High Energy Sources Observed with OMC

TL;DR

This paper reports on optical observations of high-energy sources using the INTEGRAL OMC, providing flux measurements, light curves, and identifying optical counterparts, including new ones, for various high-energy objects.

Contribution

It presents the first optical fluxes, light curves, and counterpart identifications for high-energy sources observed by INTEGRAL OMC, including new counterpart discoveries.

Findings

Detected optical counterparts for multiple high-energy sources.

Provided V-band fluxes and light curves for these sources.

Identified new optical counterparts where previously unknown.

Abstract

The INTEGRAL Optical Monitoring Camera, OMC, has detected many high energy sources. We have obtained V-band fluxes and light curves for their counterparts. In the cases of previously unknown counterparts, we have searched for characteristic variations in optical sources around the high-energy target position. Results about the Galactic Bulge Monitoring, INTEGRAL Gamma-Ray sources (IGR), and other high energy sources are presented.