A SHARP view of H0LiCOW: H0 from three time-delay gravitational lens systems with adaptive optics imaging

被引：146

作者：

Chen, Geoff C. -F. ^{[1
]}

Fassnacht, Christopher D. ^{[1
]}

Suyu, Sherry H. ^{[2
,3
,4
]}

Rusu, Cristian E. ^{[5
,6
]}

Chan, James H. H. ^{[7
]}

Wong, Kenneth C. ^{[5
,8
]}

Auger, Matthew W. ^{[9
,10
]}

Hilbert, Stefan ^{[11
,12
]}

Bonvin, Vivien ^{[7
]}

Birrer, Simon ^{[13
]}

Millon, Martin ^{[7
]}

Koopmans, Leon V. E. ^{[14
]}

Lagattuta, David J. ^{[15
]}

McKean, John P. ^{[14
,16
]}

Vegetti, Simona ^{[2
]}

Courbin, Frederic ^{[7
]}

Ding, Xuheng ^{[13
]}

Halkola, Aleksi ^{[17
]}

Jee, Inh ^{[2
]}

Shajib, Anowar J. ^{[13
]}

Sluse, Dominique ^{[18
]}

Sonnenfeld, Alessandro ^{[8
,19
]}

Treu, Tommaso ^{[13
]}

机构：

[1] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA

[2] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85740 Garching, Germany

[3] Tech Univ Munich, Dept Phys, James Franck Str 1, D-85748 Garching, Germany

[4] Acad Sinica, Inst Astron & Astrophys, 11F ASMAB,1,Sect 4,Roosevelt Rd, Taipei 10617, Taiwan

[5] Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan

[6] Natl Astron Observ Japan, Subaru Telescope, 650 N Aohoku Pl, Hilo, HI 96720 USA

[7] Ecole Polytech Fed Lausanne, Inst Phys, Astrophys Lab, Observ Sauverny, CH-1290 Versoix, Switzerland

[8] Univ Tokyo, WPI, Kavli Inst Phys & Math Universe Kavli IPMU, Chiba 2778583, Japan

[9] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England

[10] Univ Cambridge, Kavli Inst Cosmol, Madingley Rd, Cambridge CB3 0HA, England

[11] Exzellenzcluster Universe, Boltzmannstr 2, D-85748 Garching, Germany

[12] Ludwig Maximilians Univ Munchen, Univ Sternwarte, Scheinerstr 1, D-81679 Munich, Germany

[13] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA

[14] Univ Groningen, Kapteyn Astron Inst, POB 800, NL-9700 AV Groningen, Netherlands

[15] Univ Lyon 1, Univ Lyon, Ctr Rech Astrophys Lyon, Ens Lyon,CNRS,UMR5574, F-69230 St Genis Laval, France

[16] Netherlands Inst Radio Astron, ASTRON, POB 2, Dwingeloo, Netherlands

[17] Pyorrekuja 5 A, FI-04300 Tuusula, Finland

[18] STAR Inst, Quartier Agora Allee Six Aout 19c, B-4000 Liege, Belgium

[19] Leiden Univ, Leiden Observ, Niels Bohrweg 2, NL-2333 CA Leiden, Netherlands

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2019年 / 490卷 / 02期

基金：

美国国家科学基金会; 美国国家航空航天局; 瑞士国家科学基金会; 欧洲研究理事会; 加拿大自然科学与工程研究理事会;

关键词：

gravitational lensing: strong; instrumentation: adaptive optics; distance scale; EARLY-TYPE GALAXIES; BARYON ACOUSTIC-OSCILLATIONS; EDGE-ON DISC; DARK-MATTER; HUBBLE CONSTANT; SPECTROSCOPIC SURVEY; DATA RELEASE; PHOTOMETRIC REDSHIFTS; MASS STRUCTURE; EINSTEIN RING;

D O I：

10.1093/mnras/stz2547

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the measurement of the Hubble constant, H-0, with three strong gravitational lens systems, We describe a blind analysis of both PG 1115+080 and 11E0435-1223 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 Ho. 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-0 = 82.8(-8.3)(+9.4) km s(-1) Mpc(-1) for PG 1115+080, H-0 = 70.1(-4.5)(+5.3) km s(-1) Mpc(-1) for HE 0435-1223, and H-0 = 77.0(-4.6)(+4.0) km s(-1) Mpc(-1) for RXJ 1131-1231. The joint AO-only result for the three lenses is H-0 = 75.6(-3.3)(+3.2) km s(-1) Mpc(-1). The joint result of the AO + HST analysis for the three lenses is H-0 = 76.8(-2.6)(+2.6) km s(-1) Mpc(-1). All of these results assume a flat A cold dark matter cosmology with a uniform prior on Omega(m) in [0.05, 0.5] and H-0 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-0. The full time-delay cosmography results from a total of six strongly lensed systems are presented in a companion paper.

引用

页码：1743 / 1773

页数：31

共 27 条

[21] H0LiCOW-V. New COSMOGRAIL time delays of HE 0435-1223: H0 to 3.8 per cent precision from strong lensing in a flat ΛCDM model
Bonvin, V.
Courbin, F.
Suyu, S. H.
Marshall, P. J.
Rusu, C. E.
Sluse, D.
Tewes, M.
Wong, K. C.
Collett, T.
Fassnacht, C. D.
Treu, T.
Auger, M. W.
Hilbert, S.
Koopmans, L. V. E.
Meylan, G.
Rumbaugh, N.
Sonnenfeld, A.
Spiniello, C.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2017, 465 (04) : 4914 - 4930
[22] H0LiCOW-X. Spectroscopic/imaging survey and galaxy-group identification around the strong gravitational lens system WFI 2033-4723
Sluse, D.
Rusu, C. E.
Fassnacht, C. D.
Sonnenfeld, A.
Richard, J.
Auger, M. W.
Coccato, L.
Wong, K. C.
Suyu, S. H.
Treu, T.
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Birrer, S.
Bonvin, V
Collett, T.
Courbin, F.
Hilbert, S.
Koopmans, L. V. E.
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Marshall, P. J.
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Shajib, A. J.
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James, D. J.
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Krause, E.
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MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2019, 490 (01) : 613 - 633
[23] SHARP - VIII. J0924+0219 lens mass distribution and time-delay prediction through adaptive-optics imaging
Chen, Geoff C-F
Fassnacht, Christopher D.
Suyu, Sherry H.
Koopmans, Leon V. E.
Lagattuta, David J.
McKean, John P.
Auger, Matt W.
Vegetti, Simona
Treu, Tommaso
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2022, 513 (02) : 2349 - 2359
[24] A determination of H0 with the class gravitational lens B1608+656.: II.: Mass models and the Hubble constant from lensing
Koopmans, LVE
Fassnacht, CD
ASTROPHYSICAL JOURNAL, 1999, 527 (02): : 513 - 524
[25] Quasi-finite-rank approximation of compression operators on L∞[0, h) with application to stability analysis of time-delay systems
Kim, Jung Hoon
Hagiwara, Tomomichi
IET CONTROL THEORY AND APPLICATIONS, 2014, 8 (02): : 77 - 85
[26] A new quasi-finite-rank approximation of compression operators on L∞ [0 , H ) with applications to sampled-data and time-delay systems: Piecewise linear kernel approximation approach
Kwak, Dohyeok
Kim, Jung Hoon
Hagiwara, Tomomichi
JOURNAL OF THE FRANKLIN INSTITUTE-ENGINEERING AND APPLIED MATHEMATICS, 2024, 361 (18):
[27] Inverse distance ladder method for determining H0\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$H_0$$\end{document} from angular diameter distances of time-delay lenses and supernova observations
Xiaolong Gong
Tonghua Liu
Jieci Wang
The European Physical Journal C, 84 (8):

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