| Display title | Astronomy:Palomar Transient Factory |
| Default sort key | Palomar Transient Factory |
| Page length (in bytes) | 11,591 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 722760 |
| 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>NBrushPhys |
| Date of page creation | 11:38, 6 February 2024 |
| Latest editor | imported>NBrushPhys |
| Date of latest edit | 11:38, 6 February 2024 |
| 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. | The Palomar Transient Factory (PTF, obs. code: I41), was an astronomical survey using a wide-field survey camera designed to search for optical transient and variable sources such as variable stars, supernovae, asteroids and comets. The project completed commissioning in summer 2009, and continued until... |
