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Results 1 - 10
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1,520
Distributional Clustering Of English Words
- In Proceedings of the 31st Annual Meeting of the Association for Computational Linguistics
, 1993
"... We describe and evaluate experimentally a method for clustering words according to their dis- tribution in particular syntactic contexts. Words are represented by the relative frequency distributions of contexts in which they appear, and relative entropy between those distributions is used as the si ..."
Abstract
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Cited by 629 (27 self)
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as the similarity measure for clustering. Clusters are represented by average context distributions derived from the given words according to their probabilities of cluster membership. In many cases, the clusters can be thought of as encoding coarse sense distinctions. Deterministic annealing is used to find lowest
A Highly-Scalable Cluster Membership Protocol
"... Membership management (knowledge of the running processors and fault-detection mechanism) is a crucial component of any cluster-based network service. To date, existing procotols scale poorly with the number of nodes, thus limiting the scale of cluster computing. This paper describes a new membe ..."
Abstract
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Membership management (knowledge of the running processors and fault-detection mechanism) is a crucial component of any cluster-based network service. To date, existing procotols scale poorly with the number of nodes, thus limiting the scale of cluster computing. This paper describes a new
X-RAYS AND YOUNG CLUSTERS Membership, IMFs and distances
, 2005
"... Sensitive imaging X-ray observations of young stellar clusters (YSCs, ages ≤ 10 Myr) are valuable tools for the acquisition of an unbiased census of cluster members needed for Initial Mass Function (IMF) studies. Several dozen YSCs, both nearby and across the Galactic disk, have been observed with t ..."
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Sensitive imaging X-ray observations of young stellar clusters (YSCs, ages ≤ 10 Myr) are valuable tools for the acquisition of an unbiased census of cluster members needed for Initial Mass Function (IMF) studies. Several dozen YSCs, both nearby and across the Galactic disk, have been observed
Accepted to AJ A Probabilistic Quantification of Galaxy Cluster Membership
, 2000
"... Clusters of galaxies are important laboratories for understanding both galaxy evolution and constraining cosmological quantities. Any analysis of clusters, however, is best done when one can reliably determine which galaxies are members of the cluster. While this would ideally be done spectroscopica ..."
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, which, while useful in a global sense, does not provide information for specific galaxies. In this paper, we develop a more robust technique which uses photometrically estimated redshifts to determine cluster membership. This technique can either be used as an improvement over the commonly used
Value added of cluster membership for micro enterprises of the handloom sector in Ethiopia
- World Development
, 2011
"... The NetherlandsValue added of cluster membership in micro enterprises Applying Propensity Score Matching to the handloom sector in Ethiopia The purpose of this study is to investigate clustering advantages by contrasting the performance of clustered micro enterprises, in terms of profit, with that o ..."
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Cited by 3 (1 self)
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The NetherlandsValue added of cluster membership in micro enterprises Applying Propensity Score Matching to the handloom sector in Ethiopia The purpose of this study is to investigate clustering advantages by contrasting the performance of clustered micro enterprises, in terms of profit
Maximum stellar mass versus cluster membership number revisited
, 808
"... Oey & Clarke (2005)) that in the case of clusters containing fewer than ∼ 100 OB stars (i.e. those with mass < a few × 10 4 M⊙) the maximum stellar mass increases with cluster mass. At higher ..."
Abstract
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Cited by 2 (0 self)
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Oey & Clarke (2005)) that in the case of clusters containing fewer than ∼ 100 OB stars (i.e. those with mass < a few × 10 4 M⊙) the maximum stellar mass increases with cluster mass. At higher
Maximum stellar mass versus cluster membership number revisited
, 2008
"... Oey & Clarke (2005)) that in the case of clusters containing fewer than ∼ 100 OB stars (i.e. those with mass < a few × 10 4 M⊙) the maximum stellar mass increases with cluster mass. At higher ..."
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Oey & Clarke (2005)) that in the case of clusters containing fewer than ∼ 100 OB stars (i.e. those with mass < a few × 10 4 M⊙) the maximum stellar mass increases with cluster mass. At higher
Results 1 - 10
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