most citedTransit Timing Analysis in the HAT-P-32 system

51 citations · 143 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR201437 cited

Transit timing of TrES-2: a combined analysis of ground- and space-based photometry

St. Raetz, G. Maciejewski, Ch. Ginski +21

Homogeneous observations and careful analysis of transit light curves can lead to the identification of transit timing variations (TTVs). TrES-2 is one of few exoplanets, which off…

astro-ph.SR201414 cited

Superflares on the slowly rotating solar-type stars KIC10524994 and KIC07133671?

M. Kitze, R. Neuhäuser, V. Hambaryan +1

An investigation of the G-type stellar population with Kepler (as done by Maehara et al.) shows that less than 1 per cent of those stars show superflares. Due to the large pixel sc…

astro-ph.SR201451 cited

Transit Timing Analysis in the HAT-P-32 system

M. Seeliger, D. Dimitrov, D. Kjurkchieva +24

We present the results of 45 transit observations obtained for the transiting exoplanet HAT-P-32b. The transits have been observed using several telescopes mainly throughout the YE…

astro-ph.EP201421 cited

The search for transiting planets using the YETI network

R. Errmann, St. Raetz, M. Kitze +2

To search for young transiting planets in continuous light curves, we monitor young open clusters (2-200 Myr) with the YETI network. Here we report the first transiting candidates…

astro-ph.SR20148 cited

Investigation of a transiting planet candidate in Trumpler 37: an astrophysical false positive eclipsing spectroscopic binary star

R. Errmann, G. Torres, T. O. B. Schmidt +50

We report our investigation of the first transiting planet candidate from the YETI project in the young (~4 Myr old) open cluster Trumpler 37. The transit-like signal detected in t…

astro-ph.SR201212 cited

A Possible Detection of Occultation by a Proto-planetary Clump in GM Cephei

The YETI Collaboration, W. P. Chen, S. C. -L. Hu +41

GM Cep in the young (~4 Myr) open cluster Trumpler 37 has been known to be an abrupt variable and to have a circumstellar disk with very active accretion. Our monitoring observatio…