activity
20112023
most citedMasses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets

497 citations · 8.9k across the 119 of their papers we have counts for

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Showing 2019Show all

18 papers · 1 filter

astro-ph.SR2019★ 54 cited

Detection and characterisation of oscillating red giants: first results from the TESS satellite

Víctor Silva Aguirre, Dennis Stello, Amalie Stokholm +78

Since the onset of the `space revolution' of high-precision high-cadence photometry, asteroseismology has been demonstrated as a powerful tool for informing Galactic archaeology in…

astro-ph.SR2019★ 19 cited

Asteroseismology of the Multiplanet System K2-93

Mikkel N. Lund, Emil Knudstrup, Victor Silva Aguirre +14

We revisit the analysis of the bright multiplanet system K2-93, discovered with data taken by the K2 mission. This system contains five identified planets ranging in size from sub-…

astro-ph.SR2019★ 46 cited

TESS Asteroseismology of the known red-giant host stars HD 212771 and HD 203949

Tiago L. Campante, Enrico Corsaro, Mikkel N. Lund +45

The Transiting Exoplanet Survey Satellite (TESS) is performing a near all-sky survey for planets that transit bright stars. In addition, its excellent photometric precision enables…

astro-ph.SR2019★ 7 cited

Sensitivity of low-degree solar p modes to active and ephemeral regions: frequency shifts back to the Maunder Minimum

William J. Chaplin, Rachel Howe, Sarbani Basu +7

We explore the sensitivity of the frequencies of low-degree solar p-modes to near-surface magnetic flux on different spatial scales and strengths, specifically to active regions wi…

astro-ph.SR2019★ 19 cited

Signatures of magnetic activity: On the relation between stellar properties and p-mode frequency variations

A. R. G. Santos, T. L. Campante, W. J. Chaplin +12

In the Sun, the properties of acoustic modes are sensitive to changes in the magnetic activity. In particular, mode frequencies are observed to increase with increasing activity le…

astro-ph.SR2019★ 15 cited

Bayesian hierarchical inference of asteroseismic inclination angles

James S. Kuszlewicz, William J. Chaplin, Thomas S. H. North +5

The stellar inclination angle-the angle between the rotation axis of a star and our line of sight-provides valuable information in many different areas, from the characterisation o…

astro-ph.SR2019★ 33 cited

The K2 Galactic Caps Project -- Going Beyond the \textit{Kepler} Field and Ageing the Galactic Disc

B. M. Rendle, A. Miglio, C. Chiappini +21

Analyses of data from spectroscopic and astrometric surveys have led to conflicting results concerning the vertical characteristics of the Milky Way. Ages are often used to provide…

astro-ph.SR2019★ 59 cited

New light on the Gaia DR2 parallax zero-point: influence of the asteroseismic approach, in and beyond the Kepler field

Saniya Khan, Andrea Miglio, Benoît Mosser +15

The importance of studying the Gaia DR2 parallax zero-point by external means was underlined by Lindegren et al. (2018), and initiated by several works making use of Cepheids, ecli…

astro-ph.SR2019★ 10 cited

The Kepler Smear Campaign: Light curves for 102 Very Bright Stars

Benjamin J. S. Pope, Guy R. Davies, Keith Hawkins +19

We present the first data release of the Kepler Smear Campaign, using collateral 'smear' data obtained in the Kepler four-year mission to reconstruct light curves of 102 stars too…

astro-ph.SR2019★ 12 cited

KOI-3890: A high mass-ratio asteroseismic red-giantM-dwarf eclipsing binary undergoing heartbeat tidal interactions

James S. Kuszlewicz, Thomas S. H. North, William J. Chaplin +9

KOI-3890 is a highly eccentric, 153-day period eclipsing, single-lined spectroscopic binary system containing a red-giant star showing solar-like oscillations alongside tidal inter…

astro-ph.SR2019★ 56 cited

Testing asteroseismology with Gaia DR2: Hierarchical models of the Red Clump

Oliver J. Hall, Guy R. Davies, Yvonne P. Elsworth +8

Asteroseismology provides fundamental stellar parameters independent of distance, but subject to systematics under calibration. Gaia DR2 has provided parallaxes for a billion stars…

astro-ph.SR2019★ 140 cited

Abundance to age ratios in the HARPS-GTO sample with Gaia DR2: Chemical clocks for a range of [Fe/H]

E. Delgado Mena, A. Moya, V. Adibekyan +8

[ABRIDGED] The purpose of this work is to evaluate how several elements produced by different nucleosynthesis processes behave with stellar age and provide empirical relations to d…

astro-ph.SR2019★ 16 cited

Asteroseismic constraints on active latitudes of solar-type stars: HD173701 has active bands at higher latitudes than the Sun

Alexandra E. L. Thomas, William J. Chaplin, Guy R. Davies +6

We present a new method for determining the location of active bands of latitude on solar-type stars, which uses stellar-cycle-induced frequency shifts of detectable solar-like osc…

astro-ph.SR2019★ 8 cited

FliPer: In search of solar-like pulsators among TESS targets

L. Bugnet, R. A. García, S. Mathur +4

The NASA's Transiting Exoplanet Survey Satellite (TESS) is about to provide full-frame images of almost the entire sky. The amount of stellar data to be analysed represents hundred…

astro-ph.EP2019★ 34 cited

The Curious Case of KOI 4: Confirming Kepler's First Exoplanet

Ashley Chontos, Daniel Huber, David W. Latham +13

The discovery of thousands of planetary systems by Kepler has demonstrated that planets are ubiquitous. However, a major challenge has been the confirmation of Kepler planet candid…

astro-ph.SR2019★ 73 cited

The Asteroseismic Target List (ATL) for solar-like oscillators observed in 2-minute cadence with the Transiting Exoplanet Survey Satellite (TESS)

M. Schofield, W. J. Chaplin, D. Huber +21

We present the target list of solar-type stars to be observed in short-cadence (2-min) for asteroseismology by the NASA Transiting Exoplanet Survey Satellite (TESS) during its 2-ye…

astro-ph.SR2019★ 103 cited

AIMS - A new tool for stellar parameter determinations using asteroseismic constraints

B. M. Rendle, G. Buldgen, A. Miglio +12

A key aspect in the determination of stellar properties is the comparison of observational constraints with predictions from stellar models. Asteroseismic Inference on a Massive Sc…

astro-ph.EP2019★ 95 cited

A Hot Saturn Orbiting An Oscillating Late Subgiant Discovered by TESS

Daniel Huber, William J. Chaplin, Ashley Chontos +139

We present the discovery of TOI-197.01, the first transiting planet identified by the Transiting Exoplanet Survey Satellite (TESS) for which asteroseismology of the host star is po…