Abstract
PLATO is a 6 tonne completely self-contained robotic observatory that provides its own heat, electricity, and satellite communications. It was deployed to Dome A in Antarctica in January 2008 by the Chinese expedition team, and is now in its second year of operation. PLATO is operating four 14.5cm optical telescopes with 1k×1k CCDs, a wide-field sky camera with a 2k×2k CCD and Sloan g, r, i filters, a fibre-fed spectrograph to measure the UV to near-IR sky spectrum, a 0.2m terahertz telescope, two sonic radars giving 1m resolution data on the boundary layer to a height of 180m, a 15m tower, meteorological sensors, and 8 web cameras. Beginning in 2010/11 PLATO will be upgraded to support a Multi Aperture Scintillation Sensor and three AST3 0.5m schmidt telescopes, with 10k×10k CCDs and 100TB/annum data requirements.
| Original language | English |
|---|---|
| Title of host publication | Proceedings of the International Astronomical Union, 3-14 August 2009, Rio de Janeiro, Brazil |
| Publisher | Cambridge University Press |
| Pages | 627-629 |
| Number of pages | 3 |
| DOIs | |
| Publication status | Published - 2010 |
| Event | International Astronomical Union. General Assembly - Duration: 1 Jan 2010 → … |
Conference
| Conference | International Astronomical Union. General Assembly |
|---|---|
| Period | 1/01/10 → … |
Fingerprint
Dive into the research topics of 'The PLATO observatory : robotic astronomy from the Antarctic plateau'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver