Open Access
Table A.1.
Sources analysed in this work.
Source name | Chandra | XMM-Newton | NuSTAR | |||
---|---|---|---|---|---|---|
OBSID | Exp. (s) | OBSID | Exp. (s) | OBSID | Exp. (s) | |
2MASXJ01500266-0725482 | - | - | 0200431101 | 11921 | 60360005002 | 30725 |
2MASXJ04405494-0822221 | - | - | 0890690401 | 18000 | 60701043002 | 30706 |
2MASXJ04524451-0312571 | - | - | 0307002501 | 18111 | - | - |
CGCG074-129 | - | - | 0822391201 | 13600 | - | - |
ESO018-G009 | - | - | 0805150401 | 19200 | 60362029002 | 28755 |
ESO420-0131 | 10393 | 12760 | - | - | 60668003002 | 108164 |
IC4769 | - | - | 0405380501 | 35013 | - | |
IC49952 | - | - | 0200430601 | 11912 | 60360003002 | 33998 |
NGC3094 | - | - | 0655380801 | 16918 | 60668001002 | 100823 |
NGC5990 | - | - | 0655380901 | 18918 | - | |
UGC01214 | - | - | 0200430701 | 11913 | 60360004002 | 31998 |
UGC04145 | - | - | 0763460201 | 18000 | - | - |
Notes.(1)For this source XMM-Newton observations where not available. Instead we made use of chandra data. (2)X-ray spectral analysis has been presented in Osorio-Clavijo et al. (2022). Here we repeated the analysis using spectral modeling suitable to the Compton-thick nature of the source.
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