A SHARP view of H0LiCOW: H[SUB]0[/SUB] from three time-delay gravitational lens systems with adaptive optics imaging

gravitational lensing: strong; instrumentation: adaptive optics; distance scale; Astrophysics - Cosmology and Nongalactic Astrophysics; Astrophysics - Astrophysics of Galaxies

Abstract :

[en] We present the measurement of the Hubble constant, H[SUB]0[/SUB], with three strong gravitational lens systems. We describe a blind analysis of both PG 1115+080 and HE 0435-1223 as well as an extension of our previous analysis of RXJ 1131-1231. For each lens, we combine new adaptive optics (AO) imaging from the Keck Telescope, obtained as part of the SHARP (Strong-lensing High Angular Resolution Programme) AO effort, with Hubble Space Telescope (HST) imaging, velocity dispersion measurements, and a description of the line-of-sight mass distribution to build an accurate and precise lens mass model. This mass model is then combined with the COSMOGRAIL-measured time delays in these systems to determine H[SUB]0[/SUB]. We do both an AO-only and an AO + HST analysis of the systems and find that AO and HST results are consistent. After unblinding, the AO-only analysis gives H[SUB]0[/SUB]=82.8^{+9.4}_{-8.3} km s^{-1} Mpc^{-1} for PG 1115+080, H[SUB]0[/SUB]=70.1^{+5.3}_{-4.5} km s^{-1} Mpc^{-1} for HE 0435-1223, and H[SUB]0[/SUB]=77.0^{+4.0}_{-4.6} km s^{-1} Mpc^{-1} for RXJ 1131-1231. The joint AO-only result for the three lenses is H[SUB]0[/SUB]=75.6^{+3.2}_{-3.3} km s^{-1} Mpc^{-1}. The joint result of the AO + HST analysis for the three lenses is H[SUB]0[/SUB]=76.8^{+2.6}_{-2.6} km s^{-1} Mpc^{-1}. All of these results assume a flat Λ cold dark matter cosmology with a uniform prior on Ω[SUB]m[/SUB] in [0.05, 0.5] and H[SUB]0[/SUB] in [0, 150] km s^{-1} Mpc^{-1}. This work is a collaboration of the SHARP and H0LiCOW teams, and shows that AO data can be used as the high-resolution imaging component in lens-based measurements of H[SUB]0[/SUB]. The full time- delay cosmography results from a total of six strongly lensed systems are presented in a companion paper. <P />

Disciplines :

Space science, astronomy & astrophysics

Author, co-author :

Chen, Geoff C.-F.; Department of Physics, University of California, Davis, CA 95616, USA

Fassnacht, Christopher D.; Department of Physics, University of California, Davis, CA 95616, USA

Suyu, Sherry H.; Max Planck Institute for Astrophysics, Karl-Schwarzschild-Strasse 1, D-85740 Garching, Germany ; Physik-Department, Technische Universität Müchen, James-Franck-Str 1, D-85748 Garching, Germany ; Academia Sinica Institute of Astronomy and Astrophysics (ASIAA), 11F of ASMAB, No. 1, Section 4, Roosevelt Road, Taipei 10617, Taiwan

Rusu, Cristian E.; National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan ; Subaru Telescope, National Astronomical Observatory of Japan, 650 N Aohoku Pl, Hilo, HI 96720, USA

Chan, James H. H.; Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, CH-1290 Versoix, Switzerland

Wong, Kenneth C.; National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan ; Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU, WPI), University of Tokyo, Chiba 277-8583, Japan

Auger, Matthew W.; Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK ; Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK

Hilbert, Stefan; Exzellenzcluster Universe, Boltzmannstr 2, D-85748 Garching, Germany ; Ludwig-Maximilians-Universitĺat, Universitäts-Sternwarte, Scheinerstr 1, D-81679 Munchen, Germany

Bonvin, Vivien; Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, CH-1290 Versoix, Switzerland

Birrer, Simon; Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA

More authors (13 more)

Language :

English

Title :

A SHARP view of H0LiCOW: H[SUB]0[/SUB] from three time-delay gravitational lens systems with adaptive optics imaging

Publication date :

01 December 2019

Journal title :

Monthly Notices of the Royal Astronomical Society

Volume :

490

Pages :

1743-1773

Peer reviewed :

Peer reviewed

Additional URL :

https://ui.adsabs.harvard.edu/abs/2019MNRAS.490.1743C

European Projects :

H2020 - 787886 - COSMICLENS - Cosmology with Strong Gravitational Lensing

Funders :

CE - Commission Européenne

Available on ORBi :

since 31 December 2019

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