  Baikal-GVD is a next generation, kilometer-scale neutrino telescope currently
under construction in Lake Baikal. GVD consists of multi-megaton subarrays
(clusters) and is designed for the detection of astrophysical neutrino fluxes
at energies from a few TeV up to 100 PeV. The large detector volume and modular
design of Baikal-GVD allows for the measurements of the astrophysical diffuse
neutrino flux to be performed already at early phases of the array
construction. We present here recent results of the measurements on the diffuse
cosmic neutrino flux obtained with the Baikal-GVD neutrino telescope using
cascade-like events.
