most citedA heuristic derivation of the uncertainty of the frequency determination in time series data

132 citations · 360 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph200833 cited

Pulsations in the atmosphere of the rapidly oscillating Ap star 10 Aquilae

M. Sachkov, O. Kochukhov, T. Ryabchikova +4

The rapidly oscillating Ap (roAp) star 10 Aql shows one of the lowest photometric pulsation amplitudes and is characterized by an unusual spectroscopic pulsational behavior compare…

astro-ph200845 cited

MOST detects SPBe pulsations in HD 127756 & HD 217543: Asteroseismic rotation rates independent of vsini

C. Cameron, H. Saio, R. Kuschnig +7

The MOST (Microvariability and Oscillations of Stars) satellite has discovered SPBe (Slowly Pulsating Be) oscillations in the stars HD 127756 (B1/B2 Vne) and HD 217543 (B3 Vpe). Fo…

astro-ph200812 cited

Abundance analysis of seven delta Scuti Stars

L. Fossati, K. Kolenberg, P. Reegen +1

The current knowledge of the abundance pattern in delta Scuti stars is based on the analysis of just a few field stars. We aim to determine the general chemical properties of the a…

astro-ph2008132 cited

A heuristic derivation of the uncertainty of the frequency determination in time series data

T. Kallinger, P. Reegen, W. W. Weiss

Context: Several approaches to estimate frequency, phase and amplitude errors in time series analyses were reported in the literature, but they are either time consuming to compute…

astro-ph200749 cited

Nonradial p-modes in the G9.5 giant epsilon Oph? Pulsation model fits to MOST photometry

T. Kallinger, D. B. Guenther, J. M. Matthews +6

The G9.5 giant eps Oph shows evidence of radial p-mode pulsations in both radial velocity and luminosity. We re-examine the observed frequencies in the photometry and radial veloci…

astro-ph200787 cited

Late stages of the evolution of A-type stars on the main sequence: comparison between observed chemical abundances and diffusion models for 8 Am stars of the Praesepe cluster

L. Fossati, S. Bagnulo, R. Monier +5

Aims. We aim to provide observational constraints on diffusion models that predict peculiar chemical abundances in the atmospheres of Am stars. We also intend to check if chemical…