方法证据记录
Transit Photometry
Transit photometry is an observational technique that detects exoplanets by monitoring the periodic dips in stellar brightness as planets cross in front of their host stars. First systematized by William Borucki in 1984, this method became the most successful exoplanet detection technique, with the Kepler space telescope discovering thousands of confirmed exoplanets using this approach.
源记录
引文逐字复制自方法源记录。这些引文不代表任何层级的验证。
Transit Photometry Method for Exoplanet Detection
分类方法记录 · process-pipeline / astronomy
- Borucki, W. J., & Summers, A. L. (1984). The photometric method of detecting other planetary systems. Astrophysical Journal, 281, 537-553. · DOI 10.1016/0019-1035(84)90102-7
- Fressin, F., et al. (2013). The false positive rate for Kepler and the validation of Kepler objects of interest. Astrophysical Journal, 766(2), 81. · URL
- Charbonneau, D., Brown, T. M., Latham, D. W., & Mayor, M. (2000). Detection of planetary transits across a sun-like star. Astrophysical Journal, 529(1), L45-L48. · DOI 10.1086/312457
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