「XRAY」の共起表現(1語右で並び替え) - Weblio英語共起表現検索

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「XRAY」の共起表現一覧(1語右で並び替え)

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A substantial amount of the	X-ray absorbing gas may lie within 0.4 parsec (1.3 l
Dual-energy	X-ray absorptiometry (DEXA) showed mutant female mic
be performed at diagnosis, such as dual energy	X-ray absorptiometry (DXA) scanning, to identify ris
	X-ray Absorption Near Edge Structure (XANES)
	X-ray absorption spectroscopy (XAS) is a widely-used
spacecraft to investigate charged particle and	X-ray activity.
ibly owed in part to his support by his former	X-ray adviser Sir William Lawrence Bragg.
Leicester conducted an analysis of the burst's	X-ray afterglow with the XMM-Newton observatory.
e ICDD also publishes the journals Advances in	X-ray Analysis and Powder Diffraction.
In 1951, chemical and	X-ray analysis confirmed the principal constituents
scanning electron microscopes is equipped for	x-ray analysis allowing detailed elemental mapping.
	X-ray analysis shows D6h molecular symmetry with the
ientific community with the tools required for	X-ray analysis while continuing to educate and infor
ely to form crystalline compounds suitable for	x-ray analysis.
rad 8 carried aboard one experiment: the Solar	X-ray and Ultraviolet Monitor.
er in Texas noted for experimenting with early	X-ray and telegraphy equipment.
The wavelength of the impinging	x-ray and the crystal's lattice spacings are related
Eight millirem is about equal to a chest	X-ray, and 100 millirem is about a third of the aver
Solar astronomy - UV,	X-ray and possible infrared measurements of the sola
econd pulsars have been detected in the radio,	X-ray, and gamma ray portions of the electromagnetic
n important role in the evaluation of neutron,	X-ray and electron diffraction for the investigation
Note that 14" x 17" - the size of	X-Ray and MRI films - is indeed an international sta
of the Astronomical Netherlands Satellite, an	X-ray and gamma ray telescope located in space.
, surgical charges, drugs, nursing home costs,	x-ray and lab services.
ead using neutron flux, and to a lesser extent	X-ray and blast effects.
Women's Center, medical surgical, laboratory,	x-ray and health education services.
Higher energy	X-ray and Gamma-ray telescopes refrain from focusing
ysics, especially in the experimental areas of	X-ray and neutron diffraction.
Clusters of galaxies- using lensing,	X-ray and Sunyaev-Zeldovich data in conjunction to s
It will place cameras and	x-ray- and γ-detectors on the International Space Sta
Over the next few years, both	X-ray and optical emission from this remnant were al
tudent at the University of Chicago he studied	x-ray and electron scattering, and verified the Comp
MRI, CT, Plain	X-ray and Myelography is also available.
d Milislav Demerec in this very early field of	x-ray- and UV-induced mutations.
tro‐rivelatore Gamma a Immagini LEggero) is an	X-ray and Gamma ray astronomical satellite of the It
le of imaging distant celestial objects in the	X-ray and Gamma ray regions of the electromagnetic s
high throughput structural studies, including	x-ray and NMR.
icated the analysis of data from the sensitive	X-ray and gamma-ray instruments on board.
including clinical laboratory testing, general	x-ray and CT.
Techniques: Single crystal	X-ray and neutron diffraction, powder diffraction, s
The hard	X-ray and low-energy gamma-ray SIGMA telescope was a
ische Nederlandse Satelliet) was a space-based	X-ray and ultraviolet telescope.
tragalactic objects (galaxies, quasars, radio,	x-ray and infrared sources, etc.).
lectronic parts such as vacuum tubes (valves),	X-ray and microwave tubes and some lightbulbs.
ideo cameras, electronic locks, duress alarms,	x-ray, and magnetometers.
6, carrying instruments to detect ultraviolet,	X-ray and gamma ray emission.
sed gymnastics, powertherapy for treatment and	X-ray apparatus for diagnosis.
rly treadmill (Laudband), and in 1914 added an	X-ray apparatus to the machine in order to observe c
al attention at the time and failed to keep an	X-ray appointment at Sefton General Hospital.
phrenic angle can normally be seen as on chest	x-ray as a sharply-pointed, downward indentation (da
se commander, did not see the conclusion at LZ	X-Ray as the end of combat, and the Battle of la Dra
	X-ray astrometry becomes a serious concern that resu
Ray Burst Monitor (GRBM) on the Italian-Dutch	X-ray astronomy satellite BeppoSAX.
in Physics for his role in the development of	X-ray astronomy (1987)
wn as CORSA-b before launch) was Japan's first	X-ray astronomy satellite, developed by the Institut
n as Astro-B before launch, was Japan's second	X-ray astronomy satellite, developed by the Institut
He became first Director of the	X-ray Astronomy group in 1974.
The	X-ray astronomy satellite EXOSAT detected the source
The importance of	X-ray astronomy is exemplified in the use of an X-ra
Ginga was the third Japanese	X-ray astronomy mission, following Hakucho and Tenma
It was supposed to be Japan's first	X-ray astronomy satellite but was lost due to failur
Balloons for	X-ray astronomy have been used in a variety of count
Main article:	X-ray astronomy
Main article: Solar	X-ray astronomy
ird NASA Small Astronomy Satellite (SAS 3), an	X-ray astronomy mission, and then on the first High
Suzaku (formerly ASTRO-EII) is a Japanese	X-ray astronomy satellite launched on 10 July 2005 a
For example,	X-ray astronomy is nearly impossible when done from
Amateur	X-ray astronomy awaits the ingenious and determined
ng to SIMBAD, Serpens X-2 has been observed by	X-ray astronomy satellites and included in their res
He subsequently worked on	X-ray astronomy at UC Berkeley before returning to t
have been ignored during the early history of	X-ray astronomy when using sounding rocket X-ray ast
of over 700 refereed articles and head of the	X-ray astronomy group at the Institute of Astronomy.
merly named ASTRO-D) was Japan's fourth cosmic	X-ray astronomy mission, and the second for which th
Both	X-ray astronomy satellites were aimed at the J2000 c
renamed Ginga (Japanese for 'galaxy'), was an	X-ray astronomy satellite launched from the Kagoshim
Giacconi worked on the instrumentation for	X-ray astronomy, from rocket-borne detectors in the
three instruments; two of which were used for	x-ray astronomy, and one which was used to detect co
He is a pioneer	X-ray astronomy, leading the development and operati
rticular fields of expertise are astrophysics,	X-ray astronomy, cosmology and galactic astronomy.
He was a pioneer in the field of	X-ray astronomy.
ing astrophysicist who laid the foundations of	X-ray astronomy.
WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α,	X-Ray, Astrophoto, Sky Map, Articles and images
WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α,	X-Ray, Astrophoto, Sky Map, Articles and images
galaxy formation; stellar contributors to the	X-ray background and the evolution of neutral gas wi
Main article: Diffuse	X-ray background
servations of solar flares, the cosmic diffuse	X-ray background, and the observation of a single fl
g, relativistic iron line found in the diffuse	X-ray background, possibly due to a high metallicity
the	X-ray background.
ion research, including particle acceleration,	x-ray backlighting and laser-plasma instabilities (L
cattering experiments (neutron backscattering,	X-ray backscattering spectroscopy);
This star is moderately luminous in the	X-ray band, with a variable energy emission of 1032-
ss the electromagnetic spectrum as high as the	X-ray band.
ervatory dedicated to observing the sky in the	X-ray band.
5B carries ion chambers nominally covering the	X-ray bands: 0.1-0.8
The DMX is well founded	X-ray based on sound scientific principles.
oticed that something was wrong and halted the	X-ray beam, but merely displayed the word "MALFUNCTI
In 1972 the first	x-ray beamline was constructed by Ingolf Lindau and
ion sources, which provide intense and tunable	X-ray beams.
It was named Camp	X-Ray because various temporary camps in the station
, all placements should be verified by a chest	X-ray before the line can be used.
	X-ray binaries, SNR, gravitational lenses etc.
in theory of accretion and in astrophysics of	x-ray binaries, together with Rashid Sunyaev he is p
f Amsterdam in 1983 working on observations of	X-ray binaries.
cteristics strongly resemble those of accepted	X-ray binaries.
erpretation of the timing behavior of low-mass	X-ray binaries.
Circinus X-1 is an	X-ray binary star system that includes a neutron sta
Cygnus X-2 is a bright, persistent, low-mass	X-ray binary (LMXB) that varies on time-scales from
V4641 Sagittarii (V4641 Sgr) is a variable	X-ray binary star system in the constellation Sagitt
Vela X-1 is a pulsing, eclipsing high-mass	X-ray binary system, associated with the Uhuru sourc
4U 0614+091 is an	X-ray binary star system which features a neutron st
phiuchi (a DQ Herculis variable), the low-mass	X-ray binary V2293 Ophiuchi, 80 ROSAT visibly dark X
He specializes in radio galaxies,	X-ray binary systems, astrometry, and general relati
Cygnus X-3 is considered a high-mass	X-ray binary (HMXB), because V1521 Cyg is a high-mas
These candidates are all members of	X-ray binary systems in which the compact object dra
terpart of spectral type K3-K7V for a low-mass	X-ray binary (LMXB) Centaurus X-4 at about 53 amin f
The optical companion of this low-mass	X-ray binary is a subgiant F star.
ar so that the binary 4U 1755-33 is a low-mass	X-ray binary (LMXB).
lso known as 4U1656+35, is a moderately strong	X-ray binary source first studied by the Uhuru satel
4U 1642-45, according to SIMBAD is a low-mass	X-ray binary (LMXB) for which the astronomical visua
and Crab Nebula, and the Cygnus X-1 high mass	X-ray binary system, which are two of the brightest
TrA X-1 is a low-mass	X-ray binary (LMXB).
V420 Aurigae is high mass	X-ray binary star.
The system is a low-mass	X-ray binary (LMXB).
e Bursting Pulsar (GRO J1744-28) is a low-mass	x-ray binary with a period of 11.8 days.
s declination (Dec) -42° 58′ 08.1″, a low-mass	X-ray binary (LMXB).
high-mass	X-ray binary: AX J1820.5-1434 and V479 Scuti,
as how a particular protein breaks down under	X-Ray bombardment.
sounding-rocket-borne exposure to three of the	X-ray brightest binary sources in our galaxy: Her X-
	X-ray burst oscillations and quasi-periodic oscillat
A new type of	X-ray burst which emits thermal hard X-rays with a s
The solar	X-ray burst of March 30, 1969, is considered to be b
Some 150	X-ray bursts in the energy band 3.0 to 4.5 keV occur
ar gamma-ray bursts (GRBs) above 300 keV, soft	X-ray bursts (152 d), hard X-ray bursts (158 d) abov
ransfer, non-radial oscillations during Type-I	X-ray bursts and the cooling of magnetars.
al content (measured as the attenuation of the	X-ray by the bones being scanned) is divided by the
The	X-Ray Cafe was a small music venue in Portland, Oreg
The	X-Ray Cafe was the site of a small but controversial
x Rich and I engaged Leslie in 1955 to do some	x-ray calculations for us, since in those days elect
aphy equipment to include machine gun cameras,	x-ray cameras, radar cameras, gun synchronizers, and
cluding a dementia screening blood test, chest	X-Ray, CAT scan and ECG.
ooling flow in high density cooling centers of	X-ray cluster halos.
Vanguard Imaging; and Florida-based Palm Beach	X-Ray Company in 1999 with the expressed hope of rai
show no nuclear optical continuum or reflected	X-ray component, although they do occasionally show
One of the	X-ray components (A) in the Cloverleaf is brighter t
The describers of the specimens used	X-ray computed tomography scanning, or CT scanning,
symposia as well as sponsorship of the Denver	X-ray Conference.
of illumination of cold heavy elements by the	X-ray continuum.
The two	X-ray contrast media iodine and barium have ideal K
gl X-1, in turn, has been determined to be the	X-ray counterpart to V1333 Aql with a likely orbital
The	X-ray crystal structure was solved in 2003 by J. Abr
Representation of the	x-ray crystal structure of Tus-Ter protein-DNA compl
The	x-ray crystal structure of the TPP riboswitch aptame
it to catalyze this fundamental reaction, the	X-ray crystal structure has been solved.
	X-ray crystal structures have been determined for se
es with Professor Arthur J. C. Wilson, a noted	X-ray crystal physicist.
Examination of the human	X-ray crystal structure suggests that this residue (
The lack of electron density in	X-ray crystallographic studies may also be a sign of
rd was for mouse VDAC-1 crystals determined by	X-ray crystallographic techniques.
According to	X-ray crystallographic studies, the copper(I) ion is
4)PtCl3]−, the anion of Zeise's salt, based on	X-ray crystallographic data
Trinity College Cambridge and then researched	X-ray crystallography of Imperfect Crystals for his
Electron cryo-microscopy (cryoEM) and	X-ray crystallography have provided a wealth of stru
d has been characterized in the solid phase by	X-ray crystallography as a bent molecule with an ang
to the argonaute protein has been examined by	X-ray crystallography of the binding domain of an RN
ctures for the analysis of proteins using NMR,	X-ray crystallography and mass spectrometry.
It is used in the fields of	X-ray crystallography and NMR analysis.
of T4 lysozyme, determined their structure by	x-ray crystallography and measured their melting tem
s one of the smallest, yet stable, cyclophanes	X-ray crystallography shows that the aromatic bridge
Bond lengths deduced from	X-ray crystallography are consistent with a cyclohex
l structures that would fit both the available	X-ray crystallography data and a set of chemical res
tween 1982 and 1985, the three scientists used	X-ray crystallography to determine the exact arrange
and proton exchange is effected, and as yet no	X-ray crystallography structure of gamma secretase i
	X-ray crystallography indicates that this domain for
	X-ray crystallography shows that this domain forms a
Boylan did graduate research in	X-ray crystallography at the University of Illinois
rement of the molar volume of silicon, both by	X-ray crystallography and by the ratio of molar mass
ase was determined by Millard et al. (1999) by	X-ray crystallography (PDB codes: 2wfz, 2wg0, 2wg1,
in methods development and the application of	X-ray crystallography in fundamental studies.
	X-ray crystallography studies have confirmed binding
e archeael homologue of XPB has been solved by	X-ray crystallography by Dr. John Tainer and his gro
aids the structure elucidation of proteins by	X-ray crystallography using multi-wavelength anomalo
is possible because the desired pixel size for	X-ray crystallography is around 100 micrometres, and
hyde in the late 19th century, as confirmed by	x-ray crystallography in 1951.
transform relating the experimental data from	X-ray crystallography (in reciprocal space) to real-
bacillus stearothermophilus) was determined by	X-ray crystallography to a resolution of 1.9 A. The
	X-ray crystallography
	X-ray crystallography indicates that the Xe-Xe bond
he structure of Nerve Growth Factor, solved by	X-ray crystallography and published in 1991 by Tom B
A with acetylcholinesterase has been solved by	X-ray crystallography (PDB code: 1VOT; see the 3D st
His research explores ways of using	X-ray crystallography to provide rapid and accurate
In 1978, its structure was determined by	x-ray crystallography by Stephen C. Harrison.
in purple bacteria, and subsequently applying	X-ray crystallography to elucidate the protein's str
eloper teams on the PHENIX software system for	x-ray crystallography of macromolecules, and hosts t
the techniques of structural biology (such as	X-ray crystallography or NMR) to determine the 3-D s
d Raman spectroscopy, electron microscopy, and	x-ray crystallography (x-ray diffraction).
The green tetrahydrate has been determined by	X-ray crystallography to be octahedral about the cen
	X-ray crystallography indicates that zethrene is a p
Many techniques, like	X-ray crystallography and NMR spectroscopy, are wide
Structure of myoglobin determined by	x-ray crystallography

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共起表現