A Robust Determination of the Time Delay in 0957+561A, B and a Measurement of the Global Value of Hubble's Constant

Abstract

Photometric monitoring of the gravitational lens system 0957+561A,B in the g\nand r bands with the Apache Point Observatory (APO) 3.5 m telescope during 1996\nshows a sharp g band event in the trailing (B) image light curve at the precise\ntime predicted from the observation of an event during 1995 in the leading (A)\nimage with a delay of 415 days. This success confirms the "short delay," and\nthe lack of any feature at a delay near 540 days rejects the "long delay" for\nthis system, resolving a long-standing controversy. A series of statistical\nanalyses of our light curve data yield a best fit delay of 417 +/- 3 days (95%\nconfidence interval). Recent improvements in the modeling of the lens system\n(consisting of a galaxy and cluster) allow us to derive a value of the global\n(at z = 0.36) value of Hubble's constant H_0 using Refsdal's method, a simple\nand direct distance determination based on securely understood physics and\ngeometry. The result is H_0 = 63 +/- 12 km/s/Mpc (for Omega = 1) where this 95%\nconfidence interval is dominated by remaining lens model uncertainties.\n