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The transit timing variation technique (TTV) has been widely used to detect and characterize multiple planetary systems. Due to the observational biases imposed mainly by the photometric conditions and instrumentation and the high…

地球与行星天体物理 · 物理学 2016-07-14 C. von Essen , S. Cellone , M. Mallonn , B. Tingley , M. Marcussen

One of the persistent complications in searches for transiting exoplanets is the low percentage of the detected candidates that ultimately prove to be planets, which significantly increases the load on the telescopes used for the follow-up…

地球与行星天体物理 · 物理学 2011-01-12 Brandon Tingley , Aldo Bonomo , Hans-Jörg Deeg

In the effort to characterize the masses, radii, and atmospheres of potentially habitable exoplanets, there is an urgent need to find examples of such planets transiting nearby M dwarfs. The MEarth Project is an ongoing effort to do so, as…

地球与行星天体物理 · 物理学 2015-06-05 Zachory K. Berta , Jonathan Irwin , David Charbonneau , Christopher J. Burke , Emilio E. Falco

PLATO will discover exoplanets around Sun-like stars through transit photometry and characterize their host stars using asteroseismology. Since photometry for most PLATO targets will be extracted on board, an efficient strategy to detect…

地球与行星天体物理 · 物理学 2026-03-04 F. Gutiérrez-Canales , R. Samadi , A. Birch , J. Cabrera , C. Damiani , P. Guterman , C. Paproth , M. Pertenais , A. Santerne

We present a comparison of two methods of fitting solar-like variability to increase the efficiency of detection of Earth-like planetary transits across the disk of a Sun-like star. One of them is the harmonic fitting method that coupled…

天体物理学 · 物理学 2009-11-13 A. S. Bonomo , A. F. Lanza

Since 2008 we have run an observational program to accurately measure the characteristics of known exoplanet systems hosting close-in transiting giant planets, i.e. hot Jupiters. Our study is based on high-quality photometric follow-up…

地球与行星天体物理 · 物理学 2016-05-19 Luigi Mancini , John Southworth

We present a fast, efficient and easy to apply computational method for the detection of planetary transits in large photometric datasets. The code has been specifically produced to analyse an ensemble of 21,950 stars in the globular…

天体物理学 · 物理学 2009-11-10 David T. F Weldrake , Penny D Sackett

Pedestrian detection in intelligent transportation systems has made significant progress but faces two critical challenges: (1) insufficient fusion of complementary information between visible and infrared spectra, particularly in complex…

计算机视觉与模式识别 · 计算机科学 2025-02-25 Rui Zhao , Zeyu Zhang , Yi Xu , Yi Yao , Yan Huang , Wenxin Zhang , Zirui Song , Xiuying Chen , Yang Zhao

Photometric observations of exoplanet transits can be used to derive the orbital and physical parameters of an exoplanet. We analyzed several transit light curves of exoplanets that are suitable for ground-based observations whose complete…

We present an algorithm that can detect blends of bright stars with fainter, un-associated eclipsing binaries. Such systems contaminate searches for transiting planets, in particular in crowded fields where blends are common. Spectroscopic…

天体物理学 · 物理学 2009-11-10 Henk Hoekstra , Yanqin Wu , Andrzej Udalski

Despite the ever-growing number of exoplanets discovered and the extensive analyses carried out to find their potential satellites, only two exomoon candidates, Kepler-1625b-i and Kepler-1708 b-i, have been discovered to date. A…

地球与行星天体物理 · 物理学 2023-11-09 Sz. Kálmán , Sz. Csizmadia , A. E. Simon , K. W. F. Lam , A. Deline , J. -V. Harre , Gy. M. Szabó

This paper describes a simple activity for plotting and characterizing the light curve from an exoplanet transit event by way of differential photometry analysis. Using free digital imaging software, participants analyse a series of…

物理教育 · 物理学 2015-09-04 Michael Cowley , Stephen Hughes

Measuring the stellar rotation of one of the components in eclipsing binaries (EBs) or planetary systems is a challenging task. The difficulty is mainly due to the complexity of analyzing, in the same light curve, the signal from the…

A machine learning technique with two-dimension convolutional neural network is proposed for detecting exoplanet transits. To test this new method, five different types of deep learning models with or without folding are constructed and…

地球与行星天体物理 · 物理学 2019-05-15 Pattana Chintarungruangchai , Ing-Guey Jiang

To address the the problem of calibration of instrument systematics in transit light curves, we present the Python package ExoTiC-ISM. Transit spectroscopy can reveal many different chemical components in exoplanet atmospheres, but such…

天体物理仪器与方法 · 物理学 2020-07-16 Iva Laginja , Hannah R. Wakeford

The Burst Observer and Optical Transient Exploring System (BOOTES) is a network of telescopes that allows the continuous monitoring of transient astrophysical sources. It was originally devoted to the study of the optical emission from…

天体物理仪器与方法 · 物理学 2014-08-20 M. D. Caballero-Garcia , M. Jelinek , A. Castro-Tirado , R. Hudec , R. Cunniffe , O. Rabaza , L. Sabau-Graziati

A large fraction of the smallest transiting planet candidates discovered by the Kepler and CoRoT space missions cannot be confirmed by a dynamical measurement of the mass using currently available observing facilities. To establish their…

地球与行星天体物理 · 物理学 2014-05-30 Rodrigo F. Díaz , José M. Almenara , Alexandre Santerne , Claire Moutou , Anthony Lethuillier , Magali Deleuil

We present the Signal Detection using Random-Forest Algorithm (SIDRA). SIDRA is a detection and classification algorithm based on the Machine Learning technique (Random Forest). The goal of this paper is to show the power of SIDRA for quick…

地球与行星天体物理 · 物理学 2015-11-12 D. Mislis , E. Bachelet , K. A. Alsubai , D. M. Bramich , N. Parley

The Hubble Space Telescope (HST) and the Kepler space mission observed a large number of planetary transits showing anomalies due to starspot eclipses, with more such observations expected in the near future by the K2 mission and the…

地球与行星天体物理 · 物理学 2014-07-18 Bence Béky , David M. Kipping , Matthew J. Holman

Reliable estimations of ephemeris errors are fundamental for the follow-up of CoRoT candidates. An equation for the precision of minimum times, originally developed for eclipsing binaries, has been optimized for CoRoT photometry and been…

地球与行星天体物理 · 物理学 2012-06-07 H. J. Deeg , M. Seidel , the Corot Photometric Follow-Up Team