activity
20052026
most citedGravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars

612 citations · 10.2k across the 118 of their papers we have counts for

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13 papers · 1 filter

astro-ph2008★ 20 cited

MOST photometry of the enigmatic PMS pulsator HD 142666

K. Zwintz, T. Kallinger, D. B. Guenther +11

We present precise photometry of the pulsating Herbig Ae star HD 142666 obtained in two consecutive years with the MOST (Microvariability & Oscilations of STars) satellite. Previou…

astro-ph2008★ 34 cited

The nature of p-modes and granulation in HD 49933 observed by CoRoT

T. Kallinger, M. Gruberbauer, D. B. Guenther +2

Context: Recent observations of HD49933 by the space-photometric mission CoRoT provide photometric evidence of solar type oscillations in a star other than our Sun. The first publi…

astro-ph2008★ 4 cited

Oscillating red giants in the CoRoT exo-field: Asteroseismic mass and radius determination

T. Kallinger, W. W. Weiss, C. Barban +10

Context. Observations and analysis of solar-type oscillations in red-giant stars is an emerging aspect of asteroseismic analysis with a number of open questions yet to be explored.…

astro-ph2008★ 69 cited

On the detection of Lorentzian profiles in a power spectrum: A Bayesian approach using ignorance priors

M. Gruberbauer, T. Kallinger, W. W. Weiss +1

Aims. Deriving accurate frequencies, amplitudes, and mode lifetimes from stochastically driven pulsation is challenging, more so, if one demands that realistic error estimates be g…

astro-ph2008

Solar-like oscillations in red giants in the CoRoT exo-field

S. Hekker, C. Barban, T. Kallinger +4

Asteroseismic observations from space can provide us with long time series of uninterrupted high quality data for many stars at the same time. The CoRoT satellite (Convection Rotat…

astro-ph2008★ 24 cited

MOST photometry of the roAp star 10 Aql

D. Huber, H. Saio, M. Gruberbauer +12

Context: We present 31.2 days of nearly continuous MOST photometry of the roAp star 10Aql. Aims:The goal was to provide an unambiguous frequency identification for this little stud…