Multifrequency observations of a sample of very low frequency peaked BL Lacertae objects

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Table 6:

Absolute magnitudes M_R of sample sources calculated adopting R1 values from USNO-B1 (Table 1) and rest-frame peak frequencies $\nu _{\rm s}$ adopting values relative to the faint state, as reported in Table 4.
Source	m-M	M_R	$\nu _{\rm s}$
BZB J0753+5352	-42.3	-24.8	13.28
BZB J0818+4222	-43.0	-23.3	13.33
BZB J0823+2223	-44.6	-25.9	13.18
BZB J0832+4913	-42.3	-23.1	13.04
BZB J0929+8612	-42.3	-23.1	12.96
BZB J1223+8040	-42.3	-24.0	13.12
BZB J1927+6117	-42.3	-25.3	12.94
BZB J2009+7229	-42.3	-23.3	13.25

Source LaTeX | All tables | In the text

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