Table 2
List of parameters corresponding to the BL Lac objects in our sample obtained with the approach of Sbarufatti et al. (2006, 2009; see text).
| Object | R | E(B − V)Gal | α | E W min | Redshift | Log(νpeak) |
| mag. | (mag.) | (Å) | (Hz) | |||
|
|
||||||
| 1FGL J0051.4−6242 | 17.3 | 0.016 | −1.0 ± 0.1 | 0.3 | >0.30 | 15.06 |
| 1FGL J0054.9−2455* | 17.1 | 0.016 | −1.3 ± 0.3 | 1.2 | >0.12 | 15.10 |
| 1FGL J0131.2+6121 | 18.2 | 0.922 | −1.5 ± 0.4 | 1.3 | >0.08 | 15.85 |
| 1FGL J0137.8+5814 | 17.5 | 0.528 | −0.7 ± 0.2 | 0.7 | >0.12 | 14.98 |
| 1FGL J0223.0−1118 | 17.4 | 0.021 | −1.3 ± 0.4 | 1.6 | >0.20 | 14.84 |
| 1FGL J0506.9−5435 | 16.1 | 0.030 | −1.2 ± 0.2 | 0.7 | >0.40 | 15.61 |
| 1FGL J0604.2−4817 | 17.4 | 0.050 | −0.9 ± 0.2 | 1.0 | >0.37 | 15.20 |
| 1FGL J0648.8+1516 | 16.2 | 0.144 | −1.0 ± 0.2 | 0.9 | >0.13 | 15.52 |
| 1FGL J0841.4−3558 | 17.2 | 0.495 | −0.9 ± 0.3 | 1.8 | >0.15 | 15.01 |
| 1FGL J0848.6+0504 | 18.3 | 0.067 | −1.2 ± 0.4 | 1.9 | >0.57 | 16.14 |
| 1FGL J1304.3−4352* | 15.4 | 0.133 | −1.0 ± 0.2 | 0.5 | >0.19 | 15.02 |
| 1FGL J1307.6−4259 | 15.1 | 0.106 | −1.3 ± 0.2 | 0.4 | >0.10 | 15.10 |
| 1FGL J1353.6−6640 | 17.1 | 0.553 | −0.9 ± 0.3 | 0.3 | >0.15 | 15.11 |
| 1FGL J1419.7+7731 | 17.6 | 0.035 | −1.6 ± 0.3 | 1.1 | >0.27 | 15.39 |
| 1FGL J1553.5−3116* | 15.5 | 0.174 | −1.1 ± 0.2 | 0.3 | >0.28 | 14.42 |
| 1FGL J1643.5−0646* | 16.7 | 0.491 | +0.1 ± 0.4 | 2.6 | >0.12 | 14.88 |
| 1FGL J1823.5−3454 | 15.2a | 0.129 | −1.1 ± 0.2 | 0.4 | >0.17 | 15.50 |
| 1FGL J1841.9+3220 | 17.0 | 0.088 | −1.0 ± 0.2 | 0.8 | >0.20 | 15.38 |
| 1FGL J1926.8+6153* | 16.6 | 0.058 | −0.9 ± 0.2 | 0.4 | >0.16 | 15.29 |
| 1FGL J1933.3+0723 | 15.3 | 0.295 | −1.2 ± 0.2 | 0.4 | >0.20 | 14.64 |
| 1FGL J1942.7+1033 | 17.0 | 0.390 | −0.1 ± 0.2 | 0.2 | >0.20 | 14.75 |
| 1FGL J2042.2+2427* | 14.0 | 0.140 | ** | 1.9 | ** | 15.32 |
| 1FGL J2146.6−1345* | 17.5 | 0.042 | −1.1 ± 0.2 | 0.5 | >0.28 | 14.92 |
| 1FGL J2323.0−4919 | 17.1 | 0.012 | −1.1 ± 0.2 | 0.4 | >0.27 | 15.04 |
| 1FGL J2329.2+3755* | 17.0 | 0.182 | −1.3 ± 0.2 | 0.6 | >0.20 | 15.15 |
Notes. R-band magnitudes were obtained from the USNO-A2.0 catalog, while the values of E(B − V)Gal are from Schlegel et al. (1998).
Obtained from the photometry on the acquisition image of the spectrum presented in this work (see text).
Present in the BL Lac spectroscopic sample of Shaw et al. (2013).
The optical emission of the source is dominated by the host galaxy; thus, in this case it was not possible to fit the spectrum with a power law according to the method of Sbarufatti et al. (2006).
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