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Related papers: Frequent flaring in the TRAPPIST-1 system - unsuit…

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The M8V star TRAPPIST-1 hosts seven roughly Earth-sized planets and is a promising target for exoplanet characterization. Kepler/K2 Campaign 12 observations of TRAPPIST-1 in the optical show an apparent rotational modulation with a 3.3 day…

Solar and Stellar Astrophysics · Physics 2018-04-25 Brett M. Morris , Eric Agol , James R. A. Davenport , Suzanne L. Hawley

As more exoplanets are being discovered around ultracool dwarfs, understanding their magnetic activity -- and the implications for habitability -- is of prime importance. To find stellar flares and photometric signatures related to…

Solar and Stellar Astrophysics · Physics 2021-06-30 Bálint Seli , Krisztián Vida , Attila Moór , András Pál , Katalin Oláh

The nearby ultracool dwarf TRAPPIST-1 possesses several Earth-sized terrestrial planets, three of which have equilibrium temperatures that may support liquid surface water, making it a compelling target for exoplanet characterization.…

Earth and Planetary Astrophysics · Physics 2020-09-02 Amy L. Glazier , Ward S. Howard , Hank Corbett , Nicholas M. Law , Jeffrey K. Ratzloff , Octavi Fors , Daniel del Ser

Ly-$\alpha$ observations provide a powerful probe of stellar activity and atmospheric escape in exoplanetary systems. We present here an analysis of 104 HST/STIS orbits monitoring the TRAPPIST-1 system between 2017 and 2022, covering 3--5…

TRAPPIST-1 is an ultra-cool dwarf that flares frequently. These flares shape the surrounding planets' high-energy irradiation environments, with consequences for atmospheric chemistry and escape, and they can contaminate transmission…

We analyze the light curve of the M5.5 dwarf Proxima Centauri obtained by the TESS in Sectors 11 and 12. In the $\approx 50$ day-long light curve we identified and analyzed 72 flare events. The flare rate was 1.49 events per day, in total,…

Solar and Stellar Astrophysics · Physics 2019-11-06 Krisztián Vida , Katalin Oláh , Zsolt Kővári , Lidia van Driel-Gesztelyi , Attila Moór , András Pál

We present an analysis of K2 short cadence data of 34 M dwarfs which have spectral types in the range M0 - L1. Of these stars, 31 showed flares with a duration between $\sim$10-90 min. Using distances obtained from Gaia DR2 parallaxes, we…

Solar and Stellar Astrophysics · Physics 2018-08-08 L. Doyle , G. Ramsay , J. G. Doyle , K. Wu , E. Scullion

The signatures of planets hosted by M dwarfs are more readily detected with transit photometry and radial velocity methods than those of planets around larger stars. Recently, transit photometry was used to discover seven planets orbiting…

Solar and Stellar Astrophysics · Physics 2017-12-27 Rachael M. Roettenbacher , Stephen R. Kane

Although high energetic radiation from flares is a potential threat to exoplanet atmospheres and may lead to surface sterilization, it might also provide the extra energy for low-mass stars needed to trigger and sustain prebiotic chemistry.…

In the archive of the Ground Wide Angle Camera (GWAC), we found 43 white light flares from 43 stars, among which, three are sympathetic or homologous flares, and one of them also has a quasi-periodic pulsation with a period of $13.0\pm1.5$…

The TRAPPIST-1 system is the first transiting planet system found orbiting an ultra-cool dwarf star. At least seven planets similar to Earth in radius and in mass were previously found to transit this host star. Subsequently, TRAPPIST-1 was…

The TRAPPIST-1 system has 7 known terrestrial planets arranged compactly in a mean motion resonant chain around an ultra-cool central star, some within the estimated habitable zone. Given their short orbital periods of just a few days, it…

Earth and Planetary Astrophysics · Physics 2019-08-07 Alec M. Vinson , Daniel Tamayo , Brad M. S. Hansen

We present an overview of K2 short cadence observations for 34 M dwarfs observed in Campaigns 1 - 9 which have spectral types between M0 - L1. All of the stars in our sample showed flares with the most energetic reaching $3\times10^{34}$…

Solar and Stellar Astrophysics · Physics 2019-03-06 Lauren Doyle , Gavin Ramsay , John G. Doyle

The TRAPPIST-1 system provides an exquisite laboratory for advancing our understanding exoplanetary atmospheres, compositions, dynamics and architectures. A remarkable aspect of TRAPPIST-1 is that it represents the longest known resonance…

Earth and Planetary Astrophysics · Physics 2018-07-31 David Kipping

We have analyzed Kepler light curves for 849 stars with T_eff < 5200 K from our Cycle 1 Guest Observer program. We identify six new eclipsing binaries, one of which has an orbital period of 29.91 d, and two of which are probably W UMa…

Solar and Stellar Astrophysics · Physics 2015-06-03 T. E. Harrison , J. L. Coughlin , N. M. Ule , M. Lopez-Morales

Using light curves obtained by the K2 mission, we study the relation between stellar rotation and magnetic activity with special focus on stellar flares. Our sample comprises 56 bright and nearby M dwarfs observed by K2 during campaigns…

Solar and Stellar Astrophysics · Physics 2020-05-06 St. Raetz , B. Stelzer , M. Damasso , A. Scholz

For 80 days in 2017, the Kepler Space Telescope continuously observed the transitional millisecond pulsar system PSR J1023+0038 in its accreting state. We present analyses of the 59 second cadence data, focusing on investigations of the…

High Energy Astrophysical Phenomena · Physics 2018-04-11 M. R. Kennedy , C. J. Clark , G. Voisin , R. P. Breton

Although TRAPPIST-1's temperate planets have the highest transmission signals of any known system, flares contaminate 50-70% of transits at the 1000 ppm level, far above 100 ppm secondary atmospheres. Efforts to mitigate flare contamination…

Tidally locked worlds provide a unique opportunity for constraining the probable climates of certain exoplanets. They are unique in that few exoplanet spin and obliquity states are known or will be determined in the near future: both of…

Earth and Planetary Astrophysics · Physics 2023-08-02 Cody J. Shakespeare , Jason H. Steffen

Photometric space missions like Kepler and TESS continuously discover new exoplanets and advance the search for a second habitable world. The light curves recorded by these telescopes also reveal signs of magnetic activity, such as star…

Solar and Stellar Astrophysics · Physics 2021-11-16 Mirjam Bogner , Beate Stelzer , Stefanie Raetz
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