Correction of telluric absorption lines is important during the data reduction of spectroscopic observations of astronomical targets. The popular tool Molecfit1, 2 creates synthetic telluric transmission spectra based on the LBLRTM radiative transfer code3 , the HITRAN database4 , available atmospheric profiles (temperature, humidity, pressure variation with altitude), and instrumental line spread functions. Significantly improved accuracy is reached by using atmospheric profiles obtained at the same time and location as the science observations. For 9 years, a Low Humidity And Temperature Profiling (LHATPRO) Radiometer has provided profiles towards zenith every minute at Paranal. In 2019 line-of-sight support was added with the radiometer slaved to each telescope in sequence. This approach allows blind correction of water vapor telluric lines, provided some conditions are met, reducing the need to observe telluric stars.
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