H0LiCOW VIII. A weak-lensing measurement of the external convergence in the field of the lensed quasar HE 0435–1223

Tihhonova, O.; Courbin, F.; Harvey, D.; Hilbert, S.; Rusu, C. E.; Fassnacht, C. D.; Bonvin, V.; Marshall, P. J.; Meylan, G.; Sluse, D.; Suyu, S. H.; Treu, T.; Wong, K. C.

doi:10.1093/mnras/sty1040

H0LiCOW VIII. A weak-lensing measurement of the external convergence in the field of the lensed quasar HE 0435–1223

Journal Article · Thu Apr 26 04:00:00 EDT 2018 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/sty1040· OSTI ID:1461883

Tihhonova, O. ^[1]; Courbin, F. ^[1]; Harvey, D. ^[1]; Hilbert, S. ^[2]; Rusu, C. E. ^[3]; Fassnacht, C. D. ^[4]; Bonvin, V. ^[1]; Marshall, P. J. ^[5]; Meylan, G. ^[1]; Sluse, D. ^[6]; Suyu, S. H. ^[7]; Treu, T. ^[8]; Wong, K. C. ^[9]

Ecole Polytechnique Federale Lausanne (Switzlerland). Lab. d'Astrophysique
Exzellenzcluster Universe, Garching (Germany); Ludwig-Maximilians-Univ., Munchen (Germany)
Univ. of California, Davis, CA (United States). Dept. of Physics; Subaru Telescope, Hilo, HI (United States)
Univ. of California, Davis, CA (United States). Dept. of Physics
Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology
STAR Inst., Liege (Belgium)
Max Planck Society, Garching (Germany). Max Planck Inst. for Astrophysik; Academia Sinica, Taipei (Taiwan). Inst.of Astronomy and Astrophysics; Technische Univ. at Munchen, Garching (Germany)
Univ. of California, Los Angeles, CA (United States). Dept. of Physics and Astronomy
National Astronomical Observatory of Japan, Tokyo (Japan)

We present a weak gravitational lensing measurement of the external convergence along the line of sight to the quadruply lensed quasar HE 0435–1223. Using deep r-band images from Subaru Suprime Cam, we observe galaxies down to a 3σ limiting magnitude of ~26 mag resulting in a source galaxy density of 14 galaxies per square arcminute after redshift-based cuts. Using an inpainting technique and multiscale entropy filtering algorithm, we find that the region in close proximity to the lens has an estimated external convergence of κ = -0.012$$+0.020\atop{-0.013}$$ and is hence marginally under-dense. We also rule out the presence of any halo with a mass greater than M_vir = 1.6 × 10¹⁴h^-1M_⊙ (68 percent confidence limit). Our results, consistent with previous studies of this lens, confirm that the intervening mass along the line of sight to HE 0435–1223 does not affect significantly the cosmological results inferred from the time-delay measurements of that specific object

View Accepted Manuscript (DOE)

Research Organization:: SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)

Sponsoring Organization:: USDOE; National Science Foundation (NSF)

Grant/Contract Number:: AC02-76SF00515

OSTI ID:: 1461883

Journal Information:: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 4 Vol. 477; ISSN 0035-8711

Publisher:: Royal Astronomical SocietyCopyright Statement

Country of Publication:: United States

Language:: English

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Model-Independent Determination of H 0 and Ω K 0 from Strong Lensing and Type Ia Supernovae Collett, Thomas; Montanari, Francesco; Räsänen, Syksy Physical Review Letters, Vol. 123, Issue 23 https://doi.org/10.1103/physrevlett.123.231101	journal	December 2019
Constraining the microlensing effect on time delays with new time-delay prediction model in $H_{0}$ measurements Chen, Geoff C. -F.; Chan, James H. H.; Bonvin, Vivien arXiv https://doi.org/10.48550/arxiv.1804.09390	text	January 2018
Impact of the 3D source geometry on time-delay measurements of lensed type-Ia Supernovae Bonvin, V.; Tihhonova, O.; Millon, M. arXiv https://doi.org/10.48550/arxiv.1805.04525	text	January 2018
Is every strong lens model unhappy in its own way? Uniform modelling of a sample of 13 quadruply+ imaged quasars Shajib, A. J.; Birrer, S.; Treu, T. arXiv https://doi.org/10.48550/arxiv.1807.09278	text	January 2018
H0LiCOW - IX. Cosmographic analysis of the doubly imaged quasar SDSS 1206+4332 and a new measurement of the Hubble constant Birrer, S.; Treu, T.; Rusu, C. E. arXiv https://doi.org/10.48550/arxiv.1809.01274	text	January 2018
Generalised model-independent characterisation of strong gravitational lenses VI: the origin of the formalism intrinsic degeneracies and their influence on $H_0$ Wagner, Jenny arXiv https://doi.org/10.48550/arxiv.1904.07239	text	January 2019
COSMOGRAIL XVIII: time delays of the quadruply lensed quasar WFI2033-4723 Bonvin, V.; Millon, M.; Chan, J. H. H. arXiv https://doi.org/10.48550/arxiv.1905.08260	text	January 2019
A SHARP view of H0LiCOW: $H_{0}$ from three time-delay gravitational lens systems with adaptive optics imaging Chen, Geoff C. -F.; Fassnacht, Christopher D.; Suyu, Sherry. H. arXiv https://doi.org/10.48550/arxiv.1907.02533	text	January 2019

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