Microvariability Observations of Three Active Galactic Nuclei

Details Microvariability Observations of Three Active Galactic Nuclei Microvariability Observations of Three Active Galactic Nuclei

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...197.3909c&link_type=abstract

American Astronomical Society, 197th AAS Meeting, #39.09; Bulletin of the American Astronomical Society, Vol. 32, p.1457

Astronomy and Astrophysics

Astronomy

Scientific paper

Microvariability observations are presented for three objects - the BL Lac object OQ 530, the OVV quasar 3CR 345, and the very high redshift quasar PSS 1057+4555. All objects were observed using the 0.76m telescope at the Rosemary Hill Observatory. The object OQ 530 was observed in the R band during three nights in June of 1997. Observations in the V and I bands were made of the OVV quasar 3CR 345 in May of 2000. The microvariability behavior reported here for OQ 530 and 3CR 345 is compared to the previously reported behavior for these objects. In addition, observations were carried out over four nights in March and May of 2000 to search for microvariability of the very high redshift (z = 4.10) quasar PSS 1057+4555. The data presented here for these three objects are discussed in relation to current models for microvariability.

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