ライフサイエンスコーパス: radio

1 iving on a quiet road while listening to the radio.

2 ts] versus 1.0% [53 events]; adjusted hazard radio, 0.40; 95% confidence interval, 0.21-0.73; P=0.003

3 nfarction (2.5% versus 3.7%; adjusted hazard radio, 0.66; 95% confidence interval, 0.49-0.88; P=0.004

4 rombosis) (3.1% versus 4.7%; adjusted hazard radio, 0.70; 95% confidence interval, 0.55-0.88; P=0.002

5 This technique was exemplified using a radio ((14)C) isotopologue and a stable ((13)C6) isotopo

6 Cloud radio access network (C-RAN) becomes a promising scenari

7 Radio-ADP-ribosylation assays reveal that shedding refoc

8 dio transient is largely consistent with the radio afterglow of a short gamma-ray burst, and its exis

9 nd brown dwarfs, from which we have detected radio and optical auroral emissions both powered by magn

10 other fast radio bursts have similarly faint radio and optical counterparts, our findings imply that

11 Here we report simultaneous radio and optical spectroscopic observations of an objec

12 The Radio and Plasma Wave Science instrument detected a cold

13 ther electromagnetic wave regimes, including radio and sound.

14 r in vitro biosynthesis of the corresponding radio and stable isotope labeled metabolites, namely, (1

15 ndards are not required under the concept of radio and stable isotopologues using adapted LC-RAD/MS p

16 Media-based messaging (via radio and television) is now used to sensitize the publi

17 ia broadcast information channels, including radio and television; more recently, risk communication

18 From Washington to Wollongong, newspapers, radio and TV were abuzz with the story of a transgenic m

19 ltraviolet-optical-infrared, and the delayed radio and x-ray emission.

20 tive black hole in 47 Tucanae (NGC 104) from radio and X-ray observations, respectively.

21 e inductive sensing elements, high frequency radio, and/or optical circuitry and can be made signific

22 growth in mice, and have been implicated in radio- and chemo-resistance.

23 on cancer treatments currently available are radio- and chemo-therapy.

24 on of K134-substituted histone H2AX enhanced radio- and chemosensitivity of cancer cells.

25 of normal tissue complications brought on by radio- and chemotherapeutic treatment regimens.

26 Quantitative assessment of radio- and chemotherapy response with (18)F-FDG whole-bo

27 or and are thought to be highly resistant to radio- and chemotherapy.

28 e green-(99m)Tc-nanocolloid enables combined radio- and fluorescence image guidance during sentinel n

29 Intraoperatively, radio- and fluorescence-guided SN detection rates were s

30 Here we report the discovery of a fast radio burst and the identification of a fading radio tra

31 tial and frequency characterization of solar radio burst fine structures observed with the Low Freque

32 data revealing Faraday rotation in the fast radio burst FRB 110523.

33 rt the subarcsecond localization of the fast radio burst FRB 121102, the only known repeating burst s

34 tional bursts from the direction of the fast radio burst FRB 121102.

35 Every fast radio burst has a dispersion measurement, but none befor

36 observations are inconsistent with the fast radio burst having a Galactic origin or its source being

37 nate the observed spatial characteristics of radio burst images.

38 retation of another recently discovered fast radio burst, suggesting that there are at least two clas

39 Fast radio bursts (FRBs) are millisecond-duration events thou

40 Fast radio bursts are astronomical radio flashes of unknown p

41 Fast radio bursts are bright, unresolved, non-repeating, broa

42 Fast radio bursts are millisecond-duration astronomical radio

43 So far all fast radio bursts have been detected with large single-dish t

44 However, if other fast radio bursts have similarly faint radio and optical coun

45 physical origins for the population of fast radio bursts, these repeat bursts with high dispersion m

46 o have been discovered in the so-called fast radio bursts.

47 Her accompanying students hiked out, radio-called 911, and the Harborview Medical Center (Sea

48 ble to discern any impact of a complementary radio campaign on insurance claims.

49 potential of the physical properties of the radio channel itself to provide communications security.

50 that senescent cells, which accumulate after radio/chemo therapy, promote endocrine resistance in bre

51 is ~15 months despite aggressive surgery and radio-chemotherapy approaches.

52 is 15 months despite aggressive surgery and radio-chemotherapy approaches.

53 significantly better response to neoadjuvant radio/chemotherapy of the patients.

54 Neoadjuvant radio/chemotherapy regimens can markedly improve cervica

55 a novel predictive biomarker for neoadjuvant radio/chemotherapy responses.

56 which include the combination of surgery and radio/chemotherapy, the average survival rate remains po

57 GPS locations of radio-collared lions indicate that freeways are a near-a

58 icrowave devices are ubiquitous in radar and radio communication and indispensable in the readout cha

59 lasma physics and in applications related to radio-communications between the ground and spacecraft r

60 lar source has been seen in CK Vul, though a radio continuum source was identified at the expansion c

61 imes of ultrafast information processing for radio, control, and scientific computing.

62 The ultrasonic radio could serve as a useful addition to wireless commu

63 rometer hot spots; we observed the predicted radio counterpart of such hot spots.

64 ted by bats in the field, and the ultrasonic radio, coupled to electromagnetic (EM) radio, is shown t

65 processing resources effectively to maximize radio coverage.

66 Instead, the radio data require the existence of a mildly relativisti

67 , compliant systems of sensors, circuits and radios designed to intimately interface with the soft ti

68 Radio detection of cosmic rays is a rapidly developing t

69 he patient was referred to the Department of Radio-diagnosis for ultrasound.

70 All candidate signatures appear radio-dim and do not have the X-ray to radio flux ratios

71 nets, these aurorae include highly polarized radio emission at kilohertz and megahertz frequencies pr

72 The observed radio emission can be explained by either a collimated u

73 We present a detection of variable radio emission from a thermal TDF, which we interpret as

74 rgy distribution, or low-energy cutoffs, for radio emission in galaxy clusters and radio galaxies, ha

75 posed that the observed gamma-ray, X-ray and radio emission is due to an ultra-relativistic jet being

76 burst revealed circular polarization of the radio emission, but no linear polarization was detected,

77 molecular gas kinematics and features in the radio-emitting jets, has however been lacking.

78 tion technologies has delivered ultra-small, radio-enabled neuromuscular recorders and stimulators fo

79 Fast radio bursts are astronomical radio flashes of unknown physical nature with durations

80 Its radio flux and dispersion measure are consistent with va

81 ppear radio-dim and do not have the X-ray to radio flux ratios required for accreting black holes.

82 iability, quasi-periodicity and the delay of radio flux variations relative to optical changes.

83 ith a proxy for solar activity, the F10.7 cm radio flux, and therefore with the solar cycle phase.

84 sition is highly correlated with the F10.7cm radio flux.

85 Despite extensive searches, radio follow-up observations of known thermal stellar ti

86 h an external electromagnetic wave source at radio frequencies (RF) in experiment.

87 mmission was the first auction to reallocate radio frequencies between two different kinds of uses: f

88 da/78 objects is confirmed experimentally at radio frequencies by fabricating an artificial material

89 applications including surface acoustic wave radio frequencies devices and integrated optics.

90 n magnetic fields, cause copious emission at radio frequencies in both clusters of galaxies and radio

91 yrators enable new applications ranging from radio frequencies to optical frequencies, including full

92 30 seconds, and they are also detectable at radio frequencies.

93 warfs are rarely detected at far-infrared or radio frequencies.

94 hased arrays, commonly used at microwave and radio frequencies.

95 t with a uniaxial hyperbolic metamaterial at radio-frequencies revealing the directional routing effe

96 ategies employing magnetic hyperthermia in a radio frequency (RF) AMF.

97 le maintaining large mobility for high speed radio frequency (RF) applications.

98 the localized mechanical mode either with a radio frequency (RF) field through the piezo-electric ef

99 and testing of a microtoroid resonator and a radio frequency (RF) microelectromechanical systems (MEM

100 Radio frequency (RF) multipole ion guides that allow for

101 advanced pasteurization treatments based on radio frequency (RF) or microwave (MW) energy, dielectri

102 after a precisely defined delay, by a single radio frequency (rf) probe pulse.

103 emories, magnetic field sensors, and tunable radio frequency (RF)/microwave devices.

104 hniques, especially thermal approaches, e.g. radio frequency ablation (RFA).

105 pH sensing, contact/temperature monitoring, radio frequency ablation and localized photo/chemotherap

106 Our results show that logic inverters or radio frequency amplifiers can be formed by integrating

107 uch interest as a future channel material in radio frequency electronics because of its superior elec

108 oach based on the application of atmospheric radio frequency glow discharge (rf-GD) optical emission

109 's complete foraging history, obtained using radio frequency identification (RFID).

110 light mass spectrometer using novel branched radio frequency ion trap architecture.

111 describe how for the first time the use of a radio frequency ion-funnel (RFIF) in the reaction region

112 e typically continuous saturation of (1)H by radio frequency irradiation is employed.

113 the analysis of CEST effects under different radio frequency irradiation power levels was developed.

114 e ambient magnetic field with a superimposed radio frequency magnetic field of the order of 100 nT.

115 contact hole array was fabricated, to which radio frequency magnetron sputtering process was then ap

116 perlattices on SrTiO3 substrates by off-axis radio frequency magnetron sputtering.

117 Atomic spins are usually manipulated using radio frequency or microwave fields to excite Rabi oscil

118 eatures characterizing the performance of an radio frequency oscillator.

119 ime-orders of magnitude better than existing radio frequency photonic devices of similar size, weight

120 this work we demonstrate a miniature 10 GHz radio frequency photonic oscillator characterized with p

121 of animals over large areas at low levels of radio frequency power (<1 W).

122 Plasma parameters (radio frequency power and argon flow rates) were optimiz

123 ges of operation that are constrained by the radio frequency power transmission hardware.

124 A variable radio frequency proton-electron double-resonance imaging

125 The circuit operates as a radio frequency receiver performing signal amplification

126 Femtosecond laser-based generation of radio frequency signals has produced astonishing improve

127 The radio frequency sputtered nickel oxide thin film nanostr

128 hotonic crystal membrane, is controlled by a radio frequency surface acoustic wave.

129 nd-to-end user demands and globally optimize radio frequency, optical network and processing resource

130 ture ion mobility experiments performed in a radio frequency-confining drift cell.

131 e very fine patterns for large-area flexible radio-frequency (RF) applications is very desirable beca

132 amount of sample and does not need multiple radio-frequency (RF) channels.

133 Radio-frequency (RF) electronics, which combine passive

134 atic protons in free substrate for selective radio-frequency (RF) labeling and, (ii) the process of i

135 and SiNCs that were surface-treated using a radio-frequency (RF) microplasma system.

136 With a radio-frequency (RF) power source and controller, this i

137 le and conformal devices for transmission of radio-frequency (RF) signals over large distances for mo

138 The films were fabricated using radio-frequency (RF) sputtering with a single-crystal Cu

139 Conventional high-brightness radio-frequency accelerating structures operate with 30-

140 etic energy that particles in a conventional radio-frequency accelerator can reach.

141 or terahertz- to- optical devices as well as radio-frequency acoustic devices where piezoelectricity

142 esses to allow two-photon, near-infrared and radio-frequency activation.

143 iding broadly generalizable, MRI-compatible, radio-frequency analogues to optically based probes for

144 nt, on-chip inductors remains a challenge in radio-frequency and power microelectronics, where they p

145 It modulates an individual pulse in a radio-frequency burst within 4 ns, achieving a reconfigu

146 Our device can generate programmable radio-frequency bursts or continuous waveforms with only

147 Bulk niobium Superconducting Radio-Frequency cavities are a leading accelerator techn

148 250 in our device), resulting in a miniature radio-frequency circulator that exhibits reduced impleme

149 watches, scientific calculators and wireless radio-frequency communication system, which indicates th

150 gh-frequency (55 MHz) ultrasound and the raw radio-frequency data processed.

151 Here, we demonstrate that a radio-frequency deflector in combination with a dipole s

152 w sensitivity limit for atom-based, absolute radio-frequency electric field sensing of 5 muV cm(-1) H

153 sion, the negative end exhibited optical and radio-frequency electromagnetic features expected for ne

154 stigated the association between exposure to radio-frequency electromagnetic fields (RF-EMFs) from br

155 ized radioactive tracer using pulses of both radio-frequency electromagnetic radiation and magnetic-f

156 The development of transparent radio-frequency electronics has been limited, until rece

157 already find applications in such fields as radio-frequency electronics, micro-attenuators, sensors

158 rption of energy in the human brain from the radio-frequency fields emitted.

159 opose an architecture of integrated photonic radio-frequency generation and processing and implement

160 bility applications, both rigid and flexible radio-frequency graphene field-effect transistors (G-FET

161 sor was also attached to a passively-powered radio-frequency identification (RFID) tag which transmit

162 trate capable of rectifying a high-frequency radio-frequency identification signal (13.56 MHz), with

163 ehicle (rover) which can be equipped to make radio-frequency identifications, wild penguins had signi

164 Using suitable radio-frequency mesa structures, a range of IGZO thickne

165 Letter, we demonstrate direct actuation of a radio-frequency micromechanical plate-type resonator by

166 ons were grown on c-sapphire substrate using radio-frequency plasma assisted molecular beam epitaxy.

167 nthesized together with a related phase by a radio-frequency plasma reaction under near-ambient condi

168 tions, such as advanced computer processors, radio-frequency power devices, quantum cascade lasers an

169 antum (DQ) coherence excitation/reconversion radio-frequency pulses, very high-resolution proton-base

170 upling between the voltage fluctuations in a radio-frequency resonance circuit and the membrane's dis

171 and measurement of the phase of a reflected radio-frequency signal.

172 Efficient up-conversion of radio-frequency signals to an optical carrier would enab

173 However, rather than detecting weak radio-frequency signals, imaging information is obtained

174 ting in the nuclear magnetic resonance (NMR) radio-frequency spectrum, where signal attenuation and d

175 nanowires onto copper substrates followed by radio-frequency sputtering of carbon-nitride films, form

176 tude above that achievable with conventional radio-frequency structures.

177 superconducting circuits and is essential in radio-frequency superconducting quantum interference dev

178 proach to accurately manipulating individual radio-frequency waveform features without constraints se

179 Photonic methods of radio-frequency waveform generation and processing can p

180 The radio-frequency-addressable sensor assemblies presented

181 that are within 3% of those determined from radio-frequency-confining drift cell measurements.

182 e are obtainable using fp-RFDR (finite-pulse radio-frequency-driven dipolar recoupling) pulse sequenc

183 otential platform for frequency reference in radio-frequency-photonic architectures.

184 lators as a frequency reference platform for radio-frequency-photonic information processing.

185 ng hot gas shells is indirect and limited to radio galaxies at the centres of clusters, which are too

186 frequencies in both clusters of galaxies and radio galaxies through non-thermal radiation emission ca

187 s, for radio emission in galaxy clusters and radio galaxies, have not yet been determined.

188 ision between two knots in the jet of nearby radio galaxy 3C 264.

189 e we report on gamma-ray observations of the radio galaxy IC 310 obtained with the MAGIC (Major Atmos

190 r a non-thermal population of electrons in a radio galaxy jet/lobe, located at a significant distance

191 s produced by cluster mergers or injected by radio galaxy jets, which impacts the formation of large-

192 nd brain radiometabolites were studied using radio-high-performance liquid chromatography analysis.

193 l stability of (99m)Tc-RYM1 was evaluated by radio-high-performance liquid chromatography analysis.

194 A radio-hot belt exists, consisting of relatively transpar

195 asma in the highest tertile (adjusted hazard radio [HR] 1.44, 95% CI 1.14-1.83) and the presence of e

196 issue distribution were investigated by beta-radio imager whole-body mapping in mice.

197 s morphology and dynamics using high-cadence radio imaging spectroscopy.

198 dent H2O2 production in long-term persistent radio-induced DNA damage.

199 for the chromosomal rearrangements found in radio-induced papillary thyroid carcinoma.

200 wed that DUOX1 is elevated not only in human radio-induced thyroid tumors, but also in sporadic thyro

201 ing burst source, using high-time-resolution radio interferometric observations that directly image t

202 leiades cluster that uses very long baseline radio interferometry (VLBI).

203 stronomers seek to image jet formation using radio interferometry but still suffer from insufficient

204 nt on day timescales, and very long baseline radio interferometry yields an angular size of less than

205 The radio-iodinated imidazopyridine derivative (123)I-ABC577

206 sonic radio, coupled to electromagnetic (EM) radio, is shown to function as a high-accuracy rangefind

207 ur results show diversity in both stable and radio isotopes at all depths, confirming DOC cycling hid

208 in active galactic nuclei that lack powerful radio jets (such jets are an alternative way to drive mo

209 dulation on the structure of the large-scale radio jets, which provides a useful way to search for ot

210 sk encircling the black hole, and collimated radio jets.

211 nto the interstellar medium by the expanding radio jets.

212 the detection of reaction products by using radio-labeled or chemically modified nucleotides.

213 Physicians use radio-labeled sulfur colloid and/or methylene blue dye t

214 ts showed that the peak region of a pulse of radio-labelled auxin moves at a roughly constant velocit

215 correlate well with the values determined in radio ligand binding assays.

216 Radio-ligand binding and functional assays were conducte

217 an be visualized by microscopy and probed by radio-ligand binding.

218 ng 23 selected parent dust contaminants in a radio-ligand TTR binding assay; 2,2',4,4'-tetrahydroxybe

219 lts of isothermal titration calorimetry, and radio-ligand uptake and fluorescent transport assays on

220 Here we report that the radio light curve of GW170817 has no direct signature of

221 Because the cocoon model explains the radio light curve of GW170817, as well as the gamma-ray

222 Within 100 days of the merger, the radio light curves will enable observers to distinguish

223 e warm molecular hydrogen gas in the western radio lobe of the Seyfert galaxy IC 5063 is moving at hi

224 seven orders of magnitude for a sample of 76 radio-loud active galaxies.

225 es suggest an extragalactic origin and imply radio luminosities that are orders of magnitude larger t

226 Here we report radio measurements of Xmax with a mean uncertainty of 16

227 vention-clinic events, community events, and radio messaging-or to a standard care control arm, both

228 However, the radio network, optical network and processing unit cloud

229 neuronal activity while subjects listened to radio news played faster and faster until becoming unint

230 e 24 human subjects (12 females) listened to radio news uttered at different comprehensible rates, at

231 bgroups of radiosensitivity: radiosensitive, radio-normal, and radioresistant groups.

232 In the rest frame of the TDF, our radio observations are an order of magnitude more sensit

233 g simultaneous infrared, optical, x-ray, and radio observations of the Galactic black hole system V40

234 Solar radio observations provide a unique diagnostic of the ou

235 ier containing OP3-4 with BMP-2 enlarged the radio-opaque area and increased the bone mineral content

236 testinal transit time (GITT) determined with radio-opaque markers.

237 Degradation tests with radio or stable isotope labeled compounds enable the det

238 ion (MDRI) for service provisioning in cloud radio over fiber network (C-RoFN).

239 nities for the application of biodegradable (radio)peptide drugs of either natural or synthetic origi

240 ti-targeting and multi-drug strategy, chemo-/radio-/photodynamic-/ultrasound-/thermo-combined multi-m

241 FLI1 and PARP, and for chemo-potentiation or radio-potentiation.

242 with fully implantable, stretchable wireless radio power and control systems.

243 (extracurricular) Hitler Youth, and through radio, print, and film.

244 A triple system containing a radio pulsar could provide such measurements, but the on

245 ld modulate the arrival times of pulses from radio pulsars.

246 bursts are millisecond-duration astronomical radio pulses of unknown physical origin that appear to c

247 th a basic observation of Hanbury Brown that radio-pulses from two distinct antennas generate signals

248 cs, the Lyman-alpha emission surrounding the radio-quiet quasar UM 287 extends well beyond the virial

249 systemic toxicity, temporary remission, and radio-resistance in lung cancer cells.

250 The dermal macrophages were radio resistant and not replaced by monocytes or adult B

251 e cells are replenished by an extramedullary radio-resistant and UV-sensitive Bmi1(+) progenitor.

252 e these macrophages as Skin Transendothelial Radio-resistant Anti-inflammatory Macrophages (STREAM) a

253 beta) on Th17 cells and LTbetaR on meningeal radio-resistant cells were necessary for the propagation

254 MPN was delayed in animals lacking IL-33 in radio-resistant cells.

255 etermined that deletion of caspase-12 in the radio-resistant compartment was responsible for this met

256 cal yield and purity, specific activity, and radio-scalability).

257 e objects) can accurately predict organismal radio scattering characteristics from an anatomical mode

258 ull azimuthal, elevational, and polarimetric radio scattering data.

259 gents targeting HR repair as potential chemo/radio sensitizers.

260 bsorb radiation rays (e.g. X-ray) can act as radio-sensitizers to deposit radiation energy within tum

261 ystem instructions (integrated task) or to a radio show (split task).

262 In recent years, millisecond-duration radio signals originating in distant galaxies appear to

263 We report the detection of a counterpart radio source that appears 16 days after the event, allow

264 The flux density of the persistent radio source varies by around ten per cent on day timesc

265 econds of a faint 180-microJansky persistent radio source with a continuum spectrum that is consisten

266 After listening to a radio story in the scanner, participants were asked how

267 Current treatment is confined to (radio) surgery and no targeted drug therapies exist.

268 induce precocious foraging in bees and used radio tag tracking to examine the consequences of precoc

269 We used automated radio telemetry to track three songbird species (Red-eye

270 a combination of capture-mark-recapture and radio telemetry, we compared survival probabilities betw

271 ed their migration using an intercontinental radio-telemetry array.

272 ion, and we examined six years of concurrent radio-telemetry data for evidence of large-scale spatial

273 Using an automated radio-telemetry system, we compared activity patterns of

274 millisecond pulsars obtained with the Parkes radio telescope, we constrained the characteristic ampli

275 wideband microphone and a related ultrasonic radio that can be used for wireless communication.

276 The new radio-TLC method allows quality control in a short time

277 For radio-TLC quality control, various mobile phases were an

278 as far reaching implications applicable from radio to optical frequencies.

279 l SMART (species movement, acceleration, and radio tracking) collar that used accelerometry to contin

280 We used radio-tracking and ice drift data to quantify the influe

281 The ~6-day radio transient is largely consistent with the radio aft

282 dio burst and the identification of a fading radio transient lasting ~6 days after the event, which w

283 arger than those of all known short-duration radio transients.

284 to be addressed separately from the physical radio transmission aspects of wireless systems.

285 ise to a hitherto unidentified population of radio, ultraviolet, X-ray and gamma-ray transients in th

286 The observations demonstrate that radio wave propagation effects, and not the properties o

287 s of the emitting source from the effects of radio wave propagation has long been a major challenge i

288 les much shorter than those corresponding to radio wave propagation in the corona.

289 asurements, remote optical observations, and radio wave reflection experiments have produced conflict

290 Here we report the results of optical-to-radio-wavelength monitoring of the blazar CTA 102 and sh

291 Radio wavelengths can probe altitudes in Jupiter's atmos

292 rf/cool star binary that emits from X-ray to radio wavelengths.

293 Interactions of high-frequency radio waves (RF) with biological tissues are currently b

294 gulation of gene expression by low-frequency radio waves (RFs) or a magnetic field.

295 y such as lightning mapping systems based on radio waves can typically detect only some aspects of th

296 illimeter scale while ultrasound, X-ray, and radio waves have been key in aiding in the millimeter to

297 to induce neuronal activation remotely using radio waves or magnetic fields via Cre-dependent express

298 ongly affects the propagation of the emitted radio waves, so decoupling the intrinsic properties of t

299 fferent types of energy - light, ultrasound, radio waves, X-rays etc.

300 t strong luminescence and discrete-frequency radio waves.