties of the UV/optical broadband variability of quas...
We performed a new analysis of B and R light curves of a sample of PG quasars. We confirm the variab...
We investigate the optical variability of 7658 quasars from SDSS Stripe 82. Taking advantage of a la...
The relationship between variability, luminosity and redshift in the South Galactic Pole QSO sample ...
Using a sample of over 25000 spectroscopically confirmed quasars from the Sloan Digital Sky Survey, ...
We present an analysis of X-ray variability in a sample of 156 radio quiet quasars taken from the RO...
We provide a quantitative description and statistical interpretation of the optical continuum variab...
We have obtained single-epoch optical photometry for 201 quasars, taken from the FIRST Bright Quasar...
We characterize the optical variability properties of eight lobe-dominated radio quasars (QSOs): B2 ...
The long-term variability of a sample of 180 optically selected QSOs in the field of the Selected Ar...
The long-term optical variability of a composite, complete sample of quasars is investigated. While ...
The variability of 30 PG quasars has been observed in the red band during 3 years. A rest-frame stru...
We performed a new analysis of B and R light curves of a sample of PG quasars. We confirm the variab...
In previous studies we have shown that the optical variability of quasars increases, on average, wit...
Aims. The study of the ensemble properties of the UV/optical broadband variability of quasars is ham...
Aims. The study of the ensemble properties of the UV/optical broadband variability of quas...
We performed a new analysis of B and R light curves of a sample of PG quasars. We confirm the variab...
We investigate the optical variability of 7658 quasars from SDSS Stripe 82. Taking advantage of a la...
The relationship between variability, luminosity and redshift in the South Galactic Pole QSO sample ...
Using a sample of over 25000 spectroscopically confirmed quasars from the Sloan Digital Sky Survey, ...
We present an analysis of X-ray variability in a sample of 156 radio quiet quasars taken from the RO...
We provide a quantitative description and statistical interpretation of the optical continuum variab...
We have obtained single-epoch optical photometry for 201 quasars, taken from the FIRST Bright Quasar...
We characterize the optical variability properties of eight lobe-dominated radio quasars (QSOs): B2 ...
The long-term variability of a sample of 180 optically selected QSOs in the field of the Selected Ar...
The long-term optical variability of a composite, complete sample of quasars is investigated. While ...