Characterising stellar micro-variability for planetary transit searches
A method for simulating light curves containing stellar micro-variability for a range of spectral types and ages is presented. It is based on parameter-by-parameter scaling of a multi-component fit to the solar irradiance power spectrum (based on VIRGO/PMO6 data), and scaling laws derived from groun...
| Main Authors: | , , |
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| Format: | Journal article |
| Language: | English |
| Published: |
2004
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