H0LiCOW IV. Lens mass model of HE 0435-1223 and blind measurement of its time-delay distance for cosmology
Kenneth C. Wong, Sherry H. Suyu, Matthew W. Auger, Vivien Bonvin,, Frederic Courbin, Christopher D. Fassnacht, Aleksi Halkola, Cristian E. Rusu,, Dominique Sluse, Alessandro Sonnenfeld, Tommaso Treu, Thomas E. Collett,, Stefan Hilbert, Leon V. E. Koopmans, Philip J. Marshall

TL;DR
This paper presents a detailed, blind gravitational lens modeling of HE 0435-1223, measuring its time-delay distance and estimating the Hubble constant with high precision, contributing to cosmological parameter determination.
Contribution
It provides the first blind lens model analysis of HE 0435-1223, incorporating comprehensive systematics and updated measurements, advancing the use of gravitational lenses for cosmology.
Findings
Effective time-delay distance constrained to 2612 Mpc with 7.6% precision
Hubble constant estimated at 73.1 km/s/Mpc with ~8% uncertainty
Systematic uncertainties carefully accounted for in the lens modeling
Abstract
Strong gravitational lenses with measured time delays between the multiple images allow a direct measurement of the time-delay distance to the lens, and thus a measure of cosmological parameters, particularly the Hubble constant, . We present a blind lens model analysis of the quadruply-imaged quasar lens HE 0435-1223 using deep Hubble Space Telescope imaging, updated time-delay measurements from the COSmological MOnitoring of GRAvItational Lenses (COSMOGRAIL), a measurement of the velocity dispersion of the lens galaxy based on Keck data, and a characterization of the mass distribution along the line of sight. HE 0435-1223 is the third lens analyzed as a part of the Lenses in COSMOGRAIL's Wellspring (H0LiCOW) project. We account for various sources of systematic uncertainty, including the detailed treatment of nearby perturbers, the parameterization of the galaxy light…
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