... In the SIS model for the lensing mass, and using the minimum flux redshift for zl, the observed image separation of 6 > 5 12 We calculate angularsize distances in our cosmological model using the ANGSIZ code of Kayser, Helbig, & Schramm (1997). ...
... Instrument System Size at Focal Plane AngularSize \Delta p , \Delta ps (mm) \Delta ... which correspond to somewhat different angularsizes than the imaging case because ...
... Given the typical angularsize of relaxed clusters, this requires a field of view (FOV) of 5 arcmin on a side. ... Source Extent: Either point like or extended, if extended, an approximate angularsize. ...
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Ссылки http://hea-www.harvard.edu/~garcia/conx/conx_srd_001008.pdf -- 258.4 Кб -- 28.06.2011 Похожие документы
... Throughout, we assume the following cosmological parameters for distance-dependent quantities: m = 0.3, = 0.7, and H0 = 72 km s-1 Mpc-1 , 1580 which yields an angularsize scale of 5.5 kpc arcsec redshift of our system (z 0.44). ...
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... constant K of the spectral fit as follows: K= 10-14 2 4 DA ne nH dV , (1) http://cxc.harvard.edu/toolkit/pimms.jsp where DA is the angularsize distance to the source in (cm), and ne and nH are the electron and hydrogen densities per cm-3 , respectively ...
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