ivo://CDS/P/Moon/Clementine-750nm-118mCDSFernique P.2018-01-17T15:01:00Z2019-05-21T07:04:00ZCDS Helpdeskcds-question@unistra.frThe MoonThe Clementine Ultraviolet/Visible (UVVIS) Version 2 mosaic is a grayscale data set representing the albedo (brightness of the lunar surface) as measured at the 750 nanometer (nm) wavelength by the UVVIS camera (Lee 2009). In late 2008, a revised 750nm mosaic (v. 2.0) was created at USGS to refine the locations of component images by using the latest geodetic control and projecting onto a topographic model of the lunar surface (Archinal 2006). The base map was radiometrically and geometrically controlled, photometrically modeled global image mosaic compiled using more than 43,000 images from the 750nm filter observations.https://alasky.cds.unistra.fr/Planets/CDS_P_Moon_Clementine-750nm-118mSurveyResearchIsDerivedFromPlanetary Data System, from USGS Astrogeology Science Center https://astrogeology.usgs.gov/search/map/Moon/Clementine/UVVIS/Lunar_Clementine_UVVIS_750nm_Global_Mosaic_118m_v2This HiPS is distributed under ODbL license by Unistra/CNRShttps://alasky.cds.unistra.fr/Planets/CDS_P_Moon_Clementine-750nm-118mhttps://alaskybis.cds.unistra.fr/Planets/CDS_P_Moon_Clementine-750nm-118m2.6485944761985715e-19 2.6485944761985715e-19https://alasky.cds.unistra.fr/Planets/CDS_P_Moon_Clementine-750nm-118m/Moc.fits