most citedGaia's potential for the discovery of circumbinary planets

73 citations · 164 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR201473 cited

Gaia's potential for the discovery of circumbinary planets

Johannes Sahlmann, Amaury H. M. J. Triaud, David V. Martin

The abundance and properties of planets orbiting binary stars - circumbinary planets - are largely unknown because they are difficult to detect with currently available techniques.…

astro-ph.IM201413 cited

Gaia on-board metrology: basic angle and best focus

A. Mora, M. Biermann, A. G. A. Brown +21

The Gaia payload ensures maximum passive stability using a single material, SiC, for most of its elements. Dedicated metrology instruments are, however, required to carry out two f…

astro-ph.EP2014

Astrometric planet search around M8--L2 dwarfs from the ground and with Gaia

J. Sahlmann, P. F. Lazorenko, D. Segransan +4

Ultra-cool dwarfs are very low-mass stars or brown dwarfs and because of their faintness they are difficult targets for radial velocity and transit planet searches. High-precision…

astro-ph.IM20147 cited

Mid-infrared interferometry with K band fringe-tracking I. The VLTI MIDI+FSU experiment

A. Müller, J. -U. Pott, A. Mérand +11

Context: A turbulent atmosphere causes atmospheric piston variations leading to rapid changes in the optical path difference of an interferometer, which causes correlated flux loss…

astro-ph.SR201418 cited

Astrometric planet search around southern ultracool dwarfs II: Astrometric reduction methods and a deep astrometric catalogue

P. F. Lazorenko, J. Sahlmann, D. Segransan +4

We describe the astrometric reduction of images obtained with the FORS2/VLT camera in the framework of an astrometric planet search around 20 M/L-transition dwarfs. We present the…

astro-ph.SR201453 cited

Astrometric planet search around southern ultracool dwarfs I: First results, including parallaxes of 20 M8-L2 dwarfs

J. Sahlmann, P. F. Lazorenko, D. Segransan +4

Extrasolar planet searches targeting very low-mass stars and brown dwarfs are hampered by intrinsic or instrumental limitations. Time series of astrometric measurements with precis…