SPHERE: A 'Planet Finder' instrument for the VLT
| Authors |
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| Publication date | 2008 |
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| Book title | Ground-based and Airborne Instrumentation for Astronomy II |
| Book subtitle | 23-28 June 2008, Marseille, France |
| ISBN |
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| Series | Proceedings of SPIE, the International Society for Optical Engineering |
| Event | SPIE Astronomical Instrumentation 2008, Marseille, France |
| Article number | 701418 |
| Volume | Issue number | 1 |
| Number of pages | 12 |
| Publisher | Bellingham, WA: SPIE |
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| Abstract |
Direct detection and spectral characterization of extra-solar planets is one of the most exciting but also one of the most challenging areas in modern astronomy. The challenge consists in the very large contrast between the host star and the planet, larger than 12.5 magnitudes at very small angular separations, typically inside the seeing halo. The whole design of a "Planet Finder" instrument is therefore optimized towards reaching the highest contrast in a limited field of view and at short distances from the central star. Both evolved and young planetary systems can be detected, respectively through their reflected light and through the intrinsic planet emission. We present the science objectives, conceptual design and expected performance of the SPHERE instrument.
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| Document type | Conference contribution |
| Language | English |
| Related publication | SPHERE: A 'Planet Finder' Instrument for the VLT |
| Published at | https://doi.org/10.1117/12.790120 |
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