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Table 5.

Analysis results for all the observed sources.

Source name S/N Rc (BL Lac) Redshift Flux ratio Rc (gal) MR Slope
(obs) (fit) (gal)
(1) (2) (3) (4) (5) (6) (7) (8)
1RXS J011501.3−340008 20 19.4 ± 0.1 0.4824 ± 0.0007 0.9 ± 0.2 19.7 ± 0.3 −23.3 −1.8 ± 0.4
1RXS J015658.6−530208 100 17.0 ± 0.3 0.3043 ± 0.0004 3.2 ± 1.3 18.3 ± 0.5 −22.7 −1.4 ± 0.2
1RXS J020922.2−522920 160 15.4 ± 0.2 0.2110 ± 0.0002 6.0 ± 1.8 17.1 ± 0.4 −23.2 −1.5 ± 0.2
PKS 1440−389 230 15.0 ± 0.1 0.1385 ± 0.0005 8.6 ± 0.7 16.8 ± 0.2 −22.4 −1.5 ± 0.2
PMN J1457−4642 45 17.5 ± 0.2 0.1116 ± 0.0002 0.3 ± 0.2 16.7 ± 0.1 −22.2 −2.3 ± 0.2
NVSS J151148−051345 23 17.5 ± 0.1 (†) ≥0.4480 ± 0.0003 −2.5 ± 0.2
NVSS J152048−034850 43 17.2 ± 0.1 ≥0.8680 ± 0.0002 −1.6 ± 0.1
TXS 1515−273 160 15.6 ± 0.1 0.1284 ± 0.0003 3.0 ± 0.3 16.6 ± 0.2 −22.4 −1.6 ± 0.1
PMN J1539−1128 80 17.8 ± 0.1 −2.1 ± 0.3
WISE J154824.39+145702.8 42 18.2 ± 0.1 0.2308 ± 0.0002 ≤0.03 18.2 ± 0.1 −22.3
NVSS J163750−344915 80 17.5 ± 0.1 −2.3 ± 0.2
GB6 J1838+4802 250 15.8 ± 0.1 −1.1 ± 0.1
MITG J184126+2910 100 17.4 ± 0.1 0.2883 ± 0.0003 2.6 ± 0.5 18.2 ± 0.3 −22.9 −1.5 ± 0.1
1RXS J184230.6−584202 35 18.3 ± 0.2 0.421 (*) 1.7 ± 0.3 19.5 ± 0.2 −23.0 −2.4 ± 0.3
1RXS J184230.6−584202 35 18.3 ± 0.2 −1.6 ± 0.3
1RXS J195815.6−301119 110 15.8 ± 0.1 0.1190 ± 0.0003 1.2 ± 0.2 16.7 ± 0.2 −22.1 −1.9 ± 0.2
MAGIC J2001+435 105 15.9 ± 0.1 0.1739 ± 0.0004 5.0 ± 0.4 17.0 ± 0.2 −22.4 −1.0 ± 0.1
1RXS J203650.9−332817 19 17.8 ± 0.1 −1.6 ± 0.2
RBS 1751 40 16.9 ± 0.1 ≥0.618 (*) −1.6 ± 0.2
1ES 2322−409 210 16.0 ± 0.2 0.1736 ± 0.0008 9.5 ± 0.6 17.7 ± 0.2 −22.1 −1.6 ± 0.4

Notes. As the redshift of 1RXS J184230.6−584202 is based on a low-confidence detection of the CaHK feature, for this source we also present the results of a simple power-law fit. The spectral bin width is 4 Å for the sources observed with EFOSC2; 1 Å for MITG J184126+2910, MAGIC J2001+435, 1RXS J015658.6−530208, and 1RXS J020922.2−522920; and 2 Å for WISE J154824.39+145702.8. The columns are (1) Source name; (2) Median signal-to-noise ratio per spectral bin measured in continuum regions; (3) Rc, Cousins magnitude of the BL Lac spectrum corrected for reddening, telluric absorption, and slit losses with errors. Slit losses were estimated using an effective radius re = 10 kpc for all sources except for MAGIC J2001+435 for which we used re = 6.8 kpc (Aleksić et al. 2014); (4) Redshift or lower limit with error, (5) Flux ratio jet/galaxy at 5500 Å in rest frame; (6) Rc, Cousins magnitude of the galaxy with the same corrections as in Col. (3); (7) Absolute R magnitude of the galaxy, the errors are the same as those in Col. (6); (8) Power-law slope with errors. If the entry is unknown, the legend is ‘–’. (†)U Magnitude. (*)Uncertain redshift.

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