... U. Becciani, V.Antonuccio and M.Gambera . Osservatorio Astrofisico di Catania . ... computational domain is subdivided into M subdomains (proportionally to the weights ...
... 9000 е -1403.8 -13.049 a1 (X) a2 (Y) a3 (X2) a4 (XY) a5 (Y2) r.m.s. 0.046017 4.398E-4 1.231E-6 -0.15926 0.001314 -6.37E-6 -2 ... shows the difference between the two calibrations (in е) as a function of wavelength for 15 positions across the detector ...
... 1) where M A and M B are stellar masses, a - orbital separation of components, - angular velocity of the system about the z ... 2) where q = M B / M A , is the dimensionless Roche potential . ...
... 30 30 30 1515151515151515,1515,1515,1515,1515,1515,15 Texp (PR110L) (s ... M., Larsen, S. S., & Walsh, J. R., 2005, Slitless Spectroscopy with the Advanced ...
... The situation deteriorates slightly around z 15, but the result is due mainly to the insufficient sampling of the SEDs between the Ks and the M filters, in particular to the "hole" at 2.9 µm. The importance of the leaks, relative to the uncertainty due to ...
... Code for Structure Detection 495 Gambera, M., Pagliaro, A., Antonuccio-Delogu, V ... 15, 723 Grossmann, A., Morlet, J., 1987, Math. ... L94) e Lega, E., Scholl, H., Alimi, J.-M., Bijaoui, A., Bury, P., 1995, Parallel ...
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Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/pagliaroa.pdf -- 69.7 Кб -- 12.06.2006 Похожие документы