Time delay between images of the lensed quasar UM673статья

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Дата последнего поиска статьи во внешних источниках: 10 февраля 2016 г.

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[1] Time delay between images of the lensed quasar um673 / E. Koptelova, W. P. Chen, T. Chiueh et al. // ArXiv e-prints. — 1304.5396. — ArXiv e-prints, 2013. — P. 1–9. Submitted on 24 Apr 2012 (v1), last revised 26 Apr 2012 (this version, v2)) We study brightness variations in the double lensed quasar UM673 (Q0142-100) with the aim of measuring the time delay between its two images. In the paper we combine our previously published observational data of UM673 obtained during the 2003 - 2005 seasons at the Maidanak Observatory with archival and recently observed Maidanak and CTIO UM673 data. We analyze the V, R and I-band light curves of the A and B images of UM673, which cover ten observational seasons from August 2001 to November 2010. We also analyze the time evolution of the difference in magnitudes between images A and B of UM673 over more than ten years. We find that the quasar exhibits both short-term (with amplitude of ∼0.1 mag in the R band) and high-amplitude (∼0.3 mag) long-term variability on timescales of about several months and several years, respectively. These brightness variations are used to constrain the time delay between the images of UM673. From cross-correlation analysis of the A and B quasar light curves and error analysis we measure the mean time delay and its error of 89 ±11 days. Given the input time delay of 88 days, the most probable value of the delay that can be recovered from light curves with the same statistical properties as the observed R-band light curves of UM673 is 95{+5/-16}{+14/-29} days (68 and 95 % confidence intervals). Analysis of the V - I color variations and V, R and I-band magnitude differences of the quasar images does not show clear evidence of the microlensing variations between 1998 and 2010. [ DOI ]

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