Duality between (2+ 1) d quantum critical points
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 …
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 …
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)
We describe the simulated data sample for the Photometric Large Synoptic Survey
Telescope (LSST) Astronomical Time Series Classification Challenge (PLAsTiCC), a …
Telescope (LSST) Astronomical Time Series Classification Challenge (PLAsTiCC), a …
Flare statistics for young stars from a convolutional neural network analysis of TESS data
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 …
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 …
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 …
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
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 …
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 …
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 …
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 …
types between M4 and L4, from 20-s and 2-min cadence TESS light curves. We determine …