Reverberation mapping

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Seyfert Spectral Variability Behavior
Light bending?Suzaku lightcurveMiniutti & Fabian (2004) suggestcontinuum source height varies, whencont m produced close to disk gravitybends light onto accretion disk,reducing continuum flux whileenhancing reflection featuresLightBendingIron line does not respondto continuum
Page 1 and 2: Reverberation mappingOptical lines
Page 3 and 4: Reverberation mappingv =GM rGetting
Page 7 and 8: Light Crossing Time•Variations sm
Page 11 and 12: X-ray Observations of AGNWhat we ca
Page 13 and 14: Recap: The Power behind AGNSimple a
Page 15 and 16: Copious production of X-RaysUV phot
Page 17 and 18: X-ray Line ProductionGeorge & Fabia
Page 19 and 20: Chandra/XMMSuzakuAbsorptionfrom out
Page 21 and 22: Profile distorted SR & GR- probe of
Page 23 and 24: GR Effects on Spectral featuresProf
Page 25 and 26: MCG-6-30-15: Poster ChildTanaka et
Page 27: Absorption or Reflection as the ori
Page 31 and 32: Ambiguity: - X-ray AbsorptionNGC 35
Page 33 and 34: How much evidence is there forabsor
Page 35 and 36: More Evidence for ionized outflows:
Page 37 and 38: Seyfert Spectral Variability Behavi
Page 39 and 40: Partial Covering/Occultation, resur
Page 41: Summary• Large amounts of gas are

Reverberation mapping

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