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

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

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

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

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

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

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

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

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

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

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

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

14 maximize light production in dim strains of luminous bacteria.

15 ing resolve evolutionary relationships among luminous bacteria.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

74 Luminous living things are widespread and access diverse

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

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

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

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

79 % is inferred by its gravitational effect on luminous material.

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

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

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

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

84 gravitational influence on the appearance of luminous matter.

85 ios and unphysical misalignments of dark and luminous matter.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

104 Optically luminous quasars host the most prodigious accreting blac

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

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

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

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

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

110 The control of luminous radiation has extremely important implications

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

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

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

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

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

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

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

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

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

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

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

122 5 micrometers) were detected in the peculiar luminous star MWC 349A from the Kuiper Airborne Observat

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

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

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

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

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

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

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

130 The extremely luminous supernova SN 2006gy challenges the traditional

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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