activity
20172020
most citedSpectrum radial velocity analyser (SERVAL). High-precision radial velocities and two alternative spectral indicators

469 citations · 743 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.EP202053 cited

The CARMENES search for exoplanets around M dwarfs. Measuring precise radial velocities in the near infrared: the example of the super-Earth CD Cet b

F. F. Bauer, M. Zechmeister, A. Kaminski +26

The high-resolution, dual channel, visible and near-infrared spectrograph CARMENES offers exciting opportunities for stellar and exoplanetary research on M dwarfs. In this work we…

astro-ph.EP2019

The CARMENES search for exoplanets around M dwarfs. Two temperate Earth-mass planet candidates around Teegarden's Star

M. Zechmeister, S. Dreizler, I. Ribas +182

Context. Teegarden's Star is the brightest and one of the nearest ultra-cool dwarfs in the solar neighbourhood. For its late spectral type (M7.0V), the star shows relatively little…

astro-ph.SR2019205 cited

The CARMENES search for exoplanets around M dwarfs: Different roads to radii and masses of the target stars

Andreas Schweitzer, V. M. Passegger, C. Cifuentes +28

We determine the radii and masses of 293 nearby, bright M dwarfs of the CARMENES survey. This is the first time that such a large and homogeneous high-resolution (R>80 000) spectro…

astro-ph.SR201916 cited

The CARMENES search for exoplanets around M dwarfs. Chromospheric modeling of M2-3 V stars with PHOENIX

D. Hintz, B. Fuhrmeister, S. Czesla +26

Chromospheric modeling of observed differences in stellar activity lines is imperative to fully understand the upper atmospheres of late-type stars. We present one-dimensional para…

astro-ph.IM2017469 cited

Spectrum radial velocity analyser (SERVAL). High-precision radial velocities and two alternative spectral indicators

M. Zechmeister, A. Reiners, P. J. Amado +18

Context: The CARMENES survey is a high-precision radial velocity (RV) programme that aims to detect Earth-like planets orbiting low-mass stars. Aims: We develop least-squares fitti…