New PDF release: A note on bifurcation from the essential spectrum

By Badiale M.

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The Sunyaev-Zel’dovich effects Rich clusters of galaxies are the largest obvious concentrations of dark matter and baryons in the Universe. Their presence is most evident on X-ray images, where the high luminosities of their extensive hot atmospheres make them prominent sources. The well-known cluster CL 0016+16 (Figure 1) is a good example. 5455 111, the cluster is clearly seen as a bright, extended, X-ray source in a recent XMM-Newton observation [2], and the large number of X-ray counts from the cluster allows the properties of its gas to be well measured.

H. Jaffe, A. E. Lange, A. T. Lee, P. D. Mauslropf, C. B. Netterfield, S. Oh, E. Pascale, B. Rabii, P. I,. Richards, G . F. Smoot, R. Stompor, C. D. Winant, and J. H. P. Wu. MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on Angular Scales of degree. Ap. J. , 545:L5-LL9, Dec. 2000. 4. A. E. Lange, P. A. Ade, J. J. Bock, J. R. Bond, J. Borrill, A. Boscaleri, K . Coble, B. P. Crill, P. de Bernardis, P. Farese, P. Ferreira, K. Ganga, M. Giacometti, E. Hivon, V. V. Hristov, A. Iacoangeli, A.

A limitation of these retro-fitted systems is that their range of antennaantenna separations remains poor for mapping SZEs with high angular dynamic range. For this reason, a new generation of interferometers, better suited to this purpose, including AM1 [24], SZA [25], and AMiBA [26], is under construction. These interferometers will have antenna-antenna spacings optimized for measuring SZEs in known X-ray clusters of galaxies (which has dominated the work to date), and will have sufficient sensitivity to perform deep blank-field searches for SZEs.

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A note on bifurcation from the essential spectrum by Badiale M.


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