... The aim of C1109 is to survey the sky polarization at 5 GHz in the Boomerang field to provide information about polarized foregrounds in future measurements of the polarized Cosmic MicrowaveBackground (CMBP). ...
... However, the increasing interest in cosmic microwavebackground (CMB) maps provided by the on-going NASA WMAP mission and the forthcoming ESA Planck mission requires good measurements of high frequency properties of radio-sources to interpret the data ...
... is essential, however, for understanding the dynamics in our local Universe, in particular the peculiar velocity of the Local Group with respect to the Cosmic MicrowaveBackground and velocity flow fields such as in the Great Attractor (GA) region ...
... But owing to the wide-ranging knowledge of many audience members, many of the review talks were well-received - for example, the series of reviews on the Cosmic MicrowaveBackground and the Dark Matter problem. ...
... Antenna Control Computer (used in the ATCA). Array for MicrowaveBackground Anisotropy. ... CMB Cosmic MicrowaveBackground. CSIRO Commonwealth Scientific and Industrial Research Organization. ...
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Ссылки http://www.atnf.csiro.au/the_atnf/annual_reports/2000/Appendices.pdf -- 156.9 Кб -- 08.01.2002 Похожие документы
... Understanding the origin of the peculiar velocity of the Local Group and the dipole in the Cosmic MicrowaveBackground is one of the major goals of the study of large-scale structures. ...
... Way rotation Milky Way motion Local Group motion Local Supercluster motion Local Group Barycentric Virgocentric MicrowaveBackground Spectral Line Imaging ATNF Synthesis School, Narrabri 14 May 2003 Correlator Configurations Correlator Configurations ...
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Ссылки http://www.atnf.csiro.au/whats_on/workshops/synthesis2003/talks/specline.pdf -- 956.1 Кб -- 22.05.2003 Похожие документы