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(Click for frequent words.) 67 millimeter wavelengths 67 X ray wavelengths 66 Interferometric 66 submillimeter wavelength 66 submillimetre 65 fainter objects 65 interferometric 65 X ray pulses 65 infrared wavelength 64 infrared imager 64 submillimetre wavelengths 64 ultraviolet wavelengths 64 subwavelength 63 dipole moment 63 polarimetry 63 submillimeter wavelengths 63 interferometry 63 solar corona 63 helium ions 63 linearly polarized 63 faint galaxies 63 THz radiation 63 millimeter wavelength 63 QCLs 63 optical wavelengths 62 GALEX 62 filamentary structure 62 photometer 62 gamma ray detectors 62 fluorescence excitation 62 airglow 62 terahertz waves 62 visible wavelengths 62 shorter wavelengths 62 backscattered 62 SINFONI 62 VLTI 61 CMB radiation 61 ESO VLT 61 interferometers 61 #.#nm [002] 61 jovian 61 terahertz THz 61 SQUIDs 61 extragalactic 61 Spitzer infrared 61 femtosecond lasers 61 coronagraph 61 energetic electrons 61 VLBA 61 luminous galaxies 61 optical microscopy 61 lightwaves 61 IR wavelengths 61 photoemission 61 infrared ultraviolet 61 photometry 61 Corot 9b 60 emittance 60 terahertz frequencies 60 AB Aurigae 60 gravitational radiation 60 EVLA 60 ultrashort pulses 60 x ray beam 60 cosmic microwave radiation 60 spectroscopic observations 60 absorption spectra 60 infrared wavelengths 60 radar interferometry 60 diffuse aurora 60 infrared astronomy 60 electron diffraction 60 scanning electron microscopes 60 X ray binaries 60 photon counting 60 Terahertz waves 60 Geminga 60 reflectometry 60 HII regions 60 spatial resolution 60 polarimetric 60 cosmological distances 60 ultraviolet wavelength 60 Doppler shifts 60 femtosecond pulses 60 ARPES 60 multiwavelength 60 backscattering 60 radiometers 60 photomultiplier tubes 60 HD#b 60 infrared spectrometers 60 lensing galaxy 60 spectroscopic measurements 60 diffraction pattern 60 elongated orbits 60 photoelectron 60 supergiant star 60 distant supernovas 59 X ray telescopes 59 cirrus cloud 59 hyperspectral imager 59 LOFAR 59 terahertz radiation 59 x ray pulses 59 ESO telescope 59 HRTEM 59 infrared 59 unpolarized 59 x ray scattering 59 Adaptive optics 59 ultrahigh resolution 59 UV wavelengths 59 circularly polarized 59 spectroscope 59 deformable mirror 59 polarimeter 59 diffracted 59 diffraction patterns 59 stellar occultation 59 infrared interferometry 59 circumstellar 59 distant quasar 59 IR LEDs 59 Cherenkov radiation 59 widefield 59 Fomalhaut b 59 optical interferometry 59 X ray emitting 59 distant galaxy clusters 59 frequency combs 59 X ray detector 59 weak gravitational lensing 59 multiband imaging photometer 59 gamma ray flares 59 optical spectra 59 photon fluorescence 59 photon beam 59 arcminutes 59 gamma rays emitted 59 arcsecond 59 RRATs 59 auroral activity 59 infrared telescopes 59 terahertz rays 59 detect gamma rays 59 circumstellar disk 59 Keck Interferometer 59 ionised gas 59 spectrographs 59 electron neutrinos 59 micrometer scale 59 tomographic 59 collimated 59 Kuiper belt objects 59 GJ #b [002] 59 infrared spectral 58 Saturnian moons 58 photon energies 58 galaxy M# [002] 58 photon beams 58 microquasar 58 gamma ray emission 58 microwave radiation 58 femtosecond timescale 58 gravitationally lensed 58 synchrotron X ray 58 infrared radiation 58 AGNs 58 Epsilon Eridani 58 electrical resistivity 58 ionized gases 58 distant supernovae 58 Saturn magnetosphere 58 graphite whiskers 58 photon detector 58 occultations 58 Magnetic Imager HMI 58 pulsed lasers 58 photoacoustic 58 active galactic nucleus 58 arcseconds 58 photomultiplier tube 58 wavelength infrared 58 gravitational redshift 58 absorbs photons 58 electrochemical sensors 58 isotropic 58 gravitational lens 58 Submillimeter Array 58 X ray emission 58 Interferometer VLTI 58 spectroscopic 58 particle acceleration 58 foreground galaxy 58 luminosities 58 x ray beams 58 VISTA telescope 58 solar radii 58 absorption spectroscopy 58 shortwave infrared 58 Jupiter moon Io 58 neutron radiation 58 optical microscopes 58 InGaAs 58 fluorescence spectroscopy 58 Arches Cluster 58 MG J# +# 58 Fermi telescope 58 Mpc 58 retroreflector 58 synchrotron x ray 58 astronomical objects 58 prominences 58 synthetic aperture 58 meteoritic material 58 metallic nanostructures 58 microcavities 58 diffraction grating 58 microns millionths 58 high redshift galaxies 58 fluorescence microscope 58 spectroscopic analysis 58 Gamma ray 58 sub millimeter wavelengths 57 radar altimetry 57 electromagnetic flux 57 reflectance spectroscopy 57 nanometers billionths 57 Virgo Cluster 57 starquakes 57 Planck satellite 57 NASA Wilkinson Microwave 57 quantum cascade 57 Venusian atmosphere 57 spectral imaging 57 Coma Cluster 57 spatially resolved 57 infrared photons 57 ionise 57 collimators 57 ESO Paranal Observatory 57 redshifts 57 eclipsing binary 57 radiometry 57 Keck telescopes 57 blackbody 57 femtogram 57 near infrared NIR 57 Raman scattering 57 fluorophores 57 Gamma rays 57 blazars 57 distant galaxies 57 specular reflection 57 blazar 57 detect gravitational waves 57 interferometer 57 VHE gamma rays 57 superlens 57 X ray spectrometer 57 photoluminescence 57 photodetector 57 KH #D 57 Gravitational waves 57 J# +# [002] 57 spatially coherent 57 SAXS 57 Earth ionosphere 57 bolometers 57 evanescent waves 57 ESA XMM Newton 57 infrared spectra 57 Muchachos Observatory 57 microcavity 57 spectroscopy 57 diffraction limit 57 aperture telescope 57 protoplanetary 57 GJ#b 57 sub picosecond 57 mesosphere 57 Atacama Large Millimeter Array 57 APEX telescope 57 excitonic 57 RS Ophiuchi 57 frequency comb 57 chromosphere 57 intrinsic brightness 57 infrared LEDs 57 Ly alpha 57 Alfven waves 57 Chajnantor plateau 57 quantum cascade lasers 57 Synchrotron radiation 57 imaging spectrometer 57 supernova remnant 57 laser spectroscopy 57 spectroscopic technique 57 conventional optical microscopes 57 thermally induced 57 photons particles 57 QWIP 57 polariton 57 Type Ia supernovas 57 UVOT 57 confocal laser scanning 57 transmissivity 57 metallicity 57 nanometric 57 ion microscope 57 Lyman alpha 57 photolysis 57 spectral bands 57 photons emitted 57 interstellar dust clouds 57 Ultraviolet Optical Telescope 57 FWHM 57 velocimetry 57 scanning electron microscope SEM 57 MWIR 57 Saturn outermost 57 RHESSI 57 X rays gamma rays 57 elliptical orbits 57 silicate dust 57 magnetostrictive 57 Cepheid variables 57 microlens 57 corona discharge 57 attosecond 57 quantum oscillations 57 azimuthal 57 UV photons 56 VY Canis Majoris 56 Gaussian beam 56 galaxy redshift 56 elliptical galaxy 56 radiative cooling 56 auroral 56 imager 56 galactic cosmic rays 56 unpolarized light 56 refractive indices 56 distant quasars 56 atomic lattice 56 galaxy NGC 56 starburst galaxy 56 polar mesospheric clouds 56 exosphere 56 micron wavelength 56 proplyds 56 redshifted 56 phonon 56 inhomogeneities 56 pulsed laser 56 active galactic nuclei 56 panchromatic 56 ecliptic plane 56 bolometer 56 Mössbauer 56 resonance frequency 56 Nova NanoSEM 56 parabolic reflector 56 Comet 9P/Tempel 1 56 NEAs 56 brightnesses 56 diffracting 56 redshift 56 amplitudes 56 afterglows 56 pentacene molecule 56 fluorescent nanoparticles 56 illuminance 56 ionised 56 micrometre sized 56 photonic crystal 56 X ray microscopy 56 Planck telescope 56 Heterodyne Instrument 56 polaritons 56 spectroscopically 56 baryon acoustic oscillations 56 keV 56 Gravitational lensing 56 surface roughness 56 frequency electromagnetic waves 56 optical spectroscopy 56 VLBI 56 resonant cavity 56 parabolic reflectors 56 radial velocities 56 radiometer 56 GROND 56 polarizing filters 56 Kuiper Belt Objects 56 GRB #B 56 sunlike stars 56 Alfvén waves 56 subnanometer 56 magnetospheric 56 spectrometry 56 satellite altimetry 56 Doppler shift 56 orbiting gamma ray 56 Ulysses spacecraft 56 Multi Object Spectrograph 56 collimated beam 56 linearly polarized light 56 coronal loop 56 helium atoms 56 diffraction 56 Cosmic Microwave Background 56 infrared detector 56 spectral characteristics 56 ultraviolet laser 56 microlensing events 56 rubidium vapor 56 nanoribbon 56 thermal infrared 56 Beta Pictoris b 56 exoplanetary 56 optically pumped 56 multispectral 56 ionized particles 56 astrometry 56 polar vortex 56 lensless imaging 56 optical telescopes 56 planetary Transits 56 infrared rays 56 monochromators 56 emitted photons 56 spiral galaxy NGC 56 Fourier transform 56 Cat Paw Nebula 56 coronal loops 56 linewidth 56 XMM Newton 56 surface plasmons 56 Long Wavelength Array 56 NICMOS 56 X ray spectroscopy 56 HESS telescopes 56 arcsec 56 superluminal 56 velocity dispersion 56 circularly polarized light 56 waveband 56 photoelectron spectroscopy 56 confocal microscopes 56 rotational axis 56 Michelson interferometer 56 emits photons 56 HiRISE image 56 heliospheric 56 Anisotropy Probe WMAP 56 VIRTIS instrument 56 electron beams 56 transiting planet 56 superposed 56 Raman spectra 56 pyroelectric 56 X ray afterglow 55 Submillimeter 55 multispectral imager 55 synchrotrons 55 astrophysical objects 55 collimator 55 Encke gap 55 Fornax cluster 55 Delta Cephei 55 monochromator 55 infrared laser beam 55 harmful ultraviolet 55 wavelengths 55 cryogenically cooled 55 circular polarization 55 anisotropy 55 dust enshrouded 55 KBOs 55 moon Mimas 55 InAs 55 photocurrent 55 Josephson junction 55 microwave frequencies 55 spectrometric 55 GJ #b [001] 55 microwave radiometers 55 exo planets 55 birefringence 55 HiRISE camera 55 moon Enceladus 55 Epsilon Aurigae 55 photometric 55 X ray beams 55 gamma ray detector 55 optical sectioning 55 radiofrequency waves 55 Electron microscopes 55 smallest exoplanet 55 Spectroscopic 55 rotating neutron stars 55 nm spectral 55 magnetic fields 55 optomechanical 55 Rayleigh scattering 55 magnetisation 55 cosmic ray flux 55 surface plasmon 55 Jovian planets 55 nebular 55 icy moons 55 femtosecond 55 cosmological parameters 55 inhomogeneous 55 sized planets orbiting 55 cosmic gamma rays 55 sulfate aerosols 55 antineutrino 55 nm wavelength 55 2nm 55 superconducting qubit 55 Active Galactic Nuclei 55 gravity warps 55 X ray observatories 55 panchromatic imagery 55 absorbance 55 stimulated emission 55 nonthermal 55 Higgs bosons 55 polarizing filter 55 emit X rays 55 diffusion MRI 55 X ray spectra 55 Spectrograph 55 geoneutrinos 55 -# degrees Fahrenheit [002] 55 tomographic images 55 absorb photons 55 HARPS spectrograph attached 55 Mercury magnetosphere 55 mercury cadmium telluride 55 sub angstrom 55 Microlensing 55 hexagonal mirrors 55 infrared spectrograph 55 gravitational waves 55 Array ALMA 55 hyper spectral 55 spectral fingerprint 55 intracluster 55 HD# [005] 55 masers 55 quantum dot lasers 55 diffract 55 beamwidth 55 aperture lens 55 spectra 55 detector arrays 55 AU Mic 55 filamentary 55 photosphere 55 interferometric observations 55 photocatalysts 55 stellar occultations 55 mT 55 circumstellar disks 55 stylus profilers 55 spectral measurements 55 single photon detectors 55 LWIR 55 X ray beam 55 Raman spectroscopy 55 electron optics 55 Cancri e 55 cosmic ray collisions 55 earthlike planets 55 THz 55 magnetotail 55 silicon monoxide 55 isotherms 55 dI dV 55 electron density 55 radial velocity technique 55 pointings 55 cosmic ray particles 55 sodium atoms 55 Imaging Spectrometer 55 wavefront distortion 55 infrared emitters 55 supersymmetric particles 55 X ray binary 55 impactors 55 laser pulses 55 millisecond pulsars 55 SDSS II 55 ultrabright 55 scanning tunneling microscopes 55 microvolts 55 laser excitation 55 Keck Telescope 55 thermal gradients 55 retrograde orbit 55 micromirror 55 photonic circuits 55 powder diffraction 55 radial velocity method 55 ESO PR 55 ultrasonic transducers 55 GRBs 55 electroluminescence EL 55 HiRISE images 55 atmospheric turbulence 54 Hanny Voorwerp 54 inelastic scattering 54 ultraviolet photons 54 Nikon D# Kowa 54 highly collimated 54 neutrino beam 54 Triangulum Galaxy 54 barred spiral galaxy 54 Earthlike 54 Circinus X 1 54 NGC# 54 extrasolar planet 54 microlenses 54 Raman spectroscopic 54 gravitational lensing 54 silicon nanowire 54 relativistic particles 54 Red Rectangle 54 Fabry Perot 54 Descent Imager Spectral Radiometer 54 electron volt 54 photon detection 54 ionospheric 54 Mercury exosphere 54 gravitational lenses 54 SN #A 54 dynamical processes 54 constellation Hercules 54 neutron beams 54 toroid 54 emits X rays 54 Infrared spectroscopy 54 Cosmic rays 54 gravitational wave 54 μm diameter 54 protons collide 54 wavelength lasers 54 tropospheric 54 gamma ray radiation 54 starburst galaxies 54 resonance imaging 54 ROSAT 54 #nm laser [002] 54 wavefront 54 horizontally polarized 54 gamma rays 54 chemiluminescence 54 accretion disks 54 magnetic excitations 54 #x magnification [002] 54 Bragg grating 54 moonlets 54 e MERLIN 54 downwelling 54 spectroscopic imaging 54 auroral displays 54 relativistic jets 54 laser speckle 54 Cepheids 54 Hawking radiation 54 nanolaser 54 constellation Centaurus 54 detect neutrinos 54 Force Microscopy 54 infra red radiation 54 aberration correctors 54 infrared telescope 54 gaseous planet 54 interstellar clouds 54 VB #b 54 neutrino detectors 54 emission spectroscopy 54 nanobubble 54 electrons emitted 54 temperature gradient 54 asteroidal 54 supercontinuum generation 54 LiNbO3 54 pulsed Doppler 54 coronal magnetic field 54 nanosecond pulse 54 electromechanical coupling 54 Crab Pulsar 54 fluorescence quenching 54 Chajnantor 54 deformable mirrors 54 crystal lattices 54 Nd YAG 54 magnetic monopole 54 induced fluorescence 54 terahertz 54 Crab Nebula 54 interferometric technique 54 interferogram 54 LORRI 54 plasmon 54 ion thrusters 54 NIRSpec 54 meridional flow 54 planets orbiting distant 54 dispersive 54 Type Ia 54 situ measurements 54 electron flux 54 cm -1 54 Bose Einstein condensates 54 Spitzer infrared spectrograph 54 permanently shadowed regions 54 microshutters 54 earthshine 54 emission nebula 54 meV 54 CMB photons 54 stellar seismology 54 neutrino particles 54 axions 54 periodic dimming 54 planet magnetosphere 54 planetary magnetospheres 54 Milky Way halo 54 Galactic cosmic rays 54 electron spins 54 quasar 54 weakly interacting 54 #.#μm [001] 54 bandgaps 54 Proxima Centauri 54 wavebands 54 WASP #b 54 Fermi LAT 54 Bessel beam 54 Bok globules 54 ENAs 54 irradiance 54 Samuel Oschin Telescope 54 multiphoton imaging 54 ionosphere 54 ultraviolet radiation emitted 54 UKIRT 54 linear polarization 54 light refracting 54 electromagnetic EM 54 Synthetic Aperture Radar 54 Nernst 54 wavefronts 54 electrophoretic 54 ab initio calculations 54 Orion nebula 54 lunar equator 54 Martian polar 54 longwave radiation 54 micromechanical 54 hyperspectral 54 Type 1a supernovae 54 moonquakes 54 galactic nucleus 54 Laser diodes 54 aboard ESA Envisat 54 indium gallium arsenide 54 tholins 54 photomultiplier 54 zodiacal dust 54 exciton 54 magnetic coil 54 energetic gamma rays 54 multibeam 54 5μm 54 spectral radiance 54 laser altimetry 54 crystalline silicates 54 Infrared Thermal Imaging Spectrometer 54 resonant tunneling 54 Anisotropy 54 photosensors 54 VIRTIS 54 ionized gas 54 model A# 54 UV VIS 54 coronal holes 54 neutral mass spectrometer 54 TrES 4 54 comet McNaught 54 star Beta Pictoris 54 Shackleton crater 54 ray Space Telescope 54 beam splitter 54 Si substrate 54 manganite 54 helium ion 54 nondestructively 54 outer corona 54 magnetically coupled 54 LAGEOS 54 #nm wavelength [001] 54 SSRL 54 vertically polarized 54 interacting galaxies 54 magnon 54 micromachined 54 brown dwarfs 54 aurorae 54 infrared spectrums 54 TGFs 54 HARPS instrument 54 optical atomic clocks 54 #nm #nm [001] 54 Unit Telescopes 54 De Pontieu 53 photodiode 53 #μm [001] 53 donor acceptor 53 microfocus 53 Magnetars 53 noctilucent clouds 53 Coma cluster 53 ejecta 53 neutron flux 53 electron ion 53 tungsten halogen 53 Super Kamiokande 53 moon Io 53 IBEX spacecraft 53 lunar crust 53 #nm #nm [002] 53 WFPC2 53 scanning tunneling microscopy 53 type Ia supernovae 53 Near Infrared NIR 53 Roque de los 53 scanning electron 53 thermopile 53 Ritchey Chrétien 53 temperature gradients 53 amplitude modulated 53 Comet Holmes 53 GeV 53 Ultra violet 53 Atacama Large Millimeter submillimeter 53 3He 53 cosmic microwave background 53 oblique angles 53 MRFM 53 nanomesh 53 Electromagnetic radiation 53 auroral emissions 53 emission spectra 53 nanosecond pulses 53 electro optical sensors 53 spectrographic 53 collisional 53 GRB# 53 basaltic rocks 53 post perovskite 53 paramagnetic 53 waveguides 53 radial velocity 53 photodiodes 53 neutrino experiments 53 scanning optical microscopy 53 optical aberrations 53 Bug Nebula 53 crustal thickness 53 emissivity 53 transfer FRET 53 magnifications 53 unaided eye 53 planet HD #b 53 ultraviolet lasers 53 xenon lamp 53 radiometric measurements 53 Millimeter wave 53 Borexino 53 femtosecond laser pulses 53 spectroscopic methods 53 PUVA psoralen plus 53 microcantilevers 53 isotherm 53 sensor arrays 53 magnetic dipole 53 carbon nanotube membranes 53 G#.# +#.# 53 cluster NGC 53 silicon waveguide 53 AKARI 53 photochemical reactions 53 Lagoon Nebula 53 candelas 53 picometer 53 GRB #A 53 transmission electron microscope 53 relativistic protons 53 electron bunches 53 HIRES spectrometer 53 IR spectra 53 DTEM 53 microfocus X ray 53 electron doped 53 ESA Integral 53 gaseous planets 53 heliopause 53 Hubble Space Telescope HST 53 hyperlens 53 HD #b [002] 53 optical microscope 53 laser altimeter 53 cantilever deflection 53 WFC3 53 infrared observatory 53 photothermal 53 #nm laser [001] 53 photodetectors 53 diffusion coefficients 53 electronic excitations 53 nanofabricated 53 TNOs 53 scintillator 53 supernova remnants 53 eclipsing binaries 53 Cryo EM 53 accretion disk 53 asteroseismology 53 Rydberg atom 53 GEO# 53 submicrometer 53 electromagnetically induced transparency 53 UVIS 53 indium gallium arsenide InGaAs 53 tokamaks 53 transiting exoplanets 53 extrasolar 53 NASA WMAP 53 fluorescence emission 53 Photonic crystals 53 spectral fingerprints 53 diffusivity 53 Ground penetrating radar 53 antiproton 53 quasiparticle 53 gamma ray observatories 53 absorption coefficient 53 x ray microscopy 53 wavelength tunability 53 electron accelerator 53 synchrotron emission 53 RXTE 53 photomultipliers 53 monolayer graphene 53 optical waveguides 53 Solar TErrestrial RElations Observatory 53 quantum mechanically 53 Trifid Nebula 53 electron scattering 53 millisecond pulsar 53 TSN PZ camera 53 WHIM 53 CCD camera 53 scanning microscopy 53 emission wavelength 53 Plasmonic 53 VIMOS 53 Type Ia supernova 53 scanning electron microscopy 53 exoplanets orbiting 53 coronal 53 Cosmic Microwave Background CMB 53 X ray detectors 53 WIYN 53 MeV 53 Mini SAR 53 X ray absorption spectroscopy 53 astrometric 53 Paranal Chile 53 reflection nebula 53 chlorophyll fluorescence 53 planetary nebulae 53 Casimir cavity 53 Faint Object 53 gamma ray energies 53 orbital resonance 53 nanoindentation 53 C1XS 53 Earthlike planets 53 Eta Carinae 53 adaptive optics