papers

Publications (196)

astro-ph.HE2013

Energy spectra of KASCADE-Grande based on shower size measurements and different hadronic interaction models

D. Kang, W. D. Apel, J. C. Arteaga-Velazquez +54

KASCADE-Grande is dedicated for investigations of cosmic-ray air showers in the primary energy range from 10 PeV to 1 EeV. The multi-detector system allows us to reconstruct charge…

astro-ph.HE2013

Pierre Auger Observatory and Telescope Array: Joint Contributions to the 33rd International Cosmic Ray Conference (ICRC 2013)

The Telescope Array, Pierre Auger Collaborations, : +619

Joint contributions of the Pierre Auger and Telescope Array Collaborations to the 33rd International Cosmic Ray Conference, Rio de Janeiro, Brazil, July 2013: cross-calibration of…

astro-ph.SR2010

Solar-like oscillations in red giants observed with Kepler: comparison of global oscillation parameters from different methods

S. Hekker, Y. Elsworth, J. De Ridder +20

The large number of stars for which uninterrupted high-precision photometric timeseries data are being collected with \textit{Kepler} and CoRoT initiated the development of automat…

astro-ph2008

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-ph.IM2024

GRAVITY+ Wavefront Sensors: High-Contrast, Laser Guide Star, Adaptive Optics systems for the VLTI

G. Bourdarot, F. Eisenhauer, S. Yazıcı +53

We present the Wavefront Sensor units of the Gravity Plus Adaptive Optics (GPAO) system, which will equip all 8m class telescopes of the VLTI and is an instrumental part of the GRA…

astro-ph.SR2012

Accurate parameters of 93 solar-type Kepler targets

H. Bruntt, S. Basu, B. Smalley +29

We present a detailed spectroscopic study of 93 solar-type stars that are targets of the NASA/Kepler mission and provide detailed chemical composition of each target. We find that…