Related by context. All words. (Click for frequent words.) 72 GeV 71 electron volt 70 electron volts eV 69 electron volts 69 keV 68 MeV 67 electron volts GeV 67 tera electron volts 66 m z 65 cm -2 64 meV 64 petawatt 63 mJ 63 proton antiproton collisions 62 terawatt 62 mT 62 femtoseconds 62 antiparticle 61 FWHM 61 redshifts 61 cm -3 60 colliding protons 60 Wh kg 60 Mpc 60 kcal mol 60 attoseconds 60 Carina constellation 60 teraelectronvolts TeV 60 photon energies 60 picoseconds 60 photoemission 60 GFlops 60 picometers 60 ppbv 60 microwatt 59 #nm #nm [001] 59 cosmic ray electrons 59 z = 59 dipole moment 59 VLT telescope 59 kT 59 electron neutrinos 59 nucleon 59 ε 59 W/cm2 59 #mV V 58 absorption coefficient 58 sievert 58 kpc 58 cm -1 58 candelas per 58 photoelectron 58 W/m2 58 μW 58 g cm 58 quadrillionth 58 Å -1 58 Angstroms 58 micron wavelength 58 gamma ray emission 58 microwatts 58 Terawatt hours 58 Dy#O# 58 multiply accumulates 58 kelvin 58 microvolts 58 arcsec 58 Gd#O# 58 kilo watts 57 redshift 57 quasiparticle 57 orbital eccentricity 57 luminous galaxies 57 ppm boron 57 terawatts 57 gravitational acceleration 57 luminosities 57 antineutrinos 57 kVp 57 antineutrino 57 ° sec 57 xenon propellant 57 galaxy redshift 57 HARPS spectrograph attached 57 arcminutes 57 z ~ 57 μm wavelength 57 cd m 57 correlators 57 proton proton 57 cesium atom 57 W mK 57 distant quasar 56 energetic gamma rays 56 Mflops 56 curies 56 #.#nm [002] 56 electrons protons 56 J# +# [002] 56 submillimetre wavelengths 56 linewidth 56 wavelength tunable 56 Sm3 56 Brookhaven Relativistic Heavy 56 relativistic protons 56 trillion electronvolts 56 mGy 56 helium ions 56 J#.# [001] 56 kWhr 56 kW hr 56 terahertz THz 56 fin div 56 mu m 56 arcsecond 56 micro sieverts 56 nT 56 mW/cm2 56 ZrO 2 56 micromolar 56 electron positron 56 X ray pulses 56 VHE gamma rays 56 #ppm U 56 λ 56 circular dichroism 56 μS cm 56 gauss 56 ppm U 56 m/s2 56 kg/m3 56 gravitational redshift 56 millivolts 56 parsec 56 femtogram 56 CoRoT #b 56 petaFLOPS 56 nm wavelength 56 baryon 56 m 56 ms -1 56 photon absorption 56 fs pulses 56 muon neutrinos 55 Tbit s 55 arcseconds 55 2dB 55 phosphorus atom 55 electron bunches 55 picosecond 55 #,#,#,#,#,#,# [004] 55 angstroms 55 kilowatthours 55 g t Ta 55 rms noise 55 Gamma rays 55 1μm 55 cm ^ sup 55 nanometers billionths 55 η 55 kJ 55 antiprotons 55 luminous flux 55 Astronomical Units 55 orbital radius 55 excitation energies 55 Outlays totaled 55 gravitational radiation 55 picogram 55 AUs 55 praseodymium 55 Unit Telescopes 55 quadrillion BTUs 55 ohm cm 55 photon fluorescence 55 femtosecond pulses 55 MBd 55 californium 55 millimeter wavelength 55 1ppm 55 Supplementary Table 55 2ppm 55 #.# MHz [002] 55 joules 55 Georges Charpak France 55 W boson 55 Proxima Centauri 55 cosmic ray particles 55 Bulk density 55 observable universe 55 displayable colors 55 neutron spectrometer 55 Unfunded pension liability 55 particle acceleration 55 particle collisions 55 #ppm Cu 55 cm ² 55 Magnetars 55 cosmic ray protons 55 SNe Ia 55 pulse durations 55 ppm ppm 55 #.#m #.#m #.#m [003] 55 km/# miles [002] 54 terabyte TB = 54 TFlops 54 fermion 54 #cd m 2 54 nm spectral 54 1kHz 54 #.# bpa 54 bandgaps 54 ppmv 54 solar neutrinos 54 Greg Stanfield GXP 54 electron accelerator 54 spectral bands 54 positrons 54 teraelectronvolts 54 sunlike stars 54 Jeff Arend Impala 54 mmol 54 TeraFLOPS 54 dI dV 54 arcmin 54 Vpp 54 Gary Scelzi Dodge Stratus 54 corona discharge 54 microquasar 54 yttrium oxide 54 rubidium atoms 54 nanometers nm 54 GigaHertz 54 #x# ^ 54 linearly polarized 54 baryonic 54 orbiting Gliese 54 sulfur dioxide SO 54 t/m3 54 micrometre 54 μm diameter 54 ZnSe 54 cesium atoms 54 oxide thickness EOT 54 megajoules 54 cm3 54 meter panchromatic 54 gamma rays X rays 54 spherically symmetric 54 Ly alpha 54 Kepler 9c 54 solar radii 54 relativistic particles 54 χ 54 Zeta Ophiuchi 54 scanning electron microscopes 54 GFLOPs 54 tesla 54 helium nuclei 54 Eu#O# 54 tau neutrinos 54 Tflop s 54 PLoS Med 54 lanthanum La 54 bosonic 54 RUR#.# [006] 54 electrons positrons 54 CAIs 54 nanometers nanometer 54 ^ sup -1 54 antiproton 54 weakly interacting 54 Epsilon Eridani 54 sqft hr 54 microampere 54 electron scattering 54 X ray binary 54 HIRES spectrometer 53 micron diameter 53 shear modulus 53 neodymium Nd 53 Nm3 h 53 UV wavelengths 53 Raman scattering 53 supergiant star 53 Gary Densham Chevy Impala 53 μSv 53 TFLOPS 53 Kbits 53 numerical aperture NA 53 fA 53 mCi 53 optical modulators 53 spectroscopic technique 53 platinum Pt 53 actions ordinaires accréditives Prix 53 dBFS 53 mrem 53 mK 53 VLTI 53 dB insertion loss 53 QRS width 53 GPa 53 XTE J# 53 gigaflops 53 photon counting 53 polaritons 53 output voltages ranging 53 Î ¼ 53 milligauss 53 Nd 53 μm thick 53 #W halogen 53 MIL HDBK #F 53 hydrofluorocarbons HFCs perfluorocarbons PFCs 53 gluon 53 cosmic ray collisions 53 #.#t [003] 53 hyperfine 53 synthetic aperture 53 ppm Zn 53 rms jitter 53 Platform openSUSE 53 redshift z = 53 HAT P 53 nanometer wavelength 53 nH 53 cryogenically cooled 53 proton proton collisions 53 GFLOPS 53 ppm Ni 53 impactors 53 excitations 53 #.#-#.# [011] 53 Kertus Davis Chevrolet 53 5mW 53 Ryan Schnitz Buell 53 graphitic carbon 53 micrometre sized 53 synchrotron X ray 53 Muons 53 NMR spectra 53 μS 53 quadrillionths 53 lanthanum oxide 53 HOLE NO 53 anthracene 53 mtoe 53 antiparticles 53 Gigaflops 53 hafnium oxide 53 undecillion 53 Super Kamiokande 53 #ppb gold 53 Eric Medlen Mustang 53 #.#V #.#V [001] 53 ionise 53 electron beams 53 #ppb [003] 53 gravitationally lensed 53 dynamical evolution 53 dBm output 53 #.#m #.#m [004] 53 Tb s 53 x #.#cm [001] 53 leptons 53 microwave photon 53 Fomalhaut b 53 polystyrene spheres 53 #ppb Au [002] 53 neutralinos 53 Bq l 53 PLoS Biol 53 LAGEOS 53 microfarads 53 MLN EUROS 53 kwhs 53 Fourier transform 53 piconewtons 53 megaflops per 53 BLG #Lb 53 emission wavelength 53 Michelson interferometer 53 Phil Burkart Toyota Celica 52 μH 52 attosecond 52 protons 52 nanoantennas 52 photoelectric conversion 52 Main Injector Neutrino 52 CdSe 52 numerical aperture 52 oscillation frequency 52 neutrino beam 52 Tflops 52 quanta 52 optical wavelengths 52 g/cm3 52 ultraviolet wavelengths 52 phototransistors 52 radiative recombination 52 DEV DA TOMAR NEXT 52 Cu Equivalent 52 Mbp s 52 foreground galaxy 52 ppm Pb 52 teraFLOPS 52 g t Rubidium 52 exciton 52 germanium silicon 52 polarimetry 52 proton particles 52 Large Electron Positron 52 exoplanets orbiting 52 Si#DB 52 AGNs 52 microns millionths 52 #.#uF 52 resonance frequency 52 kΩ 52 micrometres 52 Lanthanum La 52 purities 52 milliwatt 52 optical spectra 52 GWs 52 irradiance 52 gamma ray energies 52 micrometers thick 52 gigahertz frequencies 52 millisecond pulsar 52 milliarcseconds 52 shorter wavelengths 52 PLoS Genet 52 gpt Pt 52 #.#μm [001] 52 multiwavelength 52 pour atteindre 52 ion traps 52 μm 52 valence electrons 52 megapascals 52 collinear 52 kilobases 52 MoS2 52 submillimeter wavelengths 52 #nm wavelength [001] 52 γ 52 #ppb [001] 52 helium atom 52 kD 52 gigabyte GB = 52 kGy 52 absorption spectra 52 sodium atoms 52 gigapixels 52 X ray binaries 52 Shutter speeds 52 #,# x1 #x# 52 fig. S2 52 interferometers 52 blazar 52 microcavity 52 #m@#.# % [002] 52 stimulated emission 52 unpolarized 52 DZero experiment 52 QCLs 52 quadrillion Btu 52 mV V 52 phonon 52 CaO 52 SMBHs 52 galactic disk 52 ppm Nb 52 ps nm 52 g t Gallium 52 star Gliese 52 Virgo Cluster 52 μF 52 Kelvins 52 LiNbO3 52 photon detection 52 μm particle 52 cd m² 52 diffract 52 2 MeV electron 52 electromagnetic flux 52 ion flux 52 quintillion bytes 52 3He 52 quadrillion bytes 52 mrad 52 √ Hz 52 κ 52 MBq 52 logarithmic scale 52 HRTEM 52 supplies SMPS 52 SMBH 52 bdrms starting 52 Amperes 52 baryons 52 μV 52 detect gamma rays 52 volt amps 52 ultraluminous galaxy 52 alpha particles 52 #Ω [002] 52 silicate dust 52 nanowatts 52 GHz POWER5 52 terahertz frequencies 52 amplitudes 52 trillion electron volts 52 Li#CO# 52 micron pixels 52 g t PGE 52 plasmon 52 isotope technetium 52 Terbium 52 X rays gamma rays 52 weak gravitational lensing 52 = #,#,#,# bytes 52 ARPES 52 massless particles 52 circularly polarized 52 deuterium atoms 52 electron proton 52 hadron 52 ohm load 51 velocity dispersion 51 photon flux 51 Sees FY# revenues 51 THz radiation 51 #.#mA [002] 51 psec 51 proton neutron 51 exajoules 51 teragrams 51 mso footer margin 51 eclipsing binary 51 ppm molybdenum 51 cosmic rays collide 51 Higgs bosons 51 X#.# [003] 51 Y#O# 51 ppm eU#O# 51 ppm indium 51 Mbits s 51 spherical particles 51 #.#g Au t [003] 51 blackbody 51 femtosecond 51 Vsby 1 51 Tb#O# 51 5μm 51 sieverts 51 CO2 eq 51 1mW 51 superpositions 51 conductivities 51 σ 51 qubit quantum 51 Entangled photons 51 spectra 51 magnetic anisotropy 51 carbon dioxide CO2 emitted 51 mU L 51 magnon 51 starburst galaxies 51 1nm 51 trillion Btu 51 electron diffraction 51 neutrino mass 51 Ron Capps Charger 51 powder diffraction 51 lp mm 51 constellation Pegasus 51 eU#O# 51 deuterium nuclei 51 ρ 51 #.#MHz [007] 51 milliampere 51 atmospheric opacity 51 transistors HEMTs 51 g t Niobium 51 Commtouch Detection Center 51 micrometers 51 SMM J# 51 submillimeter wavelength 51 #μm [001] 51 gm tonne 51 ultrashort pulse laser 51 proton antiproton 51 photometry 51 ug g 51 moduli 51 #.# [005] 51 particle detectors 51 bln kWh 51 dysprosium oxide 51 Fermi telescope 51 tonnes CO2e 51 Fig. 4a 51 AB Aurigae 51 cm ³ 51 ionization mass spectrometry 51 HREO TREO ratio 51 NASA Wilkinson Microwave 51 cm sec 51 WEEK ENDING INDEX 51 oxide TREO 51 inelastic scattering 51 Rydberg atom 51 CoRoT 51 THD + N 51 decimal digits 51 SUSY 51 chipscale 51 baryon acoustic oscillations 51 #.#Hz 51 superclusters 51 GALEX 51 #Wh [002] 51 RX J# 51 MG J# +# 51 X ray spectroscopy 51 lbs Cu 51 gamma rays emitted 51 detect gravitational waves 51 ultrashort laser pulses 51 XP fip5 ~ 51 Antennae Galaxies 51 Earth radii 51 #K LEs 51 milliohm 51 gamma ray flares 51 Bose Einstein Condensate 51 Mtoe 51 drillhole spacing 51 perigee closest 51 % Nb#O# 51 #nm wavelengths 51 mW cm 2 51 OGLE TR 51 orbital angular momentum 51 sq. mm 51 fundamental constants 51 electrons emitted 51 neutrons 51 regulated output voltages 51 Coulomb blockade 51 Teraflops 51 nm wavelengths 51 galaxy M# [002] 51 active galactic nuclei 51 Ytterbium 51 thermal EMF 51 IR spectra 51 #ppm Mo 51 blazars 51 #,#,#,#,# [011] 51 #MSPS 51 samarium 51 erbium 51 particle accelerators 51 AU Mic 51 bilayer graphene 51 #lm [002] 51 indium gallium 51 giga watt 51 neodymium oxide 51 neutralino 51 gigaflop 51 galaxy cluster 51 lepton 51 Fig. 2A 51 visible wavelengths 51 nitride semiconductor 51 Cygnus X 51 InSb 51 superconducting quantum interference 51 photocurrent 51 interparticle 51 distant supernovae 51 milioni di euro 51 multicrystalline cells 51 nm excitation 51 mso header 51 type Ia supernova 51 dipole dipole 51 isotopic ratios 51 metallicity 51 galaxies quasars 51 Z boson 51 LWIR 51 UV photons 51 # HS webwire 51 extragalactic 51 interferometric 51 galactic nucleus 51 gm t 51 dispersive 51 YU# 51 La Silla Observatory 51 Tevatron collider 51 nanomolar 51 dielectric constants 51 magnetic spectrometer 51 cubic feet scf 51 megabits sec 51 photonic bandgap 51 Wp 51 kilohertz kHz 51 nanomotors 51 atoms 51 elliptical galaxy 51 Ray Spectrometer 51 emits photons 51 Earthquake magnitudes 51 GaP 51 #.# [002] 51 azimuthal 51 ALT elevation 51 dont la moitié 51 electrons orbiting 51 optically pumped 51 Josephson junction 50 titanium sapphire 50 Wm -2 50 Quiescent current 50 globulars 50 picocurie 50 ppm arsenic 50 particle physics experiments 50 photodetectors 50 Petaflops 50 tCO2e 50 #X SSD 50 mW MHz 50 meters #.#ft 50 yr -1 50 enthalpy 50 + Pd + 50 pmol 50 WMAP satellite 50 Left ventricular ejection 50 electric dipole 50 PIN diode 50 interferometric observations 50 fluorescence intensity 50 surface plasmon 50 GRB #B 50 SN #A 50 absorbance 50 Cu Eq 50 gigahertz GHz 50 @ gn 50 uW 50 isotropic 50 Hubble Constant 50 mG 50 RS Ophiuchi 50 highly collimated 50 InAs 50 Pt + Pd 50 axions 50 orbits Saturn 50 polariton 50 Si substrate 50 Cosmologists 50 energetic electrons 50 photometer 50 Yuan Keywords MARKETS 50 cobalt atom 50 GRB# 50 -# Celsius [001] 50 Nova NanoSEM 50 mpm 50 terawatt hour 50 thermonuclear fusion 50 WIMPs 50 Coma Cluster 50 Hadron collider 50 Wilkinson Microwave Probe 50 #ppm [002] 50 mm DFN package 50 transfer FRET 50 ellipsoids 50 helium nucleus 50 nonpolar GaN 50 colliders 50 SKY# #LF 50 crystalline Si 50 photoluminescence 50 megatons 50 5nm 50 femtosecond laser pulses 50 #Wp 50 millimeter wavelengths 50 radiative cooling 50 X ray absorption spectroscopy 50 supersymmetric particles 50 La Ce Pr 50 photolysis 50 SiO 50 Rayleigh scattering 50 backscattered 50 NEAs 50 microwave frequencies 50 geosynchronous orbit reached 50 SAW oscillators 50 femtosecond pulse 50 HD# [005] 50 ppm eU 50 microbolometers 50 electron density 50 × #.#mm [002] 50 Gbytes sec 50 BiCMOS processes 50 Fermilab Tevatron 50 proton collisions 50 #.#um [001] 50 #.#g t Ag [005] 50 x ray scattering 50 VLBI 50 toneladas 50 ppm Mo 50 TrES 4 50 uL 50 2MASS 50 radial velocity method 50 μSv h 50 #.#g t Au [005] 50 Doppler shifts 50 Dysprosium 50 micrograms mL 50 m@#.# g t Au [003] 50 galactic clusters 50 Petaflop 50 WASP #b 50 chromatogram 50 quantum bits qubits 50 infrared photons 50 #.#.i#.rpm 50 2kHz 50 magnetar 50 Kw h 50 6kW 50 nanometer spatial 50 Au Eq 50 mm ² 50 microlitre 50 La#O# 50 Mn Fe 50 linewidths 50 megabyte MB = 50 nanodot 50 Panasonic Oxyride 50 lithium oxide 50 Gigahertz 50 avalanche photodiodes 50 x 7mm 50 Nd Yag 50 electron flux 50 photomultiplier tubes 50 proton decay 50 constellation Cepheus 50 Nd YAG 50 inductance values 50 Eur J Pharmacol 50 x #.#mm [001] 50 fissile isotope 50 μmol 50 NMR spectrometer 50 lutetium 50 CO -2 emissions 50 GHG emitted 50 micron thick 50 averaging #.#g t [003] 50 supermassive 50 #MW [001] 50 kHz bandwidth 50 PCT VALUE DATE 50 Fig. 2b 50 submillimetre 50 emit photon 50 laser scanning confocal 50 g carbo 50 uM 50 diatomic 50 multipartite entanglement 50 Raman spectra 50 # XN 50 thermal equilibrium 50 gamma rays 50 inch ppi 50 S2A TM 50 Gcal h 50 monodisperse 50 SAXS 50 ZrO2 50 MB DDR2 SDRAM 50 baryonic matter 50 wph 50 Planck constant 50 X ray emission 50 GaAs AlGaAs 50 0 dBm 50 #.#GHz [001] 50 meter multispectral 50 Orbitrap 50 emit photons 50 CaCO 3 50 mg/m3 50 HL Tau 50 Keck Interferometer 50 ytterbium 50 pmol L 50 Voltages 50 transmissivity 50 CMB radiation 50 W bosons 50 photoionization 50 #W #W #W 50 X ray photons 50 Calculates optimum seek 50 diffraction limit 50 anisotropy 50 MPG ESO 50 kDa 50 Anisotropy Probe 50 giant gaseous planets 50 megaflops 50 GB DDR3 50 capacitive loading 50 copper Cu 50 AngloGold Ashanti Titiribi 50 illuminance 50 nucleotide substitutions 50 Megabytes MB 50 -pass code SHOPNBC 50 reionization 50 quantum dot lasers 50 μg l 50 photons particles 50 terrawatt hours 50 ultrashort pulses 50 lumens watt 50 KwH 50 Anisotropy Probe WMAP 50 submillimeter 50 molecular orbitals 50 supercurrent 50 electronic excitations 50 centimetric 50 diamagnetic 50 Siemens SWT 50 delocalized 50 zettabytes 50 g bhp hr 50 solar corona 50 #pF [001] 50 x ray beams 50 albedo reflectivity 50 synchrotron x ray 50 spectral density 50 Phys. Rev. Lett 50 oxyhemoglobin 50 #.#mV 50 microlensing events 50 high redshift galaxies 50 μsec 50 Interferometric 50 particle beams 50 mwh 50 nsec 50 surface plasmon resonance 50 rpm spindle 49 atto 49 kilocalorie 49 gamma ray burst 49 tokamaks 49 monochromator 49 YORP effect 49 kw 49 8 Cyl 49 kw hr 49 #.#/#.#m 49 scf ton 49 mΩ 49 magnetisation 49 collide protons 49 oxides TREO 49 #Wh [001] 49 pCi l 49 INCREASED TO 49 Europium