Time delays in PG1115+080: new estimates
Abstract
We report new estimates of the time delays in the quadruple gravitationally lensed quasar PG1115+080, obtained from the monitoring data in filter R with the 1.5-m telescope at the Maidanak Mountain (Uzbekistan, Central Asia) in 2004-2006. The time delays are 16.4 days between images C and B, and 12 days between C and A1+A2, with image C being leading for both pairs. The only known estimates of the time delays in PG1115 are those based on observations by Schechter et al. (1997) -- 23.7 and 9.4 days between images C and B, C and A1+A2, respectively, as calculated by Schechter et al., and 25 and 13.3 days as revised by Barkana (1997) for the same image components with the use of another method. The new values of time delays in PG 1115+080 may be expected to provide larger estimates of the Hubble constant thus decreasing a diversity between the H_0 estimates taken from gravitationally lensed quasars and with other methods.
Cite
@article{arxiv.0910.1260,
title = {Time delays in PG1115+080: new estimates},
author = {V. G. Vakulik and V. M. Shulga and R. E. Schild and V. S. Tsvetkova and V. N. Dudinov and A. A. Minakov and S. N. Nuritdinov and B. P. Artamonov and A. Ye. Kochetov and G. V. Smirnov and A. A. Sergeyev and V. V. Konichek and I. Ye. Sinelnikov and V. V. Bruevich and T. Akhunov and O. Burkhonov},
journal= {arXiv preprint arXiv:0910.1260},
year = {2015}
}
Comments
5 pages, 2 figures, Accepted for publication in MNRAS Letters