ライフサイエンスコーパス: telescope

1 Telescope onboard the Fermi Gamma-ray Space Telescope.

2 a ring polarimeter on the robotic Liverpool Telescope.

3 this system, obtained with the Spitzer Space Telescope.

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

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

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

7 ervations taken with the James Clerk Maxwell Telescope.

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

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

10 Infrared Telescope Facility and the Keck-II telescope.

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

12 full planet rotations using the Hubble Space Telescope.

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

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

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

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

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

18 by means of differential imaging with large telescopes.

19 usters, using rotation parameters from radio telescopes.

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

21 ional study, even with the largest available telescopes.

22 brightness that could be detected by future telescopes.

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

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

25 ade by remote sensing by sophisticated space telescopes.

26 ond the sensitivity limits of existing large telescopes.

27 tem (VERITAS) array of atmospheric Cherenkov telescopes.

28 vely poor spatial resolution of far-infrared telescopes.

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

30 0.245 kiloelectron volts by the Deep Survey telescope aboard the Extreme Ultraviolet Explorer.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

72 A telescope composed of two electrically tuneable lenses e

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

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

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

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

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

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

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

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

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

82 A telescoping effect is not evident in the general populat

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

112 Hubble Space Telescope imaging observations of two nearby brown dwarf

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

140 Macrophages infiltrating glomeruli in telescoped nephrotoxic nephritis are programmed.

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

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

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

144 Hubble Space Telescope observations separated by 1.73 years reveal co

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

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

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

148 The telescoping of allyl-palladium catalyzed ketone dehydrog

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

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

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

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

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

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

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

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

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

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

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

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

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

162 Finally, a telescoped preparation of these polycyclic compounds by

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

164 The heavily telescoped process includes seven steps, two crystalliza

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

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

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

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

169 problems of light scatter and diffraction in telescopes remain.

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

171 2dc with the Galaxy Evolution Explorer space telescope reveal a radiative precursor from the supernov

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

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

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

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

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

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

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

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

180 Locking stylets and telescoping sheaths produce a technically demanding but

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

196 By telescoping the periods of effective neuronal interactio

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

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

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

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

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

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

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

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

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

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

207 Bioptic telescope usage patterns were quantified with questions

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

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

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

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

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

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

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

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

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

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

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

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

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

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