| Display title | Astronomy:K correction |
| Default sort key | K Correction |
| Page length (in bytes) | 5,307 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 375736 |
| Page content language | en - English |
| Page content model | wikitext |
| Indexing by robots | Allowed |
| Number of redirects to this page | 0 |
| Counted as a content page | Yes |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>S.Timg |
| Date of page creation | 04:04, 24 October 2022 |
| Latest editor | imported>S.Timg |
| Date of latest edit | 04:04, 24 October 2022 |
| Total number of edits | 1 |
| Recent number of edits (within past 90 days) | 0 |
| Recent number of distinct authors | 0 |
Description | Content |
Article description: (description)
This attribute controls the content of the description and og:description elements. | K correction converts measurements of astronomical objects into their respective rest frames. The correction acts on that object's observed magnitude (or equivalently, its flux). Because astronomical observations often measure through a single filter or bandpass, observers only measure a fraction of... |
