activity
20072025
most citedThe Hyper Suprime-Cam SSP Survey: Overview and Survey Design

1.1k citations · 3.4k across the 31 of their papers we have counts for

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Showing astro-ph.COShow all

14 papers · 1 filter

astro-ph.CO2025★ 1 cited

HOLISMOKES XIX: SN 2025wny at , the first strongly lensed superluminous supernova

Stefan Taubenberger, Ana Acebron, Raoul Cañameras +45

We present imaging and spectroscopic observations of supernova SN 2025wny, associated with the lens candidate PS1 J0716+3821. Photometric monitoring from the Lulin and Maidanak obs…

astro-ph.CO2025★ 38 cited

TDCOSMO 2025: Cosmological constraints from strong lensing time delays

TDCOSMO Collaboration, Simon Birrer, Elizabeth J. Buckley-Geer +30

We present cosmological constraints from 8 strongly lensed quasars (hereafter, the TDCOSMO-2025 sample). Building on previous work, our analysis incorporated new deflector stellar…

astro-ph.CO2024★ 18 cited

TDCOSMO. XVI. Measurement of the Hubble Constant from the Lensed Quasar WGD20384008

Kenneth C. Wong, Frédéric Dux, Anowar J. Shajib +17

Time-delay cosmography is a powerful technique to constrain cosmological parameters, particularly the Hubble constant (). The TDCOSMO collaboration is performing an ongoing…

astro-ph.CO2022★ 45 cited

TDCOSMO. IX. Systematic comparison between lens modelling software programs: time delay prediction for WGD 2038-4008

A. J. Shajib, K. C. Wong, S. Birrer +15

The importance of alternative methods for measuring the Hubble constant, such as time-delay cosmography, is highlighted by the recent Hubble tension. It is paramount to thoroughly…

astro-ph.CO2019★ 231 cited

TDCOSMO. I. An exploration of systematic uncertainties in the inference of from time-delay cosmography

M. Millon, A. Galan, F. Courbin +22

Time-delay cosmography of lensed quasars has achieved 2.4% precision on the measurement of the Hubble constant, . As part of an ongoing effort to uncover and control systemati…

astro-ph.CO2019★ 240 cited

STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408-5354

A. J. Shajib, S. Birrer, T. Treu +88

We present a blind time-delay cosmographic analysis for the lens system DES J04085354. This system is extraordinary for the presence of two sets of multiple images at different…

astro-ph.CO2019★ 98 cited

Cosmic dissonance: new physics or systematics behind a short sound horizon?

Nikki Arendse, Radosław J. Wojtak, Adriano Agnello +12

Persistent tension between low-redshift observations and the Cosmic Microwave Background radiation (CMB), in terms of two fundamental distance scales set by the sound horizon …

astro-ph.CO2019★ 50 cited

COSMOGRAIL XVIII: time delays of the quadruply lensed quasar WFI2033-4723

V. Bonvin, M. Millon, J. H. H. Chan +26

We present new measurements of the time delays of WFI2033-4723. The data sets used in this work include 14 years of data taken at the 1.2m Leonhard Euler Swiss telescope, 13 years…

astro-ph.CO2019★ 55 cited

The Hubble Constant determined through an inverse distance ladder including quasar time delays and Type Ia supernovae

S. Taubenberger, S. H. Suyu, E. Komatsu +7

Context. The precise determination of the present-day expansion rate of the Universe, expressed through the Hubble constant , is one of the most pressing challenges in modern…

astro-ph.CO2017★ 56 cited

H0LiCOW VIII. A weak lensing measurement of the external convergence in the field of the lensed quasar HE04351223

O. Tihhonova, F. Courbin, D. Harvey +10

We present a weak gravitational lensing measurement of the external convergence along the line of sight to the quadruply lensed quasar HE04351223. Using deep r-band images f…

astro-ph.CO2016★ 469 cited

H0LiCOW V. New COSMOGRAIL time delays of HE0435-1223: to 3.8% precision from strong lensing in a flat CDM model

V. Bonvin, F. Courbin, S. H. Suyu +15

We present a new measurement of the Hubble Constant H0 and other cosmological parameters based on the joint analysis of three multiply-imaged quasar systems with measured gravitati…

astro-ph.CO2016★ 62 cited

H0LiCOW II. Spectroscopic survey and galaxy-group identification of the strong gravitational lens system HE0435-1223

D. Sluse, A. Sonnenfeld, N. Rumbaugh +15

Galaxies located in the environment or on the line of sight towards gravitational lenses can significantly affect lensing observables, and can lead to systematic errors on the meas…

astro-ph.CO2016★ 354 cited

H0LiCOW I. Lenses in COSMOGRAIL's Wellspring: Program Overview

S. H. Suyu, V. Bonvin, F. Courbin +21

Strong gravitational lens systems with time delays between the multiple images allow measurements of time-delay distances, which are primarily sensitive to the Hubble constant that…

astro-ph.CO2009★ 62 cited

Galaxy Number Counts and Implications for Strong Lensing

C. D. Fassnacht, L. V. E. Koopmans, K. C. Wong

We compare galaxy number counts in HST/ACS fields containing moderate-redshift (0.2<z<1.0) strong gravitational lenses with those in two control samples: (1) the first square degre…