Table 3.
Chandra J1030 spectral catalog.
XID | z | CNTS | log(NH) | Γ | log(L2 − 10 keV) | cstat/d.o.f. |
---|---|---|---|---|---|---|
cm−2 | erg s−1 | |||||
1 | 3.18![]() |
252![]() |
< 22.93 | 1.52![]() |
44.63![]() |
144.1/172 |
2 | 0.6279 | 827![]() |
22.20![]() |
1.93![]() |
43.70![]() |
288.8/296 |
3 | 1.0974 | 164![]() |
22.52![]() |
2.12![]() |
43.59![]() |
99.6/134 |
4 | 2.0133 | 259![]() |
< 22.79 | 1.85![]() |
42.29![]() |
127.5/171 |
5 | 0.9679 | 37![]() |
< 22.40 | 1.9 | 42.76![]() |
265.7/289 |
6 | 0.5181 | 993![]() |
< 21.24 | 1.903![]() |
43.51![]() |
59.79/72 |
Notes. For each object, we provide the redshift (which is derived from spectroscopy when provided without uncertainties, from photometry otherwise), the (0.5–7 keV) counts (see Nanni et al. 2018) the logarithm of the column density, the photon index (which is fixed to 1.9 when there are fewer than 150 counts), the intrinsic rest-frame 2–10 keV luminosity and the value of the C-statistic over degrees of freedom. Six objects also have a redshift estimate derived from the presence of the Fe Kα line (see Table 2). This table is available in its entirety in machine-readable form at the CDS.
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