4.7 Article

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

期刊

出版社

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stw3006

关键词

gravitational lensing: strong; galaxies: individual: HE 0435-1223; cosmology: observations; distance scale

资金

  1. Swiss National Science Foundation
  2. Swiss National Science Foundation (SNSF)
  3. Max Planck Society through the Max Planck Research Group
  4. Ministry of Science and Technology in Taiwan [MOST-103-2112-M-001-003-MY3]
  5. EACOA Fellowship
  6. East Asia Core Observatories Association
  7. Academia Sinica Institute of Astronomy and Astrophysics
  8. National Astronomical Observatory of Japan
  9. National Astronomical Observatories of the Chinese Academy of Sciences
  10. Korea Astronomy and Space Science Institute
  11. US Department of Energy [DE-ACO2-765F00515]
  12. NSF [AST-1312329, AST-1450141]
  13. HST [GO-12889]
  14. Back to Belgium
  15. Belgian Federal Science Policy (BELSPO)
  16. fellowship of the Alexander von Humboldt Foundation
  17. DFG [Hi 1495/2-1]
  18. DFG cluster of excellence 'Origin and Structure of the Universe'
  19. Packard Foundation through a Packard Research Fellowship
  20. NWO-VICI career grant [639.043.308]
  21. NASA [NAS 5-26555]
  22. NASA through Space Telescope Science Institute [12889]
  23. [10158]
  24. [9744]
  25. [7422]
  26. STFC [ST/K004182/1] Funding Source: UKRI
  27. Science and Technology Facilities Council [ST/K004182/1] Funding Source: researchfish
  28. Direct For Mathematical & Physical Scien [1450141] Funding Source: National Science Foundation
  29. Direct For Mathematical & Physical Scien
  30. Division Of Astronomical Sciences [1312329] Funding Source: National Science Foundation
  31. Division Of Astronomical Sciences [1450141] Funding Source: National Science Foundation

向作者/读者索取更多资源

We present a new measurement of the Hubble Constant H-0 and other cosmological parameters based on the joint analysis of three multiply imaged quasar systems with measured gravitational time delays. First, we measure the time delay of HE 0435-1223 from 13-yr light curves obtained as part of the COSMOGRAIL project. Companion papers detail the modelling of the main deflectors and line-of-sight effects, and how these data are combined to determine the time-delay distance of HE 0435-1223. Crucially, the measurements are carried out blindly with respect to cosmological parameters in order to avoid confirmation bias. We then combine the time-delay distance of HE 0435-1223 with previous measurements from systems B1608+656 and RXJ1131-1231 to create a Time Delay Strong Lensing probe (IDSL). In flat A cold dark matter (ACDM) with free matter and energy density, we find H-0 = 71.9(-3.0)(+2.4) km s(-1) Mpc(-1) and Omega(Lambda) = 0.62(-0.35)(+0.24) This measurement is completely independent of, and in agreement with, the local distance ladder measurements of H-0. We explore more general cosmological models combining TDSL with other probes, illustrating its power to break degeneracies inherent to other methods. The joint constraints from IDSL and Planck are H-0 = 69.2(-2.2)(+1.4) km s(-1) Mpc(-1), Omega(Lambda) = 0.70(-0.01)(+0.01) and Omega(k) = 0.003(-0.006)(+0.004) in open ACDM and H-0 = 79.0(-4.2)(+4.4) km s(-1) Mpc(-1), Omega(de) = 0.77(-0.03)(+0.02) and w = -1.38(-0.16)(+0.14) in flat wCDM. In combination with Planck and baryon acoustic oscillation data, when relaxing the constraints on the numbers of relativistic species we find N-eff = 3.34(-0.21)(+0.21) in N-eff Lambda CDM and when relaxing the total mass of neutrinos we find Sigma rn(nu) <= 0.182 eV in m(nu) Lambda CDM. Finally, in an open wCDM in combination with Planck and cosmic microwave background lensing, we find H-0 = 77.9(-4.2)(+5.0) km s(-1) Mpc(-1), Omega(de) = 0.77(-0.03)(+0.03), Omega(k) = -0.003(-0.004)(+0.004) and w = -1.37(-0.23)(+0.18).

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