PPT-Period-Luminosity Relations for Small Magellanic

Author : pasty-toler | Published Date : 2016-06-09

Cloud Cepheids Based on AKARI Archival Data Abstract Background Conclusion Previous research done in the Midinfrared for the Large Magellanic Cloud LMC done by

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Period-Luminosity Relations for Small Magellanic: Transcript

Cloud Cepheids Based on AKARI Archival Data Abstract Background Conclusion Previous research done in the Midinfrared for the Large Magellanic Cloud LMC done by Ngeow et al 2010 and Madore et al 2009 showed drastically different PL relations. 2015. . Old Dominion . University. Colliders, Luminosity, & Crabbing. Todd Satogata (Jefferson Lab) / . satogata@jlab.org. Vasiliy. Morozov (Jefferson Lab) . / . morozov@jlab.org. . Alex . Castilla. 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 . 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 . Mike Lamont. Thanks for discussion: R. . Assmann. , R. Bailey, M. Ferro-. Luzzi. , S. . Fartoukh. , O. . Bruning. . The future is a strange place. Aim of the exercise is to establish some realistic numbers given accepted constraints. F. Antoniou, Y. . Papaphilippou. Beam-Beam and luminosity studies meeting, 22/6/15. Luminosity model components. 2. . Beam current decay with time . Beam size (or emittance) evolution with time . 13/4/2015. . state. . studies. I. ntroduction. Máté Szalai. 16.09.2015.. Corvinus. University of Budapest. 1. . Why. . should. . we. . study. . small. . states. ?. 2. . How. . have. . small. . states. 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. 2015. . Old Dominion . University. Colliders, Luminosity, & Crabbing. Todd Satogata (Jefferson Lab) / . satogata@jlab.org. Vasiliy. Morozov (Jefferson Lab) . / . morozov@jlab.org. . Alex . Castilla. conditions. F. Antoniou, . M. . Hostettler, . Y. Papaphilippou. , . S.Papadopoulou. ,. . G. . Papotti. . . Acknowledgements: . Beam-Beam . and Luminosity studies working group, G. . Arduini. , G. . Fossil Groups Origins (FOGO) project: . X-. ray. . scaling. . relations. in . Fossil. . systems. R. . Barrena. (IAC, Spain). , A. Biviano (OAT, Italy), S. Borgani (UT, Italy), W. Boschin (TNG, Italy), N. Castro-Rodriguez (IAC, Spain), E. M. Corsini (UP, Italy), . Bunch currentBeam energyRepetition frequency Number of bunches 4 per beamHorizontal emittanceVertical emittanceMax luminosity2 BEAM DIAGNOSTICSThe BEUV telescopes detect the synchrotron light emit-te 5 5 the data for very small radii in some synthetic Res of high luminosity the observed the luminosity R200 ie the radius encompassing their rms errors limit the uncertainties agreement between the da Bunch currentBeam energyRepetition frequency Number of bunches 4 per beamHorizontal emittanceVertical emittanceMax luminosity2 BEAM DIAGNOSTICSThe BEUV telescopes detect the synchrotron light emit-te Samir . Arfaoui. Stony Brook University. 5 December 2011. Samir Arfaoui - LAr Week. 1. Measurement principle. 7 December 2011. Samir Arfaoui - LAr Week. 2. Pros:. Trigger independent. DAQ independent.

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