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Limiting magnitude information


Visual effect of night sky's brightness.

In astronomy, limiting magnitude is the faintest apparent magnitude of a celestial body that is detectable or detected by a given instrument.[1]

In some cases, limiting magnitude refers to the upper threshold of detection. In more formal uses, limiting magnitude is specified along with the strength of the signal (e.g., "10th magnitude at 20 sigma"). Sometimes limiting magnitude is qualified by the purpose of the instrument (e.g., "10th magnitude for photometry") This statement recognizes that a photometric detector can detect light far fainter than it can reliably measure.

The limiting magnitude of an instrument is often cited for ideal conditions, but environmental conditions impose further practical limits. These include weather, moonlight, skyglow, and light pollution. The International Dark-Sky Association has been vocal in championing the cause of reducing skyglow and light pollution.

  1. ^ "FAQs about the UNH Observatory | Physics". Archived from the original on 2016-02-03. Retrieved 2016-01-28. (retrieved Jan 28 2016)

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Limiting magnitude

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In astronomy, limiting magnitude is the faintest apparent magnitude of a celestial body that is detectable or detected by a given instrument. In some...

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Apparent magnitude

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Magnitude

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object Instrumental magnitude, the uncalibrated apparent magnitude of a celestial object Limiting magnitude, the faintest apparent magnitude of a celestial...

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Bortle scale

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skies. It gives several criteria for each level beyond naked-eye limiting magnitude (NELM). The accuracy and utility of the scale have been questioned...

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List of brightest stars

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night sky at each period within the last or next 5 million years Limiting magnitude List of variable stars List of semiregular variable stars List of...

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Zenithal hourly rate

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This represents the limiting magnitude correction factor (Population index). For every change of 1 magnitude in the limiting magnitude of the observer, the...

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Surface brightness

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0.27 millinits). Araucaria Project Low-surface-brightness galaxy Limiting magnitude Sigma-D relation Daintith, John; Gould, William (2006). The Facts...

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Current limiting

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interrupting currents in its current-limiting range, reduces the current flowing in the faulted circuit to a magnitude substantially less than that obtainable...

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Limiting factor

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bring about an increase of the magnitude of the function." In population ecology, a regulating factor, also known as a limiting factor, is something that keeps...

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List of astronomical interferometers at visible and infrared wavelengths

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science which can be done. Higher limiting magnitude means that the array can observe fainter sources. The limiting magnitude is determined by the atmospheric...

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Malmquist bias

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on the limiting magnitude selected, there may be a range of distances in the data set over which all objects of any possible absolute magnitude could be...

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Star catalogue

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billion stars. Completeness and accuracy are described by the faintest limiting magnitude V (largest number) and the accuracy of the positions. From their existing...

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Hipparcos

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balance 'a priori' scientific interest, and the observing programme's limiting magnitude, total observing time, and sky uniformity constraints. For the main...

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HD 39118

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an apparent magnitude of 5.976. At this magnitude, it is visible to the naked eye only in dark skies, being close to the limiting magnitude to naked-eye...

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Very Large Telescope

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reach magnitude 4.5, significantly fainter than the Infrared Spatial Interferometer. When fringe tracking is introduced, the limiting magnitude of the...

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Distance modulus

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an apparent magnitude (m) of 5 + 24.4 = 29.4, so it would be barely visible for the Hubble Space Telescope which has a limiting magnitude of about 30...

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Guide Star Catalog

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to magnitude 11. Adding the bright star data from this catalog to the GSC produced a complete all-sky catalog down to the GSC limiting magnitude. In...

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Milky Way

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than about 20.2 magnitude per square arcsecond in order for the Milky Way to be visible. It should be visible if the limiting magnitude is approximately...

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Absolute magnitude

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astronomy, absolute magnitude (M) is a measure of the luminosity of a celestial object on an inverse logarithmic astronomical magnitude scale. An object's...

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Asteroid impact prediction

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class telescopes (which have much longer exposure times), giving a limiting magnitude of just 18. However, despite not being able to see dimmer objects...

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Messier 82

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15 through 20 January, brightening from magnitude +14.4 to +11.3; it could not be found, to limiting magnitude +17, from images caught of 14 January. It...

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Naked eye

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this number somewhat. In the center of a city, where the naked-eye limiting magnitude due to extreme amounts of light pollution can be as low as 2m, as...

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HD 37320

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a parallax from Gaia EDR3. The apparent magnitude of the star is 5.852, which is above the limiting magnitude for naked-eye vision (6.5m), making it faintly...

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Xuntian

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square degrees of the sky in various bands, reaching point-source 5σ limiting magnitudes of about 26 (AB mag) in g and r bands. The CSST's spectral resolution...

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Stellar classification

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M class main-sequence star is Lacaille 8760, class M0V, with magnitude 6.7 (the limiting magnitude for typical naked-eye visibility under good conditions being...

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Aperture masking interferometry

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high light level can be improved with aperture masks, the faintest limiting magnitude cannot be significantly improved for photon-noise limited detectors...

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Skyglow

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Night an Android app for estimating skyglow by measuring naked eye limiting magnitude Dark Sky Meter an iPhone app for measuring skyglow luminance LED light...

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