「X-Ray」の共起表現一覧(1語右で並び替え)
該当件数 : 1013件
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 |
こんにちは ゲスト さん
ログイン |
Weblio会員(無料)になると 検索履歴を保存できる! 語彙力診断の実施回数増加! |
こんにちは ゲスト さん
ログイン |
Weblio会員(無料)になると 検索履歴を保存できる! 語彙力診断の実施回数増加! |