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Microlensing in the double quasar SBS1520+530

E. R. Gaynullina·R. W. Schmidt·T. Akhunov·O. Burkhonov·S. Gottloeber·K. Mirtadjieva·S. N. Nuritdinov·I. Tadjibaev·J. Wambsganss·L. Wisotzki
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Abstract

We present the results of a monitoring campaign of the double quasar SBS1520+530 at Maidanak observatory from April 2003 to August 2004. We obtained light curves in V and R filters that show small-amplitude Δm~0.1 mag intrinsic variations of the quasar on time scales of about 100 days. The data set is consistent with the previously determined time delay of Δt=(130+-3) days by Burud et al. (2002). We find that the time delay corrected magnitude difference between the quasar images is now larger by (0.14+-0.03) mag than during the observations by Burud et al. (2002). This confirms the presence of gravitational microlensing variations in this system.

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E. R. Gaynullina, R. W. Schmidt, T. Akhunov, O. Burkhonov, S. Gottloeber, K. Mirtadjieva, S. N. Nuritdinov, I. Tadjibaev, J. Wambsganss, L. Wisotzki. 2005-05-24. Microlensing in the double quasar SBS1520+530. https://doi.org/10.1051/0004-6361%3A20052852

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