Duality between (2+ 1) d quantum critical points

T Senthil, DT Son, C Wang, C Xu - Physics Reports, 2019 - Elsevier
Duality refers to two equivalent descriptions of the same theory from different points of view.
Recently there has been tremendous progress in formulating and understanding possible …

[HTML][HTML] Gaia Data Release 3-All-sky classification of 12.4 million variable sources into 25 classes

L Rimoldini, B Holl, P Gavras, M Audard… - Astronomy & …, 2023 - aanda.org
Context. Gaia DR3 contains 1.8 billion sources with G-band photometry, 1.5 billion of which
with G BP and G RP photometry, complemented by positions on the sky, parallax, and …

Models and simulations for the photometric LSST astronomical time series classification challenge (PLAsTiCC)

R Kessler, G Narayan, A Avelino… - Publications of the …, 2019 - iopscience.iop.org
We describe the simulated data sample for the Photometric Large Synoptic Survey
Telescope (LSST) Astronomical Time Series Classification Challenge (PLAsTiCC), a …

Flare statistics for young stars from a convolutional neural network analysis of TESS data

AD Feinstein, BT Montet, M Ansdell… - The Astronomical …, 2020 - iopscience.iop.org
All-sky photometric time-series missions have allowed for the monitoring of thousands of
young (t age< 800 Myr) stars in order to understand the evolution of stellar activity. Here, we …

Flare rates, rotation periods, and spectroscopic activity indicators of a volume-complete sample of mid-to late-M dwarfs within 15 pc

AA Medina, JG Winters, JM Irwin… - The Astrophysical …, 2020 - iopscience.iop.org
We present a study of flare rates, rotation periods, and spectroscopic activity indicators of
125 single stars within 15 parsecs and with masses between 0.1 and 0.3 M⊙ observed …

Flares in open clusters with K2-II. Pleiades, Hyades, Praesepe, Ruprecht 147, and M 67

E Ilin, SJ Schmidt, K Poppenhäger… - Astronomy & …, 2021 - aanda.org
Context. Magnetic fields are a key component in the main sequence evolution of low mass
stars. Flares, energetic eruptions on the surfaces of stars, are an unmistakable manifestation …

Gaia Data Release 2-Variable stars in the colour-absolute magnitude diagram

L Eyer, L Rimoldini, M Audard, RI Anderson… - Astronomy & …, 2019 - aanda.org
Context. The ESA Gaia mission provides a unique time-domain survey for more than 1.6
billion sources with G≲ 21 mag. Aims. We showcase stellar variability in the Galactic colour …

Statistical studies of solar white-light flares and comparisons with superflares on solar-type stars

K Namekata, T Sakaue, K Watanabe… - The Astrophysical …, 2017 - iopscience.iop.org
Statistical Studies of Solar White-light Flares and Comparisons with Superflares on Solar-type
Stars - IOPscience This site uses cookies. By continuing to use this site you agree to our use …

X-ray superflares from pre-main-sequence Stars: Flare energetics and frequency

KV Getman, ED Feigelson - The Astrophysical Journal, 2021 - iopscience.iop.org
Solar-type stars exhibit their highest levels of magnetic activity during their early convective
pre-main-sequence (PMS) phase of evolution. The most powerful PMS flares, superflares …

Exploring the photometric variability of ultra-cool dwarfs with TESS

RP Petrucci, Y Gómez Maqueo Chew… - Monthly Notices of …, 2024 - academic.oup.com
We present a photometric characterization of 208 ultra-cool dwarfs (UCDs) with spectral
types between M4 and L4, from 20-s and 2-min cadence TESS light curves. We determine …