Search for sources of primary cosmic radiation at energies above 1014 eV

The results obtained at the separate installation of the Tien Shan station, intended for continuous studies, are analyzed with the aim of searching for local sources of primary cosmic radiation (PCR) at energies of 1014 − 1015 eV. Arrival directions in equatorial coordinates are determined for 35 millions of recorded extensive air showers (EAS) from PCR. The directions where the standard deviation of the number of events exceeds a certain value are separated. These can be the directions along which neutral primary cosmic particles (γ-rays and others) come from PCR sources. Some directions coincide with the results of other installations and pulsar positions.