EDP Sciences
Free Access
Volume 447, Number 3, March I 2006
Page(s) 905 - 913
Section Extragalactic astronomy
DOI https://doi.org/10.1051/0004-6361:20053574
Published online 10 February 2006

A&A 447, 905-913 (2006)
DOI: 10.1051/0004-6361:20053574

Observational determination of the time delays in gravitational lens system Q2237+0305

V. Vakulik1, R. Schild2, V. Dudinov1, S. Nuritdinov3, V. Tsvetkova4, O. Burkhonov3 and T. Akhunov3

1  Institute of Astronomy of Kharkov National University, Sumskaya 35, 61022 Kharkov, Ukraine
    e-mail: vakulik@astron.kharkov.ua
2  Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
3  Ulugh Beg Astronomical Institute of Ac.Sci. of Uzbekistan, Astronomicheskaya 33, 700052 Tashkent, Republic of Uzbekistan
4  Institute of Radio Astronomy of Nat. Ac. Sci. of Ukraine, Krasnoznamennaya 4, 61002 Kharkov, Ukraine

(Received 4 June 2005 / Accepted 26 October 2005)

We present new brightness monitoring observations of the 4 components of gravitationally lensed system Q2237+0305 , which show detection of an intrinsic quasar brightness fluctuation at a time of subdued microlensing activity, between June 27 and October 12, 2003. These data were used to determine the time delays between the arrivals of the four images. The measured delays are $\tau_{\rm BA}\approx-6$, $\tau_{\rm CA}\approx35$, and $\tau_{\rm DA}\approx2$ h, so they confirm that the long history of brightness monitoring has produced significant detection of microlensing. However the error bars associated with the delays, of order 2 days, are too large to discriminate between competing macro-imaging models. Moreover, our simulations show that for the amplitude of this intrinsic fluctuation and for photometric errors intrinsic to optical monitoring from our 1.5-m telescope or from the OGLE monitoring, a daily sampled brightness record cannot produce reliable lags for model discrimination. We use our simulations to devise a strategy for future delay determination with optical data. Nevertheless, we regard these first estimates to be significant, since they are the first direct measurements of time delays made for this system from ground-based observations in the visual wavelengths. The detected highly correlated fluctuations of the four quasar images provide an extra confirmation of the gravitational-lens nature of Q2237+0305, and give observational justification to the extensive literature which attributes the quasar's previously observed brightness fluctuations to microlensing.

Key words: gravitational lensing -- quasars: individual: Q2237+0305 -- methods: observational

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© ESO 2006

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