  The detection of the gravitational wave GW170817 defined a breakthrough in
multi-messenger astronomy. For the first time, a gravitational wave transient
detected by the Laser Interferometer Gravitational-Wave Observatory (LIGO) and
Virgo interferometer was associated with a faint electromagnetic gamma-ray
counterpart reported by the Gamma-ray Burst Monitor (GBM) aboard on the Fermi
satellite. GRB 170817A was followed up by an enormous observational campaign
covering a large fraction of the electromagnetic spectrum. In this work, we use
the data from High Altitude Water Cherenkov (HAWC) gamma-ray observatory to
search for very-high-energy (VHE) TeV photons in coincidence with the X-ray
emission from GRB 170817A. Since no counts were observed up to $\sim$120 days
after the trigger time, we derive and report the corresponding upper limits in
the energy range from 1 to 100 TeV. In addition, we extend the analysis to GRBs
with similar features proposed by A. von Kienlin.
