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相关论文: The Kepler Catalog of Stellar Flares

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We present a flare catalog of the {\it Kepler} mission using the long-cadence data of Data Release 25. This catalog comprises 3420 flare stars and 162,262 flare events. A comparison shows that the flare catalogs of previous studies are…

太阳与恒星天体物理 · 物理学 2019-04-17 Huiqin Yang , Jifeng Liu

We present the results of a search for stellar flares from stars neighbouring the target sources in the Kepler short cadence data. These flares have been discarded as contaminants in previous surveys and therefore provide an unexplored…

太阳与恒星天体物理 · 物理学 2021-02-03 James A. G. Jackman , Evgenya Shkolnik , R. O. Parke Loyd

The habitability of planets is closely connected with the stellar activity, mainly the frequency of flares and the distribution of flare energy. Kepler and TESS find many flaring stars are detected via precise time-domain photometric data,…

太阳与恒星天体物理 · 物理学 2023-01-19 Dong-Yang Gao , Hui-Gen Liu , Ming Yang , Ji-Lin Zhou

In this paper, we study stellar light curves from the TESS satellite (Transiting Exoplanet Survey Satellite) for the presence of stellar flares. The main aim is to detect stellar flares using two-minutes cadence data and to perform…

太阳与恒星天体物理 · 物理学 2022-08-31 Małgorzata Pietras , Robert Falewicz , Marek Siarkowski , Kamil Bicz , Paweł Preś

We aim to perform a statistical study of stellar flares observed by Kepler. We want to study the flare amplitude, duration, energy and occurrence rates, and how they are related to the spectral type and rotation period. To that end, we have…

太阳与恒星天体物理 · 物理学 2017-11-08 Tom Van Doorsselaere , Hoda Shariati , Jonas Debosscher

Using a recent census of flare stars from the Kepler survey, we have explored how flare activity evolves across stellar main sequence lifetimes. We utilize a sample of 347 stars with robust flare activity detections, and which have rotation…

太阳与恒星天体物理 · 物理学 2019-02-13 James R. A. Davenport , Kevin R. Covey , Riley W. Clarke , Austin C. Boeck , Jonathan Cornet , Suzanne L. Hawley

Over the past years, thousands of stellar flares have been detected by harvesting data from large photometric surveys. These detections, however, do not account for potential sources of contamination such as background stars appearing in…

Archives of long photometric surveys, like the Kepler database, are a gold mine for studying flares. However, identifying them is a complex task; while in the case of single-target observations it can be easily done manually by visual…

太阳与恒星天体物理 · 物理学 2018-09-12 Krisztián Vida , Rachael M. Roettenbacher

We aim to give a reliable estimate of the number of flaring giant stars in the Kepler field. By analyzing the flaring activity of these stars we explore their flare statistics and the released flare energies. The role of oscillation in…

太阳与恒星天体物理 · 物理学 2021-03-10 K. Oláh , Zs. Kővári , M. N. Günther , K. Vida , P. Gaulme , B. Seli , A. Pál

We embark on a study of quasi-periodic pulsations (QPPs) in the decay phase of white-light stellar flares observed by Kepler. Out of the 1439 flares on 216 different stars detected in the short-cadence data using an automated search, 56…

太阳与恒星天体物理 · 物理学 2016-04-27 C. E. Pugh , D. J. Armstrong , V. M. Nakariakov , A. -M. Broomhall

We present the largest sample of flares ever compiled for a single M dwarf, the active M4 star GJ 1243. Over 6100 individual flare events, with energies ranging from $10^{29}$ to $10^{33}$ erg, are found in 11 months of 1-minute cadence…

Kepler data from G-, K- and M-type stars are used to study conditions that lead to superflares with energies above $10^{34} {\rm erg}$. From the 117,661 stars included, 380 show superflares with a total of 1690 such events. We study whether…

太阳与恒星天体物理 · 物理学 2014-08-20 Simon Candelaresi , Andrew Hillier , Hiroyuki Maehara , Axel Brandenburg , Kazunari Shibata

We present an analysis of flare activity in wide binary stars using a combination of value-added data sets from the NASA Kepler mission. The target list contains a set of previously discovered wide binary star systems identified by proper…

太阳与恒星天体物理 · 物理学 2018-02-07 Riley W. Clarke , James R. A. Davenport , Kevin R. Covey , Christoph Baranec

We report the latest statistical analyses of superflares on solar-type (G-type main-sequence; effective temperature is 5100 - 6000 K) stars using all of the $Kepler$ primary mission data, and $Gaia$-DR2 (Data Release 2) catalog. We updated…

太阳与恒星天体物理 · 物理学 2021-01-15 Soshi Okamoto , Yuta Notsu , Hiroyuki Maehara , Kosuke Namekata , Satoshi Honda , Kai Ikuta , Daisaku Nogami , Kazunari Shibata

We apply multi-algorithm machine learning models to TESS 2-minute survey data from Sectors 1-72 to identify stellar flares. Models trained with Deep Neural Network, Random Forest, and XGBoost algorithms, respectively, utilized four flare…

太阳与恒星天体物理 · 物理学 2024-10-24 Chia-Lung Lin , Daniel Apai , Mark S. Giampapa , Wing-Huen Ip

We present a Bayesian-odds-ratio-based algorithm for detecting stellar flares in light curve data. We assume flares are described by a model in which there is a rapid rise with a half-Gaussian profile, followed by an exponential decay. Our…

太阳与恒星天体物理 · 物理学 2015-06-19 M. Pitkin , D. Williams , L. Fletcher , S. D. T. Grant

Ultra-precise light curves from Kepler provide the best opportunity to determine rates and statistical properties of stellar flares. From 11 months of data on the active M4 dwarf, GJ 1243, we have built the largest catalog of flares for a…

太阳与恒星天体物理 · 物理学 2017-01-11 James R. A. Davenport

We searched for superflares on solar-type stars using the Kepler short-cadence (1-min sampling) data in order to detect superflares with short duration. We found 187 superflares on 23 solar-type stars whose bolometric energy ranges from the…

太阳与恒星天体物理 · 物理学 2017-01-11 Hiroyuki Maehara , Takuya Shibayama , Yuta Notsu , Shota Notsu , Satoshi Honda , Daisaku Nogami , Kazunari Shibata

Superflares are flares that release total energy 10$\sim$10$^{4}$ times greater than that of the biggest solar flares with energy of $\sim$10$^{32}$ erg. We searched superflares on solar-type stars (G-type main sequence stars) using the…

太阳与恒星天体物理 · 物理学 2016-08-04 Yuta Notsu , Hiroyuki Maehara , Takuya Shibayama , Satoshi Honda , Shota Notsu , Kosuke Namekata , Daisaku Nogami , Kazunari Shibata

We analyzed Kepler short-cadence M dwarf observations. Spectra from the ARC 3.5m telescope identify magnetically active (H$\alpha$ in emission) stars. The active stars are of mid-M spectral type, have numerous flares, and well-defined…

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