{"id":1306,"date":"2021-12-17T14:14:12","date_gmt":"2021-12-17T21:14:12","guid":{"rendered":"https:\/\/www.irlabs.com\/?p=1306"},"modified":"2023-08-30T14:41:13","modified_gmt":"2023-08-30T21:41:13","slug":"ir-labs-designs-constructs-and-tests-dewar-for-shark-nir","status":"publish","type":"post","link":"https:\/\/www.irlabs.com\/ir-labs-designs-constructs-and-tests-dewar-for-shark-nir\/","title":{"rendered":"IRLabs Designs, Constructs, and Tests Dewar for SHARK-NIR"},"content":{"rendered":"

Overview<\/h4>\n

Exoplanet research and characterization are the main purposes of the Large Binocular Telescope (LBT) located on Mt. Graham in southeastern Arizona. The telescope\u2019s binocular design combined with impressive adaptive optics provides the large effective aperture, high angular resolution, low thermal background, and exceptional sensitivity for detecting faint objects. The LBT has two identical 8.4m telescopes mounted side-by-side on a common altitude-azimuth mounting.<\/p>\n

At the heart of the telescope are a pair of SHARK (S<\/strong>ystem for coronagraphy with H<\/strong>igh A<\/strong>daptive optics from R<\/strong> to K<\/strong> band) instruments. The SHARK-NIR (near infrared) and SHARK-VIS (visible light) will be used together to observe exoplanets. IRLabs designed, manufactured, and tested the dewar for the SHARK-NIR instrument and cooling platform for its HAWAII-2RG detector.<\/p>\n<\/div>

Watch Video<\/h4><\/div>