ライフサイエンスコーパス: cosmic

1 han 37 000 variants from sources of ClinVar, Cosmic, 1000 Genomes, ExAC, IntOGen, cBioPortal and IntA

2 data-download systems, new functionality in COSMIC-3D allows exploration of mutations within three-d

3 , silicon, iron, and calcium) are present in cosmic abundances, with only small grain-to-grain variat

4 ese 'standardisable candles' indeed indicate cosmic acceleration.

5 d other theories that reproduce the observed cosmic acceleration.

6 at a redshift of z = 9.6 +/- 0.2 (that is, a cosmic age of 490 +/- 15 million years, or 3.6 per cent

7 tribution of the first stars at redshift 20 (cosmic age of around 180 million years), incorporating a

8 laxies (where the bulk of stars formed) at a cosmic age of less than about 500 million years (z less,

9 galaxies seem to be abundant at such a young cosmic age, suggesting that they may be the dominant sou

10 In addition, COSMIC also details more than six million noncoding muta

11 The resistance of melanized fungi to cosmic and terrestrial ionizing radiation suggests that

12 e occupationally exposed to higher levels of cosmic and UV radiation than the general population, but

13 ns in human cancer has now been curated into COSMIC and while this is continually updated, a greater

14 he Catalogue of Somatic Mutations in Cancer (COSMIC) and Cancer Cell Line Encyclopedia (CCLE), we est

15 he Catalogue of Somatic Mutations in Cancer (COSMIC) and the spatial information in the Protein Data

16 m OMIM, 587 873 cancer-related variants from COSMIC, and 1 484 045 SNPs from dbSNP.

17 ariant data from four databases: ARDB, HGMD, Cosmic, and 1,000 genome.

18 ackground typically consists of terrestrial, cosmic, and cosmogenic radiation that may cause false po

19 sphere; they are inconsistent with volcanic, cosmic, anthropogenic, lightning, or authigenic sources.

20 ational signatures, one of which matches the COSMIC APOBEC-associated signature 2.

21 on today, will demonstrate the presence of a cosmic background of hard X-rays at that early time.

22 ost-galaxy environments(11), and we derive a cosmic baryon density of [Formula: see text] (95 per cen

23 tain fewer baryons (gas plus stars) than the cosmic baryon fraction.

24 theories and are given by the areas of dual cosmic branes.

25 ered by GWAS Catalog, PopHumanScan, OMIM and COSMIC, CADD being another major newcomer.

26 Among the mutated genes were almost 200 COSMIC Cancer Gene Census genes, many of which were recu

27 ong the ~700 cancer-related sequences in the COSMIC Cancer Gene Census, 178 sequences are predicted t

28 r the full repertoire of 715 proteins in the COSMIC Cancer Gene Census.

29 ely 470 million years ago one of the largest cosmic catastrophes occurred in our solar system since t

30 om the Cancer Cell Line Encyclopedia and the COSMIC Cell Lines Project to three renal cancer subtypes

31 o produce ionization." Ionizing radiation in cosmic chemistry includes high-energy particles (e.g., c

32 compression occurs, such as an impact from a cosmic cloud or other galaxy.

33 tifies 15% redundant indels in dbSNP, 29% in COSMIC coding, and 13% in COSMIC noncoding datasets acro

34 ore redundant indels in dbSNP; 2,118 more in COSMIC coding, and 553 more in COSMIC noncoding indel da

35 Currently (v43, August 2009), COSMIC contains details of 1.5-million experiments perfo

36 In addition to coding mutations, COSMIC covers all the genetic mechanisms by which somati

37 (n = 29) versus without (n = 38) detectable COSMIC ctDNA mutations at baseline was 407 days versus 8

38 COSMIC curates comprehensive information on somatic muta

39 ble for ionization of the Universe after the cosmic 'Dark Ages', when the baryonic matter was neutral

40 he Catalogue Of Somatic Mutations In Cancer (COSMIC) data sets.

41 All information from the COSMIC database is available freely on the COSMIC websit

42 ine calls and comparison of somatic calls to COSMIC database variants.

43 on for approximately 10 000 mutations in the COSMIC database, the method does well in assigning highe

44 -related mutation positions annotated in the COSMIC database.

45 tely 2% of RCC patient samples in the Sanger COSMIC database.

46 Catalogue of Somatic Mutations in Cancer (COSMIC) database ctDNA mutations were detected in 65% (4

47 ion years after the Big Bang, initiating the cosmic dawn.

48 esponding to the largest fluctuations in the cosmic density field.

49 ination, provide a direct measurement of the cosmic density of ionized baryons in the intergalactic m

50 ult has become the best anchor point for the cosmic distance scale(4,5).

51 inental crust (approximately 1.3) and mantle/cosmic dust (approximately 0.13).

52 In situ data from the Cosmic Dust Analyzer on board the Cassini spacecraft rev

53 This review discusses the magnitude of the cosmic dust input into the earth's atmosphere, and the r

54 Second, cosmic dust particles enter the atmosphere at high speed

55 s have terrestrial origins but also occur as cosmic dust particles.

56 , soil erosion, eolian dust, sea-salt spray, cosmic dust, volcanic emissions, and for helium, hydrody

57 c, and cosmic materials, yet consistent with cosmic ejecta, supporting the hypothesis of extraterrest

58 in agreement with the accumulation rates of cosmic-enriched elements (Ir, Pt, Os and super-paramagne

59 d Strelka obtained the largest proportion of COSMIC entries as well as the lowest rate of dbSNP prese

60 ay between dark and luminous matter in dense cosmic environments, such as galaxy clusters, is studied

61 cured to unobscured quasars as a function of cosmic epoch up to z congruent with 3 and show that a si

62 The relevance of this scenario at early cosmic epochs is not yet established.

63 scovered hundreds of galaxies at these early cosmic epochs, but their star-formation rates are more t

64 ve formed their dense stellar cores in early cosmic epochs.

65 of the IMF in other galaxies and at earlier cosmic epochs.

66 able studies of the Universe at the earliest cosmic epochs.

67 e of evidence supports the hypothesis that a cosmic event occurred at Abu Hureyra ~12,800 years ago,

68 dings do not preclude a terminal Pleistocene cosmic event.

69 emanates from a variety of sources, such as cosmic events, particle accelerators, nuclear reactors a

70 e constraint on the primordial abundance and cosmic evolution of lithium that is not susceptible to t

71 the Big Bang, and traces 13 billion years of cosmic evolution with 12 billion resolution elements in

72 city is the line-of-sight departure from the cosmic expansion and arises from gravitational perturbat

73 alaxies are inward after removal of the mean cosmic expansion and long range flows.

74 d arrivals of the supernova images probe the cosmic expansion rate, as well as the distribution of ma

75 rnovae good 'standard candles' for measuring cosmic expansion, but a correction must be applied to ac

76 be derived from the subtraction of the mean cosmic expansion, the product of distance times the Hubb

77 al lens could be used to measure the rate of cosmic expansion.

78 This high-porosity asteroid may link cosmic fluffy dust to dense celestial bodies(10).

79 ess, having a mutational status according to COSMIC, followed by the construction of PCa Interactome

80 ate that the highest-mass systems retain the cosmic fraction of baryons, a natural consequence of whi

81 tion gamma-ray bursts are intense flashes of cosmic gamma-rays, lasting less than about two seconds,

82 pha emission, discovered during a survey for cosmic gas fluorescently illuminated by bright quasars a

83 This is based on the assumption that the cosmic gas was heated by stellar remnants-particularly X

84 are known oncogenes, tumor suppressor genes, COSMIC genes, and/or transcription factors.

85 tations such as the 1000 Genomes project and COSMIC give an opportunity to investigate general princi

86 he Catalogue of Somatic Mutations in Cancer (COSMIC), GraphPAC identifies new mutational clusters in

87 mic features has become a significant focus; COSMIC has begun curating full-genome resequencing exper

88 C risk prediction after exposure to high-LET cosmic heavy ion radiation exposure is hindered due to s

89 levated natriuretic peptides enrolled in the COSMIC-HF trial (Chronic Oral Study of Myosin Activation

90 ions in the total production of photons over cosmic history and may contain faint, extended component

91 based and space-borne telescopes have probed cosmic history from the present day to a time when the U

92 s quickly, within the first billion years of cosmic history in a short, extreme starburst.

93 their centres, are the relics of a period in cosmic history when galaxies formed stars at remarkable

94 n tandem with their host galaxies throughout cosmic history, starting from the earliest times.

95 ast 20 years have revolutionized our view of cosmic history, transforming our understanding of how th

96 Star-forming galaxies trace cosmic history.

97 y galaxies probably induced a major event in cosmic history: the reionization of intergalactic hydrog

98 ically evaluate our current understanding of cosmic ice energetic processing which likely leads to th

99 Energetic processing of cosmic ices via photochemistry and radiation chemistry i

100 somatic mutation-ceRNA events from TCGA and COSMIC; (iii) 112 674 CNV-ceRNA events from TCGA; (iv) 6

101 YDB objects with melt products from a known cosmic impact (Meteor Crater, Arizona) and from the 1945

102 ounger Dryas impact hypothesis posits that a cosmic impact across much of the Northern Hemisphere dep

103 en invigorated by a hypothesis implicating a cosmic impact at the Allerod-Younger Dryas boundary or Y

104 raters, and its presence strongly supports a cosmic impact event, further strengthened by its co-occu

105 act strewnfields and consistent with a major cosmic impact event.

106 mpelling evidence to accept the claim that a cosmic impact occurred approximately 12,800 y ago and ca

107 episode known as the Younger Dryas (YD) is a cosmic impact or airburst at the YD boundary (YDB) that

108 egafaunal extinction possibly triggered by a cosmic impact over North America at approximately 12,900

109 's typical surficial processes but common to cosmic impacts.

110 s, and magnetic microspherules attributed to cosmic impacts/airbursts.

111 n Database, recurrent somatic variation from COSMIC in the context of different cancers, as well as d

112 omic information recently updated to GRCh37, COSMIC integrates many diverse types of mutation informa

113 0(6) non-synonymous mutations extracted from COSMIC, involving ~8000 genome-wide screened samples acr

114 e of mutations in cancer, the information in COSMIC is curated by expert scientists, primarily by scr

115 bers of genomic rearrangements in cancer and COSMIC is now displaying details of these analyses also.

116 COSMIC is primarily hand-curated, ensuring quality, accu

117 he catalogue of Somatic Mutations in Cancer (COSMIC) is the largest public resource for information o

118 Here we report on experiments from the Cosmics Leaving Outdoor Droplets chamber at the European

119 ticle formation experiments performed at the Cosmics Leaving Outdoor Droplets chamber at the European

120 ow, in experiments performed with the CLOUD (Cosmics Leaving Outdoor Droplets) chamber at CERN, that

121 ganic compounds conducted in the CERN CLOUD (Cosmics Leaving Outdoor Droplets) chamber.

122 we study nano-particle growth in the CLOUD (Cosmics Leaving OUtdoors Droplets) chamber, starting fro

123 The microspherules were explained as either cosmic material ablation or terrestrial ejecta from a hy

124 ith anthropogenic, volcanic, authigenic, and cosmic materials, yet consistent with cosmic ejecta, sup

125 ich are expected to be representative of the cosmic matter content of the universe (baryons and dark

126 The apparent baryon fraction exceeds the cosmic mean at larger radii, suggesting a clumpy distrib

127 an a millikelvin) that marks the rise of the cosmic mean gas temperature above the microwave backgrou

128 c approach to TDA modeling in an analysis of cosmic microwave background (CMB) nonhomogeneity.

129 around these, and through its imprint on the Cosmic Microwave Background (CMB).

130 t is consistent with values derived from the cosmic microwave background and from Big Bang nucleosynt

131 ons, which manifest in the anisotropy of the cosmic microwave background and the large-scale correlat

132 -ray binaries-to temperatures well above the cosmic microwave background at that time (about 30 kelvi

133 Observations of the cosmic microwave background indicate that baryons accoun

134 a vital role across a range of systems: from cosmic microwave background polarization to superconduct

135 lent agreement with a recent analysis of the cosmic microwave background(7).

136 teristic imprints in the polarization of the cosmic microwave background, or later with direct space-

137 the universe, gravitational lensing, and the cosmic microwave background.

138 [Formula: see text]) model as applied to the cosmic microwave background.

139 COSMIC mutational signature 18, previously associated wi

140 This indicated that COSMIC mutational signature 24, previously hypothesized

141 Unresolved anisotropies of the cosmic near-infrared background radiation are expected t

142 s in dbSNP, 29% in COSMIC coding, and 13% in COSMIC noncoding datasets across all human chromosomes,

143 2,118 more in COSMIC coding, and 553 more in COSMIC noncoding indel dataset in addition to the ones r

144 COSMIC now details the genetics of drug resistance, nove

145 The cosmic optical background is an important observable tha

146 The cosmic origin of elements heavier than iron has long bee

147 vey of the outskirts of 42 galaxies with the Cosmic Origins Spectrograph onboard the Hubble Space Tel

148 s extensive application to a wide variety of cosmic phenomena.

149 he Catalogue of Somatic Mutations in Cancer (COSMIC), QuartPAC is able to identify clusters which are

150 ure higher levels of radiation from galactic cosmic radiation (GCR) and the possibility of a large so

151 Cosmic radiation also disrupted synaptic integrity and i

152 Understanding the temporal variation of cosmic radiation and solar activity during the Holocene

153 ue opportunity to reconstruct the history of cosmic radiation and solar activity over many millennia.

154 Cosmic radiation contains protons, helium nuclei and hig

155 Extreme cosmic radiation events occurred in the years 774/5 and

156 Rodents exposed to cosmic radiation exhibit persistent hippocampal and cort

157 Of particular concern is the potential for cosmic radiation exposure to compromise critical decisio

158 ffects of heavy ionizing particles and other cosmic radiation need to be considered.

159 The new cosmic radiation record enables us to derive total solar

160 ion will result in an inevitable exposure to cosmic radiation that has been shown to cause cognitive

161 lly resolved patterns of (14)C, modulated by cosmic radiation, between 1700 and 1480 BC.

162 e and male astronauts, including exposure to cosmic radiation, microgravity, increased gravity (hyper

163 iomarker preservation against destruction by cosmic radiation.

164 he effects of microgravity, hypergravity and cosmic radiation.

165 enous thromboembolism and long-haul flights, cosmic-radiation exposure, jet lag, and cabin-air qualit

166 nmental radiation background, and monitoring cosmic radiations.

167 ang nucleosynthesis (BBN) depend only on the cosmic ratio of baryons to photons, a quantity inferred

168 s linked with either ultraviolet or galactic cosmic ray (GCR) effects on atmospheric particles.

169 er risk is an important concern for galactic cosmic ray (GCR) exposures, which consist of a wide-ener

170 agnetic field causes an increase in galactic cosmic ray (GCR) flux.

171 er began making detailed measurements of the cosmic ray and energetic particle radiation environment

172 he puzzle of the origin of ultra high energy cosmic ray electrons.

173 The presented (36)Cl Cosmic Ray Exposure ages demonstrate that the cliff over

174 We determined interstellar cosmic ray exposure ages of 40 large presolar silicon ca

175 The small intensity gradient of Galactic cosmic ray helium indicates that either the gradient is

176 hat for the processes studied, variations in cosmic ray intensity do not appreciably affect climate t

177 liosheath or the local interstellar Galactic cosmic ray intensity is lower than expected.

178 ned inside the heliosphere, the intensity of cosmic ray nuclei from outside the heliosphere abruptly

179 For data pretreatment, we developed a unique cosmic ray removal method and used an automated baseline

180 e large difference in nuclear recoil loss of cosmic ray spallation products (3)He and (21)Ne enabled

181 ltogether in looking for isolated regions of cosmic-ray acceleration.

182 of tens to hundreds of megaelectronvolts) is cosmic-ray albedo neutron decay (CRAND).

183 a were obtained by exploiting the negligible cosmic-ray background deep underground at the Laboratory

184 ent was a major contributor to the increased cosmic-ray density in the Galactic Centre, and is in tur

185 The Pierre Auger Observatory is the largest cosmic-ray detector on Earth, and as such is beginning t

186 Herein, the formation of glyoxylic acid via cosmic-ray driven, non-equilibrium chemistry in polar in

187 volts per nucleon and an increasing galactic cosmic-ray electron intensity down to ~10 x 10(6) electr

188 Here we consider neutrino and cosmic-ray emission from multiple emission regions since

189 The cosmic-ray exposure age of Ost 65 shows that it may be a

190 This interpretation relies mainly on cosmic-ray exposure dating of glacial deposits.

191 paper we review the observables generated by cosmic-ray interactions with the interstellar medium, fo

192 rge amounts of warm molecular gas(5), a high cosmic-ray ionization rate(6), unusual gas chemistry, en

193 The origin of Galactic cosmic-ray ions has remained an enigma for almost a cent

194 sequent enrichment of the gas by stellar and cosmic-ray nucleosynthesis.

195 anisotropy maps of ground-based high-energy cosmic-ray observatories (Milagro, Asgamma, and IceCube)

196 The Galaxy is filled with cosmic-ray particles, mostly protons with kinetic energi

197 The unexpectedly high flux of cosmic-ray positrons detected at Earth may originate fro

198 Cosmic-ray produced radionuclides, such as (10)Be and (1

199 of stellar evolution, binary formation, and cosmic-ray production in the Galactic Centre.

200 ources, dark matter, or unknown processes of cosmic-ray secondary production.

201 After consideration of cosmic-ray spallation and degassing processes, our resul

202 nyl alcohol (C2H3OH) act as key tracers of a cosmic-ray-driven nonequilibrium chemistry leading to co

203 Cosmic-ray-produced (3)He, (21)Ne, and (36)Ar yield conc

204 700 years ago), based on new measurements of cosmic-ray-produced beryllium and aluminium isotopes ((1

205 iving interstellar chemistry via ionization, cosmic rays also interact with the interstellar medium i

206 on of high-energy (tera-electron volts, TeV) cosmic rays and diffusive propagation from supernova sou

207 ssess the damage caused to such materials by cosmic rays and neutrons, which pose a variety of hazard

208 nsoon connection is dominated most likely by cosmic rays and oceanic circulation (both associated to

209 orbed dose and dose equivalent from galactic cosmic rays and solar energetic particles on the martian

210 Cosmic rays are charged particles arriving at the Earth

211 Cosmic rays are the highest-energy particles found in na

212 rse, demands a mechanism for ionization, and cosmic rays are the ideal candidate as they can operate

213 at hundreds to thousands of eV and galactic cosmic rays at tens of TeV has wide-ranging implications

214 the prime candidates to produce the observed cosmic rays at the highest energies.

215 ter while simultaneously being shielded from cosmic rays by overlying ice.

216 istance does not greatly exceed the distance cosmic rays can diffuse over this time, 1 kiloparsec.

217 expectations, the extragalactic component of cosmic rays contributes substantially to the total flux

218 from environmental radioactive materials and cosmic rays contributes to this observed difference.

219 We report the spectra of galactic cosmic rays down to ~3 x 10(6) electron volts per nucleo

220 he detection of supernova-produced (60)Fe in cosmic rays implies that the time required for accelerat

221 It provides an example to study the youth of cosmic rays in a superbubble environment before they mer

222 We find that ions from Galactic cosmic rays increase the nucleation rate by one to two o

223 Cosmic rays initiate air showers--cascades of secondary

224 The origin of Galactic cosmic rays is a century-long puzzle.

225 Radio detection of cosmic rays is a rapidly developing technique for determ

226 y support the idea that the bulk of galactic cosmic rays is accelerated in such remnants by a Fermi m

227 comes from accelerators capable of producing cosmic rays of these energies.

228 on that could inflict damage by accelerating cosmic rays that can deliver ionizing radiation for up t

229 50-parsec-wide cocoon of freshly accelerated cosmic rays that flood the cavities carved by the stella

230 In this process, cosmic rays that reach the upper atmosphere interact wit

231 Iron-60 ((60)Fe) is a radioactive isotope in cosmic rays that serves as a clock to infer an upper lim

232 va remnants (SNRs) hint that they accelerate cosmic rays to energies close to ~10(15) electron volts.

233 Second, beryllium-7 is a product of cosmic rays which are themselves directly linked to sola

234 uare centimetre for air showers initiated by cosmic rays with energies of 10(17)-10(17.5) electronvol

235 Measurements of the mass composition of cosmic rays with energies of 10(17)-10(18) electronvolts

236 g nucleosynthesis, interactions of energetic cosmic rays with interstellar matter, evolved low-mass s

237 mistry includes high-energy particles (e.g., cosmic rays) and high-energy photons (e.g., extreme-UV).

238 August 2012, while those of galactic origin (cosmic rays) increased by 9.3% at the same time.

239 i's classic result on the energy spectrum of cosmic rays, with the universal exponent -2, which is in

240 through observations of gamma-ray photons or cosmic rays.

241 les us to determine the mass spectrum of the cosmic rays: we find a mixed composition, with a light-m

242 s have had an important role in the epoch of cosmic reionization and the chemical evolution of early

243 f the interstellar medium in galaxies during cosmic reionization are important for understanding the

244 approximately 2), galaxies vigorously fed by cosmic reservoirs are dominated by gas and contain massi

245 Examination of COSMIC's data is primarily web-driven, focused on provid

246 In parallel with COSMIC's deep and broad variant coverage, the Cancer Gen

247 s pointed towards APOBEC deaminase activity (COSMIC signature 2) and DNA mismatch repair (COSMIC sign

248 n the Polzeta translesion polymerase, yields COSMIC signature 3 observed in BRCA1/BRCA2-mutant breast

249 o common treatments, but the contribution of COSMIC signature 3 to base substitutions, or a combined

250 se substitution signature that is similar to COSMIC signature 3.

251 Presence of this class of mutation, termed COSMIC signature 4, is responsible for the increased bur

252 tion, we show that another mutation pattern, COSMIC signature 5, is positively associated with age in

253 COSMIC signature 2) and DNA mismatch repair (COSMIC signature 6).

254 e highly enriched for ClinVar pathogenic and COSMIC somatic missense variants (Mann-Whitney U test P

255 sponsible for the most powerful and dramatic cosmic sources.

256 z approximately 4 in terms of the density of cosmic space.

257 n otherwise typical S-type micro-porphyritic cosmic spherule containing relict olivine (Fo76-90, Cr(2

258 we show that the FeNi metal in the resulting cosmic spherules was oxidized while molten, and quench-c

259 Also for the glassy cosmic spherules, overall, there was a good match betwee

260 C-ICP-MS) for Fe isotopic analysis of glassy cosmic spherules.

261 Starburst galaxies at the peak of cosmic star formation are among the most extreme star-fo

262 When cosmic star formation history reaches a peak (at about r

263 Despite the overall downturn in cosmic star formation towards the highest redshifts, it

264 Our current knowledge of cosmic star-formation history during the first two billi

265 For example, in cosmological theories, cosmic strings may have formed knotted configurations in

266 ctors, magnetic flux tubes, liquid crystals, cosmic strings, and DNA is the phenomenon of reconnectio

267 According to the current understanding of cosmic structure formation, the precursors of the most m

268 has been remarkably successful in explaining cosmic structure over an enormous span of redshift, but

269 count the milestones in our understanding of cosmic structure; summarize its impact on astronomy, cos

270 Previous simulations of the growth of cosmic structures have broadly reproduced the 'cosmic we

271 erse, and slow down in the rate of growth of cosmic structures.

272 the dynamo excitation of magnetic fields in cosmic systems; (ii) its bearing on the existence of Eul

273 COSMIC, the Catalogue Of Somatic Mutations In Cancer is

274 COSMIC, the Catalogue of Somatic Mutations in Cancer is

275 xies during the first three billion years of cosmic time (redshift z > 4) indicate a rapid evolution

276 sive black hole with its host galaxy through cosmic time is encoded in its spin.

277 h the gravitational accretion of matter over cosmic time(1).

278 rise and fall of star formation over 95% of cosmic time, back to the current observational frontier

279 ge range in cluster radius, cluster mass and cosmic time.

280 the galaxy's properties in a brief period of cosmic time.

281 ion of extragalactic magnetic fields through cosmic times (up to microgauss levels reported in nearby

282 rophysical conditions and remain stable over cosmic timescales, giving unique insights on their exist

283 her important references such as GENCODE and COSMIC using the Google Cloud Platform.

284 lly on highly characterized drugs and genes, COSMIC v78 contains wide resistance mutation profiles ac

285 The latest release, COSMIC v86 (August 2018), includes almost 6 million codi

286 We find that the baryon fraction reaches the cosmic value near the virial radius for all groups and c

287 We queried the dbSNP and COSMIC variant databases and found numerous variants ind

288 alyses of YDB spherules suggest they are not cosmic, volcanic, authigenic, or anthropogenic in origin

289 , but reside throughout the filaments of the cosmic web (where matter density is larger than average)

290 a and constrain the net magnetization of the cosmic web along this sightline to <21 nanogauss, parall

291 challenges faced as we prepare to probe the cosmic web at new wavelengths.

292 Here we report observations of a cosmic web filament in Lyman-alpha emission, discovered

293 shocked gas streaming along filaments of the cosmic web into dark-matter halos--are important.

294 The thread-like structure of this 'cosmic web' has been traced by galaxy redshift surveys f

295 smic structures have broadly reproduced the 'cosmic web' of galaxies that we see in the Universe, but

296 rse predict that galaxies are embedded in a 'cosmic web', where most baryons reside as rarefied and h

297 ssing baryons reside in the filaments of the cosmic web.

298 oing growth of clusters from the surrounding cosmic web.

299 lean probes of the baryonic component of the cosmic web.

300 e COSMIC database is available freely on the COSMIC website.