X-ray follow-up work on a set of unassociated sources listed in the Palermo Swift/BAT 100-month catalogue
Date Issued
2026
Author(s)
Abstract
In the following, we report on a preliminary study aimed at searching the X-ray counterpart to a set of still unassociated sources listed in the
Palermo Swift/BAT 100-month catalogue. By exploiting the capability of the X-ray telescope (XRT, 0.2-10 keV) onboard the Neil Gehrels Swift
Observatory to localise the sources with a positional accuracy of few arcseconds, the search for optical/UV, infrared, and radio counterparts is
more efficient and reliable. Each source is discussed in a dedicated section in which we report the log of the XRT observations, the likely
counterparts detected, their spectral behaviour, and their multi-wavelength properties.
Report number
366
Rights
open.access
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