activity
20092024
most citedThe slow spin of the young sub-stellar companion GQ Lupi b and its orbital configuration

98 citations · 895 across the 37 of their papers we have counts for

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Showing 2016Show all

6 papers · 1 filter

astro-ph.SR2016★ 13 cited

Long-Term Photometry of IC 348 with the YETI Network

D. J. Fritzewski, M. Kitze, M. Mugrauer +29

We present long-term photometric observations of the young open cluster IC 348 with a baseline time-scale of 2.4 yr. Our study was conducted with several telescopes from the Young…

astro-ph.EP2016★ 98 cited

The slow spin of the young sub-stellar companion GQ Lupi b and its orbital configuration

Henriette Schwarz, Christian Ginski, Remco J. de Kok +3

The spin of a planet or brown dwarf is related to the accretion process, and therefore studying spin can help promote our understanding of the formation of such objects. We present…

astro-ph.EP2016★ 11 cited

Direct Imaging discovery of a second planet candidate around the possibly transiting planet host CVSO 30

T. O. B. Schmidt, R. Neuhäuser, C. Briceño +11

We surveyed the 25 Ori association for direct-imaging companions. This association has an age of only few million years. Among other targets, we observed CVSO 30, which has recentl…

astro-ph.EP2016★ 18 cited

YETI observations of the young transiting planet candidate CVSO 30 b

St. Raetz, T. O. B. Schmidt, S. Czesla +32

CVSO 30 is a unique young low-mass system, because, for the first time, a close-in transiting and a wide directly imaged planet candidates are found around a common host star. The…

astro-ph.EP2016★ 4 cited

Search for transiting exoplanets and variable stars in the open cluster NGC 7243

Z. Garai, T. Pribulla, L. Hambálek +23

We report results of the first five observing campaigns for the open stellar cluster NGC 7243 in the frame of project Young Exoplanet Transit Initiative (YETI). The project focuses…

astro-ph.SR2016★ 47 cited

A lucky imaging multiplicity study of exoplanet host stars II

C. Ginski, M. Mugrauer, M. Seeliger +6

The vast majority of extrasolar planets are detected by indirect detection methods such as transit monitoring and radial velocity measurements. While these methods are very success…