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  2. Weak gravitational lensing - Wikipedia

    en.wikipedia.org/wiki/Weak_gravitational_lensing

    Galaxy-galaxy lensing is a specific type of weak (and occasionally strong) gravitational lensing, in which the foreground object responsible for distorting the shapes of background galaxies is itself an individual field galaxy (as opposed to a galaxy cluster or the large-scale structure of the cosmos). Of the three typical mass regimes in weak ...

  3. Gravitational lens - Wikipedia

    en.wikipedia.org/wiki/Gravitational_lens

    In 2009, weak gravitational lensing was used to extend the mass-X-ray-luminosity relation to older and smaller structures than was previously possible to improve measurements of distant galaxies. [29] As of 2013 the most distant gravitational lens galaxy, J1000+0221, had been found using NASA's Hubble Space Telescope.

  4. Gravitational lensing formalism - Wikipedia

    en.wikipedia.org/wiki/Gravitational_lensing...

    In weak gravitational lensing, the Jacobian is mapped out by observing the effect of the shear on the ellipticities of background galaxies. This effect is purely statistical; the shape of any galaxy will be dominated by its random, unlensed shape, but lensing will produce a spatially coherent distortion of these shapes.

  5. Dark Energy Survey - Wikipedia

    en.wikipedia.org/wiki/Dark_Energy_Survey

    The Dark Energy Survey (DES) is an astronomical survey designed to constrain the properties of dark energy.It uses images taken in the near-ultraviolet, visible, and near-infrared to measure the expansion of the universe using Type Ia supernovae, baryon acoustic oscillations, the number of galaxy clusters, and weak gravitational lensing. [1]

  6. Gravitational microlensing - Wikipedia

    en.wikipedia.org/wiki/Gravitational_microlensing

    Thus, unlike with strong and weak gravitational lenses, microlensing is a transient astronomical event from a human timescale perspective, [10] thus a subject of time-domain astronomy. Unlike with strong and weak lensing, no single observation can establish that microlensing is occurring.

  7. How astronomers used gravitational lensing to discover 44 new ...

    www.aol.com/news/astronomers-discovered-44-stars...

    A visible arc created by gravitational lensing and the bending of light beyond Abell 370 was dubbed the "Dragon Arc." After carefully analyzing the colors of each of the stars inside the Dragon ...

  8. Einstein radius - Wikipedia

    en.wikipedia.org/wiki/Einstein_radius

    For small deflections this mapping is one-to-one and consists of distortions of the observed positions which are invertible. This is called weak lensing. For large deflections one can have multiple images and a non-invertible mapping: this is called strong lensing. Note that in order for a distributed mass to result in an Einstein ring, it must ...

  9. Category:Gravitational lensing - Wikipedia

    en.wikipedia.org/wiki/Category:Gravitational_lensing

    Gravitational lensing is an effect of gravitation, most commonly associated with General relativity ... Weak gravitational lensing; X. Xallarap This page was ...