... References Cappellari M., Emsellem E., 2004, PASP, 116, 138 KЭmmel, M., Larsen, S.S., & Walsh, J.R.: "Slitless Spectroscopy with the Advanced Camera for Surveys", 2006, The 2005 HST Calibration Workshop, STScI Larsen, S.S., Walsh, J.R.: "Updated ...
... Hogbom, J. A. 1974, A&AS, 15, 417 . Steer, D. G., Dewdney, P. E., & Ito, M. R. 1984, A&A, 137, 159 . ... Hogbom, J. A. 1974, A&AS, 15, 417 . Steer, D. G., Dewdney, P. E., & Ito, M. R. 1984, A&A, 137, 159 . ...
... Object Spectrometer and Camera -BFOSC- instrument (Merighi et al. 1994), mounted at the Cassegrain focus of the Bologna Astronomical Observatory ``G.B. Cassini" 1.52 m telescope, sited near Loiano (Italy) at about 800 m altitude on the Appennine Mountains ...
... the primary component in the area # = ## 2 equal 15 16 Grocheva and Kiselev 1 as a ... Let #µ be a random vector, µ = (µ x , µ y ), where µ x = 15µ # cos #, µ y = µ # . ... We construct the matrix M whose elements will be n ij (3). ...
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Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/grochevae.ps.gz -- 100.4 Кб -- 12.06.2006 Похожие документы
... For each scale (except the slowest camera) the camera systems are split in two wavelength regions, one for 1.0 - 2.5 m and a second for 2.0 - 5.0 m. Thus, there are seven imaging systems in total, all of which can be used within the K-band (Figure 1 ). ...
... We produce m =500 pairs of the simulated light curves which have the same power ... data (Oknyanskij, 1997a,b), but for each of m pairs of the simulated light curves ... we approximately estimate the standard error 15 days/year (for V value, which has ...
... m telescope at L2 HIFI: Heterodyne single pixel system 480 to 1250 & 1410 to 1910 GHz FWHP beamsize 12" to 45" SPIRE: Spectral and Photometric Imager Bands at 250, 360 & 520 micrometers FWHP beamsizes 17", 24", & 35" Field-of -View (FOV) 4' by 8' PACS ...
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Ссылки http://www.stecf.org/coordination/esa_eso/alma-herschel/esa-feb11-05-ver4.pdf -- 2622.1 Кб -- 04.09.2008 Похожие документы