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The detection of a high energy muon neutrino on 22 September 2017 by IceCubeneutrino detector coincides with the multiwavelength flaring from the BL Lacobject TXS 0506+056, most likely confirming AGN as a source of high energycosmic rays and neutrinos. Using the photohadronic model, we have explained thevery high energy $\gamma$-rays observed by MAGIC telescopes few days after theneutrino event and extend the model to calculate the neutrino flux at differentwindows consistent with the flaring period of TXS 0506+056 and compared withthe IceCube and MAGIC estimates. We also use this model to estimate theneutrino flux from the flaring of FSRQ PKS B1424-418 which is believed to beassociated with the 2 PeV neutrino event observed by IceCube.

Photohadronic model for the neutrino and $\gamma$-ray emission from TXS 0506+056