2009 Fermi Symposium, Washington, D.C., Nov. 2-5 5 10 6 10 7 10 8 10 9 10$^{10}$10$^{11}$10$^{12}$10$^{13}$10$^{14}$10$^{15}$10$^{16}$10$^{17}$10$^{18}$10$^{19}$10$^{20}$10$^{21}$10$^{22}$10$^{23}$10$^{24}$10$^{25}$10$^{26}$10 27 10 10 10 11 10 12 10 13 10 14 10 15 10 16 10 17 10 18  Frequency (Hz) I  × Frequency (mJy·Hz) 10 6 10 7 10 8 10 9 10$^{10}$10$^{11}$10$^{12}$10$^{13}$10$^{14}$10$^{15}$10$^{16}$10$^{17}$10$^{18}$10$^{19}$10$^{20}$10$^{21}$10$^{22}$10$^{23}$10$^{24}$10$^{25}$10$^{26}$10 27 10 10 10 11 10 12 10 13 10 14 10 15 10 16 10 17 10 18  Frequency (Hz) I  × Frequency (mJy·Hz) Figure 5:: Broadband SED from radio to X-ray of 3C 309.1. The data obtained before the Fermi launch are red open circles (mostly taken from the NED), while the ones obtained later are black filled pentagons. The LAT data are not included here because this source is not in the preliminary LAT first-year catalog. Figure 6:: Broadband SED from radio to gamma-ray of 3C 380. The data obtained before the Fermi launch are red open circles (mostly taken from the NED), while the ones obtained later are black filled pentagons. The black data points are from: UMRAO, MOJAVE, Swift UVOT/XRT, and Fermi LAT. eConf C091122