Publication type: Non-refereed

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    WEAVE-Apertif project: a compound integral-field and HI spectroscopic galaxy survey
    The WEAVE-Apertif survey combines spatially resolved optical and HI spectroscopic observations to investigate galaxy evolution using a representative sample of...
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    WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope
    We present the preliminary design of the WEAVE next generation spectroscopy facility for the William Herschel Telescope (WHT), principally targeting optical...
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    Web-Based Submission of Conference Papers
    Not Available
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    WeCAPP - The Wendelstein Calar Alto Pixellensing Project Tracing Dark and Bright Matter in M31
    We present WeCAPP, a long term monitoring project searching for microlensing events towards M31. Since 1997 the bulge of M31 was monitored in two different...
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    WeCAPP Survey. M31 variables (Fliri+, 2006)
    Observations of M31 were obtained using the 0.8-m telescope at Wendelstein, Germany and the 1.2-m telescope at Calar Alto, Spain, over three observing seasons...
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    Weierstrass Transform and the Analysis of Noisy Signals
    Not Available
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    WET Observations of the DAV G185-32
    The pulsating DAV white dwarf G185-32 was observed with the Whole Earth Telescope in 1992, during XCov8. We briefly report on the weighted Fourier transform of...
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    WFPC2 Multi-color Photometry of A- and B-type Supergiants in M31 and M33 for Application to the Wind-momentum Luminosity Relation
    We report the first results of a Hubble Space Telescope (HST) program which performed WFPC2 multi-color imaging of a sample of A- and B-type supergiant stars in...
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    What Are M31 Disk Planetary Nebulae Trying to Tell Us?
    Over the past eight years we have observed optical spectra of planetary nebulae (PNe) in the disk of M31 using DIS on the 3.5-m ARC telescope at Apache Point...