「Spectra」の共起表現一覧(1語右で並び替え)

Spectra

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  • FT-VCD spectra accumulation of the selected sample solution
  • The study of particle spectra allows us to see the global picture of partic
  • ecular complex by the constancy of absorption spectra and the decrease in sensitizer fluorescence l
  • excluded by the additivity of the absorption spectra and the different dependence on concentration
  • the cloud are relatively prominently in this spectra, and the composition of the ice can be determ
  • trument that measures the intensities, energy spectra, and angular distribution of energetic electr
  • known of which are the monograph Vibrational Spectra and Structure of Polyatomic Molecules (1939)
  • nce, optical absorption and photoluminescence spectra, and the concentration of isolated nickel can
  • spectra and analytical data
  • ts when examined by means of their absorption spectra, and consequently devised a new method of pre
  • Molecular Spectra and Molecular Structure: II.
  • The database includes 14700 1H NMR spectra and 13000 13C NMR spectra as well as FT-IR, R
  • ound apparent stimulated emission in hydrogen spectra and effected the first demonstration of stimu
  • This produces higher quality spectra and allows coupling constants to be reliably
  • ialized in the digital processing of infrared spectra and was awarded seven patents in that field.
  • Her tables of atomic spectra and energy levels, published by NBS, have rem
  • nd began writing "Hyperfine Structure in Line Spectra and Nuclear Spin".
  • optical telescope as of 2005) to measure the spectra and hence redshifts of approximately 60,000 g
  • the identification of peptides based on mass spectra and genome data.
  • ion with dark, featureless and moderately red spectra, and a moderate absorption feature shortwards
  • rs are requested not to download more than 50 spectra and/or compound information in one day.
  • nalysis of thin tissue slices when sequential spectra are acquired across a tissue surface that has
  • Deuterium NMR spectra are especially informative in the solid state
  • Vibrational spectra are in the near infrared (about 1 - 5 µm) and
  • g X-7 is in close proximity to Cyg X-3, their spectra are very different.
  • h spatial arrangements require that the ENDOR spectra are recorded at different magnetic field sett
  • Their absorption spectra are non-overlapping in order to broaden the r
  • The spectra are projected vertically, i.e., perpendicular
  • The illustrated spectra are from HNcoCA and HNCA experiments; used he
  • stered across the sample while secondary mass spectra are recorded.
  • rotational states, therefore pure rotational spectra are in the far infrared region (about 30 - 15
  • id-band 'mystery' noise", and where the noise spectra are plotted.
  • charged particles, magnetic fields and solar spectra, as well as doing geodetic research.
  • rmonicity of a vibration can be read from the spectra as the distance between the diagonal peak and
  • s, over 20,000 high-resolution ESI-QTOF MS/MS spectra at four collision energies, and over 100,000
  • spectrograph for obtaining spatially resolved spectra at resolutions approaching the diffraction li
  • spectra at different engine speeds when testing engin
  • Typical spectra at these wavelengths involve rovibrational ex
  • e performed the first observations of stellar spectra at the observatory, under the direction of th
  • He was the first to measure spectra below 200 nm.
  • DAF DB250 double-decker buses, 6 with Optare Spectra bodywork and 10 with Plaxton President bodywo
  • 1995, USA, Spectra Books (ISBN 0-553-57386-1), Pub date ?
  • These are generally "stony" spectra, but with significant deviations from the usu
  • HD and H2 do have very similar emission spectra, but don't emit on exactly the same frequenci
  • It improves the resolution of 1H NMR spectra by forming diastereomeric ion pairs.
  • stances, calculated from their VIS absorption spectra by the computer algorithm “Dichromaticity ind
  • By 1905 he had acquired hundreds of spectra by tedious point-by-point measurements with a
  • The data of the MS/MS spectra can be analyzed using software that is freely
  • mitted light with the incident, an absorption spectra can be obtained.
  • there are often ions of many elements, whose spectra can be seen in visible and ultraviolet light.
  • Spectra can be made more quantitative if necessary by
  • troduced in 1973, this replaced the original, Spectra Coated version of this lens; as well as impro
  • All New FD lenses were Super Spectra Coated, and thus the distinguishing nomenclat
  • 000 GTE lines in Missouri in partnership with Spectra Communications.
  • The observed spectra consist of neutral hydrogen Lyman alpha absor
  • ENDOR spectra contain information on the type of nuclei in
  • uring this time period focused on stars whose spectra contain absorption lines of elements includin
  • Tandem mass spectra contains specific information regarding the s
  • d fragmented in a mass spectrometer; the mass spectra corresponding to the fragments of peptide pre
  • cope also the ultraviolet part of the stellar spectra could be observed.
  • The advantage is an easy interpretation ( spectra data bases) of organic vapors without fragmen
  • e visible-wavelength (0.435-0.925 micrometre) spectra data was gathered between August 1993 and Mar
  • ernational Ultraviolet Explorer New Extracted Spectra) database.
  • This class is distinguished by optical spectra devoid of the broad emission lines characteri
  • DART produces relatively simple mass spectra, dominated by protonated molecules [M+H]+ in
  • th strong emission lines, BL Lac objects have spectra dominated by a featureless non-thermal contin
  • Spectra Energy Corp (NYSE: SE) is a S&P 500 company h
  • ed DCP Midstream Partner with ConocoPhillips, Spectra Energy was reported in 2005 to emit 19,746 to
  • Spectra Energy (77.53%)
  • The Algonquin Gas Transmission is owned by Spectra Energy Corp.
  • month Texas-based El Paso Midstream Group and Spectra Energy signed a memorandum of understanding t
  • In 2010, Spectra Energy was listed in the Newsweek green ranki
  • Empress/McNeill Spectra Energy Aerodrome, (TC LID: CFL2), is located
  • Other clients include Spectra Energy (formerly Westcoast Energy), and Fluor
  • Spectra Energy may be considered the single largest p
  • tion of the Rockies Express Pipeline with the Spectra Energy owned Texas Eastern Transmission pipel
  • A Spectra Energy (NYSE: SE,TSX: UNG.PR.C) company, Unio
  • It is owned by Spectra Energy.
  • Another Spectra Energy's project, known as Northern Bridge, w
  • The New Montreal FilmFest, produced by Spectra Entertainment (owners of the Montreal Spectru
  • rns fall short to reproduce experimental mass spectra, especically relative intensities among disti
  • The study and analysis of gamma-ray spectra for scientific and technical use is called ga
  • trument used with a telescope to measure star spectra for the Doppler effect to detect the presence
  • eres on Mars and Venus, based on the infrared spectra gathered from these planets.
  • as also revealed that since the new owners of Spectra had gone bankrupt, ownership of the company h
  • sity, anticrossing of the cyclotron-resonance spectra has been observed near the GaAs transverse op
  • If the spectra have also hyperfine structure the shift refer
  • Yet quasar spectra have revealed the presence of heavy elements
  • In reality EPR spectra have many different frequencies and not all o
  • d, where he exhibits regularly, first at Nova Spectra in The Hague, then, from 1971 on, in Amsterda
  • gh spectral resolution spectrograph to obtain spectra in 5 widely separated absorption lines simult
  • atic understanding of the rules behind string spectra in cases where only closed strings are presen
  • It includes the analysis of spectra in chemical terms, and the use of spectra to
  • h as in portal situations because it captures spectra in short time segments and produces a respons
  • stimate selectivity (amount of overlapping of spectra) in quantitative manner.
  • His work on the Second Order Raman Spectra in diamond and in alkali halide crystals has
  • divalent cations have different fluorescence spectra in the bound and unbound states.
  • Phytoene has typical absorption spectra in the UVB range with maximum at 286 nm and w
  • such observations by simultaneously obtaining spectra in a two-dimensional field.
  • taken place due to the shift in the political spectra in these countries.
  • H, Giraud B, Ripka G, "Projected Hartree-Fock Spectra In Light Nuclei", Physical Review Letters 15
  • absence of iron K-emission lines in the X-ray spectra indicates a rather small circumstellar matter
  • 32− ions have been made and their vibrational spectra interpreted as showing that they have C3v sym
  • Spectra is also used as a high-end wakeboard line.
  • its chosen for expressing wavenumber in Raman spectra is inverse centimeters (cm−1).
  • Otherwise, vibrational band of O-O from Raman spectra is 1122 cm-1.
  • S-S vibrational band from Raman spectra is 715 cm-1 in a gas phase.
  • n so that a second analyzer to generate MS/MS spectra is an obligation.
  • chain reaction, and the product, based on NMR spectra, is thought to be polycyclopropane.
  • Cusson signed with Spectra Jazz in 2010 to release worldwide his single
  • Its spectra must be collected on freshly purified samples
  • tained from other sources, such as rotational spectra, NMR spectroscopy or high-quality quantum-mec
  • romic shift is a phenomenon seen in molecular spectra, not atomic spectra; it is thus more common t
  • Photometric and Arecibo echo spectra observations in 2005 confirmed a 5 km (3 mi)
  • The spectra obtained by New Horizons shows that APL is an
  • seous objects in the universe detected in the spectra of quasars, with a column density larger than
  • colors of the object, often via a controlled spectra of light, even beyond the visible spectrum in
  • n of Richard C. Lord studying the vibrational spectra of organic molecules.
  • Such effects are more common in NMR spectra of aromatic and other non-flexible systems, w
  • We have to distinguish between the spectra of di-atomic molecules, which exhibit a prono
  • he study of spectrophotometry of stars and of spectra of comets.
  • n, occurs in the high-energy induced emission spectra of all chemical elements, since it results fr
  • the same technique to the measurement of the spectra of hydrogen and helium, reproducing the distr
  • He made many observations of the spectra of stars, and in particular he also did exten
  • red by Smith College to research the emission spectra of radium, resulting in her thesis "Spectrosc
  • Sample synthetic spectra of four components
  • e IRAM radiotelescope in Spain to analyse the spectra of radiation emitted from hot regions near a
  • Infrared and Raman Spectra of Polyatomic Molecules.
  • The analysis of 31P-NMR spectra of lipids could provide a wide range of infor
  • ave is suppressed so as to remove it from the spectra of the meters used for distortion measurement
  • ns made to the interpretation of the infrared spectra of molecules in terms of their vibrational mo
  • nts for the studies of ultra-violet and x-ray spectra of the sun and of the stars.
  • The spectra of the first quasars discovered, radio source
  • telescopes where there is a need to study the spectra of extended objects as a function of position
  • hange of the shape of the absorption/emission spectra of that spectral line.
  • However, in analyzing the spectra of 773 Irmintraud for the water of hydration
  • restegard and coworkers demonstrated that NMR spectra of certain proteins (in this case cyanometmyo
  • ectral sensitivities (normalized responsivity spectra) of human cone cells, S, M, and L types
  • hiev and Andrei Irimia, of the complete lower spectra of the beryllium-like to argon-like isoelectr
  • eting the signatures of star formation in the spectra of galaxies to understand the links between t
  • Absorbance spectra of free chlorophyll a (green) and b (red) in
  • Together with Carl Runge, he examined the spectra of chemical elements.
  • re-Brion and R.W. Field, Perturbations in the Spectra of Diatomic Molecules, Academic Press, 1986.
  • of rock emit different amounts and different spectra of natural gamma radiation.
  • Normalised absorption spectra of the three human photopsins and of human rh
  • His early work was on the absorption spectra of solutions, but he soon changed to the spec
  • As the spectra of these stars vary due to the Doppler effect
  • , derived from the analysis of optical and UV spectra of CTTS.
  • A spectrometer gathers (infrared) spectra of 108 brighter galaxies than magnitude 22 of
  • this five-year survey was to take images and spectra of millions of celestial objects.
  • The action spectra of chlorophyll molecules are slightly modifie
  • The combined spectra of the components is classified as A2 and the
  • cases, mediated by detection of the infra-red spectra of substances.
  • Much of his work at OSU involved the infrared spectra of molecules; particularly with regard to the
  • l February 1981, and returned high resolution spectra of hundreds of stars along with extensive X-r
  • calalogue the spectra of 336 pulsars, discovery of a radio pulsar 1
  • There, he studied emission lines in the spectra of certain hot stars, and studied gas clouds
  • rays by known crystals in measuring the X-ray spectra of metals.
  • The spectra of the V-type asteroids, as well as the HED m
  • of the irradiation parameters, the absorbance spectra of the chemical species, and the quantum yiel
  • xcitation gives rise to spectral lines in the spectra of astronomical objects such as planetary neb
  • The spiky infrared spectra of a candle flame happens to contain a number
  • in lunar samples, as well as infrared and UV spectra of interstellar dust.
  • included laboratory experiments regarding the spectra of metals.
  • Fluorescence spectra of colloidal CdTe quantum dots of various siz
  • ection rules, but are observed in vibrational spectra of real systems due to anharmonic couplings o
  • and the Single-Particle Electronic Excitation Spectra of Crystals", Methods in Computational Physic
  • ents on the Main and Isotopic Carbon Bands in Spectra of the R-Type Stars", Publications of the Ast
  • eloped by UCLA and Montreal, images and takes spectra of any companion to the star, with a spectral
  • wrote that it pioneered a way to measure the spectra of chemical reactions on the surface of an el
  • iniscent from the broad lines observed in the spectra of O and Wolf-Rayet stars.
  • By comparing the reflectance spectra of the angrites to that of several main belt
  • This is done by measuring the spectra of a standard substance at two different pH c
  • The UV-Visible spectra of MB33 in all mixtures investigated display
  • Author of the following papers: - 'The Spectra of Metallic Arcs in an Exhausted Globe' (with
  • usually have widely spread strong absorption spectra only in the Mid-IR, and the slow development
  • One obvious advantage of 2DIR spectra over normal linear absorption spectra is that
  • Spectra owns the Texas Eastern Pipeline (TETCo), a ma
  • Line Spectra performed at 2011's Canadian Music Fest durin
  • Switched Resistor ( Spectra Physics)
  • In 2000, Trimble merged with Spectra Precision.
  • From measuring rotational and vibrational spectra properties of molecules like the distance bet
  • In January 2010, LINE SPECTRA released their first full-length album Maps &
  • In March 2011 Line Spectra released the video for City Stars in both fre
  • sphines), making it useful to measure 31P NMR spectra routinely.
  • vocals in his former bands Divina Nocturna / Spectra Selene (1997-2004).
  • al identity involves at least three different spectra, sexual orientation being only one of them (t
  • Measured spectra show a peculiar excess in the 26 - 200 MeV en
  • nded by a warm circumstellar envelope and the spectra show silicon and carbon absorption up to a di
  • However the flash spectra showed that the abundance of atoms at great h
  • Infrared spectra shows the object contains water vapor and met
  • sodium, caesium and rubidium, and vibrational spectra shows that these contain the same planar ion.
  • However, molecules have spectra similar to those of a linear molecule or a sy
  • ids, and some outer main-belt asteroids, have spectra similar to Vesta, and are thus known as vesto
  • include high quantum yields, broad absorption spectra, size-tunable emission spectra, and good resi
  • 9 Optare Spectra SLF 8 Optare Tempo 9 Irisbus Agoraline 6 Opta
  • Infrared spectra subsequently taken with the IRS instrument on
  • Using spectra taken in 1986 with the violet band of RW Leon
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