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Table A.1.

Sources in our sample for which we modified the redshift value with respect to the 3FHL catalogue.

3FHL Simulations Measured
3FHL name Source name redshift redshift adopted adopted redshift/
redshift reference lower limit redshift lower limit reference redshift

3FHL J0022.0+0006 1RXS J002200.9+000659 0.3057 (1)
3FHL J0033.5−1921 KUV 00311−1938 0.61 (2) 0.506 0.506 (3)
3FHL J0120.4−2701 PKS 0118−272 0.558 0.558 (5)
3FHL J0211.2+1051 MG1 J021114+1051 0.2 (6) 0.3
3FHL J0237.6−3602 RBS 334 0.411 (3)
3FHL J0338.9−2848 NVSS J033859−284619 0.251 (4)
3FHL J0449.4−4350 PKS 0447−439 0.205 (7) 0.3 (3),(8)
3FHL J0508.0+6737 1ES 0502+675 0.416 (9) 0.3 (10),(11)
3FHL J0521.7+2112 TXS 0518+211 0.108 (12) 0.3 (8)
3FHL J0550.5−3215 PKS 0548−322 0.069 (13)
3FHL J0612.8+4122 B3 0609+413 1.108 1.108 (12)
3FHL J0622.4−2606 PMN J0622−2605 0.414 (14) 0.3
3FHL J0650.7+2503 1ES 0647+250 0.203 (15) 0.3 (8)
3FHL J0816.4−1311 PMN J0816−1311 0.046 (14) 0.288 0.3 (3)
3FHL J1107.4+0221 NVSS J110735+022225 1.0743 1.0743 (1)
3FHL J1120.8+4212 RBS 0970 0.124 (16) 0.3 (8)
3FHL J1253.1+5300 S4 1250+53 0.664 0.664 (1)
3FHL J1410.5+1438 NVSS J141028+143841 0.144 (1)
3FHL J1427.0+2348 PKS 1424+240 0.604 0.604 (17)
3FHL J1436.9+5639 RBS 1409 0.15 (18) 0.3 (12)
3FHL J1442.5−4621 SUMSS J144236−462302 0.1026 (14)
3FHL J1443.9−3908 PKS 1440−389 0.069 (14) 0.3 (12) 0.1385
3FHL J1447.9+3608 RBS 1432 0.739 0.739 (1)
3FHL J1603.8−4903 PMN J1603−4904 0.232 (19)
3FHL J1610.6−6649 PMN J1610−6649 0.447 0.447 (1)
3FHL J1903.2+5540 TXS 1902+556 0.727 0.727 (12)
3FHL J1918.2−4111 PMN J1918−4111 1.591 1.591 (12).
3FHL J1931.1+0937 RX J1931.1+0937 0.476 0.476 (12)
3FHL J1958.3−3011 1RXS J195815.6−301119 0.119 (14) 0.3 0.119
3FHL J2243.9+2020 RGB J2243+203 0.395 0.395 (12)
3FHL J2255.2+2410 MITG J225517+2409 0.864 0.864 (1)
3FHL J2324.7−4040 1ES 2322−409 0.174 (14) 0.3 0.1738

Notes. The columns contain the source name, the redshift value in the 3FHL catalogue, the reference for that redshift value, the lower limit value, the adopted redshift value, the reference justifying the adopted value, and finally, for sources discussed in this paper, the measured redshift. If the entry (redshift, lower limit, reference) is unknown, the legend is ‘–’. There is a total of 32 sources with 7 new redshifts and 14 lower limits. The lower limit of PMN J0816−1311 (z ≥ 0.288) is smaller than the adopted value for unknown redshift z = 0.3; we therefore used z = 0.3 for this source in our simulations. The spectra of ten sources have not been published yet to our knowledge, and we present them for reference in Fig. A.1.

References. (1) Blanton et al. (2017); (2) Piranomonte et al. (2007); (3) Pita et al. (2014); (4) Halpern et al. (1997); (5) Vladilo et al. (1997); (6) Meisner & Romani (2010), imaging redshift; (7) Perlman et al. (1998), weak features, unconfirmed; (8) Paiano et al. (2017a,b); (9) Landt et al. (2002); (10) Scarpa et al. (19990; (11) Giovannini et al. (2004); (12) Shaw et al. (2013); (13) Fosbury & Disney (1976); (14) Jones et al. (2004, 2009), low S/N spectrum; (15) Rector et al. (2003), tentative value; (16) Perlman et al. (1996); (17) Furniss et al. (2013); (18) Schwope et al. (2000); (19) Goldoni et al. (2016).

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