089140

We ask for ToO observations of flaring AGNs. The scientific motivations are many: they provide unprecedented photon statistics valuable for both scoping the intrinsic spectra and variability of AGN and competing models for those (one-zone or two-zones leptonic or hadronic) as well as detecting new VHE gamma-ray emitting sources (e.g. FSRQs gravitationally lensed quasars) and source classes (e.g. NlSy1) that can only be detected during bright flares. We will take triggers from: 1. Optical (Tuorla blazar monitoring program) 2. SWIFT (GCN/ATel alerts) or MAXI (ATel) 3. Fermi-LAT (MAGIC internal analysis chain and priv. comm.) 4. VHE I?-rays flare based on MAGIC/VERITAS/H.E.S.S./HAWC/FACT 5.VHE I?-ray flare seen by MAGIC (self-trigger) 6. Fast rise/decay seen by FACT 7. ATel/GCN. [truncated! Please see actual data for full text]