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 Ne-FEO was characterized through scanning electron micro

5 Ne-lysine acetylation in the ER is an essential componen

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

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

8 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

9 Furthermore, we determine a (20)Ne/(22)Ne ratio for the primordial plume mantle of 13.23

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

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

12 with an extraterrestrial (3)He/(4)He and (20)Ne/(22)Ne ratios, along with some contaminant terrestria

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

14 Modeling predicts that the atmospheric (20)Ne/(22)Ne ratio is sensitive to solar-Ne mantle degassin

15 sions and show that a modern atmospheric (20)Ne/(22)Ne ratio was almost reached 2.7 Ga ago, implying

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

17 Our observations also indicate distinct (20)Ne/(22)Ne ratios between deep mantle plumes and mid-ocea

18 mental measurement of the (19)F(p, gamma)(20)Ne breakout reaction down to a very low energy point of

19 elvin, this thermonuclear (19)F(p, gamma)(20)Ne rate is up to a factor of 7.4 larger than the previou

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

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

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

23 tio of the two primordial neon isotopes, (20)Ne/(22)Ne, is significantly different for the three pote

24 es were detected by MS in the absence of (20)Ne and (21)Ne.

25 ents from deep mantle plumes that reveal (20)Ne/(22)Ne ratios of up to 13.03 +/- 0.04 (2 standard dev

26 Therefore, the (20)Ne/(22)Ne ratio is a powerful tool for assessing the sou

27 cosmic ray spallation products (3)He and (21)Ne enabled us to estimate that the irradiated objects in

28 ected by MS in the absence of (20)Ne and (21)Ne.

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

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

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

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

33 locity-dependent forces, by using a K-Rb-(21)Ne co-magnetometer and a tungsten ring featuring a high

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

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

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

37 For (22)Ne identification, three methods are employed.

38 tion coefficient would result in a (3)He/(22)Ne ratio of ~10(3) in the core, far higher than observed

39 All the results confirm that isotope (22)Ne and regular CO(2) really exist in the output gas from

40 Furthermore, we determine a (20)Ne/(22)Ne ratio for the primordial plume mantle of 13.23 +/- 0.

41 Therefore, the (20)Ne/(22)Ne ratio is a powerful tool for assessing the source of

42 ing predicts that the atmospheric (20)Ne/(22)Ne ratio is sensitive to solar-Ne mantle degassing over

43 nd show that a modern atmospheric (20)Ne/(22)Ne ratio was almost reached 2.7 Ga ago, implying intense

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

45 servations also indicate distinct (20)Ne/(22)Ne ratios between deep mantle plumes and mid-ocean-ridge

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

47 om deep mantle plumes that reveal (20)Ne/(22)Ne ratios of up to 13.03 +/- 0.04 (2 standard deviations

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

49 extraterrestrial (3)He/(4)He and (20)Ne/(22)Ne ratios, along with some contaminant terrestrial atmos

50 the two primordial neon isotopes, (20)Ne/(22)Ne, is significantly different for the three potential s

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

52 njecture a possible mechanism to produce (22)Ne and CO(2) and find out that (12)C and isotope (17)O a

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

54 By activating myosin II along Ne/Epi junctions ahead of the zipper and inhibiting myos

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

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

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

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

59 hile, Fe oxides do not react with Kr, Ar and Ne.

60 itioning data showing that sufficient He and Ne could have been incorporated into the core to source

61 We show that the He and Ne isotopic and elemental signatures of the Yellowstone

62 For He and Ne our calculated solubilities point to atoms occupying

63 % for Kr, 8% for Xe, and 3% for CH4, N2O and Ne.

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

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

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

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

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

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

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

71 ymous to synonymous substitutions (dN/dS) as Ne(e) proxy for 807 species including vertebrates, mollu

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

73 results show a negative correlation between Ne proxies and the genome-wide AS rates among species, c

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

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

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

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

78 emulsion film incorporating carvone (carvone-Ne) for protection of bread slices against A. flavus and

79 in-situ preservation potentiality of Carvone-Ne in bread slices with improved gas compositions, and a

80 The carvone-Ne displayed better inhibition of A. flavus (0.5 uL/mL)

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

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

83 nd transport of positron beamlets containing Ne+ >= 105 positrons in a 5% bandwidth around 600 MeV, w

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

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

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

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

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

89 Our ages, based on cosmogenic Ne-21, range from 3.9 +/- 1.6 Ma to ~3 +/- 2 Ga before t

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

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

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

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

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

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

96 in neural cells along the neural/epidermal (Ne/Epi) boundary, where RhoA and myosin are activated du

97 crystal structures of Nanoarchaeum equitans (Ne) C3PO.

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

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

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

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

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

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

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

105 and genetically depauperate (e.g., estimated Ne range = 3-9).

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

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

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

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

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

111 These data show extended [Ne VI] emission that is cospatial with the cooling peak

112 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

113 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

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

115 In contrast, the partition coefficient for Ne is three orders of magnitude lower than He.

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

117 ory traits and dN/dS as reliable proxies for Ne(e).

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

119 and inhibiting myosin II along newly formed Ne/Ne junctions behind the zipper, Cadherin2 promotes ti

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

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

122 to protein glycation (formation of furosine, Ne-(carboxymethyl)-l-lysine, Ne-(carboxyethyl)-l-lysine,

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

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

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

126 ply subducted or metasomatic components have Ne isotopes less nucleogenic than the upper mantle, henc

127 orifice can be filled with gases (H(2) , He, Ne) in the solid state, and the cage opening then contra

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

129 ched, inert 'tag' particle (for example, He, Ne, N(2))(1-3).

130 about the effect of the GC carrier gas (He, Ne, and N(2)) on the sensitivity of the analysis in the

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

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

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

134 e of the gas driving the supersonic jet (He, Ne, and N(2)) in the GC-MRR.

135 This study shows that mantle He, Ne, and Xe isotopes require that the plume mantle had lo

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

137 itio calculations on the partitioning of He, Ne, Ar, Kr and Xe between liquid iron and silicate melt

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

139 -Zehnder interferometer (MZI) employing a He-Ne laser, a mini-flow cell with two embedded channels pl

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

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

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

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

144 Thereby, the He-Ne correction, which is typically required for FTIS, can

145 To address this question, we report the He-Ne-Ar isotopic compositions of magmatic fluids trapped i

146 volatile-rich solids thus survives in the He-Ne-Xe signatures of mantle rocks today.

147 ivities were determined in laser-treated (He-Ne laser, 632 nm, 5 mW) common buckwheat (CBW) and tarta

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

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

150 edirects RhoA/myosin activity to heterotypic Ne/Epi junctions.

151 sposable elements (TEs), and those with high Ne(e) to maintain streamlined genomes as a consequence o

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

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

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

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

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

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

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

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

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

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

162 During in-situ investigation, Ne-FEO coating maintained nutritional qualities along wi

163 Here we ionized Ne atoms with few-femtosecond pulses of selected time du

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

165 ), 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

166 The large Ne of herring combined with the common occurrence of opp

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

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

169 ng mixture LD and depress estimates of local Ne.

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

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

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

173 zard Hypothesis postulates lineages with low Ne(e) to have bigger genome sizes due to the accumulatio

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

175 on of furosine, Ne-(carboxymethyl)-l-lysine, Ne-(carboxyethyl)-l-lysine, and protein-bound carbonyls)

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

177 Xe flux but has a small impact on the mantle Ne budget.

178 Ne converges on the global (metapopulation) Ne.

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

180 re essential oil into chitosan nanoemulsion (Ne-FEO) and efficacy evaluation as edible coating agains

181 in essential oil into chitosan nanoemulsion (Ne-PCEO) and its application as coating agent for anti-s

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

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

184 100 ms after the so-called error negativity (Ne), from which it was therefore distinguished.

185 rror negativity or error-related negativity (Ne/ERN), a correlate of errors in choice tasks, is relat

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

187 turn(1,3), and the depletion of He and neon (Ne) in Jupiter's atmosphere as observed by the Galileo p

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

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

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

191 ide, predicted to be dominated by He, C/O, O/Ne/Mg and O/Si/S (refs. (4,5)).

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

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

194 The speculated antifungal mode of action of Ne-TML was related to the decrease in ergosterol content

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

196 jujube fruits strengthens the application of Ne-FEO nanoemulsion as smart shelf-life enhancer in frui

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

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

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

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

201 The demographic estimate of Ne was 30, suggesting that rates of increase of inbreedi

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

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

204 on which could bias demographic estimates of Ne .

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

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

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

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

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

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

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

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

213 (2) = 0.98) function of the harmonic mean of Ne and Nb.

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

215 The antifungal mechanism of Ne-FEO was associated with ergosterol destruction, ions

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

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

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

219 53 metazoan species spanning a wide range of Ne values.

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

221 e method also enables the first synthesis of Ne@C(60) by molecular surgery, and its characterization

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

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

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

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

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

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

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

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

230 erse mechanisms, including posttranslational Ne-lysine acetylation.

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

232 opulation restriction despite a large recent Ne.

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

234 The regassed Ne flux exceeds the regassed Xe flux but has a small imp

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

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

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

238 As the effective population size (Ne(e)) reflects the intensity of genetic drift, it is ex

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

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

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

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

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

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

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

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

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

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

249 eatly reduces the effective population size (Ne) of cellular populations, increasing the role of gene

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

251 or the inverse of effective population size (Ne) we also show that the relative A + T content of cent

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

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

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

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

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

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

258 nd to have small effective population sizes (Ne), they are expected to be more affected by genetic dr

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

260 ic (20)Ne/(22)Ne ratio is sensitive to solar-Ne mantle degassing over geological time.

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

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

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

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

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

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

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

268 In-situ results revealed that Ne-TML exhibited maximum protection from fungal (75.40%)

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

270 and crustal components, which suggests that Ne isotopes are more robust tracers of deep-mantle contr

271 The Ne-PCEO coating also prevented the weight loss, starch d

272 The Ne-PCEO coating inhibited in-vivo potato sprouting and r

273 The Ne-PCEO was characterized through SEM, DLS, FTIR, and XR

274 The Ne-TML cause complete inhibition of growth and AFB(1) pr

275 The Ne-TML was assessed for its antifungal and anti-aflatoxi

276 The Ne/ERN in turn predicted alpha asymmetry on the next tri

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

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

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

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

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

282 d tested whether it predicts the size of the Ne/ERN.

283 distractor on error trials and predicted the Ne/ERN on a single-trial level.

284 that the error monitoring system scales the Ne/ERN according to the strength of error precursors to

285 potential error sources and then scaling the Ne/ERN according to the strength of the error precursor

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

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

288 g the James Webb Space Telescope to map the [Ne VI] lambda 7.652-mum emission line, enabling us to pr

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

290 oencapsulation of developed formulation TML (Ne-TML) was prepared and characterised by SEM, XRD and F

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

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

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

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

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

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

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

298 ome the most electropositive elements, while Ne, He, and F remain the most electronegative ones.

299 A + T content of centromeric DNA scales with Ne across 43 animal, fungal and yeast (Opisthokonta) spe

300 -14, -15} in the range 0.1-0.25 M Na+ yields Ne = 9.0 +/- 0.8 residues at each end, demonstrating tha