Zapis dokaza metode
Exoplanet Transmission Spectroscopy
Transmission spectroscopy is a technique for studying the atmospheres of exoplanets by analyzing the light passing through the planetary atmosphere during transit. Pioneered by David Charbonneau in 2002 with the detection of sodium in HD 209458b's atmosphere, this method has become the primary tool for characterizing exoplanet atmospheres and searching for biosignatures.
Izvorni zapis
Citati kopirani doslovno iz izvornog zapisa metode. Ne impliciraju nikakvu provjeru na razini tvrdnje.
Transmission Spectroscopy for Exoplanet Atmosphere Characterization
Taksonomski zapis metode · process-pipeline / astronomy
- Charbonneau, D., Brown, T. M., Noyes, R. W., & Gilliland, R. L. (2002). Detection of an atmospheric trace constituent in the transmission spectrum of a distant extrasolar planet. Astrophysical Journal, 568(1), 377-384. · DOI 10.1086/338770
- Kreidberg, L., et al. (2014). A precise water abundance measurement for the hot Jupiter WASP-43b. Astrophysical Journal Letters, 793(2), L15. · DOI 10.1088/2041-8205/793/2/l27
- Sing, D. K., et al. (2016). The atmospheric circulation of hot Jupiters. Nature, 529(7584), 59-62. · URL
Uređene tvrdnje
Tvrdnje pohranjene u knjigu dokaza, svaka s vlastitom procjenom.
Nema uređenih tvrdnji
Ovaj prikaz ne izmišlja procjenu tvrdnje kada knjiga dokaza nema nijednu.
Povezane metode
Generirano iz grafa metode i prikazano kao strojno predložene relacije — ne implicira se nikakva tvrdnja dokaza.