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20 Jul 2006: White. (9=) SU4 low mass point at limit of runII reach (isasugra 7.71: m0=200 geV, m12 = 160 geV, A0 = -400 geV, tan beta = 10, sgn(mu) = ). 100k Voss. (9=)

27 Apr 2006: The mean volume fraction 4,. 0 I I,,,, I0 100 200 300 400 500. ... whoseheight h ‘ H. Substituting. 0 0 100 200 300 500 M0 M= p0AH (A.4).

22 Nov 2006: IEEE TRANS. ON SAP, VOL? , NO? ,? 200? 1. Automatic Model Complexity Control Using. ... 200? 7. as the average phone correctness of all possible word sequences {W̃},.

5 May 2006: 0 20 40 60 80 100 120. 500400300200100. 0–100–200. 200300. 1000. ... 0 20 40 60 80 100 120. –100–200–300. Time (s)Time (s).

8 Jun 2006: 150. 200. 247. Supplementary Figure 2. Sequence alignments and 3D models of C.

19 Apr 2006: the range 110–200 AU with low eccentricitiesand inclinations (e < 0.01, I < 0.573). ... One problem is thatboth the 200 and 325 AU spirals have large azimuthal densityvariations which make them appear clumpy.

19 Apr 2006: higher surface brightness at r >200 AU compared to the r4 power law. ... but has slightlyhigher surface brightness at r > 200 AU compared to ther4 power law.

14 Dec 2006: 2004), we estimate for the firsttime the detection rate of cold debris disks around field M-dwarfs with ages between 20 and 200 Myr. ... al. 2005), the Castor moving group(200 Myr), the Ursa Maj moving group (500 100 Myr asrevised by King et al.

27 Nov 2006: The moments cannot be. 4. 50 100 150 200. 0.01. 0.02. ... 11 cos x e. iω(4x2x3). 50 100 150 200. 0.01. 0.02.

5 May 2006: pulses, 512 µs in duration and anacquisition width of 200 kHz was used. ... In our velocity imaging experiments the echo time TE was 10.3 ms, while theobservation time was 200 ms.