Exoplanet Transit Database. Reduction and processing of the photometric data of exoplanet transits

被引：107
|
作者：
Poddany, Stanislav [1 ,2 ]
Brat, Lubos
Pejcha, Ondrej [3 ]
机构：
[1] Charles Univ Prague, Astron Inst, Fac Math & Phys, CZ-18000 Prague 8, Czech Republic
[2] Stefanik Observ, CZ-11846 Prague 1, Czech Republic
[3] Ohio State Univ, Dept Astron, Columbus, OH 43210 USA
来源：
NEW ASTRONOMY | 2010年 / 15卷 / 03期
关键词：
Exoplanets; Planetary systems; Techniques: photometric; Database; PLANETS; PARAMETERS;
D O I：
10.1016/j.newast.2009.09.001
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We demonstrate the newly developed resource for exoplanet researchers - The Exoplanet Transit Database. This database is designed to be a web application and it is open for any exoplanet observer. It came on-line in September 2008. The ETD consists of three individual sections. One serves for predictions of the transits, the second one for processing and uploading new data from the observers. We use a simple analytical model of the transit to calculate the central time of transit, its duration and the depth of the transit. These Values are then plotted into the observed-computed diagrams (O-C), that represent the last part of the application. (C) 2009 Elsevier B.V. All rights reserved.
引用
收藏
页码：297 / 301
页数：5
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