Testing Microvariability in Quasar Differential Light Curves Using Several Field Stars
Microvariability consists of small timescale variations of low amplitude in the photometric light curves of quasars and represents an important tool to investigate their inner core. Detection of quasar microvariations is challenging because of their non-periodicity, as well as the need for high monitoring frequency and a high signal-to-noise ratio
de Diego, J. A. et al.
Fecha de publicación:
8
2015