ライフサイエンスコーパス: telescope

1 e rings in only three synthetic steps (after telescoping).

2 med using an umbilical port with a 30-degree telescope.

3 Telescope on board the Fermi Gamma-ray Space Telescope.

4 Telescope onboard the Fermi Gamma-ray Space Telescope.

5 a ring polarimeter on the robotic Liverpool Telescope.

6 this system, obtained with the Spitzer Space Telescope.

7 ly 3000-kilometer resolution with the Keck I Telescope.

8 le spectrograph on the W. M. Keck I 10-meter telescope.

9 ervations taken with the James Clerk Maxwell Telescope.

10 orial zone by Voyager 1 and the Hubble Space Telescope.

11 one (O3), was measured with the Hubble Space Telescope.

12 roved observations with the James Webb Space Telescope.

13 bserved in a C1.5 flare by the Swedish Solar Telescope.

14 at high redshifts with the James Webb Space Telescope.

15 counterparts observed with the Hubble Space Telescope.

16 ed spectrograph onboard the James Webb Space Telescope.

17 high-resolution images from the Hubble Space Telescope.

18 aging Spectrograph and the Swedish 1-m Solar Telescope.

19 Infrared Telescope Facility and the Keck-II telescope.

20 full planet rotations using the Hubble Space Telescope.

21 een more successful than NASA's Kepler space telescope.

22 including those from NASA's James Webb Space Telescope.

23 re wavelengths, obtained using the IRAM 30-m telescope.

24 ond the sensitivity limits of existing large telescopes.

25 tem (VERITAS) array of atmospheric Cherenkov telescopes.

26 vely poor spatial resolution of far-infrared telescopes.

27 merger by using a global network of 32 radio telescopes.

28 by means of differential imaging with large telescopes.

29 usters, using rotation parameters from radio telescopes.

30 y be discovered by emerging wide-field radio telescopes.

31 ional study, even with the largest available telescopes.

32 ce far too small to be resolved with today's telescopes.

33 of-detection threshold for present-day radio telescopes.

34 brightness that could be detected by future telescopes.

35 and security, medical imaging, and gamma-ray telescopes.

36 f, far too small to be resolved with current telescopes.

37 ade by remote sensing by sophisticated space telescopes.

38 ure and axial torsion of the cranium, but no telescoping.

39 bble Space Telescope (HST) and Spitzer Space Telescope(1-3).

40 ed were not possible before James Webb Space Telescope(10).

41 te intense scrutiny with the world's largest telescopes(3).

42 space observatories such as the Hubble Space Telescope(5).

43 We present Telescope, a computational software tool that provides a

44 0.245 kiloelectron volts by the Deep Survey telescope aboard the Extreme Ultraviolet Explorer.

45 mpact, from a network of citizen scientists' telescopes across the world.

46 lds, 22 examples) can be generated through a telescoped acylation/ring-expansion sequence, leading to

47 w a reduction in the size of potential space telescopes aimed at the imaging of very faint terrestria

48 A greener, telescoping alternative to the synthesis of 3,5-dialkylp

49 of Herbig-Haro 211 from the James Webb Space Telescope, an outflow from an analogue of our Sun when i

50 scans obtained in 36 adult patients with 54 telescoping anastomoses (30 right bronchus, 24 left bron

51 r collections can be a normal feature of the telescoping anastomosis and should not necessarily be in

52 Our 1.8-m Vatican Advanced Technology Telescope and charge-coupled device camera observations

53 high-sensitivity Low Frequency Array (LOFAR) telescope and establish an upper limit on the kinetic mi

54 The development of a high-efficiency telescope and follow-up optics crucially improved the li

55 posed solutions--a coronagraph internal to a telescope and nulling interferometry from formation-flyi

56 Images of the cosmos from the Hubble Space Telescope and the James Webb Space Telescope have awed t

57 a value that differs from both Hubble Space Telescope and Voyager values.

58 nt near-infrared spectra from the Very Large Telescope and W. M. Keck Observatories that reveal an en

59 logy, mostly driven by observations from new telescopes and detectors.

60 Numerous telescopes and techniques have been used to find and stu

61 l efforts, fueled by new large, ground-based telescopes and the Hubble Space Telescope, combined with

62 rs after Galileo's discoveries, ground-based telescopes and theoretical modelling furnished everythin

63 density of free electrons between source and telescope) and sky position as the original detections.

64 ts from the Kepler mission, the Hubble Space Telescope, and large ground-based telescopes opens a new

65 to their host stars with larger ground-based telescopes, and also allow a reduction in the size of po

66 days of integration time with largest space telescopes, and thus are very challenging for current in

67 ectral resolution spectroscopy for exoplanet telescope application.

68 Published data from X-ray telescopes are not adequate to reveal the fluctuations i

69 sed to establish the extent to which bioptic telescopes are used by and meet the driving needs of peo

70 The data, obtained with the Hubble Space Telescope, are sufficiently precise to detect absorption

71 tions by Swift and the Nuclear Spectroscopic Telescope Array of the EM counterpart of the binary neut

72 V) with the Very Energetic Radiation Imaging Telescope Array System (VERITAS) array of atmospheric Ch

73 renkov, and very energetic radiation imaging telescope array, combined with the future Cherenkov tele

74 pe array, combined with the future Cherenkov telescope array, will provide important complementarity

75 The majority (74%) rated the bioptic telescope as very helpful, and almost all (90%) would co

76 used the giant Arecibo and Green Bank radio telescopes as a radar to probe Titan's hidden surface.

77 hromospheric images from the 1.6-m New Solar Telescope at Big Bear Solar Observatory, supplemented by

78 vations of SNR W44 with the Fermi Large Area Telescope at energies between 2 x 10(8) electron volts a

79 Using the Goode Solar Telescope at the Big Bear Solar Observatory, we observed

80 e construction of a kilometer-scale neutrino telescope at the South Pole exemplify current efforts to

81 solution and sensitivity of even the largest telescopes at present.

82 the Advanced Technology Large-Aperture Space Telescope (ATLAST).

83 nt from a bench-stable Bi(III) precursor via telescoped B-to-Bi transmetallation and oxidation.

84 is to place an occulting shield outside the telescope, blocking the starlight before it even enters

85 nulling interferometry from formation-flying telescopes--both require exceedingly clean wavefront con

86 lar cluster Terzan 5 by using the Green Bank Telescope, bringing the total of known MSPs in Terzan 5

87 ectroscopy using the Hubble or Spitzer space telescopes, but no atmospheric features have been detect

88 uld be used for designing future space-based telescopes, but that optimistic definitions may be usefu

89 s, the system improved the resolution of the telescope by 30-50%, limited by wavefront error in the o

90 building blocks, the continuous approach was telescoped by the dehydration of the corresponding forma

91 Ground-based telescopes can in principle make such observations when

92 hnique used to overcome blur in ground-based telescopes, can also overcome blur in the eye, allowing

93 nts while not exceeding the CERN Axion Solar Telescope (CAST) experiment or other astrophysical bound

94 ground-based telescopes and the Hubble Space Telescope, combined with theoretical progress, have brou

95 ol disorders in women is often described as "telescoped" compared to that in men, with a later age at

96 A telescope composed of two electrically tuneable lenses e

97 A telescoped continuous flow process is reported for the e

98 Because LHS 1140 is nearby, telescopes currently under construction might be able to

99 We searched Fermi Large Area Telescope data for pulsations from all known millisecond

100 report an analysis of archival Spitzer Space Telescope data on ultraluminous infrared galaxies and de

101 ncluding publicly available James Webb Space Telescope data(9) and our own Hubble Space Telescope dat

102 e Telescope data(9) and our own Hubble Space Telescope data, for the same gamma-ray burst.

103 analyses of a set of three mutant SP-As with telescoping deletions from the reported NH2-terminus.

104 rnational Gamma-Ray Astrophysics Laboratory) telescopes detected a gamma-ray transient, GRB 170817A.

105 Here, we report the Fermi Large Area Telescope detection of variable gamma-ray emission (0.1

106 Telescope directly addresses uncertainty in fragment ass

107 side of Venus taken at the Anglo-Australian Telescope during February 1990 reveal four new thermal e

108 the 1-5 mum coverage of the James Webb Space Telescope early release observations to search for intri

109 This study examined evidence for such a telescoping effect in the general population and tested

110 Little evidence was found for a telescoping effect in women.

111 A telescoping effect is not evident in the general populat

112 edean spiral fibers that demonstrate exotic, telescoping elongation at break of 110%, or 30 times gre

113 types, including dorsal fin loss, long-tail, telescope-eye, albinism, and heart-shaped tail.

114 engths were carried out at the NASA Infrared Telescope Facility and the Keck-II telescope.

115 n infrared spectroscopy at the NASA Infrared Telescope Facility on Mauna Kea, Hawaii.

116 ng plane on 10 August 1995, the Hubble Space Telescope Faint Object Spectrograph detected ultraviolet

117 ddition to generate more than 30 azoles in a telescoped fashion.

118 The far-ultraviolet space telescope (FAUST) was flown on Spacelab 1 to provide wid

119 impaired people are permitted to use bioptic telescopes for driving in many states in the United Stat

120 by the Cryogenic Infrared Spectrometers and Telescopes for the Atmosphere (CRISTA) during shuttle mi

121 the DART impact ejecta with the Hubble Space Telescope from impact time T + 15 min to T + 18.5 days a

122 Using data from the Hubble and Spitzer Space Telescopes from 0.5 to 5 micrometers, we conducted a det

123 the Arecibo Observatory (AO) and Green Bank Telescope (GBT) and interpreted as evidence for liquid s

124 site angular resolution of the Chandra x-ray telescope has enabled the detection and study of resolve

125 vational progress with the NASA Hubble Space Telescope has led to the discovery and study of the earl

126 able element (TE) expression, and found that Telescope has the greatest resolution, as it estimates e

127 The Fermi Gamma-Ray Space Telescope has unveiled a radio quiet pulsar located near

128 ble Space Telescope and the James Webb Space Telescope have awed the public and astronomers alike.

129 et (1) Ceres using ground-based and orbiting telescopes have concluded that its closest meteoritic an

130 ade using large ground-based and space-borne telescopes have probed cosmic history from the present d

131 eroid (1) Ceres from ground- and space-based telescopes have provided its approximate density and sha

132 Instruments such as the Fermi large-area telescope, high-energy stereoscopic system, major atmosp

133 ited wavelength coverage of the Hubble Space Telescope (HST) and inferences of single molecules, most

134 taken on 5 August 2000 with the Hubble Space Telescope (HST) and on 6 August with the Very Large Tele

135 emission measurements from the Hubble Space Telescope (HST) and Spitzer Space Telescope(1-3).

136 The Hubble Space Telescope (HST) and the Gemini Telescope imaged this gal

137 hed data and analyze additional Hubble Space Telescope (HST) data, finding that the source is likely

138 November and December 2012, the Hubble Space Telescope (HST) imaged Europa's ultraviolet emissions in

139 Analysis of Hubble Space Telescope (HST) images of comet Hale-Bopp (C/1995 O1) su

140 ging Spectrograph (STIS) of the Hubble Space Telescope (HST) in January and February 2014 to test the

141 everal decades of planning, the Hubble Space Telescope (HST) was launched in 1990 as the first of NAS

142 Observations with the Hubble Space Telescope (HST), conducted since 1990, now offer an unpr

143 Hubble Space Telescope (HST) and the Gemini Telescope imaged this galaxy 6 to 9 months before the su

144 Based on Hubble Space Telescope images and extensive ground-based spectroscopi

145 e in winds reported from recent Hubble Space Telescope images is not a temporal change, then the feat

146 We obtained Hubble Space Telescope images of 2 Pallas in September 2007 that reve

147 Very Large Array and Australia Telescope images of the brightness distribution showed t

148 to one of the fragments in the Hubble Space Telescope images; we therefore infer that most of the co

149 Hubble Space Telescope imaging observations of two nearby brown dwarf

150 ions of Jupiter's moon Europa taken by Space Telescope Imaging Spectrograph (STIS) of the Hubble Spac

151 from Io were obtained with the Hubble space telescope imaging spectrograph (STIS).

152 st galaxy in the Local Group, with the Space Telescope Imaging Spectrograph at a resolution at least

153 th data taken in 2004, just before the Space Telescope Imaging Spectrograph failed, we find that the

154 Spitzer Space Telescope imaging spectrometer observations of comet 9P/

155 In Hubble Space Telescope imaging, we have found four images of a single

156 milton Echelle spectrograph on the 3-m Shane Telescope, implies a density in excellent agreement with

157 he deepest sky surveys with the Hubble Space Telescope in five wavebands between 0.6 and 1.6 mum.

158 images of Uranus taken with the Hubble Space Telescope in July and October 1997 revealed discrete clo

159 le plume against Jupiter by the Hubble Space Telescope in October 1999 revealed absorption due to S2

160 This demonstrates that a coronagraphic telescope in space could detect and spectroscopically ch

161 These reactions can be telescoped in a one-pot fashion to significantly simplif

162 tem as those that we can observe now through telescopes in nearby star-forming regions.

163 Observing this signal, possibly with radio telescopes in operation today, will demonstrate the pres

164 de stars has been developed at the 6.5-m MMT telescope, in Arizona.

165 as measured by a global network of 11 radio telescopes, increased dramatically during the Shoemaker-

166 We analyzed a long-term Spitzer Space Telescope infrared monitoring campaign of brown dwarfs t

167 ganisms carried by currents collide with the telescope infrastructure, resulting in the emission of l

168 Deep-sea neutrino telescopes instrumented with light detecting Photo-Multi

169 The cross-coupling can be telescoped into the one-pot synthesis of amides and alph

170 The Einstein telescope is expected to produce 10(4)-10(5) gravitation

171 However, it has been suggested that the telescope is used only to meet the visual acuity criteri

172 w generation of extremely large ground-based telescopes is under development, which, when paired with

173 SP-121 b, obtained with the James Webb Space Telescope (JWST) and the Near Infrared Imager and Slitle

174 heric observations with the James Webb Space Telescope (JWST) are enabling unprecedented characteriza

175 MIRI instruments aboard the James Webb Space Telescope (JWST) from 4 to 12 mum.

176 GJ 1214b obtained with the James Webb Space Telescope (JWST) in the mid-infrared.

177 see text] observed with the James Webb Space Telescope (JWST) Near Infrared Spectrograph (NIRSpec).

178 -infrared instrument on the James Webb Space Telescope (JWST).

179 The Fermi Large Area Telescope (LAT) has observed the star-forming region of

180 The Fermi Large Area Telescope (LAT) makes it possible to pinpoint neutron st

181 gamma-ray binaries with the Fermi Large Area Telescope (LAT) shows that 1FGL J1018.6-5856 exhibits in

182 nd exoplanetary science using transformative telescopes like the ELT will demand precise calibration

183 inent observations with the James Webb Space Telescope may enable methane detections on potentially h

184 The bioptic telescope met the (self-reported) driving needs of the m

185 Herein we report a series of telescoping methodologies for one pot synthesis of biolo

186 appendages in insects(4,5), we describe the 'telescope model', a generalized model for the developmen

187 ules from simple renewable carbon sources by telescoping multiple reactions into a single fermentatio

188 Another key feature of this synthesis is telescoping multiple steps.

189 Here we apply a telescoping multiprotein approach to the problem for 104

190 Repeated extension and retraction of telescoping nanotube segments revealed no wear or fatigu

191 Macrophages infiltrating glomeruli in telescoped nephrotoxic nephritis are programmed.

192 ll 0401 with the Low-Frequency Array (LOFAR) telescope network at 140 megahertz.

193 h resolution images from the 1.6 m New Solar Telescope (NST) equipped with high order adaptive optics

194 However, spacecraft and telescope observations have been unable to map the emiss

195 Hubble Space Telescope observations made from 15 minutes after impact

196 This effect is evident in Hubble Space Telescope observations obtained at true opposition on 13

197 Here we report Hubble Space Telescope observations of a seventh inner moon, Hippocam

198 Here we report James Webb Space Telescope observations of CH(3)(+) in a protoplanetary d

199 Event Horizon Telescope observations of M87 in 2017, at a wavelength o

200 Here we report James Webb Space Telescope observations of strong methane emission from W

201 We present Hubble Space Telescope observations of the gravitationally lensed pos

202 Hubble Space Telescope observations separated by 1.73 years reveal co

203 Here we present James Webb Space Telescope observations that clearly show that main-belt

204 Here we present James Webb Space Telescope observations that detect the 3.3 mum PAH featu

205 multaneous in situ satellite and space-based telescope observations that reveal the processes that pr

206 ellar companion with the use of Hubble Space Telescope observations.

207 913, at redshift z = 3.631, using Very Large Telescope observations.

208 uch an occulter is flown in formation with a telescope of at least one metre aperture, terrestrial pl

209 we report observations with the Swift Space Telescope of strong but declining ultraviolet emission f

210 The telescoping of allyl-palladium catalyzed ketone dehydrog

211 This approach enabled telescoping of the two steps into a single efficient pro

212 Collider, and the Gamma-ray Large Area Space Telescope offer promising opportunities within the next

213 from this source detected by the Large Area Telescope on board the Fermi Gamma-ray Space Telescope.

214 uption from the Atmospheric Imaging Assembly telescope on board the Solar Dynamic Observatory.

215 The imaging telescope on board the Transition Region and Coronal Exp

216 pp), with the use of the James Clerk Maxwell Telescope on Mauna Kea, Hawaii.

217 opp) with the use of the James Clerk Maxwell Telescope on Mauna Kea, Hawaii.

218 programme of servicing missions has kept the telescope on the cutting edge of astronomical research.

219 or a series of international low-Earth-orbit telescopes on the basis of the proposed telecommunicatio

220 nae, using data obtained with the Large Area Telescope onboard the Fermi Gamma-ray Space Telescope.

221 l resolution obtained with the Solar Optical Telescope onboard the Japanese Hinode satellite to revea

222 bble Space Telescope, and large ground-based telescopes opens a new era in searches for Earth-analog

223 s structure, the multi-lens structures (e.g. telescope or wide-angle scope) will provide very versati

224 in which 2D concentric zones in the placode telescope out to form 3D longitudinally aligned cylindri

225 ned at 24 micrometers with the Spitzer Space Telescope over a 1-year time interval show moving struct

226 Telescope performs highly accurate quantification of the

227 the speed of light, leveraging Hubble Space Telescope precision astrometry and previous radio VLBI d

228 Finally, a telescoped preparation of these polycyclic compounds by

229 The telescoped procedure reported here consists of a three-s

230 The heavily telescoped process includes seven steps, two crystalliza

231 the free-base or the hydrochloride salt in a telescoped process.

232 1,4-diazepanes, and 1,4-diazocanes through a telescoped protocol is reported.

233 llow supergiant detected by the Hubble Space Telescope, providing an independent proof for the progen

234 A subsequent telescoped reaction sequence of alkoxylation, global dep

235 s-flow synthesis, complex multistep sequence telescoping, reaction engineering equipment, and real-ti

236 latform for the simultaneous optimization of telescoped reactions.

237 Scant evidence was found of telescoping (recollection of events as more recent than

238 problems of light scatter and diffraction in telescopes remain.

239 ered outer rings of Uranus with Hubble Space Telescope results.

240 2dc with the Galaxy Evolution Explorer space telescope reveal a radiative precursor from the supernov

241 osures of Uranus taken with the Hubble Space Telescope reveal two small moons and two faint rings.

242 ons with the X-ray Multi-Mirror (XMM-Newton) telescope reveal X-ray pulsations with the same period a

243 py of Mars' atmosphere with the Hubble Space Telescope revealed the deuterium Lyman alpha line at an

244 jor Atmospheric Gamma-ray Imaging Cherenkov) telescopes, revealing variability with doubling time sca

245 e Spectrograph on the 3.9-m Anglo-Australian Telescope, reveals that the [K v] 4122.6 A line in this

246 cedented sensitivity of the James Webb Space Telescope's Mid-Infrared Instrument(10,11) in the therma

247 ed C=N reduction, the result is an efficient telescoped sequence for the preparation of diastereomeri

248 f druglike compounds in an efficient one-pot telescoped sequence in line with green chemistry princip

249 f the remaining alcohol through a three-step telescoped sequence involving an efficient cleavage of a

250 aser group with the exception that the inner telescoping sheath was replaced with the 12-F excimer la

251 Locking stylets and telescoping sheaths produce a technically demanding but

252 th the Keck Observatory and the Hubble Space Telescopes show that Dysnomia has a circular orbit with

253 tions by the Galileo spacecraft and the Keck telescope showed that Jupiter's outermost (gossamer) rin

254 umerous times by spacecraft and ground-based telescopes, showing that clouds are typically layered an

255 observations with the Swedish 1-meter Solar Telescope (SST) to quantify these twisting motions and t

256 Ground-based 1-m Swedish Solar Telescope (SST)/CRISP, Halpha 6562.8 A observations reve

257 small angles behind a small, well-corrected telescope subaperture that provides low levels of scatte

258 ptical identifications with the Hubble Space Telescope, suggest that greater, similar50 percent are M

259 iotemporal resolution of the 1.6 m New Solar Telescope, supplemented by magnetic data from the Solar

260 formation is applied to the straightforward, telescoped synthesis of alpha-sulfinamido trifluoroborat

261 maceuticals, as demonstrated by a four-step, telescoped synthesis of measles therapeutic, AS-136A, in

262 A microwave-assisted, telescoped synthesis, involving a Michael-type addition

263 ed on safe execution and the requirement for telescoped synthetic transformations (i.e., without isol

264 There are several proposed space telescope systems that could, in principle, achieve this

265 These previous results relied on space-based telescopes that do not provide spectroscopic capability

266 r-Earth planets using data from future space telescopes that were initially designed for atmospheric

267 By telescoping the periods of effective neuronal interactio

268 her 40 3-benzyl derivatives were obtained by telescoping the process with a catalytic hydrogenation r

269 mina, depressing more central neighbours to "telescope" the epithelium downwards into underlying mese

270 dividually detectable by existing or planned telescopes, they would have produced significant cosmic

271 A facile, telescoped three-step-one-flow process for the preparati

272 t performance and a continuing investment of telescope time, we are optimistic these uncharted atmosp

273 We have used the Hubble Space Telescope to blindly search for ionized high-velocity cl

274 We have built a custom telescope to detect these signals from 1 km away for nea

275 oenix cluster(17) using the James Webb Space Telescope to map the [Ne VI] lambda 7.652-mum emission l

276 We have used the Hubble Space Telescope to measure the analogous process of astrometri

277 technology of adaptive optics at the Keck II telescope to observe NGC 6240, a merger between two disk

278 an ancient molecular fossil that provides a telescope to the origins of life.

279 echnology originally applied in astronomical telescopes to combat atmospheric aberrations, to improve

280 ile, a cheap commodity solvent, by combining/telescoping two consecutive reactions-cyclotrimerization

281 In a telescoped, two-step process, S-alpha-thiobenzoyl acid 6

282 let spectroscopy and concurrent Hubble Space Telescope ultraviolet imaging in eclipse investigate the

283 A telescoped urazole oxidation and Lewis acid-catalyzed cy

284 Bioptic telescope usage patterns were quantified with questions

285 t it be possible to create mirrors for space telescopes, using nothing but microscopic particles held

286 pe (HST) and on 6 August with the Very Large Telescope (VLT).

287 A 10-mm flat laparoscopic telescope was used to capture the optical surgical field

288 econd pulsars obtained with the Parkes radio telescope, we constrained the characteristic amplitude o

289 rigins Spectrograph onboard the Hubble Space Telescope, we detected ubiquitous, large (150-kiloparsec

290 Using data from the Suzaku x-ray telescope, we determined an accurate, spatially resolved

291 Using the Chandra and Hubble Space Telescopes, we have now observed 72 collisions, includin

292 infrared spectrometers at three ground-based telescopes, we measured methane and water vapor simultan

293 inferences with the Hubble and Spitzer Space Telescopes were hindered by the observations' relatively

294 on is described of the Implantable Miniature Telescope, which is completing clinical development for

295 t to the optical taken with the Hubble Space Telescope, which simultaneously capture, in three separa

296 ale Interferometer (DASI), an array of radio telescopes, which for the past two years has conducted p

297 individual columns in the optic lobe with a telescope while recording from single T4 neurons, we fin

298 the radius of the Sun, existing and upcoming telescopes will be able to observe the composition and d

299 ike planet orbiting a nearby star requires a telescope with an extraordinarily large contrast at smal

300 ts have been detected with large single-dish telescopes with arcminute localizations, and attempts to