A measurement of the Hubble constant from angular diameter distances to two gravitational lenses

Author:

Jee Inh1ORCID,Suyu Sherry H.123ORCID,Komatsu Eiichiro14ORCID,Fassnacht Christopher D.5ORCID,Hilbert Stefan67ORCID,Koopmans Léon V. E.8ORCID

Affiliation:

1. Max-Planck-Institut für Astrophysik, 85741 Garching, Germany.

2. Institute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, No.1, Section 4, Roosevelt Road, Taipei 10617, Taiwan.

3. Physik-Department, Technische Universität München, 85748 Garching, Germany.

4. Kavli Institute for the Physics and Mathematics of the Universe, World Premier International Research Center Initiative, Todai Institutes for Advanced Study, the University of Tokyo, Kashiwa 277-8583, Japan.

5. Physics Department, University of California Davis, Davis, CA 95616, USA.

6. Exzellenzcluster Universe, 85748 Garching, Germany.

7. Ludwig-Maximilians-Universität, Universitäts-Sternwarte, 81679 München, Germany.

8. Kapteyn Astronomical Institute, University of Groningen, 9700 AV Groningen, Netherlands.

Abstract

Lensing approach to the Hubble constant The current expansion rate of the Universe is parametrized by the Hubble constant, H 0 . Different methods of measuring H 0 produce results that disagree with each other, which could be a sign of new physics or of systematic errors in the methods. Jee et al. have analyzed two gravitational lensing systems to determine their distances (see the Perspective by Davis). They use these as benchmarks for a measurement of H 0 . The precision is not sufficient to resolve the debate but does bypass some of the systematic uncertainties. Observations of more lensing systems will be required to narrow down the value of H 0 . Science , this issue p. 1134 ; see also p. 1076

Funder

National Science Foundation

Max Planck Society

German research Foundation

NWO-VICI

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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