Table 1.
The parameters for 431 nearby low-excitation radio galaxies and 75 Fermi BL Lacertae objects.
Name | Class | z | L1.4 | log Lkin | log Lline | log MBH | λ |
---|---|---|---|---|---|---|---|
erg/s | erg/s | erg/s | |||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
J0003.2+2207 | HBL | 0.1 | 39.42 | 43.28 | 41.72 | 8.10 | −4.52 |
J002900.98-011341.7 | FR I | 0.083 | 40.80 | 44.21 | 42.61 | 8.96 | −4.52 |
J003930.52-103218.6 | FR I | 0.129 | 40.13 | 43.75 | 41.10 | 8.4 | −5.44 |
J010852.48-003919.4 | FR 0 | 0.045 | 38.83 | 42.87 | 41.93 | 8.32 | −4.51 |
J001247.57+004715.8 | FR II | 0.148 | 40.65 | 44.11 | 42.01 | 8.61 | −4.73 |
… | … | … | … | … | … | … | … |
Notes. Column (1) gives the source name and Col. (2) the classification. BL Lacs are classified as low-, intermediate-, and high-synchrotron-peaked BL Lacs and referred to as LBLs, IBLs, and HBLs; low-excitation radio galaxies are classified as Fanaroff-Riley type 0 (FR 0), I (FR I), and II (FR II) radio galaxies. Col. (3) shows the redshift and Col. (4) the 1.4 GHz luminosity (in erg/s). For BL Lacs, the intrinsic 1.4 GHz luminosity is calculated by assuming a Doppler factor of δ ∼ 10 within the continuous jet model. Col. (5) gives the kinetic jet power (in erg/s) derived from 1.4 GHz radio luminosities. Col. (6) shows the total emission-line luminosity (in erg/s). Col. (7) provides the BH masses in the unit of solar mass derived from the M − σ* relation. Col. (8) shows the line accretion rate λ = Lline/LEdd. A portion of the table is presented here to offer guidance on the format and content of Table 1 available at the CDS.
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