ライフサイエンスコーパス: Venus

1 erior and the other exterior to the orbit of Venus.

2 e movement of the Moon, and perhaps Mars and Venus.

3 mation of sulfuric acid in the atmosphere of Venus.

4 nomeric Teal Fluorescent Protein (mTFP)1 and venus.

5 evidence for lightning in the atmosphere of Venus.

6 ning), no similar signals were detected from Venus.

7 s using an in vivo clock reporter, her1:her1-venus.

8 ly identified exclusively on Earth, Mars and Venus.

9 the existence of a dust ring at the orbit of Venus.

10 ently recalculated HZ boundaries are: recent Venus--1.78; runaway greenhouse--1.04; moist greenhouse-

11 3 amino acids of the SsrA degradation tag to Venus, a rapidly folding yellow fluorescent protein, we

12 We show that Jas9-VENUS abundance is dependent on bioactive JA isoforms, t

13 lular trafficking of ASTN1-Venus, with ASTN1-Venus accumulating in the forward aspect of the leading

14 hotter surface conditions, such as those on Venus, accumulation and inheritance of damage is negligi

15 erosols are ubiquitous in the atmospheres of Venus, ancient Earth, and Mars.

16 er drives the monocistronic transcription of Venus and a puromycin-resistant gene via the foot-and-mo

17 with Mars is in many ways similar to that at Venus and at an active comet, that is, primarily an iono

18 Venus and Citrine are two such variants that have been d

19 The effective halide affinity for Venus and Citrine is much reduced compared with that of

20 A super-stable core is identified for Venus and compared with that previously reported for gre

21 nce resonance energy transfer between Ggamma-Venus and giantin-Rluc8.

22 tion of spectral ratiometric imaging of ECFP/Venus and high-speed FLIM-FRET of TagRFP/mPlum can thus

23 t across the root tip as quantified with DII-VENUS and is synergistically enhanced by hypoxia and the

24 n the visible spectrum is similar for Earth, Venus and Titan, but quite different for Jupiter.

25 N-terminal fragment containing residues from Venus and yellow fluorescent protein produced either con

26 here variants of yellow fluorescent protein (Venus) and cyan fluorescent protein (Cerulean) flank eit

27 nd induce early expression of endoderm (Hhex-Venus) and neural (Sox1-GFP) reporter genes.

28 e impact cratering record of the Moon, Mars, Venus, and Mercury and from the size distributions of as

29 rs, the volcanic floodplains of the Moon and Venus, and other planetary bodies.

30 ces in the epic: to Bootes and the Pleiades, Venus, and the New Moon; we supplement them with a conje

31 ation is greater for Venus-FMRP RNA than for Venus-ARC RNA and is increased in Fmr1-knockout neurons

32 reases bursty translation for Venus-FMRP and Venus-ARC RNAs.

33 transfer (BRET) between JNK3-luciferase and Venus-arrestins.

34 fused combinations of Cerulean as donor (D), Venus as acceptor (A), and a photo-insensitive molecule

35 ign of highly optimized FRET probes that use Venus as an acceptor probe.

36 he core of smaller planets such as Earth and Venus as well as exoplanets: as planets cool off, the su

37 We tested model predictions using the DII-VENUS auxin sensor in conjunction with state-of-the-art

38 In addition, illumination of Mrgprd-ChR2-Venus(+) axon terminals in spinal cord slices evoked EPS

39 Here, we provide a protocol for a Venus-based BiFC assay to visualize protein interactions

40 d acceptor, respectively, we have combined a Venus-based BiFC system with Cerulean to develop a BiFC-

41 z) radio signals during two close fly-bys of Venus by the Cassini spacecraft.

42 dermal growth factor stimulation and an ECFP/Venus Cameleon FRET sensor for monitoring calcium transi

43 osis, pathogenesis, and treatment of central venus catheter-related thromboses are critical in the tr

44 Results show that the introduction of Venus/Cerulean itself did not alter the ability of VWF-A

45 ght-activated ion channel Channelrhodopsin-2-Venus (ChR2-Venus) to the Mrgprd locus.

46 signals generated by lightning discharges in Venus' clouds.

47 om mice expressing one or two copies of ChR2-Venus could be activated in vitro as evidenced by light-

48 Regional expression of Venus-dysferlin chimeras in A/J fibres restored the full

49 reduces Ca(2+) leak) or local expression of Venus-dysferlin prevented OSI-induced Ca(2+) waves.

50 the possibility of liquid water existing on Venus early in its history, and extends the size of the

51 2), an important planetary material found in Venus, Earth, and Mars, is vital to the study of the evo

52 sensor with a circularly permuted version of Venus enhanced sensor dynamic range nearly 2.5-fold.

53 that RGS14-Luciferase and active H-Ras(G/V)-Venus exhibit a robust BRET signal at the plasma membran

54 Toward the end of the Venus Express mission, an aerobraking campaign took the

55 Spectrometer on the European Space Agency's Venus Express spacecraft to identify compositional diffe

56 al replication and virulence in mice of this Venus-expressing influenza virus are primarily conferred

57 n enriched environment led to enhancement of Venus expression in dendritic segments of somatosensory

58 uronal activity using the coding sequence of Venus, flanked by short stretches of the 5'- and 3'-untr

59 nts of diffusion and molecular brightness of Venus fluorescent protein (FP) can be performed in solut

60 e found that an influenza virus encoding the Venus fluorescent protein acquired two mutations in its

61 rons with the mutant alleles tagged with the Venus fluorescent protein also revealed excess PM locali

62 ructed MYXV and VACV virions tagged with the Venus fluorescent protein and compared their characteris

63 d translation output from each granule using Venus fluorescent protein as a reporter.

64 yze ERAD based on mutants of split or intact Venus fluorescent protein for which fluorescence depends

65 The N-terminal fragment of the Venus fluorescent protein fused to FKBP produced constit

66 Because the renaturation of the Venus fluorescent protein results in a covalent bonding

67 N1) reporter virus that stably expresses the Venus fluorescent protein to identify antigen-bearing ce

68 rescuing transgene, VNS::SYS-1, which fuses VENUS fluorescent protein to SYS-1, we find more VNS::SY

69 ting sequences or the entire Ras proteins to Venus fluorescent protein.

70 on enables macrophages to serve as cellular "Venus fly traps", with the capacity to capture phagocyti

71 cable to other binding proteins that have a "venus-fly-trap" mechanism.

72 The Venus flytrap (Dionaea muscipula Ellis) is a marvel of p

73 endopeptidases in the digestive fluid of the Venus flytrap (Dionaea muscipula) are cysteine proteases

74 The Venus flytrap (Dionaea muscipula) possesses an active tr

75 nsor kinase BvgS is composed of four bilobed Venus flytrap (VFT) perception domains followed by alpha

76 ectrical properties of the upper leaf of the Venus flytrap and proposed the equivalent electrical cir

77 The Venus flytrap can accumulate small subthreshold charges

78 The Venus flytrap can accumulate small subthreshold charges,

79 The Venus flytrap digests and absorbs its prey, but how does

80 The Venus flytrap Dionaea muscipula captures insects and con

81 d receptor that has an extracellular bilobed venus flytrap domain (VFTD) predicted to contain five ca

82 ative ligand binding model that involved the Venus flytrap domain of T1R1 in which l-glutamate binds

83 operative ligand-binding model involving the Venus flytrap domain of T1R1, where L-glutamate binds cl

84 G protein-coupled receptors, the N-terminal Venus flytrap domain of T1R2 is required for recognizing

85 e hinge region and induce the closure of the Venus flytrap domain of T1R2, the enhancers bind close t

86 ng pocket localized in mGlu7's extracellular Venus flytrap domain, a region generally known for ortho

87 ctive interaction between XAP044 and mGlu7's Venus flytrap domain, whose three-dimensional structure

88 gth TAS1R2/TAS1R3 heterodimer, including the Venus Flytrap Domains (VFDs) [in the closed-open (co) ac

89 The Venus flytrap effectively detects, traps, digests and ab

90 When the Venus flytrap is processing its prey, the gland cell mem

91 ation, providing compelling evidence for the Venus flytrap mechanism of glutamate receptor domain clo

92 We propose a Venus flytrap model that merges the concepts of ParA pol

93 teracts with both T1R2 and T1R3 and that the Venus flytrap module of T1R2 is important for brazzein a

94 which are distinguished by an extracellular Venus flytrap module.

95 The rapid closure of the Venus flytrap upper leaf in about 0.1 s is one of the fa

96 mulus between a midrib and a lobe closes the Venus flytrap upper leaf without mechanical stimulation

97 ike type I and II PBPs, which undergo large "Venus flytrap" conformational changes upon ligand bindin

98 embers of the MBP cluster, differs from the "Venus flytrap" mechanism utilized by bacterial nonmetal

99 In a "venus flytrap" model of the receptor extracellular domai

100 ial aromatic rings which act as a molecular "Venus flytrap".

101 Although some species, such as Venus flytrap, have fast touch responses, most plants di

102 loses its holes in a manner reminiscent of a Venus flytrap, which prevents the Cs(+) ions from leachi

103 ated between two lobes and which acts like a Venus flytrap.

104 to the existence of electrical memory in the Venus flytrap.

105 rs expression of a K(+) uptake system in the Venus flytrap.

106 cated mGlu4 receptors lacking the N-terminal Venus-flytrap domain, as opposed to the mGlu4 receptor e

107 r of magnitude faster than the snap traps of Venus flytraps and catapulting tentacles of the sundew D

108 he ingenious snapping mechanism of predatory Venus flytraps that rely on concave-to-convex reconfigur

109 slation and decreases bursty translation for Venus-FMRP and Venus-ARC RNAs.

110 ability of bursty translation is greater for Venus-FMRP RNA than for Venus-ARC RNA and is increased i

111 rescent fusion of native PER2 protein (PER2::VENUS) for live imaging.

112 luding Cerulean, Dendra2, DRONPA, TagRFP and Venus, for the expression of protein fusions in plant ce

113 As an example application, Teal-Venus force sensitive biosensors integrated into E-cadhe

114 Moreover, the mTFP1-venus FRET pair can be duplexed with another FRET pair,

115 ixtures as a zero FRET control, and Cerulean-Venus FRET standards as positive FRET controls.

116 We engineered novel luciferase- and Venus-fused Galpha constructs that can be used in biolum

117 The efficiency of FRET in a zero-length LUMP-Venus fusion is 62% compared to approximately 31% in a r

118 rons express a dendritically-targeted PSD-95:Venus fusion protein under the control of a c-fos promot

119 mpared to approximately 31% in a related CFP-Venus fusion.

120 We found that reassortants with PB2 from MA-Venus-H5N1 (MA-PB2), MA-PA, or MA-NS expressed Venus mor

121 ing WT-Venus-H5N1 virus with a mouse-adapted Venus-H5N1 (MA-Venus-H5N1) virus.

122 mouse adaptation compared with the wild-type Venus-H5N1 (WT-Venus-H5N1) virus.

123 PA (R443K) increased the virulence of the WT-Venus-H5N1 virus in mice and that the presence of both o

124 lence and reporter stability by comparing WT-Venus-H5N1 virus with a mouse-adapted Venus-H5N1 (MA-Ven

125 t from the A/Puerto Rico/8/1934(H1N1) virus (Venus-H5N1 virus), became more lethal to mice, and the r

126 A-NS expressed Venus more stably than did WT-Venus-H5N1 virus.

127 n compared with the wild-type Venus-H5N1 (WT-Venus-H5N1) virus.

128 N1 virus with a mouse-adapted Venus-H5N1 (MA-Venus-H5N1) virus.

129 The existence of lightning at Venus has, however, remained controversial.

130 from the Magellan spacecraft in orbit around Venus, has established that the surface materials viewed

131 viewed at low and intermediate altitudes on Venus have a relative dielectric permittivity of 4.0 &pl

132 Up to 58% Venus(+) HSPCs with 6-16% human cell marking were observ

133 molecule, the head-to-tail interaction of NC-Venus-ICP27 locks ICP27 in a closed configuration.

134 The expression of NC-Venus-ICP27 protein was delayed compared to ICP27 expres

135 ression in wild-type HSV-1 infection, but NC-Venus-ICP27 was abundantly expressed at late times of in

136 A recombinant virus, vNC-Venus-ICP27, was constructed, and this virus was severel

137 eveloping quantitative reporters such as DII-VENUS in conjunction with parameterized mathematical mod

138 tio of the fluorescent proteins Cerulean and Venus in mammalian cells expressing a series of fusion p

139 tor, Tsr, labeled by the fluorescent protein Venus in the inner membrane of live Escherichia coli cel

140 tailed study of the stability and folding of Venus in the pH range from 6.0 to 8.0 using chemical den

141 d an Aux/IAA-based reporter, domain II (DII)-VENUS, in conjunction with a mathematical model to quant

142 Existing data for Venus indicate values of 3.6 +/- 0.6 kelvin.

143 s that the source is not associated with the Venus ionosphere.

144 Here we report observations of Venus' ionosphere that reveal strong, circularly polariz

145 Venus is a yellow fluorescent protein that has been deve

146 about 250,000 years or less, indicating that Venus is actively resurfacing.

147 The questions of whether Venus is geologically active and how the planet has resu

148 n found in space exploration missions (i.e., Venus &Jupiter planetary exploration, and heliophysics m

149 ere, but is also found in the atmospheres of Venus, Jupiter and Saturn.

150 y after photobleaching in slices from VGLUT1(Venus) knock-in mice reveal 75% of VGLUT1-containing ves

151 using wild-type, VGLUT1-3 knock-out, VGLUT1(Venus) knock-in, and VGLUT2-EGFP transgenic mice.

152 Fluorescence of an optimized reporter (Venus) lagged luminescence by 15-20 min, which is consis

153 om a cloud-free water-vapour atmosphere to a Venus-like one.

154 We found that VIP1-Venus localized in both the cytoplasm and the nucleus of

155 and new geophysical data from other planets (Venus, Mars, or Mercury) and asteroids.

156 Tectonics, volcanism, and climate on Venus may be strongly coupled.

157 a covalent bonding of the two halves of the Venus molecule, the head-to-tail interaction of NC-Venus

158 nus-H5N1 (MA-PB2), MA-PA, or MA-NS expressed Venus more stably than did WT-Venus-H5N1 virus.

159 vector BiFC system which utilizes monomeric Venus (mVenus) split at residue 210, and contains an int

160 Images of the Venus night side show similar bright and dark markings i

161 radation of the N-end rule substrate, LR-GFP(Venus), occurs with a single ClpS bound per ClpA(6); one

162 -insensitive yellow fluorescent protein [NPY-Venus] or NPY-monomeric red fluorescent protein), while

163 mTagBFP, cyan mCerulean, green CrGFP, yellow Venus, orange tdTomato and red mCherry) in the popular m

164 with spectral ratiometric imaging of an ECFP/Venus pair we were thus able to maximize the spectral se

165 tually codependent as balboa-RNAi eliminates Venus::PPK from the sensory dendrites of nociceptors.

166 Herein, local synthesis of a Venus-PSD-95 fusion protein was directly visualized in d

167 (S)-3,5-dihydroxyphenylglycine, the rate of Venus-PSD-95 mRNA translation increased rapidly in dendr

168 The basal translation rates of Venus-PSD-95 mRNA was increased in cultured hippocampal

169 e-molecule imaging of a diffusion-restricted Venus-PSD-95 reporter under control of the PSD-95 3'UTR.

170 Based on DII-VENUS quantification and direct measurement of cellular

171 ned RET efficiencies and with known Cerulean/Venus ratios were constructed and used to test sRET.

172 PER2::VENUS recapitulates the circadian functions of wild-type

173 iled to completely immobilize coexpressed D2-venus receptors (D2R-Vs), suggesting that the two did no

174 , we reported that an H5N1 virus bearing the Venus reporter gene became more pathogenic to mice and t

175 sly reported that an H5N1 virus carrying the Venus reporter gene, which was inserted into the NS gene

176 The her1:her1-venus reporter has single-cell resolution, allowing us t

177 A rescuing gon-14::GON-14::VENUS reporter is broadly expressed during development a

178 Using newly generated RANK Venus reporter mice, we identify distinct RANK(+) subset

179 PER2 and, importantly, the behavior of PER2::VENUS runs counter to the Drosophila model: it does not

180 lieved to form a domain resembling a bilobed Venus's flytrap (VFT).

181 e human Ca(2+) receptor (hCaR) consists of a Venus's-flytrap (VFT) domain and a cysteine-rich (Cys-ri

182 r (hCaR) has been speculated to consist of a Venus's-flytrap domain (VFT) and a cysteine-rich domain.

183 associated virus encoding channelrhodopsin-2-Venus showed similar fiber labeling and association with

184 occasionally detect small aggregates of the Venus signal in nuclei, but these were likely to be imag

185 evidence has been reported for lightning on Venus, some searches have been negative and the existenc

186 e basis for this difference in virulence and Venus stability was unclear.

187 of a FRET-optimized genetically encoded LUMP-Venus substrate for thrombin.

188 shares properties with the polar vortices on Venus, such as polar location, cyclonic circulation, war

189 with thrombotic disorders of arterial and/or venus systems, spontaneous abortion(s) or thrombocytopen

190 Live imaging of Venus-tagged ASTN1 in migrating cerebellar granule cells

191 his pattern was recreated upon expression of VENUS-tagged barley (Hordeum vulgare) CSLF6 and CSLH1 in

192 was used to characterize assembly mutants of Venus-tagged CaMKIIalpha to identify a dimeric CaMKII.

193 fluorescence anisotropy and FRET imaging of Venus-tagged CaMKIIalpha to test the hypothesis that neu

194 t stoichiometry or the net homo-FRET between Venus-tagged catalytic domains.

195 by inserting a 7-kb fragment consisting of a venus-tagged lac repressor gene along with a target lacZ

196 olysis was required, as was visualized using Venus-tagged lysenin probe, which specifically binds SM.

197 red for the normal polarized localization of Venus-tagged neuropeptides to axons of cholinergic motor

198 Using Cerulean and Venus-tagged proinsulins, we find that both WT-WT and WT

199 llular localization of Venus-tagged VirE2 or Venus-tagged VIP1, in the presence or absence of the oth

200 y to examine the subcellular localization of Venus-tagged VirE2 or Venus-tagged VIP1, in the presence

201 also been used to study interplanetary dust, Venus' tail and the interstellar medium.) Here we report

202 ared images and spectra of the night side of Venus taken at the Anglo-Australian Telescope during Feb

203 Five FPs: Cerulean, EGFP, Venus, tdTomato, and mCherry were concurrently used to c

204 scribe a JA perception biosensor termed Jas9-VENUS that allows the quantification of dynamic changes

205 rescent fragments of the fluorescent protein Venus that can associate to reform the fluorescent compl

206 pothalamic neurons were transfected with NPY-Venus, the distribution of the fluorescent puncta replic

207 stics of deformation in the ridged plains of Venus, the most widely preserved volcanic terrain on the

208 ss and dynamical parameters of the Earth and Venus, they fall short of explaining the small size of M

209 We demonstrate the utility of Jas9-VENUS to analyse responses to JA in planta at a cellular

210 This included using Jas9-VENUS to determine the cotyledon-to-root JA signal veloc

211 developing quantitative sensors such as Jas9-VENUS to provide high-resolution spatiotemporal data abo

212 d ion channel Channelrhodopsin-2-Venus (ChR2-Venus) to the Mrgprd locus.

213 The study introduces PPG-promoter-Venus transgenic mice as a viable and important tool to

214 el and the fluorescent proteins Cerulean and Venus, two mutant proteins of CFP and YFP with better fo

215 Transgenic mice expressing Venus under control of the PPG promoter were used to ide

216 mice expressing yellow fluorescent protein (Venus) under the control of the PPG promoter were used t

217 Under mildly acidic conditions, we show that Venus undergoes a drastic decrease in yellow fluorescenc

218 hydrogen-deuterium exchange of (15)N-labeled Venus using NMR spectroscopy over 13 months, residue-spe

219 ovincialis, Ostrea edulis, Chlamis varia and Venus verrucosa) were collected during the autumn 2011 a

220 ion, warm center, and long lifetime, but the Venus vortices have cold collars and are not associated

221 In these knock-in mice, ChR2-Venus was localized to nonpeptidergic Mrgprd(+) neurons

222 While essentially complete release of NPY-Venus was observed in 24 +/- 1% of glucose-stimulated ex

223 Using fluorescent imaging of PER2::VENUS, we acquired the first measures of mobility, molec

224 RNA sequences and an unrelated control gene, Venus, we have identified many toxic sequences - most of

225 omatographs have been flown to both Mars and Venus where detailed compositional measurements were mad

226 r AGS4-RLuc and alpha(2)-adrenergic receptor-Venus, which were Galpha(i)-dependent and reduced by ago

227 Venus, while Earth's twin in many ways, lacks such a str

228 oxygen has been observed on the nightside of Venus with HIRES, the echelle spectrograph on the W. M.

229 veals the intracellular trafficking of ASTN1-Venus, with ASTN1-Venus accumulating in the forward aspe

230 ductance in the stem of the channel, we used Venus yellow fluorescent protein as a molecular stopper