activity
20132026
most citedDISPATCH: A Numerical Simulation Framework for the Exa-scale Era. I. Fundamentals

35 citations · 44 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2026

Angular Momentum of Planet-Forming Disks: Implications for Infall Driven Misalignments

Aashish Gupta, Cristiano Longarini, L. Ilsedore Cleeves +5

Context. A significant fraction (>30%) of planet-forming disks and planetary are misaligned with respect to the rotational axis of their host stars, yet the dominant mechanism resp…

astro-ph.EP2024★ 2 cited

OGLE-2015-BLG-1609Lb: Sub-jovian planet orbiting a low-mass stellar or brown dwarf host

M. J. Mróz, R. Poleski, A. Udalski +70

We present a comprehensive analysis of a planetary microlensing event OGLE-2015-BLG-1609. The planetary anomaly was detected by two survey telescopes, OGLE and MOA. Each of these s…

astro-ph.EP2019★ 6 cited

An analysis of binary microlensing event OGLE-2015-BLG-0060

Y. Tsapras, A. Cassan, C. Ranc +83

We present the analysis of stellar binary microlensing event OGLE-2015-BLG-0060 based on observations obtained from 13 different telescopes. Intensive coverage of the anomalous par…

astro-ph.GA2017★ 1 cited

Accounting for the diversity in stellar environments

Michael Küffmeier, Troels Haugbølle, Åke Nordlund

Stars and their corresponding protoplanetary disks form in diverse environments. To account for these natural variations, we investigate the formation process around nine solar mas…

astro-ph.IM2017★ 35 cited

DISPATCH: A Numerical Simulation Framework for the Exa-scale Era. I. Fundamentals

Å. Nordlund, J. P. Ramsey, A. Popovas +1

We introduce a high-performance simulation framework that permits the semi-independent, task-based solution of sets of partial differential equations, typically manifesting as upda…

astro-ph.SR2013

Zooming in on the Formation of Protoplanetary Disks

A. Nordlund, T. Haugboelle, M. Kuffmeier +2

We use the adaptive mesh refinement code RAMSES to model the formation of protoplanetary disks in realistic star formation environments. The resolution scales over up to 29 powers…