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Prediction of flooding in distillation columns using machine learning
Published 2023-06-01Get full text
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The Barium Star HD204075: Iron Abundance and the Absence of Evidence for Accretion
Published 2019-09-01“…Spectroscopic observations of barium star ζ Capricornus (HD204075) obtained at the 8.2 m telescope of the European Southern Observatory, with a spectral resolving power R = 80,000 and signal to noise ratio greater than 300, were used to refine the atmospheric parameters. …”
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SINFONI: A near infrared AO assisted integral field spectrometer for the VLT
Published 1998“…SINFONI is a collaborative effort by the Max-Planck-Institut fur extraterrestrische Physik (MPE) and the European Southern Observatory (ESO).SINFONI will operate at the Cassegrain focus of Unit Telescope 1 (UT1) of the VLT, in conjunction with a Laser Guide Star (LGS) for almost complete sky coverage. …”
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System Analysis of Pipeline Software - a Case Study of the Imaging Survey at ESO
Published 2003-12-01“…As a case study, the development of pipeline software for the EIS (European Southern Observatory Imaging Survey) is introduced. …”
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A Large Jet Narrow-line Seyfert 1 Galaxy: Observations from Parsec to 100 kpc Scales
Published 2024-01-01Get full text
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Chemical Composition of RM_1-390 - Large Magellanic Cloud Red Supergiant
Published 2017-09-01“…A high resolution spectroscopic observation of the red supergiant star RM_1-390 in the Large Magellanic Cloud was made from a 3.6 m telescope at the European Southern Observatory. Spectral resolving power was R=20,000, with a signal-to-noise ratio S/N > 100. …”
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Quantum Astronomy at the University and INAF Astronomical Observatory of Padova, Italy
Published 2023-08-01“…The initial activities were stimulated by the project of the European Southern Observatory (ESO) to build a 100 m diameter telescope, the Overwhelmingly Large (OWL) telescope. …”
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Are Disks of Satellites Comprised of Tidal Dwarf Galaxies?
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MUSE: A second-generation integral-field spectrograph for the VLT
Published 2008“…The Multi Unit Spectroscopic Explorer (MUSE) is a second-generation instrument in development for the Very Large Telescope (VLT) of the European Southern Observatory (ESO), due to begin operation in 2011/12. …”
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Development of the HARMONI spectrograph for ESO’s Extremely Large Telescope
Published 2023“…HARMONI is the integral field spectrograph (IFS) for the European Southern Observatory's Extremely Large Telescope (ELT). …”
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Investigation of the Global Spatio-Temporal Characteristics of Astronomical Seeing
Published 2023-04-01“…The best seeing areas are generally discerned over the mid-latitude regions, consistent with the regions of the European Southern Observatory and Tibetan Plateau. In addition, the astronomical seeing values of the Tibetan Plateau in spring are better than in the other seasons. …”
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Optical Properties of Two Complementary Samples of Intermediate Seyfert Galaxies
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Long-Time Trends in Night Sky Brightness and Ageing of SQM Radiometers
Published 2022-11-01Get full text
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Identification of Bubble Nebulae around NGC 55 ULX-1 with MUSE Observations
Published 2023-01-01Get full text
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