通过光度轨道相位调制探测系外行星
Exoplanet detection through photometric orbital phase modulations
- Centro de Astrobiología (CAB), CSIC-INTA（天体生物学中心，西班牙国家技术研究委员会-国家航空航天技术研究所）
机构由 AI 辅助整理，请以论文原文为准。
AI总结：
本文综述了通过光度轨道相位调制探测系外行星的方法与方程，强调了其在传统技术难以覆盖领域的优势及未来前景。
AI中文摘要：
自从三十五年前首次探测到系外行星以来，探测信号的黎明主要由径向速度和凌星技术推动。然而，其他方法因其能够探索传统方法难以触及的特定领域而获得了显著关注。在本文中，我们聚焦于由行星引起的光度轨道相位调制，描述了相关方法和方程，并强调了它们的未来发展前景。
英文摘要：
Since the detection of the first extrasolar planets thirty-five years ago, the dawn in detected signals has been driven primarily by radial velocity and transit techniques. However, other methodologies have gained significant interest due to their ability to explore specific niches that are challenging to access with traditional approaches. In this article, we focus on the photometric orbital phase modulations induced by planets, describe the methodologies and equations and highlight their developments and prospects for the future.
