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PreprintCC BY 4.0arXiv

Exoplanet detection through photometric orbital phase modulations

  • J. Lillo-Box
  • O. Balsalobre-Ruza
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Abstract

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.

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Cite

BibTeXRIS
BibTeX
@misc{lillobox2026exoplanet,
  title = {{Exoplanet detection through photometric orbital phase modulations}},
  author = {J. Lillo-Box and O. Balsalobre-Ruza},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.20355},
  eprint = {2609.20355},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.20355},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Exoplanet detection through photometric orbital phase modulations
AU  - J. Lillo-Box
AU  - O. Balsalobre-Ruza
PY  - 2026
DA  - 2026/09/17
PB  - arXiv
DO  - 10.48550/arxiv.2609.20355
UR  - https://arxiv.org/abs/2609.20355
AB  - 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.
ER  -