activity
20162026
most citedTESS Discovery of a Transiting Super-Earth in the Mensae System

207 citations · 1.7k across the 55 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

17 papers · 1 filter

astro-ph.SR2025★ 1 cited

NGTS-EB-8: A double-lined eclipsing M+M binary discovered by citizen scientists

Sean M. O'Brien, Megan E. Schwamb, Christopher A. Watson +54

We report the identification and characterization of a new binary system composed of two near-equal mass M-dwarfs. The binary NGTS-EB-8 was identified as a planet candidate in data…

astro-ph.SR2022★ 1 cited

X-ray emission from candidate stellar merger remnant TYC 2597-735-1 and its Blue Ring Nebula

Hans Moritz Günther, Keri Hoadley, Maximilian N. Günther +3

Tight binary or multiple star systems can interact through mass transfer and follow vastly different evolutionary pathways than single stars. The star TYC 2597-735-1 is a candidate…

astro-ph.SR2022★ 5 cited

Theoretical and Observational Evidence for Coriolis Effects in Coronal Magnetic Fields Via Direct Current Driven Flaring Events

Darryl Z. Seligman, Leslie A. Rogers, Adina D. Feinstein +6

All stars produce explosive surface events such as flares and coronal mass ejections. These events are driven by the release of energy stored in coronal magnetic fields, generated…

astro-ph.SR2021★ 23 cited

The TESS View of LOFAR Radio-Emitting Stars

Benjamin J. S. Pope, Joseph R. Callingham, Adina D. Feinstein +4

The recent detection of the M dwarf GJ 1151 at 144 MHz low radio frequencies using LOFAR has been interpreted as evidence of an exoplanet magnetically interacting with its host sta…

astro-ph.SR2021★ 15 cited

NGTS clusters survey -- III: A low-mass eclipsing binary in the Blanco 1 open cluster spanning the fully convective boundary

Gareth D. Smith, Edward Gillen, Didier Queloz +27

We present the discovery and characterisation of an eclipsing binary identified by the Next Generation Transit Survey in the 115 Myr old Blanco 1 open cluster. NGTS J0002-29…

astro-ph.SR2021★ 29 cited

Testing Self-Organized Criticality Across the Main Sequence using Stellar Flares from TESS

Adina D. Feinstein, Darryl Z. Seligman, Maximilian N. Günther +1

Self-organized criticality describes a class of dynamical systems that maintain themselves in an attractor state with no intrinsic length or time scale. Fundamentally, this theoret…

astro-ph.SR2021★ 25 cited

Long-term stellar activity variations and their effect on radial-velocity measurements

Jean C. Costes, Christopher A. Watson, Ernst de Mooij +8

Long-term stellar activity variations can affect the detectability of long-period and Earth-analogue extrasolar planets. We have, for 54 stars, analysed the long-term trend of five…

astro-ph.SR2021★ 52 cited

Stellar flares detected with the Next Generation Transit Survey

James A. G. Jackman, Peter J. Wheatley, Jack S. Acton +19

We present the results of a search for stellar flares in the first data release from the Next Generation Transit Survey (NGTS). We have found 610 flares from 339 stars, with spectr…

astro-ph.SR2020★ 15 cited

An eclipsing M-dwarf close to the hydrogen burning limit from NGTS

Jack S. Acton, Michael R. Goad, Sarah L. Casewell +20

We present the discovery of NGTS J0930-18, an extreme mass ratio eclipsing M-dwarf binary system with an early M-dwarf primary and a late M-dwarf secondary close to the hydrogen bu…

astro-ph.SR2020★ 21 cited

Complex Modulation of Rapidly Rotating Young M Dwarfs: Adding Pieces to the Puzzle

Maximilian N. Günther, David A. Berardo, Elsa Ducrot +37

New sets of young M dwarfs with complex, sharp-peaked, and strictly periodic photometric modulations have recently been discovered with Kepler/K2 (scallop shells) and TESS (complex…

astro-ph.SR2020★ 138 cited

Flare Statistics for Young Stars from a Convolutional Neural Network Analysis of Data

Adina D. Feinstein, Benjamin T. Montet, Megan Ansdell +5

All-sky photometric time-series missions have allowed for the monitoring of thousands of young (Myr) to understand the evolution of stellar activity. Here we dev…

astro-ph.SR2020★ 24 cited

Superflares on the late-type giant KIC 2852961 -- Scaling effect behind flaring at different energy levels

Zs. Kővári, K. Oláh, M. N. Günther +7

The most powerful superflares reaching 10erg bolometric energy are from giant stars. The mechanism behind flaring is supposed to be the magnetic reconnection, which is close…

astro-ph.SR2020★ 23 cited

A long period (P = 61.8-d) M5V dwarf eclipsing a Sun-like star from TESS and NGTS

Samuel Gill, Benjamin F. Cooke, Daniel Bayliss +27

The Transiting Exoplanet Survey Satellite (TESS) has produced a large number of single transit event candidates which are being monitored by the Next Generation Transit Survey (NGT…

astro-ph.SR2019★ 22 cited

NGTS and WASP photometric recovery of a single-transit candidate from TESS

Samuel Gill, Daniel Bayliss, Benjamin F. Cooke +25

The Transiting Exoplanet Survey Satellite (\tess) produces a large number of single-transit event candidates, since the mission monitors most stars for only 27\,days. Such ca…

astro-ph.SR2019★ 56 cited

NGTS-7Ab: An ultra-short period brown dwarf transiting a tidally-locked and active M dwarf

James A. G. Jackman, Peter J. Wheatley, Dan Bayliss +36

We present the discovery of NGTS-7Ab, a high mass brown dwarf transiting an M dwarf with a period of 16.2 hours, discovered as part of the Next Generation Transit Survey (NGTS). Th…

astro-ph.SR2019★ 53 cited

Complex Rotational Modulation of Rapidly Rotating M-Stars Observed with TESS

Z. Zhan, M. N. Günther, S. Rappaport +23

We have searched for short periodicities in the light curves of stars with cooler than 4000 K made from 2-minute cadence data obtained in TESS sectors 1 and 2. Herein…

astro-ph.SR2018★ 47 cited

Detection of a giant flare displaying quasi-periodic pulsations from a pre-main sequence M star with NGTS

James A. G. Jackman, Peter J. Wheatley, Chloe E. Pugh +18

We present the detection of an energetic flare on the pre-main sequence M3 star NGTS J121939.5-355557, which we estimate as only 2 Myr old. The flare had an energy of $3.2\pm^{0.4}…