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A Possible New Transiting Planet

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TLDR
In this paper, a low-luminosity object transits were reported from the Optical Gravitational Lensing Experiment (OGLE), which may be caused by its unseen companion.
Abstract
Recently, 59 low-luminosity object transits were reported from the Optical Gravitational Lensing Experiment (OGLE). Our follow-up low-resolution spectroscopy of 16 candidates provided two objects, OGLE-TR-3 and OGLE-TR-10, which have companions with radii compatible with those of gas-giant planets. Further high-resolution spectroscopy revealed a very low velocity variation (<500m/s) of the host star OGLE-TR-3 which may be caused by its unseen companion. An analysis of the radial velocity and light curve results in M<2.5 M_jup, R<1.6 R_jup, and an orbital separation of about 5 R_sol, which makes it the planet with the shortest period known. This allows to identify the low-luminosity companion of OGLE-TR-3 as a possible new gas-giant planet. If confirmed, this makes OGLE-TR-3 together with OGLE-TR-56 the first extrasolar planets detected via their transit light curves.

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Journal ArticleDOI

Determining the Inclination of the Rotation Axis of a Sun-like Star

TL;DR: In this paper, the authors used Monte Carlo simulations to estimate the precision of the measurement of the inclination angle between the direction of the rotation axis of a pulsating Sun-like star and the line of sight.
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Expected Detection and False Alarm Rates for Transiting Jovian Planets

TL;DR: In this article, the detection rates of transiting Earth-sized planets were estimated for binary and multiple-star systems and of Jovian-mass extrasolar planets, and it was shown that the period distribution of the exoplanets is depressed for periods between 5 and 200 days.
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On the Star-Magnetosphere Interaction of Close-in Exoplanets

TL;DR: Numerical simulations using a resistive MHD code are performed in order to investigate the interaction of the magnetospheres of hot Jupiters (or close-in extrasolar giant planets) with the central host stars as discussed by the authors.
Journal ArticleDOI

Doppler follow-up of OGLE transiting companions in the Galactic Bulge

TL;DR: In this article, the authors conducted a radial velocity follow-up of 18 of the smallest transiting candidates in the OGLE-III survey (Optical Gravitational Lensing Experiment) to determine the true nature of these objects and to characterize their actual mass.
Journal ArticleDOI

Reassessing the radial-velocity evidence for planets around CoRoT-7

TL;DR: In this article, the authors revisited the published HARPS radial velocity measurements of the object, which were previously used to estimate the companion mass, but have been the subject of ongoing debate.
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