「SPECTROSCOPIC」の共起表現(1語右で並び替え)

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共起表現

「SPECTROSCOPIC」の共起表現一覧(1語右で並び替え)

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effects of weak gravitational lensing) and	Spectroscopic All Sky Cosmic Explorer (SPACE, to measure
A	spectroscopic analysis showed it to have a composition v
Biochemical and Mass	Spectroscopic analysis revealed that this pyroptosome is
	Spectroscopic analysis indicates the possible presence o
of predictive models for use in real-time	spectroscopic analysis of materials.
trophysics (ASCA) for a spatially resolved	spectroscopic analysis of Abell 2256 over the energy ban
Modern	spectroscopic and spectrometric techniques have since su
Xi Tauri a	spectroscopic and eclipsing triple star.
the subject of numerous X-ray diffraction,	spectroscopic and theoretical studies.
mmonly used in fluorescence microscopy and	spectroscopic applications for selection of the excitati
The	spectroscopic assignment of these states follows the Ryd
Both bright stars are	spectroscopic binaries and have at least one closer comp
binary star, whose two components are both	spectroscopic binaries themselves, making a four-star sy
-class stars, are themselves thought to be	spectroscopic binaries, bringing the total number of sta
due to the Doppler effect, they are called	spectroscopic binaries.
us Doppler shift analysis included face-on	spectroscopic binaries.
aries detected in this manner are known as	spectroscopic binaries.
ures of variable stars, cluster stars, and	spectroscopic binaries; and astrometry of minor planets
This is a single-lined	spectroscopic binary system.
3 Camelopardalis is a	spectroscopic binary in the constellation Camelopardalis
SBC7 is an acronym for	Spectroscopic Binary 7th Catalogue.
It consists of a	spectroscopic binary and a third component.
12 Camelopardalis is a	spectroscopic binary in the constellation Camelopardalis
V373 Cas is a	spectroscopic binary in the constellation Cassiopeia.
V357 Carinae (a Car, a Carinae) is a	spectroscopic binary in the constellation Carina.
Theta-1 Sagittarii is a	spectroscopic binary lying 617 light years from Earth.
θ1 Crucis (θ1 Cru, Theta1 Crucis) is a	spectroscopic binary star in the constellation Crux.
The star e Serpentis (e Ser) is a	spectroscopic binary in the constellation of Serpens.
It is a	spectroscopic binary whose components have an orbital pe
It is a	spectroscopic binary whose components have an orbital pe
It is a	spectroscopic binary with an orbital period of 143.6065
Pi Andromedae (π And, π Andromedae) is a	spectroscopic binary in the constellation Andromeda.
It is a	spectroscopic binary and has a companion located 0.12 ar
Secondary, Σ 1694 B is a	spectroscopic binary both A-type main sequence star.
It is a	spectroscopic binary whose two components are separated
104 Aqr A is a	spectroscopic binary and is suspected to be variable.
VV Corvi (VV Crv) is a close	spectroscopic binary in the Corvus constellation.
Lambda Andromedae is a	spectroscopic binary with an orbital period of 20.52 day
It is a	spectroscopic binary with an orbital period of 134 days.
θ2 Crucis (θ2 Cru / Theta2 Crucis) is a	spectroscopic binary star in the constellation Crux.
Theta Cephei is a white	spectroscopic binary star, located about 135 light-years
First discovered	spectroscopic binary in 1889 by an American astronomer E
Carl Vogel, Pickering discovered the first	spectroscopic binary stars.
Alpha Equulei is a unique	spectroscopic binary star consisting of two components.
Zeta Trianguli Australis (ζ TrA) is a	spectroscopic binary in the constellation Triangulum Aus
It is a	spectroscopic binary whose components have magnitudes of
Pi4 Orionis (π4 Ori, π4 Orionis) is a	spectroscopic binary star in the constellation Orion.
The star has been found to be a	spectroscopic binary star.
It is a	spectroscopic binary with a faint class-G companion.
31 Camelopardalis is an eclipsing	spectroscopic binary in the constellation Camelopardalis
de determination the orbital period of A's	spectroscopic binary difficult.
17 Leporis (17 Lep) is a	spectroscopic binary star in the constellation of Lepus.
Beta Cephei is a triple star comprising a	spectroscopic binary with a magnitude 8 optical companio
ilon Sagittarii (υ Sgr, υ Sagittarii) is a	spectroscopic binary star system in the constellation Sa
Theta Aquilae is a	spectroscopic binary classified as a blue-white B-type g
omponent, Iota Trianguli Australis A, is a	spectroscopic binary with a mean apparent magnitude of +
(ε Her, ε Herculis) is a fourth-magnitude	spectroscopic binary star in the constellation Hercules.
Iota Arietis is a	spectroscopic binary classified as a yellow G-type super
of the system components, A and B, form a	spectroscopic binary that completes an orbit every 76 ye
It is a	spectroscopic binary with components that are too close
anis Majoris (ζ CMa, ζ Canis Majoris) is a	spectroscopic binary in the constellation Canis Major.
Gliese 678 is a	spectroscopic binary star system approximately 60 light-
HD 176051 is a	spectroscopic binary star system located approximately 4
It is also a	spectroscopic binary star with a period of almost 273 da
resolved Pismis 24-1SW and the unresolved	spectroscopic binary Pismis 24-1NE.
In 1898 this system was reported to be a	spectroscopic binary system, with an orbital period of 2
omedae (Eta And, η Andromedae, η And) is a	spectroscopic binary star in the constellation of Androm
Rho Tucanae is a	spectroscopic binary composed of two yellow-white F-type
Nu Andromedae is	spectroscopic binary whose components are a blue-white B
Chi Aurigae is a	spectroscopic binary which is classified as a blue-white
The system consists of a	spectroscopic binary with a yellow G-type supergiant and
rferometer was used to resolve a number of	spectroscopic binary systems, including Alpha Andromedae
name HR 2422 Monocerotis or HR 2422) is a	spectroscopic binary at a distance of around 6600 light-
Kappa Velorum is	spectroscopic binary which is classified as a blue-white
The star has also been identified as a	spectroscopic binary with a period of 494 days, but the
Atik is a	spectroscopic binary star consisting of a spectral type
It is a	spectroscopic binary having a 113.8 day period, indicati
The orbit of a	spectroscopic binary is determined by making a long seri
Kappa Arietis is a	spectroscopic binary which is classified as a white A-ty
omedae was discovered to be a double-lined	spectroscopic binary in a series of spectra taken in 189
ae (V415 Car or A Carinae) is an eclipsing	spectroscopic binary of the Algol type in the constellat
s (τ CMa, τ Canis Majoris) is an eclipsing	spectroscopic binary in the constellation Canis Major an
l magnitude of approximately 5.15 and is a	spectroscopic binary star which consists of two giant st
The system itself has been identified as a	spectroscopic binary star system; this means that Delta
Tau Puppis is also a	spectroscopic binary star system in which the multiple c
This star is suspected of being a	spectroscopic binary, although this has not yet been con
It is a	spectroscopic binary, whose components are separated by
A suspected	spectroscopic binary, it has now been resolved by speckl
It is a suspected	spectroscopic binary, although this has not been confirm
The primary is a	spectroscopic binary, and its close companion completes
This is a	spectroscopic binary, which means that the individual co
This star is a	spectroscopic binary, and the primary is also a Beta Cep
They are a	spectroscopic binary, meaning the separation between the
It is a	spectroscopic binary, and the two subcomponents have app
It is a	spectroscopic binary, which means it is a binary star wi
Nu Scorpii A is itself a semi-detached	spectroscopic binary, having a fainter B-type companion
of the pair, Kappa Pegasi B, is actually a	spectroscopic binary, with the components designated Kap
It is also a	spectroscopic binary, and is composed of two stars with
At the centre of the system is a	spectroscopic binary, Iota Serpentis A and B. These are
Component A is a	spectroscopic binary.
HD 37017 is a	spectroscopic binary.
Lambda Virginis is a	spectroscopic binary.
IU Aurigae is a	spectroscopic binary.
EZ Aquarii AC is a	spectroscopic binary.
Sigma Aquilae is an eclipsing	spectroscopic binary.
rimary component, Epsilon Volantis A, is a	spectroscopic binary.
, Epsilon Ursae Minoris A, is an eclipsing	spectroscopic binary.
nt distance of 5".1 while it may also be a	spectroscopic binary.
esolved with optical telescopes, forming a	spectroscopic binary.
ve a companion, which would make Electra a	spectroscopic binary.
Wide Band Spectrometer (WBS) has	spectroscopic capabilities in a wide energy band from 3
a permanent dipole moment, which makes the	spectroscopic characterization easier.
Their individual	spectroscopic classifications are dK5e and dK7e.
A is separated from its	spectroscopic companion by 0.05 arcseconds.
B's	spectroscopic companion was discovered in 1989, and that
freely accessible, and contains extensive	spectroscopic data for organic compounds including that
nstruments, incorporating both imaging and	spectroscopic data at optical, infrared, and radio wavel
ei is a triple star system consisting of a	spectroscopic double star with a wider companion.
As an optical technique,	spectroscopic ellipsometry is non-destructive and contac
llipsometry (MOGE) is an advanced infrared	spectroscopic ellipsometry technique for studying free c
boratory, in which he assembled the latest	spectroscopic equipment.
With this	spectroscopic evidence a search for these type of molecu
Although	spectroscopic evidence is consistent with a mass of 8 ±
ars to have an orbital period of 11 years;	spectroscopic evidence indicates a third companion of A
NMR	spectroscopic experiments indicated close proximity of t
The Far Ultraviolet	Spectroscopic Explorer (FUSE) is a space-based telescope
P Cygni gives its name to a type of	spectroscopic feature called a P Cygni profile, where th
became the Reuven Ramaty High Energy Solar	Spectroscopic Imager (RHESSI), the first space mission n
The Reuven Ramaty High Energy Solar	Spectroscopic Imager (RHESSI), Explorer 81, images solar
Also called 1H-nuclear magnetic resonance	spectroscopic imaging and proton magnetic resonance spec
Magnetic resonance	spectroscopic imaging is a noninvasive imaging method th
uting is an approach to the development of	spectroscopic instruments, particularly for industrial a
harges was raised sufficiently to allow of	spectroscopic investigation.
to prove the existence of this species by	spectroscopic means
is not possible to isolate or detect it by	spectroscopic means
	Spectroscopic measurements have given an orbital period
target-of-opportunity basis, less frequent	spectroscopic measurements complement the rapid photomet
Although	spectroscopic measurements are necessary to obtain a hig
rs prefer the name TPD because it is not a	spectroscopic method.
Emission Pumping (SEP, or "PUMP and DUMP")	spectroscopic method.
	spectroscopic methods for structural characterization
He identified this gas by	spectroscopic methods to be nitrogen.
	Spectroscopic methods on a cellular and molecular level
He became interested in using	spectroscopic methods including nuclear magnetic resonan
ve diseases and the use of microscopic and	spectroscopic methods in neurosciences (“neurophotonics”
his work in development of ultrasensitive	spectroscopic methods with applications in trace gas det
In all three	spectroscopic methods, the sample usually needs to be pr
ng the structure of atoms and molecules by	spectroscopic methods.
FM can be operated in the imaging mode and	spectroscopic mode.
e closest approach to this resolution by a	spectroscopic neutron instrument type, namely the backsc
	Spectroscopic observation from orbit indicates the prese
The Hubble Space Telescope took STIS/UV	spectroscopic observations on May 3, 2010.
FOS was designed to make	spectroscopic observations of astrophysical sources from
However, more detailed	spectroscopic observations in 2005 appear to show that i
s contributions to Astronomical Physics by	spectroscopic observations of eclipses, solar pre-eminen
second per century, which corresponds from	spectroscopic observations to 20-30 km−1).
UT) was a space telescope designed to make	spectroscopic observations in the far-ultraviolet region
olume of observations produced, along with	spectroscopic observations and some pioneering attempts
	Spectroscopic observations can be used in a myriad of co
	Spectroscopic observations through 2007 indicate that it
y Notices Roy Astron Soc, vol lxv, 1905); '	Spectroscopic Observations of the Great Sunspot (Februar
The presence of water ice is supported by	spectroscopic observations, which have revealed crystall
ectrography for Rocky Exoplanet and Stable	Spectroscopic Observations, dubbed ESPRESSO, might allow
provide high resolution, multi-wavelength	spectroscopic observations.
Its orbit was computed in 1946 from	spectroscopic observations.
	Spectroscopic parallax is an astronomical method for mea
nings are the Photometric parallax method,	Spectroscopic parallax, and Dynamical parallax
solution Transmission) is a compilation of	spectroscopic parameters that a variety of computer code
The Rossiter-McLaughlin effect is a	spectroscopic phenomenon observed when either an eclipsi
th other contractors to develop an Advance	Spectroscopic Portal (ASP) to allow border officials to
ion to the new equilibrium is monitored by	spectroscopic probes such as fluorescence or less freque
The	spectroscopic properties of Proton-sponge are very inter
uctases depending on their function, their	spectroscopic properties, and their catalytic properties
ed to phycobiliproteins to confer specific	spectroscopic properties.
is its very high basicity; another is its	spectroscopic properties.
adial velocity most commonly refers to the	spectroscopic radial velocity.
The	spectroscopic radial velocity is radial component of the
This instrument had a	spectroscopic range of 82.5 to 185 nms, and a spectral r
ame logic follows to explain the identical	spectroscopic results provided by the hydrogen atoms on
Both visible and infrared	spectroscopic results indicate that Ixion's surface is a
imation of this coupling provides a direct	spectroscopic route to the distance between nuclei and h
at showed radio loud quasars have distinct	spectroscopic signatures that depend on their orientatio
purity and served as reliable reagents and	spectroscopic standards.
erally obtained empirically from gas-phase	spectroscopic studies of atoms.
RI scanner for functional, structural, and	spectroscopic studies of humans and animals.
vae, he has also worked extensively on the	spectroscopic studies of Active Galactic Nuclei
IR	spectroscopic studies have demonstrated the existence of
	Spectroscopic studies suggest that Eunomia has regions w
Donati was also a pioneer in the	spectroscopic study of the stars and the sun.
67 jointly with William Huggins, for their	spectroscopic study of the composition of stars.
In 1895, his	spectroscopic study of the rings of Saturn revealed that
ject was known as Small Main-belt Asteroid	Spectroscopic Survey, Phase II or SMASSII, which built o
Gamma rays detected in a	spectroscopic system produce peaks in the spectrum.
Linear dichroism (LD) is a	spectroscopic technique that is primarily used to study
An advantage of this	spectroscopic technique is that the ions can be detected
Reflectance difference spectroscopy is a	spectroscopic technique which measures the difference in
using a	spectroscopic technique, such as infrared spectroscopy,
ful to confirm the result, although modern	spectroscopic techniques (e.g.
und was characterized by computational and	spectroscopic techniques and found to possess a cage-lik

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