PPT-Type 1 AGN SEDs in the COSMOS

A Single Form Mixing Diagram and Outliers Heng Hao SISSA Martin Elvis CFA and COSMOS Team INAFOABO Seminar 20121025 10 90 Outline Introduction Definition and Important Questions . . Statistics. : . 1.8 . Ms. ½. . sq. .deg. . @. 160 . ksec. 1761 . sources. Dec. ’06-June ’07. Catalog. : . Elvis . et. al., . 2009, ApJS 184, 158. Martin Elvis, Francesca . Civano. , . Aldcroft. The Biblical Model. Christopher W. Ashcraft M.S., M.Ed.. Big Bang vs. Creation. Origin of Stars. Solar System: Evidence of Design. Age of the Cosmos. Are we being told all the evidence or just selected information to support a particular idea?. Smolcic. . ea. ). Compilation based on different star formation estimators (UV, IR, radio, Hα..). Large scatter: Dust obscuration is major problem. Hopkins & . Beacom. (2006) compilation. redshift. with VLBI at . Parkes. Stas Shabala. University of Tasmania. Why study AGN. . AGN physics. Brightest objects in the Universe, yet we don’t know:. Composition. Accretion / outflow connection. Details of interaction with environment. Capetti. , . R. Baldi, B. Balmaverde, S. Buttiglione. AGN 10 - Roma 10/09/2012. WHY AN AGN CENSUS?. A PROPER AGN CENSUS IS NEEDED FOR A VARIETY OF STUDIES, SUCH AS, . E.G.. , THE AGN/HOST GALAXY CONNECTION, THE PROPERTIES OF THE CENTRAL ENGINE, THE AGN LUMINOSITY FUNCTION . Sierra . Critical Zone Observatory. 3. rd. Annual COSMOS Workshop. Matthew Meadows. Sierra . Nevada Research . Institute. University . of California . Merced. Critical Zone Observatories. http://criticalzone.org. Nikos Fanidakis. and. C.M. Baugh, R.G. Bower, S. Cole, C. Done, C. S. . Frenk. 9. th. Hellenic Astronomical Conference, Athens, Greece September 20-24, 2009. RE J1034+396. Matthew Middleton. Spectral and timing similarities of AGN and . BHB. A simple scaling.... Index of -1.35 from analytical method (Vaughan et al. 2005) and large scale simulations (Middleton & Done 2010). POWER . RADIO. GALAXIES AS BEACONS FOR CLUSTERS . AT . 1<z<2. Marco Chiaberge. INAF-IRA. Space Telescope Science Institute. A. . Capetti. INAF- OATO. G. Tremblay RIT. P. . Tozzi. INAF-OATS. Hee. -Won Lee. Department of Physics and Astronomy. Sejong. University. 2015. 1. 27. Content. Introduction. Scattering . and Unification of AGN. Scattered Ly . alpha. Balmer. Wings. Discussion. Active Galactic Nuclei. Early Views about the Cosmos. Ancient Views of the Cosmos . Myths. , folklore and legends were used to explain what ancient people observed in the night . sky: . First . Nations people . – believed the night sky was a pattern on a great blanket overhead, which was held up by a spinning ‘world pole’ resting on the chest of a woman named Stone Ribs. . SOF + SMV + RBV. SOF + SMV. Randomisation. 2 : 1 : 2 : 1*. Open-label. * . Randomisation. was stratified on genotype (1a or 1b) in both cohorts, . IL28B . in cohort 1 and treatment history (naïve or non-responder) in cohort . Andrew Liu. Program Manager. Azure OSSA + NoSQL. P4010. Raghav Mohan. Program Manager. Azure OSSA + NoSQL. Topics Covered. Brief overview of Azure Cosmos DB. Brief overview of Azure HDInsight. Data at Massive Scale. Prof Chris Done. University . of Durham & ISAS/JAXA. AGN feedback. Magorrian-Gebhardt. relation gives BH mass!! Big black holes live in host galaxies with big bulges! Either measured by bulge luminosity or bulge mass (stellar velocity dispersion) or .