Tipo de publicación: Sin árbitro

  • Publicación
    The WEAVE observatory control system
    WEAVE is the next-generation spectroscopic facility for the William Herschel Telescope (WHT) 1,2. WEAVE offers multi-object (1000 fibres) and integral-field...
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    The WEAVE prime focus correction: from design to integration
    WEAVE is a new wide-field multi-object spectroscopy (MOS) facility proposed for the prime focus of the 4.2m William Herschel Telescope (WHT), situated on the...
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    The WEAVE-Apertif Survey: galaxy evolution and dynamics
    The WEAVE-Apertif (WA) survey on the William Herschel Telescope will perform dedicated large integral field unit (LIFU; 90") optical spectroscopy follow-up of...
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    The WeCAPP variable star catalogue of M31 .
    We present the WeCAPP catalogue of variable stars found in the bulge of M31 citep{wecapp05}. Observations in the WeCAPP microlensing survey (optical R and I...
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    The Western Bulge of 162173 Ryugu Formed as a Result of a Rotationally Driven Deformation Process
    162173 Ryugu, the target of Hayabusa2, is a spinning top-shaped asteroid. Observations by Optical Navigation Camera onboard Hayabusa2 have shown that the...
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    The WEUSC Operational System Implemented Using JAVA and XML Technologies
    Not Available
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    The Whole Earth Blazar Telescope and the BL Lac Campaign 2000
    We present R-band light curves of BL Lacertae from May 2000 to January 2001, obtained by 22 telescopes in 11 countries. More than 15000 UBVRI observations were...
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    The Whole Earth Blazar telescope on BL Lacertae (Poster)
    The Whole Earth Blazar Telescope (WEBT) is an international consortium of about 30 optical observatories and 2 radio observatories devoted to blazar monitoring...
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    The Wide Field Imager at the 2.2-m MPG/ESO telescope: first views with a 67-million-facette eye.
    The basic capabilities of the Wide Field Imager (WFI) were described in a previous Messenger article (No. 93, p. 13; see also Table 1) which also includes a...