ライフサイエンスコーパス: astronomical

1 h scales ranging from the microscopic to the astronomical.

2 ranging in outlook from the molecular to the astronomical.

3 because the number of possible genotypes is astronomical.

4 ral wavelength and variable bandwidth of the astronomical 2175 angstrom feature.

5 lma (dated at 776 +/- 2 kyr), agree with the astronomical age for the reversal.

6 These GEMS provide a spectral match to astronomical "amorphous" silicates, one of the fundament

7 rocycles (PANHs), has been proposed for both astronomical and combustion environments, but no suitabl

8 ore than one order of magnitude tighter than astronomical and cosmological limits on the coupling bet

9 accounted for (e.g., by independently adding astronomical and non-astronomical components, as is ofte

10 including spectroscopy, bio-medical sensing, astronomical and space detection, THz tomography, and no

11 ion metals is of interest in organometallic, astronomical, and optoelectronic device chemistry.

12 Astronomical calculations reveal the Solar System's dyna

13 The Antikythera Mechanism, an ancient Greek astronomical calculator, has challenged researchers sinc

14 is useful for applications in optical clock, astronomical calibration and biological imaging.

15 optical synthesizer, telecommunications and astronomical calibrations have been reported recently.

16 alidates measurements from the pre-encounter astronomical campaign.

17 tes the multiple roles that GA might play in astronomical chemistry.

18 dance toward an integrated picture of global astronomical climate forcing in the Late Triassic and ul

19 Unlike Earth, where astronomical climate forcing is comparatively small, Mar

20 50 and 650 ka without substantial changes in astronomical climate forcings.

21 The HAT reactions of HOSO* in astronomical CO and CO(2) ices by forming reactive acyl

22 by independently adding astronomical and non-astronomical components, as is often done in impact case

23 oglyphs are calendrical in nature and relate astronomical computations, including at least two tables

24 c CO2 between 280 and 500 ppm and a changing astronomical configuration.

25 on, placing Solar System formation within an astronomical context.

26 Animals that use astronomical cues to orientate must make continuous adju

27 d as omens, while the calm regularity of the astronomical cycles must have been philosophically attra

28 Astronomical data analytics has rapidly expanded given t

29 y laboratory studies of Mg silicates and the astronomical data for comets and for protoplanetary disk

30 Laboratory spectra have been compared to astronomical data in order to gain further insight into

31 oratory spectra are needed for comparison to astronomical data.

32 KODAMA is then applied to an astronomical dataset, revealing unexpected features.

33 izing the central circadian pacemaker to the astronomical day by conveying information about ambient

34 We present the astronomical detection of a chiral molecule, propylene o

35 However, the astronomical detection of specific aromatic molecules is

36 Here we report the astronomical detection of this t = 0 moment, capturing t

37 Due to its microscopic nature at astronomical distances and stringent requirements in lab

38 l, precise, and mature tools for determining astronomical distances.

39 The non-stoichiometric binding and astronomical diversity characteristic of carbohydrates c

40 pread access to advanced AI capabilities for astronomical education and research.

41 sufficient to enable their identification in astronomical environments by radio astronomy.

42 s play an important role in the chemistry of astronomical environments such as the cold interstellar

43 cules and benzo-N-pentalene(+) structures in astronomical environments.

44 portant insights concerning the chemistry in astronomical environments.

45 utron star mergers, which are multimessenger astronomical events that have been observed both in grav

46 Geochemical and astronomical evidence demonstrates that planet formation

47 heric properties with present-day and future astronomical facilities.

48 rrelations can enhance coding performance by astronomical factors.

49 ly Pleistocene, in response to both external astronomical forcing and internal climate dynamics.

50 mate system of Earth responds nonlinearly to astronomical forcing by frequency modulating eccentricit

51 favoring high temperatures, indicating that astronomical forcing could have played a role in trigger

52 n the basis of their distinctive response to astronomical forcing depending on greenhouse gas concent

53 Marine delta(18)O data reveal astronomical forcing of the climate and cryosphere durin

54 ese variations in the climatic expression of astronomical forcing produced latitudinal climatic zones

55 However, it has not been clear how astronomical forcing translates into the observed sequen

56 esponses of temperature and precipitation to astronomical forcing under different ice/CO(2) boundary

57 ontent and magnetic susceptibility indicates astronomical forcing was involved and the PETM onset las

58 quasi-synchronization in the interaction of astronomical forcing, carbon cycling and glacial events

59 onmental conditions, possibly as a result of astronomical forcing.

60 h-frequency Antarctic ice sheet dynamics and astronomical forcing.

61 response of the oceanic carbon reservoir to astronomical forcing.

62 A long-standing astronomical goal is to resolve structures in the innerm

63 spacing is readily resolvable using typical astronomical grating spectrographs.

64 tituted PAHs preclude their definitive radio astronomical identification.

65 etal and sulfides), which is consistent with astronomical identifications of crystalline and amorphou

66 These trails already affect astronomical images across the complete electromagnetic

67 The oral presentation included about 130 astronomical images which cannot be reproduced here.

68 here ice sheets and oceanic, atmospheric and astronomical influences in initiating climate change in

69 ss of circumstellar silicon carbide based on astronomical infrared spectra is controversial.

70 e realization that many emission features in astronomical infrared spectra probably arise from polycy

71 Hence, astronomical insolation forcing likely contributed to th

72 The constant improvement of astronomical instrumentation provides the foundation for

73 h in astronomy, astrophysics, cosmology, and astronomical instrumentation.

74 e in either the sensitivity or resolution of astronomical instruments have always brought revolutiona

75 The observed astronomical line strengths are generally consistent wit

76 nprecedented accuracy by a new generation of astronomical measurements.

77 ublic money to industrial contracts to build astronomical missions.

78 The astronomical number of accessible discrete chemical stru

79 s that may be associated with the trait from astronomical number of all possible combinations; and (2

80 or experimentally intractable because of the astronomical number of combinations in design space.

81 Mammals are colonized by an astronomical number of commensal microorganisms on their

82 find its unique native state in spite of the astronomical number of configurations in the denatured s

83 It faces a fundamental obstacle in the astronomical number of genotypes whose fitness needs to

84 small proteins is inherently limited by the astronomical number of possible amino acid sequences.

85 To delineate the astronomical number of possible interactions of all gene

86 sents about 15 per cent of the population of astronomical objects near the Sun.

87 for predicting the properties of far-distant astronomical objects such as accretion disks around blac

88 articularly attractive candidate among known astronomical objects to potentially host life.

89 disparities in the opportunity to see these astronomical objects with the naked eye.

90 is a unique phenomenon observed in condensed astronomical objects, including the Wolf-Rayet star EZ-C

91 red emission bands that are observed in many astronomical objects.

92 ore accurate estimation of the total mass of astronomical objects.

93 ethod for a star tracker based on the direct astronomical observation is proposed here.

94 s in autonomous driving, biomedical imaging, astronomical observation, and more.

95 ons has been in critical demand for frontier astronomical observation, spectroscopic imaging and wave

96 These findings strongly correlate with astronomical observations and explain a higher [c-C3H]/[

97 Astronomical observations and isotopic measurements of m

98 In this special issue, astronomical observations and theories constraining circ

99 ive model of interstellar dust inferred from astronomical observations and theory.

100 aints from particle physics nor cosmological/astronomical observations are sufficient to rule out thi

101 Astronomical observations captured solar transits by Pho

102 line in dust opacity during the mission, and astronomical observations captured solar transits by the

103 Recent astronomical observations have revealed what may prove t

104 These astronomical observations motivate us to understand exop

105 Astronomical observations now reach far enough back in t

106 Astronomical observations of elemental and isotopic abun

107 Although astronomical observations of primordial deuterium abunda

108 This provides a link between astronomical observations of star formation and cosmoche

109 h rapid formation is broadly consistent with astronomical observations of young stellar objects, whic

110 matter which has been postulated to explain astronomical observations through its gravitational effe

111 the gaseous disk dissipated, constrained by astronomical observations to be a few to ten million yea

112 ntensity of emission profiles used widely in astronomical observations, and necessary for star and pl

113 ith H(2), critical for interpreting infrared astronomical observations, are lacking for most molecule

114 Mendel carried out daily meteorological and astronomical observations, cared for the monastery's fru

115 on observations of geological field studies, astronomical observations, laboratory experiments, and a

116 ide new insights into the Doppler effect for astronomical observations, laser cooling, and light-matt

117 ed to the absolute calendar by a few ancient astronomical observations, which remain a source of deba

118 through its gravitational impact is clear in astronomical observations--from the early observations o

119 ing of solid structures, and comparison with astronomical observations.

120 meteorites to theoretical-computational and astronomical observations.

121 condensation site, as similarly suggested by astronomical observations.

122 t are challenging to simulate or measure via astronomical observations.

123 r design that is practical for adaptation to astronomical observatories.

124 cecraft and the NASA Goddard Geophysical and Astronomical Observatory (GGAO).

125 The narrowness of the peak does suggest an astronomical origin; however the shape of the peak is in

126 lengths; each has provided insights into new astronomical phenomena (e.g., quasars, pulsars, and the

127 n eclipse, and search for dates matching the astronomical phenomena we believe they describe.

128 They are applicable in astronomical, planetary science, space weather, light po

129 their hierarchical relation, we estimate an astronomical precession frequency of 108.6 +/- 8.5 arcse

130 d allow a precision as high as 1 cm s(-1) in astronomical radial velocity measurements.

131 Fast radio bursts are astronomical radio flashes of unknown physical nature wi

132 Fast radio bursts are millisecond-duration astronomical radio pulses of unknown physical origin tha

133 orms, the genome databases are growing at an astronomical rate.

134 disputed eclipse reference, we analyze other astronomical references in the Epic, without assuming th

135 We use three overt astronomical references in the epic: to Bootes and the P

136 as kept the telescope on the cutting edge of astronomical research.

137 Our findings suggest that the astronomical response in delta(2)H(wax) is attributable

138 1.4+/-0.3 and to correlate with the Infrared Astronomical Satellite (IRAS) 100- map.

139 deviant from their actual values in infrared astronomical satellite (IRAS) galaxy samples.

140 hift surveys of galaxies [e.g., the Infrared Astronomical Satellite (IRAS)] with velocity fields deri

141 ity of the atomic nucleus with the shapes of astronomical-scale, gravitationally-bound masses.

142 de complex phenomena ranging from quantum to astronomical scales and in disciplines as diverse as met

143 instability (RTI), present from tabletop to astronomical scales, is an iconic example characterized

144 n of rotating bodies in both terrestrial and astronomical settings.

145 dying optical speckle in both laboratory and astronomical settings.

146 pherical or elongated grains that consist of astronomical silicates or organic refractory material.

147 particles (IDPs) were compared with those of astronomical silicates.

148 te and local RNA fitness landscapes, but the astronomical size of sequence space limits purely experi

149 Here, we present geologic data and a new astronomical solution (ZB18a) showing exceptional agreem

150 Our astronomical solution requires a chaotic resonance trans

151 o a great eccentricity cycle consistent with astronomical solutions.

152 icles that can be associated with a discrete astronomical source, and they pose challenges to particl

153 Transient astronomical sources are typically powered by compact ob

154 wave band and has detected a wide variety of astronomical sources at considerable distances, includin

155 A new class of extragalactic astronomical sources discovered in 2021, named odd radio

156 hose observed in most other classes of radio astronomical sources, and are consistent with coherent e

157 there has been no direct evidence for FeS in astronomical sources, which poses a considerable problem

158 FRBs) are brief radio emissions from distant astronomical sources.

159 ds (DIBs), ubiquitous absorption features in astronomical spectra, have been known since early this c

160 llar medium is one of the oldest problems in astronomical spectroscopy, as DIBs have been known since

161 Astronomical studies of CH in higher rotational levels a

162 By mining astronomical survey data, we have now found 195 compact

163 Astronomical surveys have identified numerous exoplanets

164 A number of astronomical systems have been discovered that generate

165 of resolved x-ray jets in a wide variety of astronomical systems.

166 These apparently represent early astronomical tables and may shed light on the later book

167 Maya astronomical tables are recognized in bark-paper books f

168 But 40 years ago after radio astronomical techniques uncovered the high-energy univer

169 e optics, a technology originally applied in astronomical telescopes to combat atmospheric aberration

170 atics from Plato's Academy and ancient Greek astronomical theories.

171 le is consistent with the predictions of the Astronomical Theory.

172 tidal constituents, a proxy for the highest astronomical tide (HAT), changes over seasonal and inter

173 nded to an elevation higher than the highest astronomical tide datum - captured the biotic and edaphi

174 the parameters determined from the first-day astronomical tide height (ATH) data.

175 ewed vigilance, with systematic reference to astronomical time (including year zero) or, at the very

176 These records lead to an astronomical time calibration of the environmental chang

177 An absolute, fully calibrated astronomical time scale has hitherto been hampered beyon

178 the variability of atmospheric CO2 levels on astronomical time scales that is not yet captured in exi

179 recent availability of large collections of astronomical time series of flux measurements (light cur

180 he Olenekian in South China that defines the astronomical time-scale for the critical interval of maj

181 Earth, using an integrated radioisotopic and astronomical timescale from the Cretaceous Western Inter

182 f fast radio bursts (FRBs), which are bright astronomical transient phenomena, contains information a

183 imes brighter than the current International Astronomical Union recommendation of magnitude 7 (refs.

184 es, and the endorsement of the International Astronomical Union.

185 r disk), in addition to the dust, within one astronomical unit (1 au, the Sun-Earth distance) of the

186 ntation via thermal processing within 2 to 3 astronomical unit (au) of the Sun (1 au being the Earth-

187 etized immediate environment within about an astronomical unit (AU; Earth-Sun distance) of the source

188 wa) was observed near its perihelion of 0.19 astronomical unit by the Ultraviolet Coronagraph Spectro

189 of 113.5 astronomical units from the Sun (1 astronomical unit equals 1.5 x 10(8) kilometres).

190 he comet is headed toward perihelion at 0.92 astronomical unit in April 1997 and is widely expected t

191 the Sun of about 2.8 astronomical units (one astronomical unit is the Earth-Sun distance).

192 (One astronomical unit is the Earth-Sun distance.) The main c

193 prevalence of exoplanets orbiting within one astronomical unit of their host stars in support of the

194 To divert grains out of the 2- to 4-astronomical unit region, the solar radiation pressure m

195 the Sun (performed mostly at a distance of 1 astronomical unit) indicate that solar energetic particl

196 interstellar objects (2.4 x 10(-4) per cubic astronomical unit) suggests that some should have been d

197 100 picodynes per square centimeter AU (AU, astronomical unit), which is significantly larger than t

198 At a distance of one astronomical unit, the wind is mixed and evolved, and th

199 ius A* of 1.4 x 10(4) solar masses per cubic astronomical unit.

200 tric observations that spatially resolve the astronomical-unit-scale distribution of hot material aro

201 cember 2004 at a distance from the Sun of 94 astronomical units (1 AU = 1.5 x 10(8) km).

202 hich itself is a close binary A/B) by 15,000 astronomical units (1 AU is the distance from Earth to t

203 lattened shape with a diameter of a thousand astronomical units (1 AU is the distance from Earth to t

204 (C/1996 B2), at a distance of more than 3.8 astronomical units (550 million kilometres) from its nuc

205 The AU Mic disk is detected between 50 astronomical units (AU) and 210 AU radius, a region wher

206 The disk has a radius of about 330 astronomical units (Au) and a mass of 1 to 8 M(o).

207 ple with a tertiary companion at least 3,500 astronomical units (AU) away from the inner binary.

208 s (twice Earth's) and lies projected at ~0.8 astronomical units (AU) from its host star, about the di

209 istic electrons are observable up to several astronomical units (au) from the planet.

210 Fomalhaut b lies about 119 astronomical units (AU) from the star and 18 AU of the d

211 Hydra and HD163296, at distances of about 30 astronomical units (au) from the star.

212 anets including the asteroids at 0.39 to 4.2 astronomical units (AU) from the Sun (where 1 AU is the

213 presence of fields of 0.54 0.21 G at ~1 to 3 astronomical units (AU) from the Sun and 0.06 G at 3 to

214 mal formation-extending possibly hundreds of astronomical units (AU) from the sun-and that the compos

215 cs imaging with a physical resolution of 0.4 astronomical units (AU) resolves the inner (15 to 80 AU)

216 s and instead predict that a planet near 1.5 astronomical units (AU) should roughly be the same mass

217 in which Jupiter migrates inward from a > 5 astronomical units (AU) to a approximately 1.5 AU before

218 by an accretion disk with a diameter of 130 astronomical units (AU).

219 densed matter at or beyond approximately 2.7 astronomical units (au-the Sun-Earth distance) from thei

220 at a mean distance from the Sun of about 2.8 astronomical units (one astronomical unit is the Earth-S

221 and 9.6 days, respectively, compared to 0.81 astronomical units and 154 days, respectively, for plane

222 anets in phase space overdensities are 0.087 astronomical units and 9.6 days, respectively, compared

223 r the centre of the disk are separated by 61 astronomical units and a tertiary protostar is coinciden

224 n pressure if the LOS approximately 30 to 60 astronomical units and B(LISM) approximately 2.5 microga

225 Voyager 1 was then about 20 astronomical units beyond the shock that terminates the

226 projected separation of 0.275 arc second (5 astronomical units for a distance of 18 parsecs).

227 ion of the asteroid belt between 1.7 and 2.1 astronomical units from Earth.

228 The planet, HIP 99770 b, orbits 17 astronomical units from its host star, receiving an amou

229 s of several to tens of Earth masses at 2-16 astronomical units from the central star.

230 ) place such objects at distances of several astronomical units from the parent star, whereas all but

231 n debris disk extending from about 35 to 210 astronomical units from the star(4), and with clumps exh

232 disk, with a dust-free region less than 9.5 astronomical units from the star, qualitatively and quan

233 city after April 2010 at a distance of 113.5 astronomical units from the Sun (1 astronomical unit equ

234 d on 16 December 2004 at a distance of 94.01 astronomical units from the Sun, becoming the first spac

235 n of one to four gas giants between 5 and 15 astronomical units from the Sun, in agreement with the o

236 idplane of classical T Tauri disks at 2 to 3 astronomical units from their central stars.

237 t fragmentation on scales of more than 1,000 astronomical units has recently emerged.

238 , with sizes of tens, sometimes hundreds, of astronomical units have been resolved with high-spatial-

239 The extracted CO snow line radius of ~30 astronomical units helps to assess models of the formati

240 rger than any intensities since V1 was at 15 astronomical units in 1982.

241 ight speed, and reaches a radius of about 50 astronomical units in only 1.5 days.

242 Between 3.6 and 3.4 astronomical units inbound, GIADA and OSIRIS (Optical, S

243 The magnetic field on a scale of 80 astronomical units is coincident with the major axis (ab

244 8998-760-1 b at greater than or equal to 160 astronomical units is far beyond the CO snowline, we pos

245 Activity at a distance from the Sun of >3 astronomical units is predominantly from the neck, where

246 is coincident with the major axis (about 210 astronomical units long) of the disk.

247 t here that the protoplanetary disk within 3 astronomical units of AA Tauri possesses a rich molecula

248 of around 0.01 solar masses within about 100 astronomical units of the star.

249 ary activity despite an approach within 0.25 astronomical units of the Sun.

250 ragmentation on length scales of about 5,000 astronomical units offers a viable pathway to the format

251 s of approximately 2.3 and approximately 4.6 astronomical units orbiting a primary star of mass appro

252 crafts at heliocentric distances from 2 to 4 astronomical units show a deficit of grains with masses

253 /1995 O1) at a heliocentric distance of 6.45 astronomical units showed emission from cyanogen gas.

254 ssion observations with a resolution of five astronomical units that show four annular substructures

255 simenko from a heliocentric distance of >3.6 astronomical units through perihelion passage at 1.25 as

256 On 25 August 2012, Voyager 1 was at 122 astronomical units when the steady intensity of low-ener

257 and from space at distances as small as 0.3 astronomical units(2-5) to the Sun.

258 ght KIV subgiant star in a very close (0.062 astronomical units) and rapid (2.86 day) orbit with a ma

259 and the orbit of the wide (4 arcseconds, 635 astronomical units) companion are both consistent with e

260 r 1, located at 18.5 billion kilometers (123 astronomical units) from the Sun, decreased by a factor

261 rized, biconical nebula 10 arc seconds (6000 astronomical units) in diameter around the star LkHalpha

262 g the first two perihelion passes (0.16-0.25 astronomical units) of the Parker Solar Probe spacecraft

263 ons of a wide-separation (greater than 1,000 astronomical units) quadruple system composed of a young

264 egion of space extending from Neptune (at 30 astronomical units) to well over 100 AU and believed to

265 mpared to other young disks (greater than 50 astronomical units)(10).

266 he water snowline radii are less than 10 AU (astronomical units)(4,5).

267 imately 10(3) times Saturn's radius RS (0.43 astronomical units), a weak but persistent signal was ob

268 sphere begins repelling the solar wind (~3.3 astronomical units), and we report the spatial structure

269 ar (with a separation of less than a hundred astronomical units), theory predicts the presence of cir

270 gh it is still far from the sun (presently 6 astronomical units).

271 od of 8.46 days, an orbital distance of 0.07 astronomical units, a radius of 0.4 Jupiter radii, and a

272 4, at a heliocentric radial distance of 91.0 astronomical units, and continued sporadically with a gr

273 ructure with a size of approximately 13 x 19 astronomical units, consistent with a disk seen at an in

274 on 2004/351 (during a tracking gap) at 94.0 astronomical units, evidently as the shock was moving ra

275 nresolved (having a size of the order of 100 astronomical units, except at periapse, where the tidal

276 orbital distances of only approximately 0.02 astronomical units, have strong tidal interactions, and

277 fragment, at a distance of approximately 800 astronomical units, is also optically thick to its own c

278 event occurred on 15 December 2004, at 94.1 astronomical units, just before the spacecraft crossed t

279 inity of Neptune's 2:1 resonance at about 48 astronomical units, Neptune's eccentricity can damp to i

280 k fragmentation at radii between 150 and 320 astronomical units, overlapping with the location of the

281 the disk, at projected separations of 10-60 astronomical units, persisting over intervals of 1-4 yea

282 cal units through perihelion passage at 1.25 astronomical units, spanning low and maximum activity le

283 tidally locked because they are close (<0.05 astronomical units, where 1 au is the average Sun-Earth

284 around HD 172555 between about six and nine astronomical units-a region analogous to the outer terre

285 imately 500-metre radius at a distance of 45 astronomical units.

286 tion shock on about 16 December 2004 at 94.0 astronomical units.

287 f Herbig Ae/Be stars on scales of 100 to 300 astronomical units.

288 en cleared out to a distance of more than 17 astronomical units.

289 ursor dust near its midplane inside of a few astronomical units.

290 detected at a separation larger than about 4 astronomical units.

291 ams relative to grains intercepted outside 4 astronomical units.

292 an an earth mass of material out to about 75 astronomical units.

293 comet was at a heliocentric distance of 4.1 astronomical units.

294 arm in the outer disk at a separation of 183 astronomical units.

295 in the system are separated by less than 200 astronomical units.

296 at a semi-major-axis distance of around 0.05 astronomical units.

297 r 51 Eridani at a projected separation of 13 astronomical units.

298 midplane of the disk beyond a distance of 20 astronomical units.

299 ion content of crystalline materials becomes astronomical when collective electronic behavior and the

300 A familiar joke in the astronomical world is that you can sleep through somebod