PPT-Quasar Luminosity Functions at High

Redshifts Gordon Richards Drexel University With thanks to Michael Strauss Xiaohui Fan Don Schneider and Linhua Jiang Quasar Luminosity Function Croom et al 2004 Space density of quasars as a function of . Quasars. Quasars were . discovered by the . radio waves that they give off. Scientists at first had no idea what to these disruptions could possibly be. They still really don’t know.. Because of the initial ambiguity surrounding the Quasars they . Massive Black Holes. Stephen Fine. Outline. What is a quasar. How do we study quasar black holes. Why do we study quasar black holes. What are the current difficulties in studying black holes. How can we improve on the current situation. at . Brookhaven . National Laboratory . 1. Vl. adimir N. Litvinenko . for eRHIC team. Stony Brook University, Stony Brook, NY, USA. Brookhaven National Laboratory, Upton, NY, USA. Center for Accelerator Science and Education. Brittany Vamvakias. Quasars and blazars. A quasar is an active galactic nucleus with a supermassive black hole as the center.. It is thought to be formed by the collision of two galaxies.. A blazar is a more compact and energetic quasar, with the jet pointing towards the Earth.. Jack . Singal. University of Richmond. Stat. . Chall. . In 21. st. Century Cosmology. May 25, 2016. J. Singal, U. Richmond. V. . Petrosian. , Stanford. Orientation. What we have. :. Flux-limited survey catalogs. Gordon Richards. Drexel University. With thanks to. Michael Strauss, . Yue. . Shen. (Princeton), Don Schneider, Nic Ross (Penn State), Adam . Myers (Illinois. ), Phil Hopkins (. Berkeley. ), . and a host of other people from the SDSS Collaboration. e. +. e. –. Collider in the LHC tunnel to study the Higgs Boson. M. Koratzinos. On behalf of the . LEP3 proto-working group. HEP2012: Recent Developments in High Energy Physics and Cosmology. . Ioannina. Division of Particle and Astrophysical Science, Nagoya University, JAPAN. with. SKA-Japan high-. z. galaxy and cosmology WG. East-Asian SKA WS, 30 . Nov. .-2 Dec., 2011, KASI, . Daejeon. , Korea. Formation and Evolution of Galaxies:. Mark Kidger. European Space Agency. European Space Astronomy Centre. Herschel Science Centre. What is a Quasar?. Quasar is a contraction of . Quasi-Stellar Object. .. They are objects that look like faint, blue stars, but are really incredibly distant.. Chandra. and the Inner Structure of AGNs. Warm Absorbers, X-ray Eclipses and . Broad Line Region Inflows, a unification. Martin Elvis. Harvard-Smithsonian Center for Astrophysics. Chandra. taught us about AGN structure. , . are.  . canonical.  solutions . y. (. x. ) of . Bessel's . differential equation. :. α (the . order.  of the Bessel function). Bessel functions are also known as . cylinder functions.  or . conditions. F. Antoniou, . M. . Hostettler, . Y. Papaphilippou. , . S.Papadopoulou. ,. . G. . Papotti. . . Acknowledgements: . Beam-Beam . and Luminosity studies working group, G. . Arduini. , G. . Bunch currentBeam energyRepetition frequency Number of bunches 4 per beamHorizontal emittanceVertical emittanceMax luminosity2 BEAM DIAGNOSTICSThe BEUV telescopes detect the synchrotron light emit-te Charles L. Steinhardt. 1. , . Heng. . Hao. 2. , . Monica . Young. 3. , . Guido Risaliti. 4. , . Francesca . Civano. . Harvard-Smithsonian . Center. for Astrophysics. and. 1. IPMU, Univ. Tokyo; 2..