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We perform a search for sources of gamma-rays with energies E>100 GeV at lowGalactic latitudes |b|<10 deg using the data of Fermi telescope. To separatecompact gamma-ray sources from the diffuse emission from the Galaxy, we use theMinimal Spanning Tree method with threshold of 5 events in inner Galaxy(Galactic longitude |l|<60 deg) and of 3 events in outer Galaxy. Using thismethod, we identify 22 clusters of very-high-energy (VHE) gamma-rays, which weconsider as "source candidates". 3 out of 22 event clusters are expected to beproduced in result of random coincidences of arrival directions of diffusebackground photons. To distinguish clusters of VHE events produced by realsources from the background we perform likelihood analysis on each sourcecandidate. We present a list of 19 higher significance sources for which thelikelihood analysis in the energy band E>100 GeV gives Test Statistics (TS)values above 25. Only 10 out of the 19 high-significance sources can be readilyidentified with previously known VHE gamma-ray sources. 4 sources could beparts of extended emission from known VHE gamma-ray sources. Five sources arenew detections in the VHE band. Among these new detections we tentativelyidentify one source as a possible extragalactic source PMN J1603-4904 (a blazarcandidate), one as a pulsar wind nebula around PSR J1828-1007. Highsignificance cluster of VHE events is also found at the position of a sourcecoincident with the Eta Carinae nebula. In the Galactic Center region, strongVHE gamma-ray signal is detected from Sgr C molecular cloud, but not from theGalactic Center itself.

Galactic sources of E>100 GeV gamma-rays seen by Fermi telescope