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「Microlensing」の共起表現一覧(1語右で並び替え)
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ray light can be explained by gravitational | microlensing, an effect which has been used to search fo |
the galactic bulge undergoing gravitational | microlensing by intervening foreground stars (or other c |
Microlensing by an isolated object was first detected in | |
ed on December 8, 2009 by the gravitational | microlensing by Sumi. |
Since 2005, PLANET performs a common | microlensing campaign with RoboNet-1.0, |
r of intervening stars that can be used for | microlensing during a stellar transit. |
A gravitational | microlensing event occurs when a planet accompanying thi |
rs when it became the lens of gravitational | microlensing event MOA-2009-BLG-387L, in which it eclips |
After a | microlensing event in progress has been identified, the |
analysis of another team revealed that the | microlensing event could be interpreted as being caused |
-41 or MACHO-97-BLG-41, was a gravitational | microlensing event located in Sagittarius which occurred |
MOA-2009-BLG-387 was a gravitational | microlensing event detected by the Microlensing Observat |
On June 7, 2010, long after the | microlensing event had subsided, the science teams study |
In 2009 during the | microlensing event, a Neptune-mass planet was found orbi |
fact that the star acted as the lens in the | microlensing event, which compromised the ability to col |
microlensing events, supernovae and gamma-ray bursts | |
nates the observation of high-magnification | microlensing events. |
The | Microlensing Follow Up Network (μFUN) has not yet positi |
Microlensing has also been proposed as a means to find d | |
Since then, | microlensing has been used to constrain the nature of th |
discovered simultaneously by gravitational | microlensing in a common effort by the Optical Gravitati |
The technique of gravitational | microlensing is used to monitor large numbers of stars i |
serve millions of stars each night, and see | microlensing many times each year. |
t was discovered by using the gravitational | microlensing method on August 4, 2009. |
is planet was detected by the gravitational | microlensing method based on an event recorded in Septem |
For events detected by the gravitational | microlensing method, year stands for OGLE season, BLG me |
As it is typical for exoplanets detected by | microlensing method, the orbital period and eccentricity |
et was discovered orbiting this star by the | microlensing method. |
The | Microlensing Observations in Astrophysics (MOA) telescop |
The star is named for the | Microlensing Observations in Astrophysics group, which s |
f an extrasolar planet was announced by the | Microlensing Observations in Astrophysics (MOA) Collabor |
Microlensing Observations in Astrophysics (MOA) is a col | |
d observing resources is very important for | microlensing researchers today. |
s a quasar that is undergoing gravitational | microlensing, resulting in double, triple or quadruple i |
is the fact that for every star undergoing | microlensing, there are thousands of stars changing in b |
They use | microlensing to observe dark matter, extra-solar planets |
ett was an innovative user of gravitational | microlensing to search for extrasolar planets-dark matte |
S.V.H. Haugan, "Separating intrinsic and | microlensing variability using parallax measurements". |
idate was detected using a technique called | microlensing, which is caused by the deflection of light |
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