Table 1.
Frequency dependent constraints on Tint.
| νo | log10Tint | ||
|---|---|---|---|
| (GHz) | (log10K) | ||
| H0 = 67.4km/s/Mpc | |||
| 15 | 10.13< (a) | log10Tint | < 11.56 |
| 24 | 9.73< | log10Tint | |
| 43 | 9.12< | log10Tint | < 11.65 |
| 86 | 9.29< | log10Tint | |
Notes. Constraints on log10Tint of AGN radio cores. Upper limits come from source variability (Section 2.1) and lower limits from a population analysis (Section 2.2). For all values, a uniform disk was assumed for the core geometry. Each column corresponds to νo (the observing frequency in GHz) and log10Tint (the lower and upper bounds on the logarithm of Tint).
Value from Lee (2014).
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