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30 Nov 1998: 35.2 68P10 06 23 56.0 42 50 42 369 408 0.09 12.5 68P11 06 24 21.0 43 22 37 186 235 0.13 8.1 68P12 ... 06 24 28.4 43 53 42 179 221 0.15 8.8 68P13 06 24 29.0 43 01 30 243 278 0.11 10.0 68P14 06 24

15 Jan 1998: 139 (E) 394 412 (Ta3) 2.64 (9)4 490 495 (Ta4) 5 6 205 222 (F) 525 534 (Ta5) 2.24 (5)60 536 545 (Ta50) 7 243 263 (G) ... 24%. Despite this relatively weak con-servation both enzymes share a very similar three-dimensional structure (Moser et al., 1997).

30 Nov 1998: 53P1 10 01 04.41 46 40 51.9 34.0 32.6 0.20 24.5 53P2 10 01 51.97 46 19 57.6 20.6 21.2 ... 0.26 13.6 53P107 10 15 33.70 46 24 17.6 14.6 33.3 0.24 12.2.

30 May 1998: Nature. 365: 65–68. 24. Gordon, D. A., J. R. Wetterau, and R. ... J. Lipid Res. 24: 1243–1250. 33. Rouser, G., A. N. Siakatos, and S.

9 Sep 1998: 10.2 (24.1) 9.0 (17.9)Riso (%). c 32.5Phasing power 1.29 (0.77)Anomalous phasing power 1.33 (0.57)Resolution in outer shell (Å) ... 2.20 3.24–3.0Rfactor 0.190Rfree (10% of data) 0.258.

30 Nov 1998: that magnitude that gives 1 detected photon/s) are: CCD U B V R I Z #1 23.8 25.6 25.7 25.6 24.9 #2 23.8

14 Oct 1998: 1.24) δ(p) = limn. {n(d1)/d log Pp(|C|= n). }exists and is strictly positive when p > pc. ... The existence of the limit in (1.24) has been proved when d = 2 by Alexander,Chayes, and Chayes (1990), and when d = 3 by Cerf (1998b).

30 Nov 1998: 24.6 48 39 43 824 877 0.11 17.2 52P4 10 24 02.8 45 01 10 566 612 0.18 20.8 52P5 10 24 12.8 46 ... 18 15 4169 4461 0.25 80.0 52P6 10 24 29.4 48 32 38 2652 2988 0.20 50.4 52P7 10 25 25.2 47 20 06 168

29 Nov 1998: The image detection thresholds on the O and E plates were around 24 mag arcsec. ... and 24 mag arcsec. Detected images were parameterised to preserve coordinate, intensity and general shape information.

1 Mar 1998: shows. Table 1. Comparison of RIDOS with other Optical Surveys Survey Limiting Mag Sky Area Resolution Availability (R) (sq deg) arcsec (to community) ----------------------------------------------------------------------- RIDOS 24.5 100-200 1 from