The MONOS project has obtained WEAVE LIFU observations to study the cores of nine stellar clusters containing O and B stars. Most O stars form in multiple...
WEAVE is the next-generation wide-field optical spectroscopy facility for the William Herschel Telescope (WHT) in La Palma, Canary Islands, Spain. WEAVE mainly...
WEAVE spectrograph cameras: the polishing of the spherical lenses
WEAVE is the new wide field multi-object and integral field survey facility for the prime focus of the 4.2 m William Herschel Telescope. WEAVE fiber-fed...
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...
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...
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...
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...