activity
19982024
most citedTransiting exoplanets from the CoRoT space mission VIII. CoRoT-7b: the first Super-Earth with measured radius

598 citations · 9.7k across the 144 of their papers we have counts for

collaborators

136 papers

astro-ph.SR2024

Low-amplitude solar-like oscillations in the K5 V star Indi A

Mia S. Lundkvist, Hans Kjeldsen, Timothy R. Bedding +17

We have detected solar-like oscillations in the mid K-dwarf Indi A, making it the coolest dwarf to have measured oscillations. The star is noteworthy for harboring a…

astro-ph.SR2021★ 26 cited

Age and helium content of the open cluster NGC 6791 from multiple eclipsing binary members. III. Constraints from a subgiant

K. Brogaard, F. Grundahl, E. L. Sandquist +18

Models of stellar structure and evolution can be constrained using accurate measurements of the parameters of eclipsing binary members of open clusters. Multiple binary stars provi…

astro-ph.SR2020★ 12 cited

Extremely precise age and metallicity of the open cluster NGC 2506 using detached eclipsing binaries

E. Knudstrup, F. Grundahl, K. Brogaard +10

Accurate stellar parameters of stars in open clusters can help constrain models of stellar structure and evolution. Here we wish to determine the age and metallicity content of the…

astro-ph.SR2019

Chromospheric emission of solar-type stars with asteroseismic ages

R S Booth, K. Poppenhaeger, C. A. Watson +3

Stellar magnetic activity decays over the main-sequence life of cool stars due to the stellar spin-down driven by magnetic braking. The evolution of chromospheric emission is well-…

astro-ph.SR2018★ 25 cited

The blue straggler V106 in NGC6791: A prototype progenitor of old single giants masquerading as young

K. Brogaard, S. M. Christiansen, F. Grundahl +18

We determine the properties of the binary star V106 in the old open cluster NGC6791. We identify the system to be a blue straggler cluster member by using a combination of ground-b…

astro-ph.SR2018★ 101 cited

Establishing the accuracy of asteroseismic mass and radius estimates of giant stars. I. Three eclipsing systems at [Fe/H]~ -0.3 and the need for a large high-precision sample

K. Brogaard, C. J. Hansen, A. Miglio +12

We aim to establish and improve the accuracy level of asteroseismic estimates of mass, radius, and age of giant stars. This can be achieved by measuring independent, accurate, and…