as tr o - ph / 9 41 10 33 8 N ov 1 99 4

ar X iv : h ep - l at / 9 41 10 15 v 1 9 N ov 1 99 4 1 Instanton size distributions from calibrated cooling

Using an under-relaxed cooling algorithm we investigated the vacuum in the 2d O(3) model and 4d pure gauge SU (2). We calibrated the amount of cooling performed to have similar physical effect at different lattice spacings.

as tr o - ph / 9 80 81 94 19 A ug 1 99 8 Magnetic Field Effects on the Structure of Radiatively

Vol 10 Nos. 3 & 4 #1

m ag ni tu de o f M L = 1. 9. T he n um be r of S tr an dl in e La ke ev en ts lo ca te d du rin g N ov em be rD ec em be r w as lo w er th an th e 35 s uc h ev en ts lo ca te d du rin g th e pr ev io us tw om on th p er io d. R ed ou bt : S ep te m be rO ct ob er 1 99 8: A to ta l o f 1 0 ea rt hq ua ke s w er e lo ca te d in th e R ed ou bt r eg io n du rin g S ep te m be rO ct ob er 1 99 8

ar X iv : a st ro - p h / 99 11 43 8 v 1 2 3 N ov 1 99 9 H 2 molecules and cold clouds in cooling flow clusters †

as tr o - ph / 9 71 20 07 30 N ov 1 99 7

Using a novel two-dimensional coordinate system, we have derived a particularly simple way to express the redshift distortions in galaxy redshift surveys with arbitrary geometry in closed form. This method provides an almost ideal way to measure the value of = 0:6 0 =b in wide area surveys, since all pairs in the survey can be used for the analysis. In the limit of small angles, this result str...