activity
20182022
most citedMagnetic Twists of Solar Filaments

28 citations · 45 across the 5 of their papers we have counts for

collaborators

13 papers

astro-ph.GA20221 cited

A vast population of wandering and merging IMBHs at cosmic noon

Tiziana Di Matteo, Yueying Ni, Nianyi Chen +5

Massive black holes in the centers of galaxies today must have grown by several orders of magnitude from seed black holes formed at early times. Detecting a population of intermedi…

astro-ph.CO20221 cited

Robust field-level inference with dark matter halos

Helen Shao, Francisco Villaescusa-Navarro, Pablo Villanueva-Domingo +13

We train graph neural networks on halo catalogues from Gadget N-body simulations to perform field-level likelihood-free inference of cosmological parameters. The catalogues contain…

astro-ph.GA202212 cited

Ultramassive black holes formed by triple quasar mergers at

Yueying Ni, Tiziana DiMatteo, Nianyi Chen +2

The origin of rare and elusive ultramassive black holes (UMBH, with MBH > 1e10 Msun) is an open question. Using the large volume cosmological hydrodynamic simulation ASTRID, we rep…

astro-ph.SR202128 cited

Magnetic Twists of Solar Filaments

Jinhan Guo, Yiwei Ni, Ye Qiu +3

Solar filaments are cold and dense materials situated in magnetic dips, which show distinct radiation characteristics compared to the surrounding coronal plasma. They are associate…

astro-ph.GA20213 cited

The Diversity of Environments Around Luminous Quasars at Redshift

Keven Ren, Michele Trenti, Madeline A. Marshall +2

Significant clustering around the rarest luminous quasars is a feature predicted by dark matter theory combined with number density matching arguments. However, this expectation is…

astro-ph.CO2021

AI-assisted super-resolution cosmological simulations II: Halo substructures, velocities and higher order statistics

Yueying Ni, Yin Li, Patrick Lachance +4

In this work, we expand and test the capabilities of our recently developed super-resolution (SR) model to generate high-resolution (HR) realizations of the full phase-space matter…