output
20062025
most citedSMILEI: a collaborative, open-source, multi-purpose particle-in-cell code for plasma simulation

580 citations

Showing astro-ph.SRShow all

20 papers · 1 filter

astro-ph.SR2024★ 42 cited

The JWST Weather Report from the Nearest Brown Dwarfs I: multi-period JWST NIRSpec + MIRI monitoring of the benchmark binary brown dwarf WISE 1049AB

Beth A. Biller, Johanna M. Vos, Yifan Zhou +22

We report results from 8 hours of JWST/MIRI LRS spectroscopic monitoring directly followed by 7 hours of JWST/NIRSpec prism spectroscopic monitoring of the benchmark binary brown d…

astro-ph.SR2023★ 40 cited

Exploring the Extremes: Characterizing a New Population of Old and Cold Brown Dwarfs

A. M. Meisner, S. K. Leggett, S. E. Logsdon +3

Mapping out the populations of thick disk and halo brown dwarfs is important for understanding the metallicity dependence of low-temperature atmospheres and the substellar mass fun…

astro-ph.SR2020★ 29 cited

Rotational spectral modulation of cloudless atmospheres for L/T Brown Dwarfs and Extrasolar Giant Planets

P. Tremblin, M. W. Phillips, A. Emery +5

The rotational spectral modulation (spectro-photometric variability) of brown dwarfs is usually interpreted as a sign of the presence of inhomogeneous cloud covers in the atmospher…

astro-ph.SR2020★ 319 cited

A new set of atmosphere and evolution models for cool T-Y brown dwarfs and giant exoplanets

Mark W. Phillips, Pascal Tremblin, Isabelle Baraffe +6

We present a new set of solar metallicity atmosphere and evolutionary models for very cool brown dwarfs and self-luminous giant exoplanets, which we term ATMO 2020. Atmosphere mode…

astro-ph.SR2019★ 45 cited

WISE J072003.20-084651.2B Is A Massive T Dwarf

Trent J. Dupuy, Michael C. Liu, William M. J. Best +21

We present individual dynamical masses for the nearby M9.5+T5.5 binary WISE J072003.20084651.2AB, a.k.a. Scholz's star. Combining high-precision CFHT/WIRCam photocenter astromet…

astro-ph.SR2019★ 12 cited

3D MHD simulations and synthetic radio emission from an oblique rotating magnetic massive star

Simon Daley-Yates, Ian R. Stevens, Asif ud-Doula

We have performed 3D isothermal MHD simulation of a magnetic rotating massive star with a non-zero dipole obliquity and predicted the radio/sub-mm observable lightcurves and contin…