Combining laser frequency combs and iodine cell calibration techniques for Doppler detection of exoplanets
Exoplanets can be detected from a time series of stellar spectra by looking for small, periodic shifts in the absorption features that are consistent with Doppler shifts caused by the presence of an exoplanet, or multiple exoplanets, in the system. While hundreds of large exoplanets have already bee...
| Main Authors: | , , , |
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| Format: | Article |
| Language: | en_US |
| Published: |
SPIE - The International Society for Optical Engineering
2017
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| Subjects: | |
| Online Access: | http://hdl.handle.net/1721.1/110927 |