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Exoplanet Detection by Astrometric Method
Bibcode: 2016AcASn..57..422X

Xu, W. W.; Liao, X. H.; Zhou, Y. H. +1 more

As we known, the exoplanets are mostly detected by the methods of radial velocity and transit, only one is found by the astrometric method. As the data of the gaia to be released, astrometry will become one of the most important method for detecting exoplanets gradually. Based on the position sequence of stars, this paper discusses the calculation…

2016 Acta Astronomica Sinica
Gaia 6
Analogue Simulation and Orbital Solving Algorithm of Astrometric Exoplanet Detection
Bibcode: 2016AcASn..57..568H

Ji, J. H.; Huang, P. H.

Astrometry is an effective method to detect exoplanets. It has many advantages that other detection methods do not bear, such as providing three dimensional planetary orbit and determining the planetary mass. Astrometry will enrich the sample of exoplanets. As the high-precision astrometric satellite Gaia (Global Astrometry interferometer for Astr…

2016 Acta Astronomica Sinica
Gaia 4
Identifying and Tracking Solar Photospheric Bright Points Based on Three-dimensional Segmentation Technology
Bibcode: 2016AcASn..57...29X

Feng, S.; Ji, K. F.; Xiong, J. P. +3 more

Photospheric bright points (PBPs) are tiny and short-lived phenomena which can be seen within dark inter-granular lanes. In this paper, we develop a new method to identify and track the PBPs in the three-dimensional data cube. Different from the previous way such as Detection-Before-Tracking, this method is based on the Tracking-While-Detection. U…

2016 Acta Astronomica Sinica
Hinode 1