Compton-thick AGN in the 70-month Swift-BAT All-Sky Hard X-ray Survey: A Bayesian approach

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Table 1

Literature Compton-thick sources not confirmed by this work.

Name¹	Γ ²	N _H ³	EW _{FeK_α} ⁴	C/d.o.f.⁵	Reference⁶

2MASXJ03502377-5018354			–	58.3/59	Ricci et al. (2015)
CGCG420-015				134.28/135	Severgnini et al. (2011)
ESO565-G019			< 1000	66.2/72	Gandhi et al. (2013)
ESO406-G004			–	33.6/11	Ricci et al. (2015)
NGC 7582			<400	197.3/204	Rivers et al. (2015)
NGC 4939			–	204/211	Maiolino et al. (1998)
MRK 1210			< 233	415.16/521	Ohno et al. (2004)
NGC 1365				816.1/739	Risaliti et al. (2009)

Notes.

⁽¹⁾

Source name.

⁽²⁾

Photon index.

⁽³⁾

N_H value in units of 10²² cm^-2.

⁽⁴⁾

Equivalent width of the FeK_α line in units of eV.

⁽⁵⁾

C statistic value over degrees of freedom.

⁽⁶⁾

Previous evidence suggesting Compton thickness.

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