Characterization of a multi-etalon array for ultra-high resolution spectroscopy

The upcoming Extremely Large Telescopes (ELTs) are expected to have the collecting area required to detect potential biosignature gases in the atmosphere of rocky planets around nearby low-mass stars. Some efforts are currently focusing on searching for molecular oxygen (O2), since O2 is a known bio...

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Veröffentlicht in:	arXiv.org 2020-12
Hauptverfasser:	Rukdee, Surangkhana, Ben-Ami, Sagi, Szentgyorgyi, Andrew, López-Morales, Mercedes, Charbonneau, David, García-Mejía, Juliana
Format:	Artikel
Sprache:	eng
Schlagworte:	Arrays Celestial bodies Earth analogs Etalons Extrasolar planets Extremely large telescopes High resolution Low mass stars Oxygen Resolution Spectral resolution Spectrographs Spectroscopic telescopes Spectroscopy Spectrum analysis Terrestrial planets
Online-Zugang:	Volltext
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