ライフサイエンスコーパス: Ne

1 Ne curves of all study species converged 1.0 million yr

2 Ne reflects the effect of random sampling on the genetic

3 Ne(-)max = 4.4(1.0) x 10(20) cm(-3) for CoCp*2 and 1.3(0

4 t risk of acquisition of HIV (4.7, 2.2-10.1; Ne=6).

5 among higher-risk populations (1.7, 1.4-2.1; Ne=25).

6 the form Ni(+)(C(2)H(2))(n), Ni(+)(C(2)H(2))Ne, and Ni(+)(C(2)H(2))(n)Ar(m) (n = 1-4) are produced i

7 differences in elemental abundances and (20)Ne/(22)Ne ratios between the Iceland mantle plume and th

8 rrelated with (129)I-derived (129)Xe and (20)Ne/(22)Ne ratios that are higher than the atmospheric (2

9 te yielded atmospheric (38)Ar/(36)Ar and (20)Ne/(22)Ne.

10 ios that are higher than the atmospheric (20)Ne/(22)Ne ratio.

11 epletion of all atmospheric noble gases ((20)Ne, (36)Ar, (84)Kr, (132)Xe) with respect to air-saturat

12 e gases and their isotopes (e.g., (4)He, (20)Ne, (36)Ar) in groundwater near shale-gas wells.

13 Ar fractionation levels along with (4)He/(20)Ne with distance to the nearest gas production wells doe

14 icantly more enriched in crustal (4)He*, (21)Ne*, and (40)Ar* than Barnett gas.

15 osed-system radiogenic noble-gas ((4)He, (21)Ne, (40)Ar, (136)Xe) residence times.

16 Cosmic-ray-produced (3)He, (21)Ne, and (36)Ar yield concordant surface exposure ages of

17 ositively correlated with crustal (4)He, (21)Ne, and (40)Ar and suggest that noble gases and methane

18 etermined to be the carrier of anomalous (22)Ne in ancient meteorites.

19 Atmospheric (22)Ne/(36)Ar ratios of stray gas mimic also that of Strawn,

20 That exotic (22)Ne is, in fact, the decay isotope of relatively short-li

21 t are higher than the atmospheric (20)Ne/(22)Ne ratio.

22 ences in elemental abundances and (20)Ne/(22)Ne ratios between the Iceland mantle plume and the MORB

23 d with (129)I-derived (129)Xe and (20)Ne/(22)Ne ratios that are higher than the atmospheric (20)Ne/(2

24 ded atmospheric (38)Ar/(36)Ar and (20)Ne/(22)Ne.

25 w that sequential hermaphroditism may affect Ne differently over varying time frames, and that demogr

26 An Ne of 48 over a 32-year period would imply that this pop

27 owledge, of entrapment of atmospheric Ar and Ne in phengite and omphacite.

28 Earth to determine the composition of Ar and Ne returned from mantle depths to the surface by forearc

29 We measured Ar and Ne trapped in phengite and omphacite from the youngest k

30 % for Kr, 8% for Xe, and 3% for CH4, N2O and Ne.

31 mples should be equally influenced by Nb and Ne and confirm this with simulated results: [Formula: se

32 e contrasting effects of T and Vk* on Ne and Ne/N are jointly considered with respect to d and phi.

33 arameters effective population size (Ne) and Ne/N is revisited for iteroparous species with overlappi

34 dances of light elements such as C, N, O and Ne has, however, broken this accordance: models adopting

35 Na, and S and highly ionized solar C, O, and Ne.

36 e mass of the colliding gas species (He, Ar, Ne, Kr, Xe, CH4, and N2).

37 inity to <0.1% of the true value (defined as Ne based on 100% sampling).

38 ns designed to evaluate the bias of LD-based Ne estimates ([Ncirc ]e).

39 n one gene pool, which would downwardly bias Ne and (2) reductions in drift LD (and hence upward bias

40 umulating genetic estimates in terms of both Ne (which influences long-term evolutionary processes) a

41 effect of Nn on Ne was well approximated by Ne=N/(1-FIS), where FIS (determined by Nn) was evaluated

42 Repeated measurements of C = Ne/DeltaV with this method have a relative standard devi

43 nation, which if not accounted for can cause Ne estimates to be downwardly biased.

44 tic shunt, which was confirmed using cholyl-(Ne-NBD)-lysine as a tracer.

45 mbined with LD data to estimate contemporary Ne at various times in the past.

46 enetic approaches that estimate contemporary Ne, the method based on linkage disequilibrium (LD) assu

47 , LD-based method of estimating contemporary Ne to include linkage information and show via simulatio

48 antify the bias in estimates of contemporary Ne associated with the assumption that all loci in a lar

49 Estimates of contemporary Ne were significantly lower in the protogynous species,

50 f adsorption of several small gases (H2, D2, Ne, N2, CO, CH4, C2H6, Ar, Kr, and Xe) on the metal-orga

51 to demographic variance and thus decreasing Ne /N in a small age-structured population inhabiting a

52 broadening analysis of the electron density Ne and temperature Te in a laser-induced plasma (LIP), u

53 (3) dependence, so the density of electrons (Ne(-)max) is constant over a range of NC sizes.

54 Cell contact rearrangements (Ne/Epi + Ne/Epi --> Ne/Ne + Epi/Epi) just behind the zipper lower

55 rior to anterior along the neural/epidermal (Ne/Epi) boundary just ahead of the advancing zipper.

56 crystal structures of Nanoarchaeum equitans (Ne) C3PO.

57 esponse-locked error-related negativity (ERN/Ne), and response-locked error positivity (Pe), measured

58 d beyond other measures (i.e., N2, P300, ERN/Ne, age, sex, IQ, impulsivity, depression, anxiety, moti

59 error-monitoring, as indexed by smaller ERN/Ne; and adjusting response strategy posterror, as indexe

60 r than a method designed to jointly estimate Ne and m.

61 od and detailed demographic data to estimate Ne /N for a small and apparently isolated red-billed cho

62 am fir, Abies balsamea, in order to estimate Ne/N.

63 In this study, we estimate Ne from genetic data collected from two ecologically sim

64 RR 2.7, 95% CI 2.2-3.4; number of estimates [Ne]=22) and was roughly doubled among higher-risk popula

65 developed areas in predicting and estimating Ne for future research.

66 port, we introduce a strategy for estimating Ne dynamics, allowing the exploration of large multi-loc

67 However, estimating Ne , and identifying key demographic mechanisms that und

68 phisticated demographic method of estimating Ne /N, which uses Fisher's reproductive value to account

69 ilbrium), the accuracy is 0.7% or better for Ne/Kr, Ne/Ar, and Ar/Kr, and 2.5% or better for Ne/Xe, A

70 Kr, Ne/Ar, and Ar/Kr, and 2.5% or better for Ne/Xe, Ar/Xe, and Kr/Xe using air as the only calibratio

71 ield accuracy improves to 0.6% or better for Ne/Xe, Ar/Xe, and Kr/Xe when the data is calibrated usin

72 for many generations, with consequences for Ne estimates that remain to be evaluated.

73 We use an electron energy of 35 V for Ne to eliminate isobaric interferences, and a higher ele

74 tion in the effective populations size (from Ne=500 to Ne=75).

75 excellent agreement with that derived from [Ne iv], formed in the same region of the nebula as [K v]

76 s reflect the effective size per generation (Ne).

77 s a consequence, never approached the global Ne, even when the geographic scale of sampling was large

78 contact rearrangements (Ne/Epi + Ne/Epi --> Ne/Ne + Epi/Epi) just behind the zipper lower tissue res

79 he simultaneous measurement of dissolved He, Ne, Ar, Kr, Xe, SF6, N2, and O2 concentrations in a sing

80 Here I present new noble gas (He, Ne, Ar, Xe) measurements from an Icelandic OIB that reve

81 endohedral atoms and ions (X = H(+), H, He, Ne, Ar, Li(0,+), Be(0,+,2+), Na(0,+), Mg(0,+,2+)) have b

82 f endohedral atoms and ions including H, He, Ne, Li(0,+), Be(0,+,2+), Na(0,+), and Mg(2+).

83 uantificaton of the partial pressures of He, Ne (in dry gas), Ar, Kr, N2, O2, CO2, and CH4 in gaseous

84 In DCDB MIBD, a He-Ne laser beam passes through a half-wave plate onto the

85 optical response was calibrated using an He-Ne laser at 632 nm.

86 gratings were irradiated with a 632.8-nm He-Ne laser.

87 corded as a function of incident angle of He-Ne laser beam using a laboratory assembled SPR setup.

88 llary cell and detected using a low-power He-Ne laser.

89 Samples were excited with a He/Ne laser at 632.8 nm and SERS was detected by a CCD came

90 um concentrations and elemental ratios of He/Ne and He/Ar in OIBs are an order of magnitude lower tha

91 ion, this formula is a good approximation if Ne >> 1.

92 ctions in drift LD (and hence upward bias in Ne) caused by an increase in the number of parents respo

93 hat even relatively small, recent changes in Ne can be detected reliably with a modest number of sing

94 g, so the timing and amplitude of changes in Ne differed among species and even among conspecific lin

95 ne fish where a recent, temporary decline in Ne is known to have occurred.

96 angrove species further shows the decline in Ne to be strongly associated with the speed of past chan

97 , might have led to the early differences in Ne detected in our analyses.

98 d Muller's ratchet, result in a reduction in Ne, which increase the likelihood of fixation of deleter

99 te loci data to compare historical trends in Ne with population dynamic parameters.

100 n only had a notable influence of increasing Ne as it became smaller (16).

101 either continuous or pulsed beams of 500 keV Ne, Ar, Kr, or Xe ions.

102 ), the accuracy is 0.7% or better for Ne/Kr, Ne/Ar, and Ar/Kr, and 2.5% or better for Ne/Xe, Ar/Xe, a

103 E is quantified by its characteristic length Ne (specified in charged residues) and its consequences

104 different from that of simpler targets like Ne or CH4, which is not the case for fluorene.

105 ng mixture LD and depress estimates of local Ne.

106 Similarly, a low Ne was also evident for the colonization of pneumococcus

107 However, low Ne for the Y should be counterbalanced to some extent by

108 could be a factor determining some very low Ne/N that have been published.

109 ons are theoretically expected to have lower Ne than gonochorists (separate sexes), assuming all othe

110 With higher m, Ne converges on the global (metapopulation) Ne.

111 Ne converges on the global (metapopulation) Ne.

112 mitting medium, formation of nanocrystalline Ne inside hollow NPs is not detected by XRD, indicating

113 aw [Formula: see text] based on the ratio Nb/Ne, which can be estimated from two or three simple life

114 e used to evaluate the influence of d on Ne, Ne/N and the factors that determine these parameters: ad

115 100 ms after the so-called error negativity (Ne), from which it was therefore distinguished.

116 ity on errors, the error-related negativity (Ne/ERN), in a task in which two types of errors could oc

117 num (Pt), the NaCl-B2 phase, and solid neon (Ne) at 300 K and high temperatures up to megabar pressur

118 ration variation of reproductive success (Nt/Ne(i)), population dynamics (ki), and the proportion of

119 of effective population size/census number (Ne/N).

120 r detection are responsible for the observed Ne/ERN amplitude reductions.

121 hown to be a robust predictor (R(2)=0.78) of Ne/N in an empirical data set of life tables for 63 anim

122 a mass spectrometer (GC-MS) for analysis of Ne, Ar, Kr, Xe, N2, and O2 and an electron capture detec

123 They thereby demonstrate how assessments of Ne can incorporate stochastic sex- and age-specific demo

124 rotons per NC and the dramatic dependence of Ne(-)max on the nature of the cation (H(+) vs MCp*2(+))

125 different elements, given determinations of Ne and Te based on appropriate parameters for at least o

126 The demographic estimate of Ne /N was 0.21, reflecting a high total demographic vari

127 The demographic estimate of Ne was 30, suggesting that rates of increase of inbreed

128 entire interval, 1961-1993, the estimate of Ne was 48 when based on a weighted mean derived from the

129 with short adult lifespans, the estimate of Ne/N is largely unbiased because biases in T are compens

130 on which could bias demographic estimates of Ne .

131 Molecular genetic estimates of Ne computed from linkage disequilibrium and approximate

132 Estimates of Ne for the time intervals 1961-1977 and 1977-1993 were 3

133 n samples (T=1-32 generations), estimates of Ne ranged from infinity to <0.1% of the true value (defi

134 the surge of genetically based estimates of Ne that has been fueled by the genomics revolution.

135 LD estimates of Ne therefore accurately reflect local (subpopulation) Ne

136 single-sample molecular genetic estimates of Ne to corroborate the demographic estimate and examine e

137 st, the effect of Nn on genetic estimates of Ne was substantial.

138 Although Nn is independent of Ne, the reverse is not true.

139 (2) = 0.98) function of the harmonic mean of Ne and Nb.

140 ovides continuous, real-time measurements of Ne, Ar, Kr, and Xe mole ratios in natural waters.

141 ression in the short term is of the order of Ne approximately 70 for a wide range of species' reprodu

142 a recent origin of In(3R)P, on the order of Ne generations.

143 Our data revealed a pattern of Ne/ERN amplitudes that closely mirrored the amount of mo

144 This promotes rapid shortening of Ne/Epi junctions, driving the zipper forward and drawing

145 g and normal forests our estimated values of Ne/N were about twice those previously reported for annu

146 s are used to evaluate the influence of d on Ne, Ne/N and the factors that determine these parameters

147 lants, it was found that the effect of Nn on Ne was well approximated by Ne=N/(1-FIS), where FIS (det

148 ime, the contrasting effects of T and Vk* on Ne and Ne/N are jointly considered with respect to d and

149 r, with estimated effective sizes 500 < or = Ne < or = 1000, were selected for increased performance

150 s Rcr3 is allelic to the L. pimpinellifolium Ne gene, which suppresses the Cf-2-dependent autonecrosi

151 between the effective size of a population (Ne) and the effective size of its neighborhoods (Nn) has

152 ound in the successively sampled population (Ne = 5-20).

153 Cell contact rearrangements (Ne/Epi + Ne/Epi --> Ne/Ne + Epi/Epi) just behind the zip

154 opulation restriction despite a large recent Ne.

155 Estimates of recent Ne in two solanaceous species differed by an order of ma

156 A population's effective size (Ne ) is a key parameter that shapes rates of inbreeding

157 ies of changes in effective population size (Ne ) and used a Bayesian-coalescent based approach that

158 rienced a steady decline in population size (Ne ) thereafter.

159 ionary parameters effective population size (Ne) and Ne/N is revisited for iteroparous species with o

160 and the estimated effective population size (Ne) based on synonymous sites was approximately 1.8-4.2

161 Contemporary effective population size (Ne) can be estimated using linkage disequilibrium (LD) o

162 n of contemporary effective population size (Ne) from linkage disequilibrium (LD) between unlinked pa

163 ctor that reduces effective population size (Ne) in natural populations.

164 Effective population size (Ne) is a key parameter in population genetics.

165 Effective population size (Ne) is an important genetic parameter because of its rel

166 ajor reduction in effective population size (Ne) is observed from approximately 240 years ago to pres

167 thods to estimate effective population size (Ne) is rapidly increasing, but all approaches make simpl

168 Effective population size (Ne) of a natural fish population was estimated from temp

169 Low effective population size (Ne) of paternal genes due to polygyny and female-biased

170 ent and long-term effective population size (Ne) were determined for two solanaceous species by exami

171 by its long-term effective population size (Ne).

172 ng changes in the effective population size (Ne).

173 Refinement with ensemble sizes (Ne) of >or=2 to represent the atomic motions reconciles

174 hence very small effective population sizes (Ne ) in all populations.

175 ed to historical effective population sizes (Ne), and can provide insights into the genetic diversity

176 d for estimating effective population sizes, Ne, and selection coefficients, s, from time-series data

177 tions of state of Au, Pt, NaCl-B2, and solid Ne.

178 f targets (GaSb, GaAs, GaP) and ion species (Ne, Ar, Kr, Xe) to determine new parametric trends regar

179 ore accurately reflect local (subpopulation) Ne unless m> approximately 5-10%.

180 ive population size of these subpopulations (Ne = 205) and the average generation time of this specie

181 onflict with expectations based on long-term Ne alone.

182 here is a single difference in the long-term Ne, or overall strength of selection, between the two sp

183 imited to encapsulating species smaller than Ne and Na(+).

184 Furthermore, our analyses show that Ne for the focal chough population is critically small,

185 ependent change in posterror slowing and the Ne/ERN amplitude, questioning a direct link between the

186 ccurs via a specific interaction between the Ne of the His imidazole, forming a 1:1 stoichiometric co

187 If the Ne/O abundance in these stars is adopted for the Sun, th

188 ects, we found an amplitude reduction in the Ne/ERN, contradicting the existence of a direct relation

189 ror slowing and whether the amplitude of the Ne/ERN predicts posterror slowing in the current task se

190 day 4 of colonization was comparable to the Ne during day 4 to day 8.

191 key demographic mechanisms that underlie the Ne to census population size (N) ratio, remains challeng

192 Performance of these Ne estimates could be improved by incorporating data fro

193 e effective populations size (from Ne=500 to Ne=75).

194 ficant correlations between the single-trial Ne/ERN amplitude and error-related reaction times.

195 The single-trial Ne/ERN distribution showed a reduced variance for middle

196 We calculated true Ne and Nb, using the model species' vital rates, and ver

197 In high-pressure DAC experiments using Ne as pressure-transmitting medium, formation of nanocry

198 n even large populations (e.g., SD=0.5% when Ne=10,000) and is likely to be the most powerful method

199 number of heterozygous sites is 4Neu, where Ne denotes the migration effective population number and

200 -14, -15} in the range 0.1-0.25 M Na+ yields Ne = 9.0 +/- 0.8 residues at each end, demonstrating tha