  Active galactic nuclei (AGNs) are considered to be one of the most
appropriate sources of ultra high energy cosmic rays (UHECRs, $E \gtrsim
10^{18} \mathrm{~eV}$). Radiogalaxy Virgo A (M87) in the centre of a cluster of
galaxies Virgo Cluster (VC) can be a prominent source of UHECRs. We investigate
the possible contribution of Virgo A and the VC to the flux of events with
trans-GZK energies - extremely high energy cosmic rays (EHECRs) - from the
recent Auger and Telescope Array (TA) data sets ($E > 52 \mathrm{~EeV}$ and $E
> 57 \mathrm{~EeV}$, respectively). We simulate EHECR propagation from Virgo A
and the VC taking into account their deflections in galactic (GMF) and
extragalactic (EGMF) magnetic fields and show that there is no excess of EHECR
arrival directions from images of Virgo A/VC at different EHECR rigidities. By
means of event-by-event analysis we recover the extragalactic arrival
directions of EHECR events detected by Auger and TA for representative set of
nuclei H(p), He, N, Si, Fe, and find evidences of enhanced fluxes of N-Si-Fe
EHECRs from the Local Filament and Hot/Cold Spot regions. The Local Filament
with its enhanced magnetic field is an expected contributor to the UHECR flux
as the closest to the Earth last scattering centre, whereas Hot/Cold Spot
region is a part of a larger arc-like spot, possibly created by diffusively
spreading jet of UHECRs, accelerated in the relativistic jet of Virgo A during
a prominent nuclear outburst about 10 - 12 Myr ago.
