「X-ray」の共起表現(2語左で並び替え)

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共起表現

「X-ray」の共起表現一覧(2語左で並び替え)

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Eight millirem is about equal to a chest	X-ray, and 100 millirem is about a third of the aver
winds from this pair makes the system a strong	X-ray source.
The knot is a prominent	X-ray feature, consisting of a number of filaments c
V4641 Sagittarii (V4641 Sgr) is a variable	X-ray binary star system in the constellation Sagitt
different ROSAT sources within 1° and a Rossi	X-ray Timing Explorer source designated XTE J1704-44
T observed that τ Sco was a star with a harder	X-ray spectrum than usual for B0V stars.
al Netherlands Satellite (ANS) detected a soft	X-ray flare on YZ CMi which is unaccompanied by visu
, all placements should be verified by a chest	X-ray before the line can be used.
al inspection methods would require using a 2D	X-ray of the component or the use of destructive tes
Cygnus X-3 is considered a high-mass	X-ray binary (HMXB), because V1521 Cyg is a high-mas
Development of a novel	X-ray detector technique for use in medical imaging;
A knee	x-ray of a patient with ACDC reveals calcification i
InFOCμS (2004+) - a hard	X-ray telescope with a 49 cm2 collecting area.
es with Professor Arthur J. C. Wilson, a noted	X-ray crystal physicist.
s X-4, and that Scorpius X-4 is not a separate	X-ray source.
analysis (NCESS), which has a high-resolution	x-ray photoelectron spectroscopy machine to probe ne
s built between 1978 and 1980 as a synchrotron	x-ray facility tied to the Cornell Electron Storage
The detector end of a simple	x-ray diffractometer with an area detector.
terpart of spectral type K3-K7V for a low-mass	X-ray binary (LMXB) Centaurus X-4 at about 53 amin f
atmospheric temperature and moisture, a solar	x-ray imager to detect solar flares, and instruments
oratory was established in 1975 and a portable	X-ray machine purchased.
ar so that the binary 4U 1755-33 is a low-mass	X-ray binary (LMXB).
Suzaku (formerly ASTRO-EII) is a Japanese	X-ray astronomy satellite launched on 10 July 2005 a
A soft	X-ray solar imaging telescope is on board the GOES-1
ts of a mirror spacecraft that carries a large	X-ray telescope, with a mirror area of about 5 m² an
4U 1642-45, according to SIMBAD is a low-mass	X-ray binary (LMXB) for which the astronomical visua
1989 the Japanese Ginga Team discovered a new	X-ray source that was cataloged as GS 2023+338.
iting Solar Observatory, OSO 3, carried a hard	X-ray experiment (7.7 to 210 keV) and an MIT gamma-r
A faint	X-ray halo has been detected around Venus.
AGR 1627-41 is a persistent	X-ray source.
A transient	X-ray source first discovered in 1996 by the Italian
A second	X-ray source detected on only one scan during the Ap
The detectors will include a wide-field	X-ray imager with an energy resolution of 150 eV at
TrA X-1 is a low-mass	X-ray binary (LMXB).
He is a pioneer	X-ray astronomy, leading the development and operati
The system is a low-mass	X-ray binary (LMXB).
Finally, it is a soft	X-ray transient because it periodically emits short
ische Nederlandse Satelliet) was a space-based	X-ray and ultraviolet telescope.
is granted sentience/sapience from a dentist's	x-ray machine.
e Bursting Pulsar (GRO J1744-28) is a low-mass	x-ray binary with a period of 11.8 days.
On board is a hard	X-ray detector (27-189 keV) with a 5.1 cm2 NaI(Tl) s
ography unit: The CBCT unit uses a cone-shaped	X-ray rather than a linear one to create three-dimen
s declination (Dec) -42° 58′ 08.1″, a low-mass	X-ray binary (LMXB).
n of gas and dust near the AGN that absorb the	X-ray emission.
According to	X-ray crystallographic studies, the copper(I) ion is
According to	X-ray diffraction analysis, the reagent traded under
nd is reported as stable and with according to	X-ray crystallography a chairlike tricyclic silicon
According to	X-ray crystallography, it binds Fe3+as a 1:1 complex
These accreting millisecond	X-ray pulsars are thought to be the evolutionary pro
A total of thirteen accreting millisecond	X-ray pulsars have been discovered as of January 201
He was selected by NSF to acquire an	X-ray diffractometer and has been a pioneer in apply
rly treadmill (Laudband), and in 1914 added an	X-ray apparatus to the machine in order to observe c
e ICDD also publishes the journals Advances in	X-ray Analysis and Powder Diffraction.
estion remained unanswered until the advent of	x-ray diffraction in the 20th century.
gator on television consumer affairs programme	X-Ray.
After an	X-ray examination, doctors diagnosed Yang's injury a
es are universally used as contrast agents for	X-ray procedures.
ectroscopy, and Circular Dichroism, along with	X-ray crystallography.
by the Sojourner rover using its Alpha Proton	X-ray Spectrometer.
and performed another overnight alpha particle	X-ray spectrometer integration.
physical properties package, an alpha particle	X-ray spectrometer, a magnetometer, a seismometer, a
An Alpha Particle	X-Ray Spectrometer (APXS) (or Alpha Proton X-Ray Spe
Alpha particle	X-ray Spectrometer (APXS) (Courtesy NASA/JPL-Caltech
See also: Astrophysical	X-ray source
s atmosphere, X-radiation from an astronomical	X-ray source has been discovered coming from Scorpiu
ulum Australe X-1 (TrA X-1) is an astronomical	X-ray source discovered in November 1974 after the X
Bromide is also radiopaque, so an abdominal	x-ray may also help in the diagnosis.
0426-10 is the designation for an astronomical	X-ray source detected by the X-ray observatory satel
An advanced	X-ray imaging technique called called X-ray tomograp
Hydra A is an astronomical	X-ray source.
(22 March 1924 - 28 May 1997) was an American	x-ray engineer, competition rower and Olympic champi
ho invented a method of fabricating an imaging	X-ray spectrometer.
Coolidge - Physicist who invented an improved	X-ray tube, developed the tungsten filament for the
2 pm on April 2, 1997, is from an astronomical	X-ray source never seen before in the constellation
nal astrometry to confirm that an astronomical	X-ray source really is the same as an astronomical v
aterials using neutron radiation analogical to	X-ray techniques.
Microprobe analyses and	X-ray powder-diffraction studies indicate extensive
was successfully crystallized and analyzed by	X-ray diffraction in 2003.
West Pacific LORAN-C Chain ( GRI 8930) and the	X-Ray Secondary of the East Asia LORAN-C chain ( GRI
October 11, 1966, is to localize and identify	X-ray sources in the Cygnus region.
ions of IC 2497 with the XMM-Newton and Suzaku	X-ray space telescopes to probe the current activity
to show the wave nature of gamma rays, and on	X-ray spectra.
esigned jointly by the USSR and France, and an	X-ray spectroscope onboard.
lications such as capsule endoscopy and dental	x-ray systems, scientific imaging, automotive safety
the Crimean Astrophysical Observatory, and two	X-ray telescopes.
ace (they would have been detected and medical	X-ray machines would not work if this was not the ca
t (dye) is injected through the cervix, and an	x-ray technologist takes photos of the Essure coils
less energetic in the soft gamma-ray and hard	X-ray range, and repeated bursts came from the same
for visible, near infrared, and soft and hard	X-ray frequencies.
In 1979, he and fellow	X-Ray Spex drummer BP Hurding formed alongside singe
fraction, electron microscopy, and synchrotron	x-ray diffraction.
ion sources, which provide intense and tunable	X-ray beams.
Another early	X-ray observatory satellite Uhuru detected TrA X-1 a
She first appears when	X-ray gets credit for a gold tube of Kate Barlow's l
in methods development and the application of	X-ray crystallography in fundamental studies.
phic research pioneering optical approaches to	x-ray diffraction based on the Fourier transform.
several modified versions of the APS (without	X-ray spectrometer) or APXS have been flown: Surveyo
But, there are several	X-ray objects near the position of Oph XR-1.
ts for unknown reasons, so these are transient	X-ray pulsars that are observed only intermittently,
Intermediate polar systems are strong	X-ray emitters.
thin the error box for Cyg X-4 are twenty-four	X-ray sources in the SIMBAD database.
Within 2° of Ara XR-1 are forty	X-ray sources including 4U 1705-44 and [ KRL2007b] 2
rticular fields of expertise are astrophysics,	X-ray astronomy, cosmology and galactic astronomy.
ysics, especially in the experimental areas of	X-ray and neutron diffraction.
radio wavelengths by the Very Large Array, and	X-ray wavelengths by the XMM-Newton satellite.
Main article: Solar	X-ray astronomy
Main article: Extrasolar	X-ray source astrometry
Main article: Astronomical	X-ray source
Main article: Astronomical	X-ray sources
Main article: Astronomical	X-ray source catalog
Main article: Lockheed	X-ray source
Main article: Diffuse	X-ray background
Zinc iodide is often used as an	x-ray opaque penetrant in industrial radiography to
aries at the same 4.8-hour orbital rate as the	X-ray emissions, and they occur a few days before th
ss the electromagnetic spectrum as high as the	X-ray band.
That Vega is regarded as an	X-ray source rests on one 4.8 s star-tracking observ
As an	X-ray source, NGC 4151 was apparently first so detec
Speed Observations of Be Stars Associated with	X-Ray Sources.
in theory of accretion and in astrophysics of	x-ray binaries, together with Rashid Sunyaev he is p
Al Yafi (born c.1970), Yemeni prisoner at Camp	X-ray
se commander, did not see the conclusion at LZ	X-Ray as the end of combat, and the Battle of la Dra
of the final major North Vietnamese push at LZ	X-Ray on the former C Company line which was then he
t contribute to anomalous scattering at normal	X-ray wavelengths used for X-ray crystallography .
Detainees upon arrival at Camp	X-Ray, January 2002
nsity of the Crab Nebula is various at various	X-ray energies, conversion of the Crab to another un
olution, as long as crystals are available, as	x-ray diffraction needs numerous copies of the molec
her husband on the team of BAFTA award winning	X-Ray.
Balloons for	X-ray astronomy have been used in a variety of count
A detailed atomic structure for hERG based on	X-ray cystallography is not yet available, so struct
he central carbon atom of around 130° based on	X-ray diffraction.
ost often used to identify substances based on	x-ray diffraction data, and is designed for use with
4)PtCl3]−, the anion of Zeise's salt, based on	X-ray crystallographic data
gl X-1, in turn, has been determined to be the	X-ray counterpart to V1333 Aql with a likely orbital
any of the ROSAT sources are likely to be the	X-ray source detected by the March 15, 1963, Aerobee
According to SIMBAD, there may be five	X-ray sources either on the border between Sagittari
, electron lithography, electron beam welding,	X-Ray tubes, and free electron lasers.
He also became a	X-Ray technician working in Nevada.
reason for the invention, is that because the	X-ray source-point is swept electronically, not mech
ill capture material and temporarily become an	X-ray pulsar.
rs to believe that GRB 031203 may have been an	X-ray flash, viewed off-axis, or a member of a previ
It is injected intravenously before taking	X-ray images to increase arterial contrast in the fi
ith the Associated Press, and instead began an	x-ray equipment business.
The local doctor then shows Ben an	X-ray of Quish's head, which reveals that there is a
ents and to postulate correlations between the	X-ray structure and the physical properties of fibro
rement of the molar volume of silicon, both by	X-ray crystallography and by the ratio of molar mass
The Broad Band	X-ray Telescope (BBXRT) was flown on the space shutt
She is the brother of	X-Ray.
data from NASA's Swift Gamma-Ray Burst Mission	X-ray space telescope, from a precursor star in the
reen converts the photon energy emitted by the	x-ray tube into visible light on the diodes.
be damaged or destroyed by near-instantaneous	x-ray vaporization of its surface resulting in an in
detected and quantified in mixtures by powder	x-ray diffraction.
and are often discovered incidentally by chest	X-ray.
s in the crystal, frequently measured by using	X-Ray Photoelectron Spectroscopy to compare the rati
of illumination of cold heavy elements by the	X-ray continuum.
hether the ionization energy is provided by an	X-ray photon, an ultraviolet photon, EUV photon, or
Oph X-1 is an observation by the	X-ray observatory satellite Uhuru during its first y
e hospital and it was caused by nitrocellulose	x-ray film that ignited when an exposed light bulb w
pounds are usually evaluated by single-crystal	X-ray crystallography, focusing both on the overall
It will place cameras and	x-ray- and γ-detectors on the International Space Sta
a Renal Dialysis Unit, Cardiac Catheter Suite,	X-ray, CT, PET and MRI Scanners, with extensive outp
.2V) that shows O VI superionization caused by	X-ray ionization and the Auger ionization effect.
which especially pertain to the use of CCDs in	X-ray detectors can be coupled with practical books
a detector plane of 32,768 four mm CdZnTe hard	X-ray detector tiles; it is purpose-built for Swift.
ooling flow in high density cooling centers of	X-ray cluster halos.
orphous solids were initially characterised by	X-ray diffraction.
tobacter vinelandii has been characterised via	x-ray crystallography in both ADP tetrafluoroalumina
researcher in materials characterization with	x-ray diffraction and on the structural analysis of
aesium and rubidium have been characterized by	X-ray crystallography.
roduct mixture was more fully characterized by	X-ray crystallography and Nuclear Magnetic Resonance
In 1951, chemical and	X-ray analysis confirmed the principal constituents
reveal "filarial dance sign" in chylus fluid;	X-ray tests can show calcified adult worms in lympha
ies were subsequently discovered as a class of	X-ray emitters.
kely black hole systems that are classified as	X-ray novae.
diation" after he first discovered it close to	X-ray tube anodes.
An all-ages and community-oriented club, the	X-Ray played a "heavyweight role in shaping Portland
A combined Hubble/Spitzer/Chandra	X-Ray Observatory image of M 82.
tention more to his own record company, called	X-Ray Records/Rayvano Productions.
tmosphere are sometimes blind when compared to	X-ray telescopes.
ties such as CT, MR, and Computed Radiography (	x-ray) devices for image capture.
ce the 1950s or earlier , but was confirmed by	X-ray diffraction analysis only in 2005
ch as NaCl and CsCl were later confirmed using	X-ray crystallography.
ReB2 without any other phases, as confirmed by	X-ray crystallography.
ve-like nature of X-rays was confirmed through	X-ray scattering experiments on crystalline solids.
hyde in the late 19th century, as confirmed by	x-ray crystallography in 1951.
c synthesis and the structure was confirmed by	x-ray crystallography.
Sco X-6 is considered an	X-ray transient, black hole candidate.
5, on November 12, 1974, and is considered an	X-ray transient, possibly an X-ray nova or long-peri
n observed by Ariel 5 (A), it is considered an	X-ray transient (T), AT 0214+013.
It also contains several	X-ray sources, thought to be close binary star syste
The image at the right contains 56	X-ray objects: 36 are visibly dark X-ray sources det
The fourth Uhuru catalog contains one	X-ray source detected early within the constellation
em in their native environment, in contrast to	X-ray crystallography, which generally requires plac
The terminal has cooling rooms,	X-ray equipment, radiation detection, dangerous good
servations of solar flares, the cosmic diffuse	X-ray background, and the observation of a single fl
ANS could measure	X-ray photons in the energy range 2 to 30 KeV, with
, 30 parking bays, 72 immigration counters, 15	X-ray screening areas, for less waiting times, duty-
5B carries ion chambers nominally covering the	X-ray bands: 0.1-0.8
d been defined, Delhaize and coworkers applied	X-Ray Fluorescence (XRF) for the successful multi-el
d in 1984 for his innovation and creativity in	X-ray laser physics.

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「X-ray」の共起表現一覧(2語左で並び替え)