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...

Deskribapen osoa

Xehetasun bibliografikoak
Egile Nagusiak: Aigrain, S, Favata, F, Gilmore, G
Formatua: Journal article
Hizkuntza:English
Argitaratua: 2004