... Up: Algorithms . ... Non-linear and non-parametric algorithms for data averaging, smoothing and clipping in the RATAN-600 flexible astronomical data processing system are proposed. Algorithms are based on robust methods and non-linear filters using an iterative approach to smoothing and clipping. ... The history of algorithms, based on the robust methods and non-linear filters using an iterative approach to smoothing and clipping, began twelve years ago in the data reduction at the RATAN-600. ...

LRG) .. ... 1 III 28.09.2010 ~100 Mpc/h . ... 2 III 28.09.2010 WMAP 3 III 28.09.2010 (2- ) Kazin E. et. al. 2010, A&A) 2- SDSS main galaxies 4 III 28.09.2010 (GOODS) Balestra I. et al. ... 2- ) (GOODS) ( ) 8 III 28.09.2010 9 III 28.09.2010 10 III 28.09.2010 11 III 28.09.2010 LRG ( ) SDSS DR7. ... 12 III 28.09.2010 LRG Kazin et al. ... 3 : 102±8 Mpc/h, 51±4 Mpc/h, 29±3 Mpc/h 14 III 28.09.2010 15 III 28.09.2010 ? ... 17 III 28.09.2010 102 Mpc/h 80 Mpc/h , 3 18 III 28.09.2010 102 Mpc/h 80 Mpc/h , . ...

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Выберите: 1-101 1-102 2-101 3-101 3-102 4-101 4-103 4-104 5-101 5-102 5-103 6-101 6-102 6-103 7-101 7-102 10-101 10-102 10-103 11-101 12-101 12-102 АНТК - 21 АНТК - 41 АНТК - 61 1- 21 1- 22 2- 21 3- 21 3- 22 4- 21 4- 22 5- 21 5- 22 6- 21 6- 22 7- 21 7- 22 8- 21 8- 22 9- 21 9- 22 10- 21 10- 22 11- 21 12 ...

To: file acf-to-spectrum.wpd From: Jon Hagen Date: April 2, 2004 Subject: Transforming correlation functions to spectra I. Recovering a Power Spectrum from a Sampled Autocorrelation Function The power spectrum, by definition, is the Fourier Transform of the autocorrelation function (ACF). ... Note also that the sampled ACF points extend only to some max, so the spectrum we calculate will have been effectively convolved with a smoothing function. ... Let us denote the cross spectrum as U() + jV(). ...

... 0.5 ( ) , 0.0 ­ . ... R. P. Fender, E. Gallo, D. Russell, MNRAS, 2010 : Lbol GM = Mc , RH = c2 2 BH 2 [1 + 1 - ax ], ax - _ M BH M M BH M L 5100 6.91 = 10 44 10 erg / s L 5100 7, 69 = 10 44 10 erg / s 0.5 FWHM ( H 3 10 km / s 0.5 ) 2 FWHM ( MgII ) 3000km / s 2 L M BH = 2 в 106 42 H M 10 erg / s L M BH = 3.37 44 3000 M 10 erg / s 0.47 0.55 FWHM ( H 3 10 km / s ) 2.06 FWHM ( MgII ) km / s 2 AGN (Equipartition) R.-Y. Ma, F. Yuan, arXiv:0706.0124. ...

Краткие характеристики . ... Нептун . ... Основные параметры: . ... ОСНОВНЫЕ ПАРАМЕТРЫ ПЛАНЕТЫ . ... Экваториальный радиус (км) . ... Вторая космическая скорость (км/с) . ... Температура абсолютно черного тела (k) . ... ОСНОВНЫЕ ПАРАМЕТРЫ ОРБИТЫ . ... Сидерический период орбиты (дней) . ... ОСНОВНЫЕ ПАРАМЕТРЫ ОБСЕРВАТОРИЙ . ... ОСНОВНЫЕ ПАРАМЕТРЫ АТМОСФЕРЫ . ... ОСНОВНЫЕ ПАРАМЕТРЫ СПУТНИКОВ . ... Наяда (NIII - 1989) . ... Наклон орбиты - угол между плоскостью орбиты и основной координатной плоскостью. ...

. CTA 102 = 2230+114 . R.A. ( J2000.0) =22 32 36.4 . Dec. (J2000.0)= +11 43 51 . J band, 4x4 arcmin . Recommended standard stars . star . J . err J . H . err H . K . err K . 1 . 14.607 .004 . 14.102 .009 . 14.078 .004 . 2 . 13.313 .004 . 12.762 .009 . 12.591 .004 .

... SIEMENS, 1 ф. 6А-40А . ... 600 . ... SIEMENS, 3 ф. 50А, 63A . ... УЗО SIEMENS, 1 ф. (Германия) . ... MERLIN GERIN 1 ф. 30 . ... Legrand (ABB), 1 п. 1A-5А . ... Legrand (ABB), 1 п. 10А-25А . ... Legrand (ABB), 1 п. 32А . ... Legrand (ABB), 1 п. 40А . ... Legrand (ABB), 1 п. 50А, 63A . ... Legrand (ABB), 3 п. 6А-25А . ... Legrand (ABB), 3 п. 80А . ... Legrand (ABB), 3 п. 100А . ... Legrand (ABB), 3 п. 50А; 63А . ... Диф. авт. ... MERLIN GERIN (Франция) 1 ф. 1800 . ... MERLIN GERIN (Франция) 3 ф. 2400 ...

Search this album . ... Comet Halley 1985-86 . Halley 24-02-86 6m IIIaJ . ... 12m IIIaJ" class="g-sb-preview g-hide" rel="g-preview" href="/gallery3/var/albums/first100years/album34/Halley131185.jpg?m=1378189632"> 15m IIIaJ" class="g-sb-preview g-hide" rel="g-preview" href="/gallery3/var/albums/first100years/album34/Halley161185.jpg?m=1378189632"> 8m IIIaJ" class="g-sb-preview g-hide" rel="g-preview" href="/gallery3/var/albums/first100years/album34/Halley131285.jpg?m=1378189632"> . ...