Table 1.
X-ray spectral fit results of Mrk 335 (see Sect. 3.2).
| Model | NH | ΓX | kT or log ξ | η |  |
|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) |
| High state, 2020 June 23 – July 1 | |||||
| pl | 2.49 ± 0.06 | 3.2 | |||
| zpcf * pl | 6.3 |
2.95 |
0.86 |
1.4 | |
| bbdy+(zpcf * pl) (1) | 4.3 |
2.97 ±0.20 | 0.15 | 0.88 |
1.5 |
| zxipcf * pl | 16.1 |
2.3 |
2.1 |
0.87 |
1.1 |
| Deep low state, 2019 May (2) | |||||
| pl | 2.34 ±0.20 | 1.6 | |||
| zpcf * pl | 13.95 |
3.07 ±0.21 | 0.94 |
1.0 | |
| pl + bbdy | 0.50 |
0.15 ±0.02 | 0.9 | ||
Notes. Columns are as follows: (1) Models: pl = powerlaw, bbdy = black body, zpcf = partial covering absorber, and zxipcf = ionized absorber model. (2) Absorption in units of 1022 cm−2; (3) power-law photon index; (4) kT in units of keV of the black body, or ionization parameter log ξ of the ionized absorber; (5) covering factor; and (6) goodness of fit, reduced χ2. If no errors are reported, the quantity was fixed. For all fits the column density at z = 0 was fixed to the Galactic value of 3.96×1020 cm−2.
(1)bbdy parameters fixed at low-state value.
(2)Fits using Cash statistics (Cash 1979).
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