「lensing」の共起表現一覧(1語右で並び替え)
該当件数 : 48件
"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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