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Radio Loud Quasars and GLAST Aneta Siemiginowska Harvard-Smithsonian Center for Astrophysics.

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Presentation on theme: "Radio Loud Quasars and GLAST Aneta Siemiginowska Harvard-Smithsonian Center for Astrophysics."— Presentation transcript:

1 Radio Loud Quasars and GLAST Aneta Siemiginowska Harvard-Smithsonian Center for Astrophysics

2 GLAST WorkshopAneta Siemiginowska Blazar Sequence: FSRQ ? Opt-UV LBL HBL SYN Compton FSQR HBLLBL Donato et al 2000

3 GLAST WorkshopAneta Siemiginowska X-rays vs. Gamma-ray Emission Unified picture:  What process dominates X-ray emission? Jet vs. Corona  FSRQ - optical/UV lines => Can determine the BH mass  UV emission - an accretion state?

4 GLAST WorkshopAneta Siemiginowska Multi-wavelength DATA: PKS1127-145 z=1.187 X-rays: Beppo SAX - 1999 Chandra - 2000/2005 XMM - 2002 Swift - 2007 (140ksec) EGRET(?) - 1993/1995

5 GLAST WorkshopAneta Siemiginowska MODELS: SSC model fit to the radio and BeppoSAX data SSC Giommi et al 2002

6 GLAST WorkshopAneta Siemiginowska Model Components: SYN - synchrotron SSC - Compton scattering of SYN ERC(IR) - IC/IR field due to dust ERC(UV) - IC/UV field from AD ERC(BEL) - IC/BEL Clouds Inverse Compton on an External Photon Field - Sikora Model Blazejowski et al 2004 LAT energy Band: - Critical for this Model - Jet vs. Corona-Disk contribution to the X-ray band

7 GLAST WorkshopAneta Siemiginowska

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