Gost Na Asu Tp -

The is for high-resolution optical spectroscopy. It studies exoplanet atmospheres to determine the vertical thermal structure, or T-P profile .

: GHOST covers a wide wavelength range from 363 to 950 nm. This lets researchers detect different chemical species and thermal features in one observation. gost na asu tp

: Researchers use the GHOST Data Reduction Pipeline to process raw spectra. This removes instrumental noise and "telluric" (Earth's atmospheric) interference to isolate the planetary signal. The is for high-resolution optical spectroscopy

A technical report or academic write-up on this topic could use the following structure: gost na asu tp

: Define the exoplanet (e.g., WASP-189 b) and the use of high-resolution spectroscopy for atmospheric characterization.