ToO observations of flaring AGNs based on optical comma X-ray and I-ray triggers

We ask for ToO observations of flaring AGNs. The scientific motivations aremany: they provide unprecedented photon statistics, valuable for both scopingthe intrinsic spectra and variability of AGN and competing models for those(onezone or twozones, leptonic or hadronic) as well as detecting new VHEgammaray emitting sources (e.g. FSRQs, gravitationally lensed quasars) andsource classes (e.g. NlSy1), that can only be detected during bright flares. Wewill take triggers from: 1. Optical (Tuorla blazar monitoring program) 2. SWIFT(GCN/ATel alerts) or MAXI (ATel) 3. FermiLAT (MAGIC internal analysis chain andpriv. comm.) 4. VHE I?rays flare based on MAGIC/VERITAS/H.E.S.S./HAWC/FACT5.VHE I?ray flare seen by MAGIC (selftrigger) 6. Fast rise/decay seen by FACT 7. ATel/GCN. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]