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Table 1.

Main properties of the targets and observing log.

(1) (2) (3) (4) (5) (6) (7) (8)
Target z Type TeV AR Nfrms Nobs Ref.
det? (mag)
1ES 0033+595 HBL y 1.911 1501 387 1
1ES 0120+340 0.272 HBL 0.125 1183 300
RGB 0136+391 HBL y 0.168 1556 393
RGB 0214+517 0.049 HBL 0.381 1183 309
3C 66A 0.444 IBL y 0.182 2726 644 2,3
1ES 0647+250 0.41 HBL y 0.214 1134 303
1ES 0806+524 0.138 HBL y 0.096 1188 328 4
OJ 287 0.306 LBL y 0.062 3308 699 5,6,7,8
1ES 1011+496 0.212 HBL y 0.027 1509 426 9,10,11
1ES 1028+511 0.360 HBL 0.027 1040 273
Mkn 421 0.031 HBL y 0.033 2797 683 12–20
RGB 1117+202 0.139 0.043 780 230
Mkn 180 0.045 HBL y 0.029 1323 379 21
RGB 1136+676 0.135 HBL y 0.019 908 244
ON 325 0.130 IBL/HBL y 0.052 1031 272 22
1ES 1218+304 0.182 HBL y 0.045 941 273
RGB 1417+257 0.237 HBL 0.041 907 246
1ES 1426+428 0.129 HBL y 0.027 825 219
1ES 1544+820 HBL 0.108 169 46
Mkn 501 0.034 HBL y 0.042 3958 749 23–28
OT 546 0.055 HBL y 0.064 1496 401 29
1ES 1959+650 0.047 HBL y 0.384 2784 734 30,31
BL Lac 0.069 LBL y 0.714 3122 771 32–34
1ES 2344+514 0.044 HBL y 0.468 1584 451 35,36

S5 0716+714 0.31 LBL y 0.067 2789 511 37–41
ON 231 0.102 IBL y 0.049 757 196 42
3C 279 0.536 FSRQ y 0.062 1198 316 43–50
PG 1424+240 0.604 IBL/HBL y 0.127 408 141 51
PKS 1510−089 0.360 FSRQ y 0.209 994 272 52–54
PG 1553+113 HBL y 0.113 1610 444 55–60
PKS 2155−304 0.116 HBL y 0.047 1097 190

Notes. Targets above the dividing horizontal line belong to the long-term monitoring sample of 24 targets drawn from Costamante & Ghisellini (2002). Columns: (1) target name, (2) redshift, (3) broadband type (FSRQ/BL division from the Roma-BZCAT (5th Edition, Massaro et al. 2015), LBL/IBL/HBL classification from this work), (4) is the target detected at TeV energies?, (5) galactic extinction in the R-band, obtained from the NED, (6) number of CCD frames, (7) number of data points, and (8) references to papers where parts of these data have been used before.

References. (1) Aleksić et al. (2015a); (2) Aliu et al. (2009); (3) Böttcher et al. (2009); (4) Aleksić et al. (2015f); (5) Villforth et al. (2010); (6) Valtonen et al. (2009); (7) Pihajoki et al. (2013b); (8) Valtonen et al. (2008); (9) Albert et al. (2007b); (10) Ahnen et al. (2016b); (11) Aleksić et al. (2016); (12) Lichti et al. (2008); (13) Donnarumma et al. (2009); (14) Acciari et al. (2009a); (15) Aleksić et al. (2010b); (16) Abdo et al. (2011b); (17) Acciari et al. (2011b); (18) Aleksić et al. (2012a); (19) Aleksić et al. (2015c); (20) Aleksić et al. (2015d); (21) Albert et al. (2006b); (22) Aleksić et al. (2012b); (23) Aleksić et al. (2015b); (24) Acciari et al. (2011a); (25) Abdo et al. (2011a); (26) Aleksić et al. (2010c); (27) Anderhub et al. (2009b); (28) Albert et al. (2007e); (29) Aleksić et al. (2014a); (30) Albert et al. (2006a); (31) Tagliaferri et al. (2008); (32) Albert et al. (2007d); (33) Villata et al. (2009); (34) Raiteri et al. (2013); (35) Albert et al. (2007c); (36) Aleksić et al. (2013); (37) Pian et al. (2005); (38) Ostorero et al. (2006); (39) Anderhub et al. (2009a); (40) Villata et al. (2008); (41) Bhatta et al. (2013); (42) Acciari et al. (2009b); (43) Böttcher et al. (2007); (44) MAGIC Collaboration et al. (2008); (45) Larionov et al. (2008); (46) Abdo et al. (2010b); (47) Aleksić et al. (2011); (48) Hayashida et al. (2012); (49) Aleksić et al. (2014b); (50) Kiehlmann et al. (2016); (51) Aleksić et al. (2014c); (52) D’Ammando et al. (2009); (53) D’Ammando et al. (2011); (54) Aleksić et al. (2014d); (55) Albert et al. (2007a); (56) Albert et al. (2009); (57) Aleksić et al. (2010a); (58) Aleksić et al. (2012c); (59) Aleksić et al. (2015e); (60) Ackermann et al. (2015).

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