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「lensing」の共起表現一覧(1語右で並び替え)

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"The Origin of Gravitational Lensing: A Postscript to Einstein's 1936 Science pape
ss contours (dominated by dark matter) from a lensing analysis overlaid.
ests include applications using gravitational lensing and high-redshift supernovae.
quences of TeVeS in relation to gravitational lensing and cosmology.
ion, galaxy clustering and weak gravitational lensing, and the implications of these observations f
nded to measure effects of weak gravitational lensing) and Spectroscopic All Sky Cosmic Explorer (S
The experiments testing gravitational lensing and light time delay limits the same post-New
ct and helped in the development of explosive lensing and the Urchin initiator.
The Probing Lensing Anomalies NETwork (PLANET) collaboration coor
great distance was credited to gravitational lensing by the galaxy cluster Abell 1835 between it a
Gravitational lensing- combining strong and weak lensing analysis te
Lensing currently serves on several committees in the
he amount of brightening due to gravitational lensing doesn't vary with the wavelength, this means
curate for most measurements of gravitational lensing, due to the smallness of the ratio rs/r.
inary evidence from the Optical Gravitational Lensing Experiment (OGLE) survey.
was discovered when the Optical Gravitational Lensing Experiment (OGLE) survey observed the smaller
lanet discovered by the Optical Gravitational Lensing Experiment (OGLE) and others in 2005, using g
ern surveys such as the Optical Gravitational Lensing Experiment (OGLE) observe millions of stars e
However, in 2003 the Optical Gravitational Lensing Experiment (OGLE) detected periodic dimming i
project manager of the Optical Gravitational Lensing Experiment and editor of the quarterly journa
In 2002 the Optical Gravitational Lensing Experiment (OGLE) survey detected that the li
iences, a member of the Optical Gravitational Lensing Experiment (OGLE), co-discoverer (together wi
a common effort by the Optical Gravitational Lensing Experiment, microFUN, MOA, PLANET and RoboNet
QSO 2237+0305 A), the lensing galaxy is sometimes referred to as QSO 2237+0
Huchra's Lens is the lensing galaxy of the Einstein Cross (Quasar 2237+30)
t 8 billion light years from Earth, while the lensing galaxy is located at a distance of 400 millio
n is mainly useful for studying gravitational lensing in a strong gravitational field (see here for
Measuring weak gravitational lensing in the deep sky to detect signatures of dark
h average power (100 W to kWs) due to thermal lensing in the laser gain medium.
e is best known for her work on gravitational lensing, including the Chang-Refsdal lens.
t known for his pioneer work on gravitational lensing, including the Chang-Refsdal lens.
Weak gravitational lensing is thus an intrinsically statistical measurem
ic alignment of background sources around the lensing mass.
Gravitational lensing occurs when a distant object and a massive in
Gravitational lensing occurs when light from a distant star is bent
e Einstein ring produced by the gravitational lensing of light from two distant galaxies.
h for the HOLIGRAIL (Hoher List Gravitational Lensing) project.
ht in the universe are thoroughly in the weak lensing regime, in which the deflection is impossible
ncing as the dark matter model, gravitational lensing studies may provide the means to separate the
ns Survey (DLS, short for "Deep Gravitational Lensing Survey") is an ultra-deep multi-band optical
millions of galaxies in a weak gravitational lensing survey.
It exhibits the phenomenon of gravitational lensing that was postulated by Albert Einstein when h
redshift, it is possible to use galaxy-galaxy lensing to see how several different types of galaxie
research uses the phenomenon of gravitational lensing to probe the nature and distribution of the p
Lensing was re-elected in 2006 with 11,000 votes, run
ucted from measurements of weak gravitational lensing with the Hubble Space Telescope.
Clusters of galaxies- using lensing, X-ray and Sunyaev-Zeldovich data in conjunct
                                                                                                   


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