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24 Apr 2007: stars at 24,70,160μm• Akari (2006-) currently doing all-sky survey 2-180μm• Herschel (2008-) observations at 60-670μm• Spica (2017+) planned 5-200μm. ... Structure is wavelength dependent!850μm. (Holland et al. 2006)24 and 70μm. (Su et al.

5 Jun 2007: To demonstrate the power of adding the VISTA IR data to the planned DESoptical data, we have constructed mock magnitude-limited galaxy samples (with 20 < i < 24 and redshifts0 < z < 2)

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20 Jun 2007: Structure” is the only choice for Costing level. Enter the Cost Code, this must be 24 characters.

31 May 2007: 24). In this case the covariance matrix Σ has the relatively simple form.

2 Jul 2007: yi = c1/%( 1. 0Ɛ#t % dt. )1/%1. 10Ɛ#t %1#it dt (24). ... parameter %: If % = 1,the optimal choice of contract quantity (24) dependsonly on the expectation.

27 Jun 2007: First, notice that. (δdw, w) = ‖dw‖2, w C0 (Mint); (3.24)thus, δd is a non-negative operator. ... Let σp(P) stand for the principal symbolof P. Then (3.24) implies that for any such w and a fixed x. (

16 Nov 2007: 2.4.1.2 Minimum Phone Error (MPE) 23. 2.4.1.3 Minimum Classification Error (MCE) 24. ... 2.4.2 Weak-Sense Auxiliary Function and Parameter Re-estimation 24. 2.5 Bayesian Training of HMMs 29.

5 Jun 2007: The DESdesign reference survey strategy is to survey the full 5000deg2 in year 1 for 200secs per bandreaching 10sigma limits[AB mags] in g, r, i and z of 24.1, ... The goal for the full 5 years is a total exposure of 400, 400,1200, 2000 secs in g, r i

18 Jan 2007: 37 36 35 34 33 32 31 12. lastmove 37 36 35 34 33 32 31 30 29 28 27 26 25 24 23 22 21 20 19 18 17 16