Optical corrector for Dark Energy Survey
THALES SESO manufactured one of largest lens in the world the Dark Energy Survey (DES) project with a diameter of 980mm. This project included the grinding, polishing, control and coat and AR coatings of 5 large lenses (some evenaspheres).
DES is a major ground-based Astronomy project designed to probe the origin of the accelerating universe. To do that, an extremely sensitive high resolution/high field of view camera (DECAM) is mounted at the focal plane of the existing Φ 4m Blanco Telescope (location Cerro Tololo Observatory in Chile).
Courtesy of UCL-UK and Fermilab-USA
Key- requirements of these lenses:
Element | Type | Size | Optical Quality per surface |
C1 | CX spherical /CV spherical | Φ 980mm | |
C2 | CX spherical / CV aspherical | Φ 690mm | <60/250nm RMS (spherical/aspherical sides) |
C3 | CX spherical /CV spherical | Φ 650mm | |
C4 | CX spherical /CV spherical | Φ 600mm | <60/250nm RMS (spherical/aspherical sides) |
C5 | CX spherical /CV spherical | Φ 550mm |
Other optical specifications were almost the following ones:
• Radii tolerances within about +/-0.5mm
• Thickness tolerances within about +/-0.2mm
• Tilts/wedges < 0.05mm
• S/D quality better than 60/40 (relaxed up to 80/50 for the largest C1 element)
• Microroughness better than 2nm RMS