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Galactic PeVatrons are astrophysical sources accelerating particles up to afew PeV ($\sim$10$^{15}$ eV) energies. The primary signature of 100 TeV$\gamma$ rays may come from PeV protons or multi-hundred TeV (not PeV)electrons. The search for PeVatrons has been one of the key science topics forVERITAS and HAWC. In 2021, LHAASO detected 14 steady $\gamma$-ray sources withphoton energies above 100 TeV, up to 1.4 PeV. This provides a clear list ofPeVatron candidates for further study with VERITAS and HAWC. Most of thesesources contain possible source associations, such as supernova remnants,pulsar wind nebulae, and stellar clusters. However, two sources: LHAASOJ2108+5157 and LHAASO J0341+5258, do not have any such counterparts. Therefore,multiwavelength observations are required to identify the objects responsiblefor the UHE $\gamma$ rays, to understand the source morphology and association,and to shed light on the emission processes. Here, we will present the statusof VERITAS/HAWC observations and results for the LHAASO PeVatron candidateJ0341+5258, and also discuss the VERITAS PeVatron search in general.

Searching for TeV emission from LHAASO J0341+5258 with VERITAS and HAWC