This bundle contains two sets of albedo maps, one from 2015, one from 2017. For each map the publication is provided. A summary of the data product is procided below. 

The first set is from 2015 (Vincendon et al., Icarus, 2015, doi: 10.1016/j.icarus.2014.10.029) and provides the data from figures 3, 4 and 9 of the article. Albedo is obtained by integrating OMEGA wavelengths to derive bolometric albedo from 0.43 μm and 2.5 μm (corresponds to 85% of the solar flux), UV contribution is extrapolated, aerosol contribution is accounted for. Corrections include aerosol contribution removal, and accounting for the non-lambertian surface behaviour. Maximum albedo coverage (98.5%) derived by averaging data from LS 330° MY26 to LS 135° MY30. Mismatches between observations are apparent due to surface albedo changes over the period and uncertainty in the aerosols correction. All maps are non polar extending up to +/- 60° in latitude, and generated either at 32 ppd (pixels per degree) or 8 ppd. Raster format is geotiff with real (float) values of the albedo. Maps with the following index "lev0", "lev1", "lev2" correspond to the quality level of the data, lev0 behind the highest (most reliable albedo retreival) and lev2 the lowest. Addtionally, more partial coverage maps are provided per season of several mars years: MY27, MY28, MY29 and MY30. The index "c/d" behind the MY indicates if the weather was "clear" or "dusty" for this particular MY. 
 
The second set if from 2017 (Audouard et al., 2017, LPSC Abstract #1980), it is also an OMEGA albedo map at 60 ppd (nearly 1km/pix at equator) and provides full (including polar) coverage. Two version exist, one with OMEGA data online showing some gaps (94.8% coverage), and another with full coverage using TES albedo data to fill in the OMEGA coverage gaps. Raster format is geotiff with real (float) values of the albedo.