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Table 3.

Results of the X-ray spectral fitting for ABC sources with a complex (non power-law) model.

Name ALMA Other name Object type Detector Model NH ΓX K ΓR KR kT KT E1 K1 E2 K2 χ2 (d.o.f.)
J0029+3456 B2 0026+34 AGN EPIC A * PL 0.47(28)
J0057+3021 NGC 0315 AGN ACIS PL+T 0.83(115)
EPIC PL+T 0.79(356)
J0111−7302 PMN J0111−7302 AGN EPIC PL+T 0.81(14)
J0242−2132 PKS 0240−217 QSO ACIS A * PL 0.88(37)
EPIC A * (PL+L) 0.80(969)
J0702−2841 NGC 2325 AGN EPIC PL+T 0.64(323)
J0758+3747 NGC 2484 QSO EPIC PL+T 0.57(360)
J0928−0409 PKS J0928−0408 QSO EPIC PL+L 1.18(8)
J1044+0655 PKS 1042+071 QSO ACIS PL+L 0.94(115)
J1109−3732 NGC 3557 AGN ACIS PL+T 0.60(9)
J1215−1731 PKS 1213−17 Blazar XRT A * (PL+R) > 7.79 < −2.63 < 0.01 0.86(9)
J1230+1223 M 87 AGN XRT PL+T 1.05(212)
ACIS PL+T 0.87(141)
EPIC A * (PL+T) 1.14(1153)
J1305−4928 NGC 4945 RS ACIS A * (T+R+L+L) 1.08(183)
EPIC A * (T+R+L+L) 0.90(227)
J1319−1239 NGC 5077 AGN ACIS PL+T 0.27(6)
J1321−4342 NGC 5090 RG EPIC A * (T+R) 0.66(189)
J1336−3357 IC 4296 AGN ACIS PL+T 0.78(89)
EPIC PL+T 0.69(392)
J1347+1217 PKS 1345+12 QSO ACIS A * (PL+L) 0.82(53)
J1553+2348 PKS 1551+23 QSO XRT A * PL 0.84(7)
J1558−1409 PKS 1555−140 AGN ACIS T 0.85(75)
EPIC PL+T 0.90(1434)
J1627−2426 PMN J1626−2426 AGN ACIS R+L+L −1.72∗ < 0.01 3.11∗ < 0.01 0.90(11)
J1711−3744 PMN J1711−3744 No type ACIS A * PL <28.93e4 1.10(22)
J1723−6500 NGC 6328 QSO EPIC A * PL 0.65(309)
J2033+2146 PKS 2031+21 QSO XRT A * PL 0.98(55)
J2157−6941 PKS 2153−69 QSO ACIS PL+T 0.88(272)
J2212−2518 CRATES J221220.71−251828.4 AGN ACIS P+T 0.30(16)

Notes. For each source we list the ALMA name (Name ALMA), the alternate name (Other name), the ABC type (Object type), and the X-ray detector (Detector). The column Model shows the model components used to fit the spectrum, namely an intrinsic photoelectric absorption component ZWABS (A), a power-law component (PL), a thermal component APEC (T), a gaussian line ZGAUSS (L), and a power law spectrum reflected from neutral material PEXRAV (R). We then list the intrinsic hydrogen column density (NH), the power-law spectral index (ΓX) and normalization K, the reflection component spectral index ΓR and normalization KR, the thermal component temperature (kT) and normalization KT, and the line(s) rest-frame energy (E1, E2) and normalization(s) (K1, K2). Finally, we list the fit χ2 and degrees of freedom (χ2, d.o.f.). NH is in 1022 cm−2. K is 10−4 keV cm−2 s−1. KR is 10−2 keV cm−2 s−1. kT, E1, and E2 are in keV. KT is 10−4 cm−5. K1 and K2 are in 10−4 cm−2 s−1. Parameters indicated with an asterisk (*) are unconstrained and fixed to their best fit value.

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