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emcee : The MCMC Hammer
- Foreman-Mackey, Daniel; Hogg, David W.; Lang, Dustin
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Publications of the Astronomical Society of the Pacific, Vol. 125, Issue 925
https://doi.org/10.1086/670067
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PURELY DRY MERGERS DO NOT EXPLAIN THE OBSERVED EVOLUTION OF MASSIVE EARLY-TYPE GALAXIES SINCE z ∼ 1
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In the realm of the Hubble tension—a review of solutions *
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Dark Matter Contraction and the Stellar Content of Massive Early-Type Galaxies: Disfavoring “Light” Initial mass Functions
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Dark matter haloes of massive elliptical galaxies at z ∼ 0.2 are well described by the Navarro–Frenk–White profile
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Automated galaxy–galaxy strong lens modelling: No lens left behind
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Beyond the bulge–halo conspiracy? Density profiles of early-type galaxies from extended-source strong lensing
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The bulge–halo conspiracy in massive elliptical galaxies: implications for the stellar initial mass function and halo response to baryonic processes
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Is every strong lens model unhappy in its own way? Uniform modelling of a sample of 13 quadruply+ imaged quasars
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H0LiCOW – IX. Cosmographic analysis of the doubly imaged quasar SDSS 1206+4332 and a new measurement of the Hubble constant
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Astrometric requirements for strong lensing time-delay cosmography
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Early-type galaxy density profiles from IllustrisTNG – II. Evolutionary trend of the total density profile
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H0LiCOW – XIII. A 2.4 per cent measurement of H0 from lensed quasars: 5.3σ tension between early- and late-Universe probes
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Early-type galaxy density profiles from IllustrisTNG – I. Galaxy correlations and the impact of baryons
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lenstronomy II: A gravitational lensing software ecosystem
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Finding Strong Gravitational Lenses in the DESI DECam Legacy Survey
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Gravitational Lensing Formalism in a Curved Arc Basis: A Continuous Description of Observables and Degeneracies from the Weak to the Strong Lensing Regime
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The Hubble Constant from Strongly Lensed Supernovae with Standardizable Magnifications
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Identification of Galaxy–Galaxy Strong Lens Candidates in the DECam Local Volume Exploration Survey Using Machine Learning
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An Extended Catalog of Galaxy–Galaxy Strong Gravitational Lenses Discovered in DES Using Convolutional Neural Networks
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Could Quasar Lensing Time Delays Hint to a Core Component in Halos, Instead of H 0 Tension?
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A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km s−1 Mpc−1 Uncertainty from the Hubble Space Telescope and the SH0ES Team
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New Strong Gravitational Lenses from the DESI Legacy Imaging Surveys Data Release 9
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text
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Strong Lensing by Galaxies
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Strong gravitational lensing's 'external shear' is not shear
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TDCOSMO XV: Population Analysis of Lines of Sight of 25 Strong Galaxy-Galaxy Lenses with Extreme Value Statistics
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text
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January 2024 |