Using the Rossiter–McLaughlin Effect to Observe the Transmission Spectrum of Earth’s Atmosphere
Due to stellar rotation, the observed radial velocity of a star varies during the transit of a planet across its surface, a phenomenon known as the Rossiter–McLaughlin (RM) effect. The amplitude of the RM effect is related to the radius of the planet which, because of differential absorption in the planetary atmosphere, depends on wavelength
Yan, F. et al.
Fecha de publicación:
6
2015