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20152026
most citedH0LiCOW V. New COSMOGRAIL time delays of HE0435-1223: to 3.8% precision from strong lensing in a flat CDM model

469 citations · 1k across the 31 of their papers we have counts for

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Showing 2021Show all

8 papers · 1 filter

astro-ph.GA2021

The effect of spiral arms on the Sérsic photometry of galaxies

Alessandro Sonnenfeld

Context. The Sérsic profile is a widely-used model to describe the surface brightness distribution of galaxies. Spiral galaxies, however, are qualitatively different from a Sérsic…

astro-ph.GA2021

GAlaxy Light profile convolutional neural NETworks (GaLNets). I. fast and accurate structural parameters for billion galaxy samples

R. Li, N. R. Napolitano, N. Roy +5

Next generation large sky surveys will observe up to billions of galaxies for which basic structural parameters are needed to study their evolution. This is a challenging task that…

astro-ph.GA2021

The dark matter halo masses of elliptical galaxies as a function of observationally robust quantities

Alessandro Sonnenfeld, Crescenzo Tortora, Henk Hoekstra +9

Context. The assembly history of the stellar component of a massive elliptical galaxy is closely related to that of its dark matter halo. Measuring how the properties of galaxies c…

astro-ph.GA2021

Statistical strong lensing. IV. Inferences with no individual source redshifts

Alessandro Sonnenfeld

Context. Strong lensing mass measurements require the knowledge of the redshift of both the lens and the source galaxy. Traditionally, spectroscopic redshifts are used for this pur…

astro-ph.GA2021

Statistical strong lensing. III. Inferences with complete samples of lenses

Alessandro Sonnenfeld

Context. Existing samples of strong lenses have been assembled by giving priority to sample size, at the cost of having a complex selection function. With the advent of the next ge…

astro-ph.CO2021

Statistical strong lensing. II. Cosmology and galaxy structure with time-delay lenses

Alessandro Sonnenfeld

Context. Time delay lensing is a powerful tool to measure the Hubble constant . In order to obtain an accurate estimate of from a sample of time delay strong lenses, how…