Achieving high-precision ground-based photometry for transiting exoplanets

Olivier Guyon, Frantz Martinache

Research output: Chapter in Book/Report/Conference proceedingConference contribution

1 Citation (Scopus)

Abstract

Detection of transiting exoplanets requires high precision photometry, at the percent level for giant planets and at the 1e-5 level for detection of Earth-like rocky planets. Space provides an ideally stable - but costly - environment for high precision photometry. Achieving high precision photometry on a large number of sources from the ground is scientifically valuable, but also very challenging, due to multiple sources of errors. These errors can be greatly reduced if a large number of small wide field telescopes is used with an adequate data analysis algorithm, and the recent availability of low cost high performance digital single lens reflex (DSLR) cameras thus provides an interesting opportunity for exoplanet transit detection. We have recently assembled a prototype DSLR-based robotic imaging system for astronomy, showing that robotic high imaging quality units can be build at a small cost (under $10000 per deg2m2 of etendue), allowing multiple units to be built and operated. We demonstrate that a newly developed data reduction algorithm can overcome detector sampling and color issues, and allow precision photometry with these systems, approaching the limit set by photon noise and scintillation noise - which can both average as the inverse square root of etendue. We conclude that for identification of a large number of exoplanets, a ground-based distributed system consisting of a large number of DSLR-based units is a scientifically valuable cost-effective approach.

Original languageEnglish (US)
Title of host publicationProceedings of SPIE - The International Society for Optical Engineering
Volume8151
DOIs
StatePublished - 2011
EventTechniques and Instrumentation for Detection of Exoplanets V - San Diego, CA, United States
Duration: Aug 23 2011Aug 24 2011

Other

OtherTechniques and Instrumentation for Detection of Exoplanets V
CountryUnited States
CitySan Diego, CA
Period8/23/118/24/11

Fingerprint

Photometry
Exoplanets
extrasolar planets
reflexes
photometry
Lens
lenses
Planets
robotics
Unit
Robotics
planets
Lenses
Camera lenses
costs
Costs
Scintillation
Astronomy
Data Reduction
Limit Set

Keywords

  • Exoplanets
  • Photometry

ASJC Scopus subject areas

  • Applied Mathematics
  • Computer Science Applications
  • Electrical and Electronic Engineering
  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics

Cite this

Guyon, O., & Martinache, F. (2011). Achieving high-precision ground-based photometry for transiting exoplanets. In Proceedings of SPIE - The International Society for Optical Engineering (Vol. 8151). [81511C] https://doi.org/10.1117/12.894321

Achieving high-precision ground-based photometry for transiting exoplanets. / Guyon, Olivier; Martinache, Frantz.

Proceedings of SPIE - The International Society for Optical Engineering. Vol. 8151 2011. 81511C.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Guyon, O & Martinache, F 2011, Achieving high-precision ground-based photometry for transiting exoplanets. in Proceedings of SPIE - The International Society for Optical Engineering. vol. 8151, 81511C, Techniques and Instrumentation for Detection of Exoplanets V, San Diego, CA, United States, 8/23/11. https://doi.org/10.1117/12.894321
Guyon O, Martinache F. Achieving high-precision ground-based photometry for transiting exoplanets. In Proceedings of SPIE - The International Society for Optical Engineering. Vol. 8151. 2011. 81511C https://doi.org/10.1117/12.894321
Guyon, Olivier ; Martinache, Frantz. / Achieving high-precision ground-based photometry for transiting exoplanets. Proceedings of SPIE - The International Society for Optical Engineering. Vol. 8151 2011.
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