Search Results - "Lund, M. N"
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Automated preparation of Kepler time series of planet hosts for asteroseismic analysis
Published in Monthly notices of the Royal Astronomical Society (11-12-2014)“…One of the tasks of the Kepler Asteroseismic Science Operations Center (KASOC) is to provide asteroseismic analyses on Kepler Objects of Interest. However,…”
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Confirming chemical clocks: asteroseismic age dissection of the Milky Way disc(s)
Published in Monthly notices of the Royal Astronomical Society (01-04-2018)“…Abstract Investigations of the origin and evolution of the Milky Way disc have long relied on chemical and kinematic identifications of its components to…”
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Asteroseismic inference on rotation, gyrochronology and planetary system dynamics of 16 Cygni
Published in Monthly notices of the Royal Astronomical Society (21-01-2015)“…The solar analogues 16 Cyg A and B are excellent asteroseismic targets in the Kepler field of view and together with a red dwarf and a Jovian planet form an…”
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Detection of solar-like oscillations in relics of the Milky Way: asteroseismology of K giants in M4 using data from the NASA K2 mission
Published in Monthly notices of the Royal Astronomical Society (01-09-2016)“…Asteroseismic constraints on K giants make it possible to infer radii, masses and ages of tens of thousands of field stars. Tests against independent estimates…”
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Ages and fundamental properties of Kepler exoplanet host stars from asteroseismology
Published in Monthly notices of the Royal Astronomical Society (11-09-2015)“…We present a study of 33 Kepler planet-candidate host stars for which asteroseismic observations have sufficiently high signal-to-noise ratio to allow…”
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The BAyesian STellar algorithm (BASTA): a fitting tool for stellar studies, asteroseismology, exoplanets, and Galactic archaeology
Published in Monthly notices of the Royal Astronomical Society (01-01-2022)“…ABSTRACT We introduce the public version of the BAyesian STellar Algorithm (BASTA), an open-source code written in Python to determine stellar properties based…”
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Oscillation frequencies for 35 Kepler solar-type planet-hosting stars using Bayesian techniques and machine learning
Published in Monthly notices of the Royal Astronomical Society (21-02-2016)“…Kepler has revolutionized our understanding of both exoplanets and their host stars. Asteroseismology is a valuable tool in the characterization of stars and…”
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Hot super-Earths stripped by their host stars
Published in Nature communications (11-04-2016)“…Simulations predict that hot super-Earth sized exoplanets can have their envelopes stripped by photoevaporation, which would present itself as a lack of these…”
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First Results from the Hertzsprung SONG Telescope: Asteroseismology of the G5 Subgiant Star μ Herculis
Published in The Astrophysical journal (10-02-2017)“…Abstract We report the first asteroseismic results obtained with the Hertzsprung Stellar Observations Network Group Telescope from an extensive high-precision…”
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SPIN-ORBIT ALIGNMENT OF EXOPLANET SYSTEMS: ENSEMBLE ANALYSIS USING ASTEROSEISMOLOGY
Published in The Astrophysical journal (01-03-2016)“…ABSTRACT The angle between a planet's orbital axis and the spin axis of its parent star is an important diagnostic of planet formation, migration, and tidal…”
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Damping rates and frequency corrections of Kepler LEGACY stars
Published in Monthly notices of the Royal Astronomical Society (21-07-2019)“…ABSTRACT Linear damping rates and modal frequency corrections of radial oscillation modes in selected LEGACY main-sequence stars are estimated by means of a…”
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The K2 Galactic Caps Project – going beyond the Kepler field and ageing the Galactic disc
Published in Monthly notices of the Royal Astronomical Society (21-12-2019)“…ABSTRACT Analyses of data from spectroscopic and astrometric surveys have led to conflicting results concerning the vertical characteristics of the Milky Way…”
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Establishing the accuracy of asteroseismic mass and radius estimates of giant stars – II. Revised stellar masses and radii for KIC 8430105
Published in Monthly notices of the Royal Astronomical Society (01-11-2022)“…ABSTRACT Asteroseismic scaling relations can provide high-precision measurements of mass and radius for red giant (RG) stars displaying solar-like…”
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WHAT ASTEROSEISMOLOGY CAN DO FOR EXOPLANETS: KEPLER-410A b IS A SMALL NEPTUNE AROUND A BRIGHT STAR, IN AN ECCENTRIC ORBIT CONSISTENT WITH LOW OBLIQUITY
Published in The Astrophysical journal (10-02-2014)“…We confirm the Kepler planet candidate Kepler-410A b (KOI-42b) as a Neptune-sized exoplanet on a 17.8 day, eccentric orbit around the bright (K sub(p) = 9.4)…”
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Extremely precise age and metallicity of the open cluster NGC 2506 using detached eclipsing binaries
Published in Monthly notices of the Royal Astronomical Society (01-11-2020)“…ABSTRACT Accurate stellar parameters of stars in open clusters can help constrain models of stellar structure and evolution. Here, we wish to determine the age…”
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Seismic and spectroscopic analysis of nine bright red giants observed by Kepler
Published in Monthly notices of the Royal Astronomical Society (01-01-2024)“…ABSTRACT Photometric time series gathered by space telescopes such as CoRoT and Kepler allow to detect solar-like oscillations in red giant stars and to…”
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Signatures of Magnetic Activity: On the Relation between Stellar Properties and p-mode Frequency Variations
Published in The Astrophysical journal (20-09-2019)“…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…”
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The host stars of Kepler's habitable exoplanets: superflares, rotation and activity
Published in Monthly notices of the Royal Astronomical Society (21-01-2016)“…We embark on a detailed study of the light curves of Kepler's most Earth-like exoplanet host stars using the full length of Kepler data. We derive rotation…”
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Study of chemically peculiar stars – I. High-resolution spectroscopy and K2 photometry of Am stars in the region of M44
Published in Monthly notices of the Royal Astronomical Society (01-03-2022)“…ABSTRACT We present a study based on the high-resolution spectroscopy and K2 space photometry of five chemically peculiar stars in the region of the open…”
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