[INGNEWS] ING ANNOUNCEMENT OF OPPORTUNITY FOR OBSERVING TIME IN SEMESTER 2008B

From: Rene Rutten (rgmr@ing.iac.es)
Date: Thu Feb 21 2008 - 14:29:22 PST

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    ING ANNOUNCEMENT OF OPPORTUNITY FOR OBSERVING TIME IN SEMESTER 2008B

    The semester 2008B announcement of opportunity for observing time at the
    Isaac Newton Group of Telescopes on La Palma can be found at:

    http://www.ing.iac.es/Astronomy/observing/2008B_AO.html

    Please feel free to distribute this announcement in your institute.

    I would like to bring to your special attention the following aspects
    related to the ING telescopes.

    1. Last year the laser guide beacon for Adaptive Optics on the WHT was
    commissioned. During the next several months science verification and system
    characterization will take place, and a special call for service observing
    time has been issued (deadline 29 Feb 2008; see
    http://www.ing.iac.es/Astronomy/observing/2008AServiceAO.html ).
    The GLAS laser system is also available for general applications for
    observing time in semester 2008B.

    2. I highlight here the advent of a new detector for the ISIS spectrograph,
    QUCAM. This frame-transfer L3CCD (or EMCCD) allows very fast spectroscopy
    with virtually zero read noise. It opens a new window at the WHT on the
    highly variable universe. For details please see the ISIS web page under
    http://www.ing.iac.es/Astronomy/ or contact the instrument specialist
    (prguez@ing.iac.es).

    3. Although the future of the 2.5-m Isaac Newton Telescope remains uncertain
    beyond 2009, we still welcome in particular large proposals for observing
    time. The observatory will continue to support this telescope and its
    instrumentation into the foreseeable future.

    4. INGs future:
    Recent developments in the UK have resulted in rumors over the future of the
    ING telescopes on La Palma. Although the future in the longer term is indeed
    not guaranteed, there is no indication that the observatory is under
    immediate threat. This is probably best indicated by the active development
    programme for the WHT, specifically of the ACAM imager that will be
    completed this year, and the fact that we expect to sign an agreement very
    soon over the deployment of a world-class high-resolution spectrograph
    HARPS-NEF that will become available from 2010 onwards.

    Further details of the proposal submission process and current
    instrumentation at ING can be found at:

    http://www.ing.iac.es/Astronomy/observing/INGinfo_home.html
    and
    http://www.ing.iac.es/Astronomy/

    Rene Rutten
    Director, ING
    21 February 2008

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