Vrba et al., 1995), and supplementing these data with our own deep optical observations of the [$\gamma$]{}–ray box GRB790613, we will show here that an object of blue optical candidate type for Geminga can, in principle, be detected in study of such an IPN [$\gamma$]{}–box in the three standard filters [*B, V, R*]{}.

In Section 2 the statement of a problem of the deep CCD photometric search for weak blue stellar–like objects in relatively small [$\gamma$]{}–ray boxes at the 6 m telescope is expounded. The obtained photometric data for the GRB790613 event field are adduced in Section 3.2. The method of photometric search for such objects in the [$\gamma$]{}–ray box GRB790613, which are “black body”–like by [*BVR*]{}, and the discussion of the results of deep optical observations of this box are presented in Section 3.3. The estimates of a probable value of proper motions per year for all objects up to $V = 25^m$ are presented in Section 3.4. Section 3.5 is devoted to some other interesting objects found in (or near) the region of localization of the GRB790613 event.

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I & II & III & IV & V & VI\
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23:13 & I 