Table A.1
Sources observed during the first three S band epochs.
Name | Alternative name | Class(a) | z | X band first epoch | Association |
---|---|---|---|---|---|
0011–191 | SHBLJ001355.9–185406 | HBL | 0.095 (1) | - | TeV |
0031–196 | KUV 00311–1938 | HBL | 0.610 (2) | - | TeV |
0236–314 | 1RXSJ023833.1–311808 | HBL | 0.233 (3) | - | TeV |
0301–243 | HBL | 0.260 (2) | - | TeV | |
0347–121 | 1ES 0347–121 | EHBL | 0.185 (2) | - | TeV |
0426–380 | FSRQ | 1.111 (2) | (16) | TeV | |
0447–439 | HBL | 0.107 (4) | (16) | TeV | |
0548–322 | EHBL | 0.069 (2) | - | TeV | |
0625–354 | OH–342 | RG | 0.056 (5) | (17) | TeV |
0903–573 | IBL | 0.695 (6) | - | TeV | |
1008–310 | 1RXS J101015.9–311909 | HBL | 0.143 (1) | - | TeV |
1101–232 | 1ES 1101–232 | EHBL | 0.186 (7) | - | TeV |
1248–350 | U | 0.410 (8) | - | neutrino | |
1253–053 | 3C279 | FSRQ | 0.538 (7) | - | neutrino/TeV |
1312–423 | 1ES 1312–423 | HBL | 0.105 (2) | - | TeV |
1322–428 | Cen A, NGC 5128 | RG | 0.002 (9) | (17) | TeV |
1424–418 | [HB89] 1424–418 | FSRQ | 1.520 (10) | (17) | neutrino |
1440–389 | HBL | 0.065 (11) | (16) | TeV | |
1510–089 | FSRQ | 0.360 (10) | - | TeV | |
1514–241 | AP Librae | LBL | 0.049 (1) | - | TeV |
1515–273 | TXS 1515–273 | HBL | 0.140 (11) | - | TeV |
1600–489 | PMN J1603–4904 | CSO | 0.232 (12) | (18) | TeV |
1921–293 | BLLac | 0.353 (1) | - | calibrator | |
1934–638 | CSO | 0.183 (13) | (19) | calibrator | |
2005–489 | [HB89] 2005–489 | HBL | 0.071 (14) | (17) | TeV |
2155–304 | [HB89] 2155–304 | HBL | 0.116 (15) | (17) | TeV |
2322–409 | 1ES 2322–409 | HBL | 0.174 (1) | - | TeV |
2356–309 | EHBL | 0.165 (1) | - | TeV |
Notes. (a) Source class abbreviations: LBL - low frequency peaked blazar; IBL - intermediate frequency peaked blazar; HBL - high frequency peaked blazar; EHBL - extremely high frequency peaked blazar; RG - radio galaxy; FSRQ - flat spectrum radio quasar; CSO - compact symmetric object; U - unidentified.
References. (1) Jones et al. (2009); (2) Mao (2011); (3) Arsioli et al. (2015); (4) Craig & Fruscione (1997); (5) Lauer et al. (2014); (6) Thompson et al. (1990); (7) Neeleman et al. (2016); (8) Jackson et al. (2002); (9) Lavaux & Hudson (2011); (10) Truebenbach & Darling (2017); (11) Chang et al. (2019); (12) Goldoni et al. (2016); (13) Paturel et al. (2002); (14) Keeney et al. (2018); (15) Ganguly et al. (2013); (16) Müller et al. (2018); (17) Ojha et al. (2010); (18) Müller et al. (2014); (19) Ojha et al. (2004).
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