activity
20182022
most citedPyAutoLens: Open-Source Strong Gravitational Lensing

91 citations · 455 across the 15 of their papers we have counts for

collaborators

18 papers

astro-ph.GA20229 cited

The far-infrared/radio correlation for a sample of strongly lensed dusty star-forming galaxies detected by Herschel

M. Giulietti, M. Massardi, A. Lapi +6

We investigate the radio-far infrared (FIR) correlation for a sample of bright high-redshift () star-forming galaxies selected in the FIR from the Her…

astro-ph.CO202252 cited

A new estimate of the cosmic star formation density from a radio-selected sample, and the contribution of -dark galaxies at

A. Enia, M. Talia, F. Pozzi +13

The Star Formation Rate Density (SFRD) history of the Universe is well constrained up to redshift . At earlier cosmic epochs, the picture has been largely inferred from U…

astro-ph.GA202232 cited

The Bright Extragalactic ALMA Redshift Survey (BEARS) I: redshifts of bright gravitationally-lensed galaxies from the Herschel ATLAS

S. A. Urquhart, G. J. Bendo, S. Serjeant +53

We present spectroscopic measurements for 71 galaxies associated with 62 of the brightest high-redshift submillimeter sources from the Southern fields of the Herschel Astrophysical…

astro-ph.GA202159 cited

The ALPINE-ALMA [CII] survey: The contribution of major mergers to the galaxy mass assembly at z~5

M. Romano, P. Cassata, L. Morselli +25

Galaxy mergers are thought to be one of the main mechanisms of the mass assembly of galaxies. Recently, many works have suggested a possible increase in the fraction of major merge…

astro-ph.IM202191 cited

PyAutoLens: Open-Source Strong Gravitational Lensing

James. W. Nightingale, Richard G. Hayes, Ashley Kelly +14

Strong gravitational lensing, which can make a background source galaxy appears multiple times due to its light rays being deflected by the mass of one or more foreground lens gala…

astro-ph.GA202143 cited

The ALPINE-ALMA [CII] survey: Dust mass budget in the early Universe

F. Pozzi, F. Calura, Y. Fudamoto +32

The dust content of normal galaxies and the dust mass density (DMD) at high-z (z>4) are unconstrained given the source confusion and the sensitivity limitations of previous observa…