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    Chapter

    Self-Assembled Dimeric Containers Based on Calix[4]arene, Resorcin[4]arene and Calix[4]pyrrole Scaffolds

    The understanding of the basic principles controlling reversible encapsulation processes is a key point for the development of valuable applications of synthetic molecular containers. Over the last decades, su...

    G. Aragay, P. Ballester in Calixarenes and Beyond (2016)

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    Chapter and Conference Paper

    Recent Developments in the Optimal Extraction of UVES Spectra

    J. M. Larsen, P. Ballester, V. D’Odorico in The 2007 ESO Instrument Calibration Worksh… (2008)

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    Chapter and Conference Paper

    IOT Overview: Calibrations of the VLTI Instruments (MIDI and AMBER)

    We present here a short review of the calibration processes that are currently applied to the instruments AMBER and MIDI of the VLTI (Very Large Telescope Interferometer) at Paranal. We first introduce the gen...

    S. Morel, F. Rantakyrö, T. Rivinius in The 2007 ESO Instrument Calibration Worksh… (2008)

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    Chapter and Conference Paper

    The PRIMA Astrometric Planet Search Project

    R. Launhardt, E. J. Bakker, P. Ballester in The Power of Optical/IR Interferometry: Re… (2008)

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    Chapter and Conference Paper

    The Detector Monitoring Project

    Many detectors, optical CCDs and IR arrays, are currently in operation onboard ESO instruments at the La Silla Paranal Observatory. A unified scheme for optical detector characterization has been adopted since...

    P. Amico, P. Ballester, W. Hummel in The 2007 ESO Instrument Calibration Worksh… (2008)

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    Chapter and Conference Paper

    A Bottom-Up Approach to Spectroscopic Data Reduction

    Any reference object identification based both on pattern-recognition techniques and on kee** to a minimum any instrument-specific assumption, goes in the direction of fulfilling the essential requisites of ...

    C. Izzo, Y. Jung, P. Ballester in The 2007 ESO Instrument Calibration Workshop (2008)

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    Article

    The VLTI – A Status Report

    The Very Large Telescope (VLT) Observatory on Cerro Paranal (2635 m) in Northern Chile is approaching completion. After the four 8-m Unit Telescopes (UT) individually saw first light in the last years, two of ...

    A. Glindemann, J. Algomedo, R. Amestica, P. Ballester in Astrophysics and Space Science (2003)

  8. No Access

    Chapter

    The VLTI — A Status Report

    The Very Large Telescope (VLT) Observatory on Cerro Paranal (2635 m) in Northern Chile is approaching completion. After the four 8-m Unit Telescopes (UT) individually saw first light in the last years, two of ...

    A. Glindemann, J. Algomedo, R. Amestica in The Very Large Telescope Interferometer Ch… (2003)