Identification of objects in the optical range in areas of hard radiation near red dwarf stars

TL;DR

This paper investigates optical objects near red dwarf stars in regions emitting TeV gamma radiation, aiming to identify potential sources and candidates through spectral analysis.

Contribution

It presents a method for localizing TeV gamma-ray sources in optical and X-ray ranges and suggests possible identifications with red dwarfs and other objects.

Findings

Distances from gamma-ray maxima to candidate red dwarfs are estimated.

Possible identifications of weaker TeV sources are proposed.

Localization regions for high-energy sources are analyzed.

Abstract

The analysis of the localization regions of TeV gamma-radiation sources in the X-ray and optical spectral ranges is carried out. The distances from the position of the maxima in the distribution of high-energy fluxes to the probable candidates for identification with red dwarfs are indicated. Possible identifications of weaker TeV sources and other field objects are also considered.