ライフサイエンスコーパス: luminous

1 a hundred times larger and 10(7) times more luminous.

2 exhibits a smooth (<10% excess variability), luminous (2 x 10(45) to 7 x 10(45) erg per second), and

3 These observations reveal an exceptionally luminous (8.2 x 10(45) erg s(-1)) galaxy cluster that ho

4 mbined with a contribution by hot coronae in luminous active galactic nuclei, these accretion flows c

5 thermal-like feature in the X-ray spectra of luminous active nuclei(6-8).

6 distant of the two galaxies is unexpectedly luminous and is spatially resolved with a radius of 260

7 observations concerning the distribution of luminous and nonluminous matter in the Milky Way, in gal

8 We interpret the luminous and supersoft X-rays as resulting from helium b

9 Most of the matter in the Universe is not luminous, and can be observed only through its gravitati

10 o near-infrared) counterpart is powered by a luminous (approximately 10(42) erg per second) kilonova

11 (45) ergs s(-1), which is more than twice as luminous as any previously known supernova.

12 This signal is luminous at optical and infrared wavelengths and is call

13 It is similar to, but six times more luminous at peak than, an enigmatic transient in the gal

14 the first report of two different species of luminous bacteria co-occurring within a single light org

15 Luminous bacteria contain three types of NAD(P)H-FMN oxi

16 ypothesis, based mostly on the prevalence of luminous bacteria in fish guts, has not been tested expe

17 an and Atlantic squids--are known to recruit luminous bacteria into light organ symbioses.

18 ed FMN substrate required by luciferase from luminous bacteria is provided in vivo by NAD(P)H-FMN oxi

19 hat occur between the juvenile squid and the luminous bacteria that colonize it.

20 The phenomenon is thought to be caused by luminous bacteria, but details of milky sea composition,

21 ing resolve evolutionary relationships among luminous bacteria.

22 maximize light production in dim strains of luminous bacteria.

23 between the squid Euprymna scolopes and its luminous bacterial partner, Vibrio fischeri, to define t

24 ort of merodiploidy of lux or rib genes in a luminous bacterium and the first indication that a natur

25 cterium leiognathi; and (iv) a strain of the luminous bacterium Photobacterium mandapamensis was foun

26 The association between the luminous bacterium Vibrio fischeri and the sepiolid squi

27 between the squid Euprymna scolopes and the luminous bacterium Vibrio fischeri offers the opportunit

28 nization of its light organ by the symbiotic luminous bacterium Vibrio fischeri.

29 btail squid Euprymna scolopes and the marine luminous bacterium Vibrio fischeri.

30 mna scolopes, which harbors a culture of the luminous bacterium Vibrio fischeri.

31 between the squid Euprymna scolopes and the luminous bacterium Vibrio fischeri.

32 it is unlikely to be a giant eruption from a luminous blue variable star.

33 It appears similar to the giant outbursts of luminous blue variable stars (LBVs) of 60-100 solar mass

34 their mass in violent precursor eruptions as luminous blue variables (LBVs) before reaching their mos

35 Here we report the detection of the luminous, blue progenitor system of the type Iax SN 2012

36 Quasi-periodic eruptions (QPEs) are luminous bursts of soft X-rays from the nuclei of galaxi

37 The luminous, but brief, accretion phases shown by transient

38 star makes a supernova, because it seems too luminous by more than a factor of ten.

39 servations of HCN emission from the infrared-luminous 'Cloverleaf' quasar (at a redshift zeta = 2.557

40 ) objects have been known for 50 years to be luminous condensations of gas in star-forming regions, b

41 Blue stragglers are anomalously luminous core hydrogen-burning stars formed through mass

42 which, the TADF unit contains a typical TADF luminous core structure, the "Host" unit exhibits effect

43 The subclass type IIn supernovae are luminous core-collapse explosions of massive stars and,

44 idize ortho-phenylenediamine (OPD) to create luminous DAP.

45 rity to the luciferin-binding protein of the luminous dinoflagellate Lingulodinium polyedrum, encoded

46 three-domain luciferases found in all other luminous dinoflagellates studied.

47 in the atmospheres of brown dwarfs and self-luminous, directly imaged exoplanets(5).

48 larly viewed either a 5-minute or a 1 degree luminous disk reflected from a horizontally oscillating

49 ions up to 3 h, whereas extended use of self-luminous displays in the home prior to sleep can.

50 etween the growth of massive black holes and luminous dusty galaxies.

51 as been revolutionized by the discovery that luminous, dusty starburst galaxies were 1,000 times more

52 h an external quantum efficiency of 23.3%, a luminous efficacy of 33.4 lm W(-1), and a luminance of a

53 ry color-rendering index (up to 93) and high luminous efficacy of radiation (268-318 lm.W(-1)) are ob

54 les could become a light source that reaches luminous efficiencies ( approximately 40%) surpassing ex

55 ximum luminance >/=10 000 cd m(-2) , maximum luminous efficiency </=50 cd A(-1) , and maximum luminou

56 monochromatic spectral lights that optimizes luminous efficiency and color gamut.

57 hereby enhances both operating stability and luminous efficiency based on its retardation effect in r

58 To obtain the maximum luminous efficiency from an organic material, it is nece

59 nverted polymer light-emitting diodes have a luminous efficiency of 61.6 cd A(-1) and an external qua

60 Sprites are large, luminous electrical discharges in the upper atmosphere c

61 essing the synchronous formation of the most luminous elliptical galaxies found today at the centres

62 ) at the centers of galaxies actively powers luminous emission, but most MBHs are considered dormant.

63 llenging sources to explain are those at the luminous end of the range (more than 10(40) ergs per sec

64 e, collectively experiencing their bodies as luminous energetic essences with diffuse spatial boundar

65 Optical observations of transient luminous events and remote-sensing of the lower ionosphe

66 These long-lived, ultraviolet-luminous events can be observed out to redshifts z > 4.

67 y last for tens of seconds, and are the most luminous events in the universe.

68 Gamma-ray bursts (GRBs) are short-lived, luminous explosions at cosmological distances, thought t

69 In recent years, certain luminous extragalactic optical transients have been obse

70 rent powering mechanism from the most common luminous extragalactic transients (supernovae), whose ti

71 for on-axis jetted TDEs on the basis of the luminous, fast-fading red component, thus providing a me

72 Recently, a large and luminous filament, consistent with such a cold accretion

73 that the outflow is not associated with the luminous flares in the data.

74 e interferometry reveal a rich morphology of luminous flat-spectrum radio sources.

75 cesses that determine the critical scales of luminous galaxies and the generation of their morphology

76 But at redshifts z > 5 even the most luminous galaxies appear faint; the interpretation of lo

77 This demonstrates that very luminous galaxies are quite rare 700 Myr after the Big B

78 In addition, the discovery of many luminous galaxies at Cosmic Dawn (z > 10) has suggested

79 servations have provided large samples of UV luminous galaxies at redshift (z) greater than 6 (refs.

80 ntinuum emission as companions to typical UV-luminous galaxies at the same redshift.

81 ectrograph spectroscopic confirmation of two luminous galaxies at z = 14.32-0.20+0.08 and z = 13.90 +

82 erse is just too young to have built up many luminous galaxies at z approximately 7-8 by the hierarch

83 studies have found that the oldest and most luminous galaxies in the early Universe are surprisingly

84 ntinuum emission, showing that the excess of luminous galaxies in the early Universe cannot be entire

85 tal Sky Survey, and they are among the least luminous galaxies in the known Universe.

86 t 1,000 times greater than that of similarly luminous galaxies in the present-day Universe, so they r

87 erse and b is a measure of the 'bias' of the luminous galaxies in the survey.

88 emove 100% of the atomic hydrogen content of luminous galaxies like the Milky Way within 100 million

89 d to address the existence of such large and luminous galaxies so early in cosmic history.

90 emitted in the early Universe came from very luminous galaxies that are largely hidden at optical wav

91 This discovery proves that luminous galaxies were already in place 300 million year

92 for the early, rapid formation of remarkably luminous galaxies while also highlighting the necessity

93 roscopy that confirms redshifts for two very luminous galaxies with z > 11, and also demonstrates tha

94 es have been limited to the largest and most luminous galaxies, which may have fundamentally differen

95 redshift z > 1; >8 billion light years away) luminous galaxies.

96 axies, ASASSN-15lh appears to be hosted by a luminous galaxy (MK approximately -25.5) with little sta

97 position 4 kiloparsecs from the center of a luminous galaxy at redshift 0.3214.

98 NIRSpec spectrum of GN-z11, an exceptionally luminous galaxy at z = 10.6, revealing the detection of

99 t grains in a strongly lensed, intrinsically luminous galaxy that is forming stars at a rate more tha

100 Uhuru and OSO-7 revealed highly luminous (> 10(36) ergs(-1)) x-ray sources in globular c

101 only 0.156 arcseconds (2.3 au) from the more luminous (> 120 times brighter) star AB Doradus A.

102 North Star is a luminous, gut-honest reflection by a pediatric oncologis

103 II in time-resolved UV spectroscopy during a luminous hard state, which we interpret as a warm, moder

104 right galaxies at high redshift are the most luminous, heavily star-forming galaxies in the Universe

105 past decade have discovered a population of luminous, high-redshift, dusty starburst galaxies.

106 cal scales of about 400 kpc around the hyper-luminous hot dust-obscured galaxy W0410-0913, at redshif

107 identified with the rare population of hyper-luminous, hot dust-obscured galaxies.

108 The host galaxy is more luminous in dust emission than any other known object at

109 ift z approximately 1), GRB 980425 was under-luminous in gamma-rays by three orders of magnitude.

110 dicate that the background objects are ultra-luminous infrared galaxies, powered by extreme bursts of

111 relationship between Stx2 concentrations and luminous intensity of GFP, imaged by the CCD camera (R(2

112 ht and dark, current responses to changes in luminous intensity, and electrically evoked postsynaptic

113 Here, we present a high luminous-intensity photobleacher that is based on rigoro

114 , can be tapped, thereby producing even more luminous jets powered by the interaction of the black ho

115 Luminous living things are widespread and access diverse

116 CVs are both, in part, overabundant like the luminous LMXBs.

117 the autoinducers of luciferase synthesis in luminous marine bacteria as well as of pathogenesis func

118 ontrol quorum sensing in the closely related luminous marine bacterium Vibrio harveyi.

119 companions to be engulfed, possibly powering luminous mass ejections from the host star(3-5).

120 ture of dark matter remains mysterious, with luminous material accounting for at most approximately 2

121 % is inferred by its gravitational effect on luminous material.

122 f bacteria by attracting fish to consume the luminous material.

123 -performance turn-on sensing for Ln-MOFs and luminous materials driven by other metal chromophores.

124 ec (kpc); Ho = 50 km.sec-1.megaparsec-1] the luminous matter constitutes only 1% of the closure densi

125 past 20 years has convinced astronomers that luminous matter in a spiral galaxy constitutes no more t

126 The interplay between dark and luminous matter in dense cosmic environments, such as ga

127 ore than 4 x 10(11) solar masses of dark and luminous matter in this region, consistent with that exp

128 gravitational influence on the appearance of luminous matter.

129 ios and unphysical misalignments of dark and luminous matter.

130 Otherwise Carina, the eighth most luminous Milky Way dwarf, would be expected to inhabit a

131 Quasars are the most luminous non-transient objects known and as a result the

132 Its position on the sky is near a luminous, non-star-forming elliptical galaxy at a redshi

133 gravity, which may explain why the windy and luminous O stars have not yet blown away those gases.

134 ere we report observations of a far-infrared-luminous object at redshift 6.900 (less than 800 million

135 ith the former being the second most distant luminous object ever observed.

136 ightest cluster galaxies, which are the most luminous objects emitting stellar light, some 9 billion

137 uminous infrared galaxies are among the most luminous objects in the local Universe and are thought t

138 ar-powered eruptions thousands of times more luminous occur in classical novae, accompanied by signif

139 ue can be used to generate holograms of self-luminous or remote objects using a local reference, thus

140 we report the first complete life cycle of a luminous ostracod (Vargula tsujii Kornicker & Baker, 197

141 Bringing a luminous ostracod into laboratory culture sets the stage

142 smological model the bulk of the mass of the luminous parts of the large galaxies likely had been ass

143 ay to broad use of these advanced miniature "luminous pearls" in photonics and biophotonics.

144 The lack of both a comparably luminous persistent radio counterpart and a high Faraday

145 ere we report the detection of a third, less luminous persistent radio source associated with the rep

146 orts have appeared about unusual large-scale luminous phenomena above thunderclouds and, more than 80

147 s in spectacular starbursts, which should be luminous phenomena when observed at submillimetre wavele

148 que light curve of which transitioned into a luminous plateau within days.

149 lly modulated excitation source (under equal luminous power conditions).

150 nous efficiency </=50 cd A(-1) , and maximum luminous power efficiency </=55 lm W(-1) are demonstrate

151 a brightness that exceeds 300 cd/m(2) and a luminous power efficiency that exceeds 10 Lm/W at just 3

152 driven image synthesis method, we found that luminous power patterns (i.e., images) can be applied to

153 over more than 13 megaparsecs and contains a luminous quasar as well as a system rich in molecular ga

154 asurement of the mass of the black hole in a luminous quasar at a redshift of 2, with a look back in

155 ed gas in the broadband x-ray spectra of the luminous quasar PDS 456.

156 ely massive galaxies that can be observed as luminous quasars and starbursts.

157 st that GNz7q is an antecedent to unobscured luminous quasars at later epochs.

158 tarbursts that then transition to unobscured luminous quasars by expelling gas and dust(5).

159 challenge(1,2) since it was discovered that luminous quasars existed only 700 million years after th

160 Optically luminous quasars host the most prodigious accreting blac

161 times that of the Sun have been detected in luminous quasars less than one billion years after the B

162 nk between early massive black holes and the luminous quasars observed at z = 6.

163 ing emergence of supermassive BHs that power luminous quasars so soon after the Big Bang.

164 stellar-mass BH seeds into the supermassive luminous quasars that are observed when the universe is

165 massive black holes; the detection of highly luminous quasars with redshifts greater than z = 6 sugge

166 een black hole seeds(6) and one of the first luminous quasars(7).

167 The most luminous quasars, however, are not confined to such high

168 The control of luminous radiation has extremely important implications

169 Here we report the discovery of luminous radio emission from the seemingly ordinary type

170 signals bear similarities with the much less luminous radio emission generated by pulsars within our

171 d covering the first month of evolution of a luminous radio transient associated with Swift J164449.3

172 We report a luminous radio transient, VT J121001+495647, found in th

173 progenitor systems, allowing us to rule out luminous red giants and almost all helium stars as the m

174 paper uses pre-explosion images to rule out luminous red giants and most helium stars as companions

175 ery of ionized gas nebulae surrounding three luminous red quasars at z ~ 0.4 from Gemini integral fie

176 During October 2019 and March 2020, the luminous red supergiant Betelgeuse demonstrated an unusu

177 o a larger clade that includes them plus non-luminous relatives.

178 rates of species accumulation than their non-luminous relatives.

179 y timescales, so that most blazars appear as luminous sources characterized by noticeable and fast ch

180 as no instance in which the lux genes of one luminous species had replaced the lux genes of another l

181 strikingly different from that of the seven luminous species previously characterized, all of which

182 pecies had replaced the lux genes of another luminous species.

183 Archival images of the field do not show a luminous star at that position with an upper limit in th

184 5 micrometers) were detected in the peculiar luminous star MWC 349A from the Kuiper Airborne Observat

185 by star formation within the cores of highly luminous starburst galaxies in the distant Universe.

186 cates that those orbiting very close to more-luminous stars might be evaporatively destroyed or that

187 e sustained hydrogen fusion that powers self-luminous stars--are born hot and slowly cool as they age

188 During the rising stage, one or more luminous steps are revealed at 32-40 km, before a contin

189 idus, respectively; (iii) the lux genes of a luminous strain of Photobacterium damselae, BT-6, were c

190 at of gene replacement, we constructed a non-luminous strain of V. fischeri (delta luxA::erm).

191 follows: (i) the lux genes of the only known luminous strain of Vibrio vulnificus, VVL1 (ATCC 43382),

192 of Vibrio harveyi; (ii) the lux genes of two luminous strains of Vibrio chagasii, 21N-12 and SB-52, w

193 Three hundred three luminous strains, most of which were recently isolated f

194 The extremely luminous supernova SN 2006gy challenges the traditional

195 h (SN 2015L), which we interpret as the most luminous supernova yet found.

196 es characteristic of the hydrogen-poor super-luminous supernovae (SLSNe-I), whose energy sources and

197 Super-luminous supernovae that radiate more than 10(44) ergs p

198 eport observations of two slow-to-fade super-luminous supernovae that show relatively fast rise times

199 Here we report observations of a class of luminous supernovae whose properties cannot be explained

200 pe of the continuum resembles those of super-luminous supernovae, but extends further down into the r

201 losely resemble typical fast-declining super-luminous supernovae, which are not powered by radioactiv

202 volves much more rapidly than those of super-luminous supernovae.

203 o been proposed as the explanation for super-luminous supernovae.

204 we report the draft genome of the uncultured luminous symbiont of an anomalopid flashlight fish, 'Can

205 flare from SGR 1806-20, which was much more luminous than any previous transient event observed in o

206 milarity to 'red transients', which are more luminous than classical novae and thought to be the resu

207 frozen planet because the young Sun was less luminous than it is today.

208 fs. (5,6)), which is at least 2-6 times less luminous than model predictions given its dynamical mass

209 asses and therefore more than 400 times less luminous than the Sun.

210 round the same time), but typically are more luminous than the turn-off stars and therefore long ago

211 This supernova is more than three times more luminous than type Ic supernovae associated with long-du

212 rs in galaxies that are >/= 10(6) times more luminous than typical galactic maser sources.

213 enables the two-dimensional imaging of self-luminous (that is, incoherent) objects with high through

214 Because these stars are very luminous, they can be observed in other galaxies, and th

215 tive cooling automatically while maintaining luminous transparency and near-infrared (NIR) modulation

216 uasi-spherical outflows similar in size from luminous type 1 and type 2 quasars at concordant redshif

217 Here we report a luminous ultraviolet-optical flare from the nuclear regi

218 xamples are dust-obscured galaxies which are luminous when observed at sub-millimetre wavelengths and

219 ime of the explosion, marked by an extremely luminous X-ray outburst.

220 Young, low-mass stars are luminous X-ray sources whose powerful X-ray flares may e

221 This region contains luminous young stars and protostars but, like most star-

222 Radiation pressure and winds from luminous young stars should disperse the star-forming ga