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Mathias Zechmeister

Researcher at University of Göttingen

Publications -  127
Citations -  6531

Mathias Zechmeister is an academic researcher from University of Göttingen. The author has contributed to research in topics: Planet & Radial velocity. The author has an hindex of 33, co-authored 108 publications receiving 5204 citations. Previous affiliations of Mathias Zechmeister include Max Planck Society.

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Journal ArticleDOI

The generalised Lomb-Scargle periodogram. A new formalism for the floating-mean and Keplerian periodograms

TL;DR: The Lomb-Scargle periodogram is a common tool in the frequency analysis of unequally spaced data equivalent to least-squares fitting of sine waves as discussed by the authors, and it can be used to detect eccentric orbits of exoplanets.
Proceedings ArticleDOI

CARMENES instrument overview

A. Quirrenbach, +132 more
- 10 Jul 2014 - 
TL;DR: CARMENES (Calar Alto high-resolution search for M dwarfs with Exoearths with Near-infrared and optical Echelle Spectrographs) is a next-generation radial-velocity instrument under construction for the 3.5m telescope at the Calar Alto Observatory by a consortium of eleven Spanish and German institutions as discussed by the authors.
Journal ArticleDOI

The CARMENES search for exoplanets around M dwarfs - High-resolution optical and near-infrared spectroscopy of 324 survey stars

Ansgar Reiners, +180 more
TL;DR: In this article, the CARMENES radial velocity (RV) survey is observing 324 M dwarfs to search for any orbiting planets and the authors present an atlas of high resolution M-dwarf spectra and compare the spectra to atmospheric models.
Journal ArticleDOI

The CARMENES search for exoplanets around M dwarfs: High-resolution optical and near-infrared spectroscopy of 324 survey stars

Ansgar Reiners, +172 more
TL;DR: In this paper, the authors present an atlas of high-resolution M-dwarf spectra and compare the spectra to atmospheric models and demonstrate that in this spectroscopic range, the large amount of absorption features compensates for the intrinsic faintness of an M7 star.