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Table 2
Extreme synchrotron peaked sources.
Source | log ν peak | log ν peak f ν peak | Note |
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2WHSPJ003322.3−203907 | 17.9 | –11.9 | New HSP |
2WHSPJ004013.7+405003 | >17.5 | >–11.5 | 5BZU, lower limit |
2WHSPJ012308.5+342048 | 18.0 | –10.8 | 5BZB, TeV source |
2WHSPJ013803.7−215530 | >17.5 | >–12.0 | blazar candidate lower limit |
2WHSPJ015657.9−530159 | 18.0 | –11.1 | 5BZB |
2WHSPJ020412.9−333339 | 17.9 | –11.7 | 5BZB, new γ-ray identification |
2WHSPJ023248.5+201717 | 18.5 | –11.0 | 5BZG, TeV source* |
2WHSPJ032056.2+042447 | 17.9 | –11.7 | Blazar candidate, new γ-ray identification |
2WHSPJ032356.5−010833 | >17.5 | >–11.9 | 5BZB, TeV source, lower limit |
2WHSPJ034923.1−115926 | 17.9 | –11.0 | 5BZB, TeV source |
2WHSPJ035257.4−683117 | 18.1 | –11.0 | Previously known BL Lac* |
2WHSPJ050419.5−095631 | 17.9 | –11.6 | New HSP, new γ-ray identification |
2WHSPJ050709.2−385948 | >17.5 | >–12.2 | Blazar candidate, lower limit |
2WHSPJ050756.0+673723 | 17.9 | –10.7 | 5BZB, TeV source |
2WHSPJ055040.5−321615 | 18.1 | –10.7 | 5BZG, TeV source |
2WHSPJ055716.7−061706 | 17.9 | –11.5 | Blazar candidate, new γ-ray identification |
2WHSPJ064710.0−513547 | 17.9 | –11.2 | Blazar candidate |
2WHSPJ071029.9+590820 | 18.1 | –10.7 | 5BZB, TeV source |
2WHSPJ073326.7+515354 | 17.9 | –11.3 | Blazar candidate |
2WHSPJ081917.5−075626 | 18.0 | –11.5 | 5BZB, TeV source |
2WHSPJ083251.4+330011 | 18.0 | –12.0 | 5BZB, new γ-ray identification |
2WHSPJ084452.2+280409 | 17.9 | –12.3 | New HSP |
2WHSPJ092057.4−225720 | >17.5 | >–11.6 | New HSP, lower limit |
2WHSPJ094620.2+010450 | 17.9 | –11.8 | 5BZB, TeV source |
2WHSPJ095849.0+013218 | 17.9 | –12.3 | New HSP, new γ-ray identification |
2WHSPJ102212.6+512359 | 18.2 | –11.7 | 5BZG, new γ-ray identification |
2WHSPJ104651.4−253544 | >18.0 | >–11.5 | 5BZB |
2WHSPJ105606.6+025213 | 17.9 | –11.5 | 5BZG |
2WHSPJ110357.1+261117 | 17,9 | –12.2 | New HSP |
2WHSPJ110651.7+650603 | 17.9 | –12.7 | Blazar candidate |
2WHSPJ110804.9+164820 | 17.9 | –12.7 | New HSP |
2WHSPJ112313.2−090424 | 17.9 | –12.4 | Blazar candidate |
2WHSPJ113209.1−473853 | >17.5 | >–11.6 | Blazar candidate, lower limit |
2WHSPJ113630.1+673704 | 18.1 | –11.1 | 5BZB, TeV source |
2WHSPJ121323.0−261806 | 17.9 | –11.2 | 5BZB |
2WHSPJ122044.5+690525 | >17.5 | >–12.0 | Blazar candidate, lower limit |
2WHSPJ122208.6+030718 | >17.5 | >–11.8 | New HSP, lower limit |
2WHSPJ122514.2+721447 | >17.5 | >–11.8 | Lower limit, 5BZB |
2WHSPJ125341.2−393159 | 17.9 | –11.3 | 5BZG, new γ-ray identification |
2WHSPJ125708.2+264924 | >17.5 | >–12.3 | New HSP, lower limit |
2WHSPJ132239.1+494336 | >17.5 | >–12.1 | New HSP, lower limit |
2WHSPJ132541.8−022809 | 17.9 | –12.0 | 5BZB, new γ-ray identification |
2WHSPJ140027.0−293936 | >17.5 | >–12.1 | Blazar candidate, lower limit |
2WHSPJ140121.1+520928 | >17.5 | >–12.0 | 5BZB, lower limit |
2WHSPJ142832.5+424020 | 18.1 | –10.7 | 5BZB, TeV source |
2WHSPJ143342.7−730437 | >17.5 | >–11.5 | Blazar candidate, lower limit, new γ-ray identification* |
2WHSPJ151041.0+333503 | >17.5 | >–11.5 | 5BZG, lower limit, new γ-ray identification |
2WHSPJ151618.7−152344 | 18.0 | –11.7 | 5BZB, new γ-ray identification |
2WHSPJ153646.6+013759 | >18.0 | >–11.7 | 5BZB |
2WHSPJ160519.0+542058 | 17.9 | –12.0 | 5BZB, new γ-ray identification |
2WHSPJ161004.0+671026 | >17.5 | >–11.8 | 5BZB, lower limit, new γ-ray identification |
2WHSPJ161414.0+544251 | 17.9 | –12.6 | Blazar candidate |
2WHSPJ161632.8+375603 | 18.0 | –12.1 | 5BZG |
2WHSPJ161632.8+375603 | 18.0 | –12.1 | 5BZG |
2WHSPJ162330.4+085724 | >17.5 | >–12.1 | New HSP, lower limit, new γ-ray identification |
2WHSPJ165352.2+394536 | 17.9 | –10.2 | Variability, flaring, 5BZB, TeV source* |
2WHSPJ171902.2+552433 | 17.9 | –12.5 | Known blazar |
2WHSPJ194333.7−053352 | >17.5 | >–11.8 | Blazar candidate |
2WHSPJ194356.2+211821 | 18.1 | –11.0 | New HSP, TeV source |
2WHSPJ205528.2−002116 | >18.0 | >–10.9 | 5BZB, TeV source, lower limit |
2WHSPJ214410.0−195559 | 17.9 | –12.4 | Blazar candidate |
2WHSPJ215305.2−004229 | >18.0 | >–11.4 | 5BZB, lower limit* |
2WHSPJ223248.7−202226 | 17.9 | –11.7 | Blazar candidate |
2WHSPJ225147.5−320611 | >18.0 | >–11.3 | 5BZU, lower limit, new γ-ray identification |
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