Abstract The VST Photometric Hα Survey of the Southern Galactic Plane and Bulge
(VPHAS+) is surveying the southern Milky Way in u, g, r, i and Hα at∼ 1 arcsec angular …

ABSTRACT WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility
for the William Herschel Telescope, saw first light in late 2022. WEAVE comprises a new 2 …

ABSTRACT The INT/WFC Photometric Hα Survey of the Northern Galactic Plane (IPHAS) is
a 1800 deg2 imaging survey covering Galactic latitudes| b|< 5° and longitudes ℓ= 30°–215° …

Context. The Gaia-ESO Survey (GES) is a public, high-resolution spectroscopic survey,
conducted with the multi-object spectrograph Fibre Large Array Multi Element Spectrograph …

We have compiled a significantly updated and comprehensive census of massive stars in
the nearby Cygnus OB2 association by gathering and homogenizing data from across the …

We present a 3D map of extinction in the northern Galactic plane derived using photometry
from the INT/WFC Photometric Hα Survey of the northern Galactic plane. The map has fine …

Asteroseismology has the capability of precisely determining stellar properties that would
otherwise be inaccessible, such as radii, masses, and thus ages of stars. When coupling this …

The INT Galactic Plane Survey (IGAPS) is the merger of the optical photometric surveys,
IPHAS and UVEX, based on data from the Isaac Newton Telescope (INT) obtained between …

We present an astrometric and photometric wide-field study of the Galactic open star cluster
M37 (NGC 2099). The studied field was observed with ground-based images covering a …

We present the motivations for and methods we used to create a new ground-based
photometric survey of the field targeted by the NASA Kepler Mission. The survey contains …