Level 1A BepiColombo/PHEBUS EUV observations data of the disk-integrated solar reflected light from the Mercury surface

On October 9th and 10th 2021, nine days after the first flyby of Mercury by the ESA-JAXA mission BepiColombo, the EUV spectrograph of Probing the Hermean Exosphere by UV Spectroscopy (PHEBUS) instrument aboard BepiColombo observed the disk-integrated solar reflected light from the surface of Mercury between 90 and 160 nm at a distance of 4.5 million kilometers. These observations are used to derive the EUV reflectance of the surface of Mercury in this wavelength range for the first time since the Mariner 10 observations in 1974-1975. This dataset contains the partially processed (level 1A) science data version 0.1 of these observations, compliant with the PDS4 archiving standard format (i.e data that have been processed beyond the raw stage but which have not yet reached calibrated status). Data from other observations possible at several periods during the rest of the cruise may be added later. Note: version 0.1 is the unofficial version of Phebus data maintained and archived by the PHEBUS team before data ingestion into the ESA Planetary Science Archive (PSA).