Correction de la dispersion atmosphérique dans l’imagerie par les grands télescopes et les interféromètres astronomiques by Koechlin, Laurent, Dettwiller, Luc

“…The very large telescopes and the various optical interferometers provide access to unparalleled angular resolutions and provide scientific data of primary importance, but at the price of instrumental constraints that require complex equipment. …”
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System Analysis of Pipeline Software - a Case Study of the Imaging Survey at ESO by Young-Soo Kim

“…The EIS team has been conducting a sky survey to provide candidate targets to the ESO VLTs (Very Large Telescopes) observations. The survey data have been processed in a sequence of five major data corrections and reductions, i.e. preprocessing, flat fielding, photometric and astrometric corrections, source extraction, and coaddition. …”
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Dispersion Characteristics of the Multi-mode Fiber-fed VIPA Spectrograph by Xiaoming Zhu, Dong Lin, Zhongnan Zhang, Xintong Xie, Jinping He

“…This makes the VIPA spectrograph a promising instrument to attain an ultra-high spectral resolution ( ${ \mathcal R }\gt 3\times {10}^{5}$ ) on very large telescopes.…”
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