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1 ular structure, with distinct parameters for intracluster and intercluster coupling, also yields pred
2 on an unusual competition between inter- and intracluster bonds.
3  distance between branch points on the short intracluster chains were similar for all genotypes howev
4                      Furthermore, changes in intracluster closed time distributions were the single b
5 effective opening rate (increase in the mean intracluster closed time duration) in single-channel rec
6                                          The intracluster closed-time histograms contained four compo
7                    Only 12 (20%) reported an intracluster coefficient (median 0.047 [interquartile ra
8 tivation of neural clusters with potentiated intracluster connections, with the firing rate in each c
9 many polymorphisms, consistent with frequent intracluster conversion.
10 ect of cluster sampling is estimation of the intracluster correlation coefficient (rho): the degree o
11 tors across study sites assessed using model intracluster correlation coefficient was substantial at
12 ferences, risk ratios (RRs) and 95% CIs, and intracluster correlation coefficients for each outcome.
13 nt clusters, analyses of such data must take intracluster correlation into account rather than assumi
14 w event rates, low participant numbers, high intracluster correlation) and major contextual changes r
15 dds ratios were obtained with correction for intracluster correlation.
16 iptional networks that convey information on intracluster correlations and intercluster connections o
17                                          The intracluster correlations and the cluster-framework corr
18 l loss with odds ratios, with adjustment for intracluster correlations as appropriate.
19 n sites and their spatial arrangement affect intracluster dynamics preventing conversion to amyloids.
20 induces the generation of Fe(1+) centers via intracluster electron transfer, wherein a neighboring pa
21 in Mossbauer spectra, spin ground state, and intracluster Fe-Fe separation.
22  electrons are highly effective at mediating intracluster ferromagnetic exchange coupling between the
23 til now, however, direct observations of the intracluster gas have been limited only to mature cluste
24 itting 'bubbles' rising buoyantly in the hot intracluster gas, before later falling back.
25 ting processes (such as shock-heating of the intracluster gas, supernovae, and Active Galactic Nuclei
26 SC 122, thus confirming the existence of hot intracluster gas, while deep imaging spectroscopy from t
27 s that produces shocks and turbulence in the intracluster gas.
28 g GRNs to cluster-level analyses that ignore intracluster heterogeneity.
29 s on the nanocluster form local tetramers by intracluster interactions of C-H...pi and pi...pi stacki
30                                              Intracluster light (ICL) is diffuse light from stars tha
31 nteraction of jets with the intergalactic or intracluster media, and in studying the energy generatio
32  hot (10(7) to 10(8) kelvin), X-ray-emitting intracluster medium (ICM) is the dominant baryonic const
33 s of galaxies and pervaded by a diffuse, hot intracluster medium (ICM) that dominates the baryonic co
34 s of the interaction between the hot ionized intracluster medium and the cold interstellar medium of
35 usters, the hot (approximately 10(7) kelvin) intracluster medium can become dense enough that it shou
36                           Cooling of the hot intracluster medium in cluster centers can feed the supe
37 aboratory experiments, support the idea that intracluster medium turbulence may have significantly co
38               Stars and gas in galaxies, hot intracluster medium, and intergalactic photo-ionized gas
39 is cluster may form through accretion of the intracluster medium, rather than (as is currently though
40 at is cospatial with the cooling peak in the intracluster medium, the coolest gas phases and the site
41 xies and a hot, metal-rich gas composing the intracluster medium.
42 highly compressible low-entropy gas from the intracluster medium.
43 the physical properties and evolution of the intracluster medium.
44 uences with seven other group O isolates (5% intracluster nucleotide sequence diversity) similar to c
45                                          The intracluster open durations elicited by beta-alanine cou
46                     The distributions of the intracluster open durations elicited by GABA could be de
47  concentration of cysteamine that elicits an intracluster open probability of >0.9.
48                                  The maximal intracluster open probability was 0.35, with a half-maxi
49 e cores of some clusters of galaxies the hot intracluster plasma is dense enough that it should cool
50                                  Associative intracluster proton transfer Bz(.+)(H2O)(n+1) + H2O-->C6
51                   This suggests a barrier to intracluster proton transfer, and as a result, the [Bz(.
52                                          The intracluster reactions are highly advantageous for appli
53 Louvain clusters of complications with dense intracluster relationships.
54  by sequential addition of HIO3, followed by intracluster restructuring to I2O5 and recycling of wate
55  GDP-protofilaments result in differences in intracluster tension, determining both clustering propen
56 ir ability to identify both intercluster and intracluster variability on a simple bivariate synthetic
57  represent behaviorally distinct stimuli and intracluster variability represents sensory or neuronal