Unveiling the nature of INTEGRAL objects through optical spectroscopy - X. A new multi-year, multi-observatory campaign

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Fig. 2

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Similar to Fig. 1 but for nine more INTEGRAL sources of our sample (see Table 1). For IGR J16058−7253 (bottom right panel), we indicate the two optical objects likely responsible for the total hard X-ray emission detected for this source (see Landi et al. 2012b and Sect. 4.1 of this paper).

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