2009 Fermi Symposium, Washington, D.C., Nov. 2-5 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 1:: Broadband SED from radio to gamma-ray of NRAO 140. 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, Effelsberg, IRAM Plateau de Bure Interferometer, Swift UVOT/XRT, and Fermi LAT. Figure 2:: Broadband SED from radio to gamma-ray of PKS 0403 − 13. 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 3