Measuring the color dependent Rossiter-McLaughlin effect from 0.38 to 1.71 micrometer using ground based observations

Mahmoudreza Oshagh - Instituto de Astrofísica de Canarias (IAC)Dec 16, 2020
Atmospheric characterization
Instrumentation & Observational techniques
Chromatic Rossiter-McLaughlin, Transmission spectroscopy, HD 189733b, stellar activity, SOAP
Transmission spectroscopy has been proven to be the most powerful technique in detecting and characterizing atmospheres of exoplanets. So far, mostly ground and space-based multi-band transit photometry have been used to retrieve the exoplanets' broadband transmission spectra. An alternative technique has been proposed for retrieving the broadband transmission spectra using ...
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