ライフサイエンスコーパス: Venus

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

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

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

4 mation of sulfuric acid in the atmosphere of Venus.

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

6 evidence for lightning in the atmosphere of Venus.

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

8 l data void in current atmospheric models of Venus.

9 ved in Earth's magnetotail and near Mars and Venus.

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

11 ly identified exclusively on Earth, Mars and Venus.

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

13 n layers of a specific N95 respirator model (Venus-4400) after treatment with one and five cycles of

14 Despite Venus' 700 K surface temperature being too hot for any p

15 3 amino acids of the SsrA degradation tag to Venus, a rapidly folding yellow fluorescent protein, we

16 upon gravistimulation as visualized with DII-VENUS, a sensor for auxin signaling and proxy for relati

17 evealed Davydov splitting when the yellow FP Venus(A206) dimerizes, and a novel approach combining ph

18 We conclude that excitonic coupling between Venus(A206) fluorophores is possible at physiological te

19 ed to confirm that the two fluorophores in a Venus(A206) homodimer behave as a single-photon emitter.

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

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

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

23 The analysis of quantitative DII-Venus, an auxin signaling reporter, indicates that low b

24 A Venus-analogue atmosphere with sulfuric acid clouds is a

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

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

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

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

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

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

31 mate models for a cool, wet climate on early Venus and could be an attractive research theme for futu

32 for interpreting the distinct properties of Venus and Earth (for example, tectonism, atmospheric com

33 the divergence between the sibling planets, Venus and Earth.

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

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

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

37 binant (r)SARS-CoV-2 expressing fluorescent (Venus and mCherry) or luciferase (Nluc) reporter genes a

38 ll fluorophores FITC and Rhodamine B or with Venus and mCherry, they bound mostly nonoverlapping sets

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

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

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

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

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

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

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

46 We utilize fluorescent reporter mice (Otr(venus/+)) and find that cortical regions show temporally

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

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

49 Coronae on Venus are key to understanding the planet's geodynamics.

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

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

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

53 Here, we explore Venus as an example of a planet that recently transition

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

55 e tested the model predictions using the DII-VENUS auxin response reporter, comparing the predicted a

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

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

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

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

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

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

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

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

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

65 quence of the presence of NH(3) is that some Venus cloud droplets must be semisolid ammonium salt slu

66 solvent and most organic covalent chemistry, Venus' cloud-filled atmosphere layers at 48 to 60 km abo

67 signals generated by lightning discharges in Venus' clouds.

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

69 t trigger rapid DR5-reporter activation, DII-Venus degradation or Ca(2+) signalling.

70 er, comparing the predicted and observed DII-VENUS distributions using genetic and chemical perturbat

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

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

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

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

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

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

77 ity in the Venusian atmosphere obtained from Venus Express and Akatsuki radio occultation profiles pe

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

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

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

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

82 Layer 5, whereas CGE-derived Lhx6-Cre::Dlx1-Venus(fl) cells are least abundant in that layer.

83 rs at P8) whereas CGE-derived Lhx6-Cre::Dlx1-Venus(fl) cells are the sparsest (2% of NEUN+ cells acro

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

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

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

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

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

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

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

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

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

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

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

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

96 uch as in the prey-trapping mechanism of the Venus fly trap (Dionaea muscipula).

97 Most known sugars and sweeteners bind to the Venus Fly Trap domain of T1R2 subunit of the sweet taste

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

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

100 gnetic field data acquired during the fourth Venus flyby of the Parker Solar Probe (PSP) mission and

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

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

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

104 Certainly, in land plants, such as the Venus flytrap (Dionaea muscipula) where fast electrical

105 ns of GABA(B)R identified amino acids of the Venus flytrap (VFT) domains with which the alpha-conotox

106 subunit is characterized by an extracellular Venus flytrap (VFT) module, a descending peptide linker,

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

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

109 l principles for fast snapping in the iconic Venus flytrap are not yet fully understood.

110 The Venus flytrap can accumulate small subthreshold charges

111 The Venus flytrap can accumulate small subthreshold charges,

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

113 The Venus flytrap Dionaea muscipula captures insects and con

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

115 agonist binding leads to the closure of the Venus flytrap domain of GB1, triggering a series of tran

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

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

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

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

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

121 Each subunit possesses an extracellular Venus flytrap domain, which is connected to a canonical

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

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

124 ers and possess extracellular ligand-binding Venus flytrap domains, which are linked by cysteine-rich

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

126 x structures presented here exhibit a closed Venus flytrap fold, with the enzyme exploiting the chara

127 nals by measuring the action potentials of a Venus flytrap is demonstrated.

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

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

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

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

132 which are distinguished by an extracellular Venus flytrap module.

133 echanosensitive (MS) ion channel involved in Venus flytrap prey recognition.

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

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

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

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

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

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

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

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

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

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

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

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

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

147 Our results show that agonist binding at the Venus flytraps leads to a compaction of the intersubunit

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

149 ansmission of signals from the extracellular Venus flytraps to the G protein-coupling domains-the 7-t

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

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

152 ibility of Earth-like climatic conditions on Venus for much of its earlier history, prior to catastro

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

171 Venus has a thick atmosphere that rotates 60 times as fa

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

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

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

175 nd atmospheres similar to those of Earth and Venus-high-molecular-weight (secondary) atmospheres-on r

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

177 uced auxin response, increased levels of DII:VENUS, IAA18:GUS, and HS::AXR3-NT:GUS were also observed

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

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

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

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

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

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

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

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

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

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

188 ys, coimmunoprecipitation, and in situ split Venus interaction assays.

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

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

191 Venus is a yellow fluorescent protein that has been deve

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

193 ts Earth-like size and source material(1,2), Venus is extremely dry(3,4), indicating near-total water

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

195 is less than 29 km, unless the heat flux on Venus is less than the radiogenic lower bound of 34 [For

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

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

198 Venus kinase receptors (VKRs) constitute a Receptor Tyro

199 Taking inspiration from Venus kinase receptors (VKRs), an atypical family of RTK

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

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

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

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

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

205 the nightside and downstream portion of the Venus magnetosphere (i.e., the magnetotail).

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

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

208 Design limitations prevented past Venus missions from measuring both HCO(+) and the escapi

209 d be an attractive research theme for future Venus missions.

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

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

212 a total of 181 proteins co-purifying with a Venus multifunctional (VM)-tagged CK1delta and/or CK1eps

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

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

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

216 Firstly, for validation, we applied Venus on well-studied viral datasets, such as HBV- hepat

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

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

219 Fluorescent cells from CHGA-Venus organoids were purified by flow cytometry and anal

220 SAPIEN 3 (ES3) balloon-expandable valves or Venus-P self-expandable valves.

221 an age of 36.3 years; 64.1% of ES3, 35.9% of Venus-P.

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

223 At least some of this deformation on Venus postdates the emplacement of the locally youngest

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

225 l erosion is usually assumed to be absent on Venus, precluded by a high surface temperature of ~450 d

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

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

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

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

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

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

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

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

234 Using a CRISPR/Cas9 Zebrafish her6::Venus reporter combined with mathematical and in vivo ex

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

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

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

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

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

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

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

242 mineralogy will place firmer constraints on Venus's heat flux.

243 Consistency with Venus's modern atmospheric composition occurs in less th

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

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

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

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

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

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

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

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

252 From orbit, Venus' surface is only observable on the nightside throu

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

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

255 Here we show that VENUS-tagged AtDRO1 driven by the native AtDRO1 promoter

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

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

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

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

260 Using a Venus-tagged Gbetagamma and nanoluciferase-tagged trunca

261 receptor-specific assays for recruitment of Venus-tagged Gs protein through fusion of luciferase to

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

281 arshall Ethanol for Untreated Persistent AF (VENUS) trial was an investigator-initiated, National Ins

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

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

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

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

286 we update an existing photochemical model of Venus' upper atmosphere by including the photochemistry

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

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

289 Venerupis corrugata, Polititapes rhomboides, Venus verrucosa, Dosinia exoleta, Glycymeris glycymeris,

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

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

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

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

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

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

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

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

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

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

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