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The GAPS Programme at TNG
2022
Astronomy and Astrophysics
The detection of lines in emission in planetary atmospheres provides direct evidence of temperature inversion. We confirm the trend of ultra-hot Jupiters orbiting A-type stars that show temperature inversions on their daysides by detecting metals emission lines in the dayside of KELT-20b. We first detected the planetary emission by using the G2 stellar mask of the HARPS-N pipeline, which is mainly composed of neutral iron lines, as a template. Using neutral iron templates, we performed a
doi:10.1051/0004-6361/202142768
fatcat:mcealm5snfdvrctti6n4scj26e