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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.
Naked-eye visibility, Modelling magnitude limits & Large observatories
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magnitude limiting sky light telescope crumey stars brightness limit background displaystyle dark pupil magnification visibility eye one mag seen visible
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Limiting magnitude | is a | faintest apparent magnitude of a celestial body that is detectable or detected by a given instrument.In some cases | 0.90 | text |
| a galaxy or comet.Various authors have stated the limiting magnitude of a telescope with entrance pupil D | instance of | Point sources such as a star will be easier to detect than a diffuse object | 0.80 | text |
| his eye pupil diameter | instance of | Bowen did not record parameters | 0.80 | text |
| naked-eye magnitude limit | instance of | Bowen did not record parameters | 0.80 | text |
| or the extent of light loss in his telescopes | instance of | Bowen did not record parameters | 0.80 | text |
| Limiting magnitude | related to External links | Estimating Limiting Magnitude | 0.60 | section |
| Limiting magnitude | related to External links | NinePlanets | 0.60 | section |
| Limiting magnitude | related to External links | Limiting Magnitude CalculatorLoss | 0.60 | section |
| Limiting magnitude | related to External links | Night | 0.60 | section |
| Limiting magnitude | related to External links | Astronomical Magnitude ScaleAstronomical Visibility | 0.60 | section |
| Limiting magnitude | related to External links | Andrew Crumey | 0.60 | section |
| Limiting magnitude | related to Large observatories | Telescopes | 0.60 | section |
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