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20162026
most citedDetection of stellar light from quasar host galaxies at redshifts above 6

127 citations · 1.2k across the 49 of their papers we have counts for

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Showing 2022Show all

12 papers · 1 filter

astro-ph.GA2022★ 10 cited

Dynamical evolution of massive black hole pairs in the presence of spin-dependent radiative feedback

Francesco Bollati, Alessandro Lupi, Massimo Dotti +1

The putative ubiquity of massive black holes (MBH) at the center of galaxies, and the hierarchical progress of structure formation along the cosmic history, together necessarily im…

astro-ph.SR2022★ 5 cited

Non-ideal magnetohydrodynamics of self-gravitating filaments

Nicol Gutiérrez-Vera, Tommaso Grassi, Stefano Bovino +3

Filaments have been studied in detail through observations and simulations. A range of numerical works have separately investigated how chemistry and diffusion effects, as well as…

astro-ph.GA2022★ 127 cited

Detection of stellar light from quasar host galaxies at redshifts above 6

Xuheng Ding, Masafusa Onoue, John D. Silverman +41

The detection of starlight from the host galaxies of quasars during the reionization epoch () has been elusive, even with deep HST observations. The current highest redshift q…

gr-qc2022★ 3 cited

A general relativistic extension to mesh-free methods for hydrodynamics

Alessandro Lupi

The detection of gravitational waves has opened a new era for astronomy, allowing for the combined use of gravitational wave and electromagnetic emissions to directly probe the phy…

astro-ph.GA2022★ 50 cited

Morphological decomposition of TNG50 galaxies: methodology and catalogue

Tommaso Zana, Alessandro Lupi, Matteo Bonetti +6

We present MORDOR (MORphological DecOmposeR, a new algorithm for structural decomposition of simulated galaxies based on stellar kinematics. The code measures the properties of up…

astro-ph.GA2022★ 38 cited

Sub-parsec resolution cosmological simulations of star-forming clumps at high redshift with feedback of individual stars

F. Calura, A. Lupi, J. Rosdahl +7

We introduce a new set of zoom-in cosmological simulations with sub-pc resolution, intended to model extremely faint, highly magnified star-forming stellar clumps, detected at z=6.…