activity
20072025
most citedPreparation of Kepler lightcurves for asteroseismic analyses

286 citations · 1.5k across the 21 of their papers we have counts for

collaborators

22 papers

physics.ins-det2025

Testing a Computed Tomography Imaging Spectrometer for Earth Observations on the HEIMDAL Stratospheric Balloon Mission

Mads Juul Ahlebæk, Albertino Antonio Almeida Bach, Loui Collin-Enoch +13

Stratospheric High Altitude Balloons (HABs) have great potential as a remote sensing platform for Earth Observations that complements orbiting satellites and low flying drones. At…

astro-ph.IM2024★ 13 cited

The PLATO Mission

Heike Rauer, Conny Aerts, Juan Cabrera +842

PLATO (PLAnetary Transits and Oscillations of stars) is ESA's M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large numb…

astro-ph.SR2015★ 10 cited

On the current solar magnetic activity in the light of its behaviour during the Holocene

F. Inceoglu, R. Simoniello, M. F. Knudsen +3

Solar modulation potential (SMP) reconstructions based on cosmogenic nuclide records reflect changes in the open solar magnetic field and can therefore help us obtain information o…

astro-ph.SR2013★ 4 cited

Comparison of photometric variability before and after stellar flares

C. Karoff

The energy in the solar acoustic spectrum is known to be correlated with flares, but it is not known if the same is true for stellar flares? In order to answer this question, we ha…

astro-ph.SR2013★ 1 cited

Kepler White Paper: Asteroseismology of Solar-Like Oscillators in a 2-Wheel Mission

W. J Chaplin, H. Kjeldsen, J. Christensen-Dalsgaard +53

We comment on the potential for continuing asteroseismology of solar-type and red-giant stars in a 2-wheel Kepler Mission. Our main conclusion is that by targeting stars in the ecl…

astro-ph.SR2013★ 254 cited

Rotation periods of 12 000 main-sequence Kepler stars: Dependence on stellar spectral type and comparison with v sin i observations

M. B. Nielsen, L. Gizon, H. Schunker +1

Aims: We aim to measure the starspot rotation periods of active stars in the Kepler field as a function of spectral type and to extend reliable rotation measurements from F-, G-, a…