Table 1.
Results of the linear fits to the –MBH relation (in log–log space), for the different datasets used in this work.
Survey | Tobs | Δtmin, obs | ![]() |
α(Tobs) | β(Tobs) |
---|---|---|---|---|---|
(days) | (days) | (days) | |||
CDF-S | 654 | 0.25 | 334[±87] | −1.07±0.12 | −0.2±0.2 |
128 | 0.95 | 65[±17] | −1.36±0.16 | −0.3±0.3 | |
COSMOS | 555 | 0.40 | 240[![]() |
−1.36±0.10 | −0.16±0.14 |
” | 891 | 0.38 | 413[![]() |
−1.29±0.07 | −0.21±0.13 |
CAIXA | 0.926 | 0.003 | 0.926 | −2.9±0.2 | −0.71±0.16 |
...+TARTARUS | 0.463 | ” | 0.463 | −2.98±0.14 | −0.75±0.14 |
Long-term RXTE | 5110 | 300 | 5110 | −1.38±0.09 | −0.15±0.12 |
Swift+RXTE | 9.45 | ∼0.5 | 9.45 | −1.81±0.08 | −0.42±0.07 |
Notes. Tobs and Δtmin, obs represent the maximum and minimum sampled timescales in the observer reference frame, while is the median value of the maximum rest-frame timescale over all sources; in square brackets we quote the Trest range for high-z samples (differences in Trest for the low-z samples are not significant). α(Tobs) and β(Tobs) represent the best-fit intercept and slope of Eq. (4).
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