Blazar studies

- Identification:
analysis methods
existing catalogs 
- Redshift and Luminosity Distributions, log N/log S
- Spectral Indices as a function of redshift
- EBL
- Correlations: Epeak vs Flux, Epeak vs Index, Index vs Flux
- Time properties:
                  Series analysis, Power Spectral Density
                  gamma vs X timing correlation
- Multiwavelength:
         Target of opportunity campaigns, preplanned MW campaigns:
               Monitoring of "Flaring sources": simultaneous observation in
                   - Radio (VLBA)
                   -  Optical (Whole Year Blazar Telescope, GLAST Telescope Network)
                   -  X (ASM,Swift)
                   - "European Network for the Investigation of Glactic Nuclei through
                      Multifrequency Analysis" (ENIGMA)
                HBL:  simultaneous observation in the  "TeV" range
      
- Sambrina-Fossati trend: Power decreases as Epeak increases                 
- Detection/upper limits on radio-quiet galaxies ("Seyfert")
- Detection/upper limits on radio-galaxies:Cen A, M87,  3EGJ1621+8203-NGC6251,
3EGJ1735-1500-J1737-15
-Microquasars:

- Modeling (SSC, EC)

-Simulations