Open AccessExtremely violent optical microvariability in blazars: fact or fiction? ★
Author(s) -
Cellone Sergio A.,
Romero Gustavo E.,
Araudo Anabella T.
Publication year - 2007
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1111/j.1365-2966.2006.11140.x
Subject(s) - physics , photometry (optics) , spurious relationship , blazar , astrophysics , light curve , amplitude , stars , astronomy , systematic error , statistics , optics , gamma ray , mathematics
Variability amplitudes larger than 1 mag over time‐scales of a few tens of minutes have recently been reported in the optical light curves of several blazars. In order to independently verify the real occurrence of such extremely violent events, we undertook an observational study of a selected sample of three blazars: PKS 0048−097, PKS 0754+100 and PKS 1510−089. Possible systematic error sources during data acquisition and reduction were carefully evaluated. We indeed found flux variability at intra‐night time‐scales in all the three sources, although no extremely violent behaviour, as reported by other authors, was detected. We show that an incorrect choice of the stars used for differential photometry will, under fairly normal conditions, lead to spurious variability with large amplitudes on short time‐scales. Wrong results of this kind can be avoided with the use of simple error‐control techniques.