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Table 1

Analysis results for the observed sources.

Source name (1) S/N (2) Rc (BL Lac) (obs) (3) Redshift (4) Flux ratio (5) Rc(gal) (fit) (6) MR (gal) (7) Slope (8)
1RXS J032342.6-011131 132 17.4 ± 0.1 −1.2 ± 0.1
RX J0338.4+1302 60 17.6 ± 0.2 −2.5 ± 0.4
SUMSS J052542-601341 3 21.2 ± 0.1 −0.8 ± 1.0
GB6 J0540+5823 42 16.8 ± 0.3 −1.3 ± 0.1
PMN J0622-2605 89 17.5 ± 0.1 0.4150 ± 0.0001 −0.4 ± 0.1
TXS 0700-197 110 16.7 ± 0.1 −0.4 ± 0.1
NVSS J080405-362919 70 17.1 ± 0.1 >1.4454 ± 0.0003 −1.0 ± 0.1
RX J0819.2-0756 61 18.5 ± 0.2 0.3214 ± 0.0002 1.8 ± 0.6 19.4 ± 0.4 −22.0 −1.2 ± 0.2
NVSS J084121-355506 96 16.7 ± 0.2 >1.0196 ± 0.0001 −1.2 ± 0.1
1RXS J094709.2-254056 126 16.2 ± 0.1 −0.9 ± 0.2
NVSS J105534-012617 79 18.2 ± 0.1 −1.0 ± 0.2
NVSS J123341-014426 144 18.0 ± 0.1 −0.7 ± 0.1
1RXS J130737.8-425940 109 16.7 ± 0.1 −1.1 ± 0.1
4C +29.48 43 19.7 ± 0.2 1.1427 ± 0.0001 −0.4 ± 0.2
1RXS J144037.4-384658 75 17.7 ± 0.2 0.3583 ± 0.0002 4.8 ± 0.9 19.5 ± 0.2 −22.3 −1.2 ± 0.1
PMN J1544-6641 70 17.7 ± 0.1 0.2595 ± 0.0004 4.9 ± 0.3 19.1 ± 0.1 −21.7 −1.1 ± 0.1
NVSS J160756-203942 62 18.3 ± 0.1 0.5479 ± 0.0001 −0.5 ± 0.1
NVSS J163750-344915 93 16.8 ± 0.1 −0.9 ± 0.1
NVSS J164011+062827 112 17.7 ± 0.2 −0.9 ± 0.1
1RXS J171405.2-202747 65 17.6 ± 0.1 0.5222 ± 0.0002 3.5 ± 0.5 19.4 ± 0.2 −23.8 −1.4 ± 0.1
RXJ1754.1+3212 170 16.5 ± 0.2 −1.1 ± 0.04
NVSS J182338-345412-Gr600 110 15.8 ± 0.2 0.1826 ± 0.0002 ~17.8 ~-22.1 −1.2 ± 0.1
NVSS J182338-345412-Gr300 98 15.8 ± 0.2 0.1826 ± 0.0002 −1.4 ± 0.3
NVSS J184919-164723 46 19.0 ± 0.1 0.3485 ± 0.0005 2.0 ± 0.4 19.9 ± 0.2 −21.8 −1.0 ± 0.1
NVSS J192502+28154 65 16.5 ± 0.1 0.1636 ± 0.0003 17.6 ± 0.4 −22.2 −1.3 ± 0.1
1RXS J194246.3+103339 97 16.0 ± 0.2 −0.7 ± 0.1
1RXS J194422.6-452326 75 17.2 ± 0.1 0.2358 ± 0.0002 5.3 ± 0.6 18.2 ± 0.1 −22.3 −1.1 ± 0.1
NVSS J194455-214320 76 17.8 ± 0.1 0.4263 ± 0.0003 1.9 ± 0.1 18.8 ± 0.1 −23.6 −1.1 ± 0.2
NVSS J224753+441317 133 16.6 ± 0.3 −1.4 ± 0.1
1RXS J230437.1+370506 95 17.9 ± 0.3 −1.5 ± 0.1

Notes. Two separate FORS observations of NVSS J182338-345412 were performed, one using Grism 600RI and the other using Grism 300I. In these spectra absorption features of the host galaxy have been detected but their S/N was too weak to allow formal fitting with a galaxy model. We therefore fit the spectra with a power law and roughly estimated the host galaxy magnitude from the intensity of the features. The spectral bin width is 1 Å for sources observed with Keck/ESI and SALT/RSS and 1.66 Å for sources observed with VLT/FORS. 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 Galactic reddening, telluric absorption, and slit losses with errors. Slit losses were estimated using an effective radius re = 10 kpc for all sources; (4) Redshift or lower limit with errors; (5) Flux Ratio of jet to galaxy at 5500 Å in rest frame; (6) Rc, Cousins magnitude of the galaxy with the same corrections as in column (3); (7) Absolute R Magnitude of the galaxy, the errors are the same as those in column (6); (8) Power-Law Slope α with fλ ∝ λα with errors. For α, 3-sigma errors are shown; all other quantities are shown with 1-sigma errors. If the entry is unknown, the legend is ‘-’.

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