ライフサイエンスコーパス: astronomical

1 ranging in outlook from the molecular to the astronomical.

2 because the number of possible genotypes is astronomical.

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

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

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

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

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

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

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

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

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

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

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

14 oratory spectra are needed for comparison to astronomical data.

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

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

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

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

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

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

21 rrelations can enhance coding performance by astronomical factors.

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

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

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

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

26 response of the oceanic carbon reservoir to astronomical forcing.

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

28 spacing is readily resolvable using typical astronomical grating spectrographs.

29 tituted PAHs preclude their definitive radio astronomical identification.

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

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

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

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

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

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

36 The observed astronomical line strengths are generally consistent wit

37 nprecedented accuracy by a new generation of astronomical measurements.

38 The astronomical number of accessible discrete chemical stru

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

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

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

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

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

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

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

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

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

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

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

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

51 Astronomical observations captured solar transits by Pho

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

53 Recent astronomical observations have revealed what may prove t

54 Astronomical observations now reach far enough back in t

55 Astronomical observations of elemental and isotopic abun

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

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

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

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

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

61 condensation site, as similarly suggested by astronomical observations.

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

63 meteorites to theoretical-computational and astronomical observations.

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

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

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

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

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

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

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

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

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

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

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

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

76 1.4+/-0.3 and to correlate with the Infrared Astronomical Satellite (IRAS) 100- map.

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

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

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

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

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

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

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

84 o a great eccentricity cycle consistent with astronomical solutions.

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

86 Transient astronomical sources are typically powered by compact ob

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

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

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

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

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

92 Astronomical studies of CH in higher rotational levels a

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

94 A number of astronomical systems have been discovered that generate

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

117 100 picodynes per square centimeter AU (AU, astronomical unit), which is significantly larger than t

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

163 /1995 O1) at a heliocentric distance of 6.45 astronomical units showed emission from cyanogen gas.

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

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

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

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

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

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

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

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

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

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

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

175 4, at a heliocentric radial distance of 91.0 astronomical units, and continued sporadically with a gr

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

193 ams relative to grains intercepted outside 4 astronomical units.

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

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

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

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

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

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