منابع مشابه
MOPS installation at Mopra and first light
Investigating grain growth in southern protoplanetary disks Page 18 As we enter the 2006 millimetre observing season at the ATNF, the installation of the ATNF’s newest and most versatile spectrometer is now complete. The MOPra Spectrometer (MOPS) recently completed the final stages of testing on the Mopra millimetre telescope and observations have commenced for 2006, with fascinating results al...
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Research is increasingly collaborative and global in nature and efforts to manage the vast amounts of research data generated daily require global solutions. The Digital Object Identifier (DOI) system provides a means of persistent identification of research data collections and datasets that is global, standardised and widely used. The Australian National Data Service (ANDS) partnered with Dat...
متن کاملLaser Development for Sodium Laser Guide Stars at ESO
A breakthrough in the development of sodium laser guide star technology at ESO was made in 2009. The laser research and development programme has led to the implementation of a narrowband Raman fibre laser emitting at the wavelength of the sodium lines at 589 nm with demonstrated power beyond 50 W. Fibre lasers are rugged and reliable, making them promising candidates for use in the next genera...
متن کاملFirst results from the ESO VLTI Calibrators Program ⋆
The ESO Very Large Telescope Interferometer (VLTI) is one of the leading interferometric facilities. It is equipped with several 8.2 and 1.8m telescopes, a large number of baselines up to 200m, and with several subsystems designed to enable high quality measurements and to improve significantly the limits of sensitivities currently available to long-baseline interferometry. The full scientific ...
متن کاملFinding the First Stars: The Hamburg/ESO Objective Prism Survey
The Hamburg/ESO survey (HES; [4]) is an objective-prism survey for bright quasars based on IIIa-J plates taken with the ESO Schmidt telescope and its 4◦ prism. It covers the total southern extragalactic sky (δ <+2◦. 5; |b| & 30◦). All 380 Schmidt plates (effective area ∼ 7 000 square degrees) have been taken, and have been digitized and reduced in Hamburg. The spectral range of the HES plates i...
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ژورنال
عنوان ژورنال: EPJ Web of Conferences
سال: 2018
ISSN: 2100-014X
DOI: 10.1051/epjconf/201818604003