Multiwavelength light curve of PKS 1510–089 between 2012 and 2017. From top to bottom panels: Fermi-LAT flux above 1 GeV; Swift-XRT flux 2–10 keV; U band flux from UVOT; KVA, SMARTS and MAPCAT optical flux in R-band; IR flux from REM and SMARTS in J band; radio 229 GHz flux measured by POLAMI; radio 37 GHz flux measured by Metsähovi; 15 GHz flux measured by OVRO. The red points show the observations within 12 h (or 3 days for the radio measurements) when MAGIC data have been taken during the time that Fermi-LAT flux is above 3 × 10⁻⁸ cm⁻² s⁻¹, while the blue points are observations in time bins with Fermi-LAT flux below this flux value (i.e., the low-state sample). IR, optical and UV data have been dereddened using Schlafly & Finkbeiner (2011).