'2 kev' diaporamas de présentation

X-ray bursters

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X-Ray Polarimetry Programs in Italy

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Collaborators: - Brian McNamara (Waterloo University & Ohio University)

X-ray cavities in galaxy clusters. Myriam Gitti (UniBO,INAF-OABo). Collaborators: - Brian McNamara (Waterloo University & Ohio University) - Paul Nulsen (Harvard-Smithsonian Center for Astrophysics). ?? Arcetri, 7 Maggio 2009 ??. Plan of the talk Introduction galaxy clusters

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Neutrino Mass and Mixing

Neutrino Mass and Mixing. David Sinclair Carleton University PIC2004. Outline . History of neutrino mass and mixing Recent results and current status Future Prospects. History. Original proposal by Pauli, Fermi Neutrino mass must be small Only 1 neutrino proposed so no mixing.

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The XMM Large Scale Structure (XMM-LSS) Survey

The XMM Large Scale Structure (XMM-LSS) Survey. Andy Read University of Leicester (for the XMM-LSS Consortium). Marseille (LAM) Milano (AOB) Milano (IFCTR) Munich (MPA) Paris (IAP) Santiago (Uni. Cato.). A Europe /Chile Consortium. PI : Saclay, France. Birmingham Bristol

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The hard X-ray Extra-Galactic sky with INTEGRAL/IBIS

The hard X-ray Extra-Galactic sky with INTEGRAL/IBIS. De Rosa on behalf of the INTEGRAL/AGN survey team. High-z QSOs. INTEGRAL (INTErnational Gamma-Ray Astrophysics Laboratory). Astronomical satellite for observing the gamma-ray sky launched on October 17, 2002. Imager IBIS

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Detectability of warm intergalactic medium and the DIOS mission

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Marie Machacek Smithsonian Astrophysical Observatory

Probing the Dynamics of Galaxy-Gas Interactions in Groups and Clusters with Chandra and XMM-Newton. Marie Machacek Smithsonian Astrophysical Observatory. IGM Workshop 3/8/2005. Thanks to my collaborators. Christine Jones William R. Forman Paul Nulsen Ralph Kraft

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369 views • 23 slides

Finding a Logo

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Science motivation of the searching for ? ?

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Surface events suppression in the germanium bolometers EDELWEISS experiment

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Supernova Remnants in the ChASeM33 X-ray Survey of M33

Supernova Remnants in the ChASeM33 X-ray Survey of M33. Knox S. Long, William P. Blair, P. Frank Winkler, and the ChASeM33 team. Background . X-ray H ? [S II] v.

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2. Focusing

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Preliminary Analysis Results of PoGO Argonne Beam Test

Preliminary Analysis Results of PoGO Argonne Beam Test. December 10, 2003 Tsunefumi Mizuno mizuno@SLAC.Stanford.EDU. Data Files. 212 data files and the log (txt and pdf format) can be obtained through the web: http://www.slac.stanford.edu/~mizuno/PoGO/Argonne/index.html

284 views • 17 slides

F. Cappella INFN-Roma

New observation of 2 b 2 n decay of 100 Mo to the 0 + 1 level of 100 Ru in the ARMONIA experiment. SILAFAE Valparaiso , CHILE 6-12 December 2010. F. Cappella INFN-Roma. Roma2,Roma1,LNGS,IHEP/Beijing. + by-products and small scale experiments.: INR-Kiev

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262 views • 16 slides

Study Systematics on the ICM metallicity measurements

Study Systematics on the ICM metallicity measurements. Elena Rasia Chandra Fellow Physics Department, University of Michigan, Ann Arbor. In collaboration with Mazzotta P., Moscardini L., Borgani S., Dolag K., Ettori S., Tornatore L., Bourdin H. (submitted ApJ).

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Simulation for TW FEL @ LCLS-II

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Early Type Stars Observed with ASCA

Early Type Stars Observed with ASCA. Classification Wind Collision & Single Star Objection on the Standard Line Driven Instabilities Elemental Abundance. Six Single Stars. Classification. Colliding Wind Shock HD19379 3.2 keV ?2 Vel 0.3keV+1.4keV V444 Cyg 0.6keV+2 keV

179 views • 9 slides