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  2. Redshift - Wikipedia

    en.wikipedia.org/wiki/Redshift

    High-redshift galaxy candidates in the Hubble Ultra Deep Field, 2012 [19] The spectrum of light that comes from a source (see idealized spectrum illustration top-right) can be measured. To determine the redshift, one searches for features in the spectrum such as absorption lines, emission lines, or other variations in light intensity. If found ...

  3. Lyman-break galaxy - Wikipedia

    en.wikipedia.org/wiki/Lyman-break_galaxy

    The technique may be adapted to look for galaxies at other redshifts by choosing different sets of filters; the method works as long as images may be taken through at least one filter above and below the wavelength of the redshifted Lyman limit. In order to confirm the redshift estimated by the color selection, follow-up spectroscopy is ...

  4. Quasars, Redshifts and Controversies - Wikipedia

    en.wikipedia.org/wiki/Quasars,_Redshifts_and...

    Arp has interpreted these connections to mean that these objects are in fact physically connected. He further hypothesized that the higher redshift objects are ejected from the lower redshift objects - which are usually active galactic nuclei (AGN)- and that the large observed redshifts of these "ejected" objects is dominated by a non ...

  5. Photometric redshift - Wikipedia

    en.wikipedia.org/wiki/Photometric_redshift

    A photometric redshift is an estimate for the recession velocity of an astronomical object such as a galaxy or quasar, made without measuring its spectrum.The technique uses photometry (that is, the brightness of the object viewed through various standard filters, each of which lets through a relatively broad passband of colours, such as red light, green light, or blue light) to determine the ...

  6. Lyman-alpha emitter - Wikipedia

    en.wikipedia.org/wiki/Lyman-alpha_emitter

    The baryonic acoustic oscillation signal should be evident in the power spectrum of Lyman-alpha emitters at high redshift. [6] Baryonic acoustic oscillations are imprints of sound waves on scales where radiation pressure stabilized the density perturbations against gravitational collapse in the early universe.

  7. Gravitational redshift - Wikipedia

    en.wikipedia.org/wiki/Gravitational_redshift

    Gravitational redshift can be interpreted as a consequence of the equivalence principle (that gravitational effects are locally equivalent to inertial effects and the redshift is caused by the Doppler effect) [5] or as a consequence of the mass–energy equivalence and conservation of energy ('falling' photons gain energy), [6] [7] though there ...

  8. We Know Sexuality Is a Spectrum —Here's What That Means - AOL

    www.aol.com/news/know-sexuality-spectrum-heres...

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  9. Tired light - Wikipedia

    en.wikipedia.org/wiki/Tired_light

    Tired light was an idea that came about due to the observation made by Edwin Hubble that distant galaxies have redshifts proportional to their distance.Redshift is a shift in the spectrum of the emitted electromagnetic radiation from an object toward lower energies and frequencies, associated with the phenomenon of the Doppler effect.