Wiki Markup high \|b\|, non pulsar LAT bright source are associated to radio sources - 98/106 (92%) in LBAS have 8.4 GHGHz flux density > 100 mJy - Log of radio luminosity is 39.0 < Log Lr < 45.3 \[erg s^-1\]
- radio luminosity distribution is different for BL Lacs and FSRQ:
Wiki Markup Log Lr, BLL = 42.8 \+/\- 1.1 \[erg s^-1\]
Wiki Markup Log Lr, FSRQ = 44.4 \+/\- 0.6 \[erg s^-1\]
Wiki Markup RG: NGC 1275 similar to BL Lacs (Log Lr = 42.2 \[erg s^-1\]), Cen A much less luminous (Log Lr = 39.1 \[erg s^-1\])
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- 8.4 GHz data are representative of radio flux density in general - negligible extended emission - flat spectrum compact cores, overluminous with respect to radio galaxies (except Cen A)
- We have already a significant improvement over EGRET numbers, so we want to address the existence of actual correlation between radio and gamma ray properites. There's a number of bias/effects that we have to keep in mind, so we tried to look into different pairs of quantities
- when we have z, we calculate luminosity and K-correct - else we just use S_848.4 and SF_E>100 >100 MeV
- BL Lacs and FSRQ tend to populate different regions, so we make correlation analysis for full population and single classes separately
- Spearman rank is used - partial analysis is used as far as luminosity are concerned
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