... 3t 9i e Ѕг q 3 t !g 3 3 P Ё{ } °m Pd Hg 1h Ё 8 8t i H{ Ё І} 9 y S !p 8 'i { Ѕ Hp ' f ... v 3 % !v t !g 'e p fh Py l Іm xi i Ґ 1h Ё t s} Py 8 8t r !v 8 ft І u Ё{ i} 9 9y z ...
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Ссылки http://www.adass.org/adass/proceedings/adass98/reprints/guillaumedr.pdf -- 340.5 Кб -- 16.07.1999 Похожие документы
... Using the most sensitive instrumental configuration (the broad band filter LW2, covering a wavelength range between 5-8.5 m, and 6 PFOV), sources with a flux down to 0.5 mJy can be detected. ...
... atlas, GLIMPSE has used Montage as an engine to co-register 2MASS images in the J, H and K bands and MSX images at 8m. SWIRE will perform a wide area imaging survey of high galactic latitude fields to study the evolution of stellar populations up to z=3 ...
... H jn ЎG 0n VU 8Q Ґi m lP "G Ўk G ji g cH 0h g fe d p 0 ёx ёr x 8 ёv Ґ 8 wv 0u ёr I ... j j ё Y Ўe E Y D ё B° 8Ї ® ¬ ё ts " & Up ¤ @ uj {m Y " u ¦ lj }г !e (e u ¤ ё us Wm ...
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Ссылки http://www.adass.org/adass/proceedings/adass98/reprints/sallkb.pdf -- 214.1 Кб -- 16.07.1999 Похожие документы
... software was originally written for high dispersion spectroscopy, i.e., plates that were 8 in long taken, at 2.5--6.5 љ Amm \Gamma1 , and (under)sampled every 7--8 Їm. Later, the software was modified to handle low dispersion spectra---(80 љ Amm \Gamma1 ...
... n2 sin2 ( t/2) m2 sin2 ( T/2) (10) It is easy to find that the frequencies j = 2 j, m T j = 1, 2, ... (11) satisfy Eq. (8), provided that j = m/2,m,... if m is even and j = m, 2m, ..., if m is odd. ...
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Ссылки http://www.adass.org/adass/proceedings/adass96/reprints/vityazevv1.pdf -- 144.6 Кб -- 14.01.1998 Похожие документы