A hot Jupiter transiting a mid-K dwarf found in the pre-OmegaCam Transit Survey

Autor(en)
J. Koppenhoefer, Roberto P Saglia, Luca Fossati, Miguel Anibal Verdugo Olivares, Y. Lyubchik, Markus Mugrauer, Ralf Bender, Chi-Hon Lee, A. Riffeser, P. Afonso, Jochen Greiner, Thomas Henning, Ralph Neuhäuser, I. A. G. Snellen, Y. Pavlenko, N. Vogt
Abstrakt

We describe the pre-OmegaTranS project, a deep survey for transiting extra-solar planets in the Carina region of the Galactic disc. In 2006–2008, we observed a single dense stellar field with a very high cadence of ∼2 min using the European Southern Observatory Wide Field Imager at the La Silla Observatory.

Using the Astronomical Wide-field Imaging System for Europe environment and the Munich Difference Imaging Analysis pipeline, a module that has been developed for this project, we created the light curves of 16 000 stars with more than 4000 data points which we searched for periodic transit signals using a box-fitting least-squares detection algorithm. All light curves are publicly available. In the course of the pre-OmegaTranS project, we identified two planet candidates – POTS-1b and POTS-C2b – which we present in this work.

With extensive follow-up observations we were able to confirm one of them, POTS-1b, a hot Jupiter transiting a mid-K dwarf. The planet has a mass of 2.31 ± 0.77 MJup, a radius of 0.94 ± 0.04 RJup and a period of P = 3.16 d. The host star POTS-1 has a radius of 0.59 ± 0.02 R⊙ and a mass of 0.70 ± 0.05 M⊙. Due to its low apparent brightness of I = 16.1 mag, the follow-up and confirmation of POTS-1b was particularly challenging and costly.

Organisation(en)
Institut für Astrophysik
Externe Organisation(en)
Max-Planck-Institut für extraterrestrische Physik, Ludwig-Maximilians-Universität München, Rheinische Friedrich-Wilhelms-Universität Bonn, National Academy of Sciences of Ukraine (NASU), American River College, Leiden University, Universidad de Valparaíso, Friedrich-Schiller-Universität Jena, Max-Planck-Institut für Astronomie
Journal
Monthly Notices of the Royal Astronomical Society
Band
435
Seiten
3133-3147
Anzahl der Seiten
14
ISSN
0035-8711
DOI
https://doi.org/10.1093/mnras/stt1512
Publikationsdatum
09-2013
Peer-reviewed
Ja
ÖFOS 2012
103004 Astrophysik, 103003 Astronomie
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/4570254b-2ffd-46c5-8062-00633e9bbeb2