Here are the results of the 2018 LARGE campaign in terms of passes and NPs collected by the network. It appears that stations of the Russian network did not participate in the campaign (they only tracked GLONASS satellites), so they have not been included in the statistics.
We believe that the inferior tracking coverage of the Galileo constellation is to a great extent explained by the lower cross section of the retroreflector arrays relative to those mounted on the Glonass satellites. Our experience tracking these objects tells us that the LRAs mounted on the first Galileo spacecraft (Galileo 101-104) are obviously superior to the ones that suceeded them (Galileo 2XX). Among both the primary and secondary groups of Galileo targets there is one spacecraft carrying the first LRA versions (Galileo-102 and Galileo-103). Both of them have received significantly higher tracking coverage than the rest of spacecraft in their respective groups (~60% more NP data for Galileo-102, ~40% more NP data for Galileo-103). Meanwhile, the data yield for Galileo-103 and Galileo-104 is lower than for Glonass satellites by approximately 20% in terms of NP data. It must be noted that the LRAs onboard the Glonass satellites selected for the LARGE campaign have a higher cross section than the previously employed ones, and superior to those used in any of the Galileo constellation.
Except for Compass-M3, coverage for the Compass constellation has been low as a) the geosynchronous satellites are only partially visible from Europe (if at all); b) prediction quality for Compass-MS1 and MS2 is not adequate for intensive SLR tracking (http://sgf.rgo.ac.uk/forumNESC/index.php?topic=43.0).
(http://sgf.rgo.ac.uk/media/20180530_large_campaign.png)