Development of a test rig for the active control of a segmented mirror support system
Within the preliminary developments related to the Gran Telescopio Canarias, a test rig is being designed for the active control of the support system of the...
Development of configurable slit unit for GTC-EMIR
The Configurable Slit Unit (CSU) for EMIR shall enable the possibility to generate a multi-slit configuration, a long slit, or an imaging aperture at the...
Development of cryogenic components based on COTS parts for the HARMONI instrument
HARMONI is an integral field spectrograph working at visible and near-infrared wavelengths. The instrument will be part of the first-light complement at the E...
Development of gas absorption cells for infrared echelle spectrographs
High-resolution spectroscopy in the near-infrared could become the leading method for discovering extra-solar planets around very low-mass stars and brown...
Development of the camera for the large size telescopes of the Cherenkov Telescope Array
The Large Size Telescopes, LSTs, located at the center of the Cherenkov Telescope Array, CTA, will be sensitive for low energy gamma-rays. The camera on the LST...
Development status of the telescope for the Ingenio/SEOSAT mission primary payload
Ingenio/SEOSAT is the flagship mission for the Spanish Space Plan 2007-2011, as is currently under development by a Spanish industrial consortium in the...
Developments in fiber-positioning technology for the WEAVE instrument at the William Herschel Telescope
WEAVE is the next-generation wide-field optical spectroscopy facility for the William Herschel Telescope (WHT) on La Palma in the Canary Islands, Spain. It is a...
DG Leo uvby differential photometry (Lampens+, 2005)
The first table (dataset1) contains 1590 data points collected with 1.5m telescopes equipped with conventional photometers at the observatories of San Pedro...