Abstract
CCD imaging photometry data has been obtained on a sample of sources to search for rapid variability. Light curves and photometric data are presented for the QSO PG 0117+213 and the BL Lacertae objects 0414+009 and 0836+182. The B and V magnitudes of the QSO PG 0117+213 decreased by 0.86 and 0.30 in a time interval of 46 hours. In the rest frame of the QSO (z=1.493) these variations occurred in only 18.5 hours. Furthermore this QSO varied significantly over a period of only 25 minutes. No short timescale variability was detected in the two BL Lacertae objects.
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© 1991 Springer-Verlag
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Ekins, R., Plunkett, S., McBreen, B. (1991). Optical observations of rapid variability in the QSO PG 0117+213. In: Duschl, W.J., Wagner, S.J., Camenzind, M. (eds) Variability of Active Galaxies. Lecture Notes in Physics, vol 377. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0030058
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DOI: https://doi.org/10.1007/BFb0030058
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