First Planet Confirmation with the Exoplanet Tracker

J. C. Van Eyken, J. Ge, S. Mahadevan, C. DeWitt, D. Ren

Research output: Contribution to journalConference article

4 Scopus citations

Abstract

The Exoplanet Tracker (ET) is a new concept of instrument for measuring stellar radial velocity variations. ET is based on a dispersed fixed-delay interferometer, a combination of Michelson interferometer and medium resolution (R ∼ 6700) spectrograph which overlays interferometer fringes on a long-slit stellar spectrum. By measuring shifts in the fringes rather than the Doppler shifts in the absorption lines themselves, we are able to make accurate stellar radial velocity measurements with a high throughput and low cost instrument. The single-order operation of the instrument can also in principle allow multi-object observations. We plan eventually to conduct deep large scale surveys for extra-solar planets using this technique. We present confirmation of the planetary companion to 51Peg from our first stellar observations at the Kitt Peak 2.1m telescope, showing results consistent with previous observations. We outline the fundamentals of the instrument, and summarize our current progress in terms of accuracy and throughput.

Original languageEnglish (US)
Pages (from-to)250-261
Number of pages12
JournalProceedings of SPIE - The International Society for Optical Engineering
Volume5170
DOIs
StatePublished - Dec 1 2003
EventTechniques and Instrumentation for Detection of Exoplants - San Diego, CA, United States
Duration: Aug 5 2003Aug 7 2003

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All Science Journal Classification (ASJC) codes

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

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