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Table 1.
Sample of hard-TeV BL Lacs collected by Xue et al. (2019a).
| Object |  |
Log MBH | Rs | R |
|---|---|---|---|---|
| (erg s−1) | (M⊙) | (cm) | (cm) | |
| 1ES 0229+200 | 1.00 × 1045 | 9.16 ± 0.11 (Meyer et al. 2012) | 4.29 × 1014 | 7.00 × 1014 |
| 1ES 0347−121 | 1.63 × 1045 | 8.02 ± 0.11 (Meyer et al. 2012) | 3.10 × 1013 | 2.25 × 1012 |
| 1ES 0414+009 | 1.54 × 1045 | 9 | 2.96 × 1014 | 2.17 × 1014 |
| 1ES 1101−232 | 1.02 × 1045 | 9 | 2.96 × 1014 | 3.30 × 1014 |
| 1ES 1215+303 | 2.11 × 1045 | 8.4 (Gupta et al. 2012) | 7.45 × 1013 | 1.00 × 1013 |
| 1ES 1218+304 | 5.45 × 1045 | 8.04 ± 0.24 (Meyer et al. 2012) | 3.25 × 1013 | 7.40 × 1011 |
| S5 0716+714 | 3.33 × 1046 | 8 (Zdziarski & Bottcher 2015) | 2.96 × 1013 | 1.01 × 1011 |
| W Comae | 6.00 × 1044 | 8.7 (Zdziarski & Bottcher 2015) | 1.49 × 1014 | 1.41 × 1014 |
| TXS 0506+056 | 1.74 × 1045 | 9 | 2.96 × 1014 | 1.92 × 1014 |
Notes. Columns from left to right: the source name; the observed luminosity of the TeV spectrum; logarithm of the SMBH mass in units of the solar mass, M⊙; the Schwarzschild radius of the SMBH; the maximum R obtained by Eq. (9).
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