TY - JOUR
T1 - The WAGGS project - I. The WiFeS Atlas of Galactic Globular cluster Spectra
AU - Usher, Christopher
AU - Pastorello, Nicola
AU - Bellstedt, Sabine
AU - Alabi, Adebusola
AU - Cerulo, Pierluigi
AU - Chevalier, Leonie
AU - Fraser-McKelvie, Amelia
AU - Penny, Samantha
AU - Foster, Caroline
AU - McDermid, Richard M.
AU - Schiavon, Ricardo P.
AU - Villaume, Alexa
N1 - 25 pages, 15 figures. Accepted for publication in the Monthly Notices of the Royal Astronomical Society
PY - 2017/7/1
Y1 - 2017/7/1
N2 - We present the WiFeS Atlas of Galactic Globular cluster Spectra, a library of integrated spectra of Milky Way and Local Group globular clusters. We used the WiFeS integral field spectrograph on the Australian National University 2.3 m telescope to observe the central regions of 64 Milky Way globular clusters and 22 globular clusters hosted by the Milky Way's low mass satellite galaxies. The spectra have wider wavelength coverage (3300 to 9050 Å) and higher spectral resolution (R = 6800) than existing spectral libraries of Milky Way globular clusters. By including Large and Small Magellanic Cloud star clusters, we extend the coverage of parameter space of existing libraries towards young and intermediate ages. While testing stellar population synthesis models and analysis techniques is the main aim of this library, the observations may also further our understanding of the stellar populations of Local Group globular clusters and make possible the direct comparison of extragalactic globular cluster integrated light observations with well understood globular clusters in the Milky Way. The integrated spectra are publicly available via the project website.
AB - We present the WiFeS Atlas of Galactic Globular cluster Spectra, a library of integrated spectra of Milky Way and Local Group globular clusters. We used the WiFeS integral field spectrograph on the Australian National University 2.3 m telescope to observe the central regions of 64 Milky Way globular clusters and 22 globular clusters hosted by the Milky Way's low mass satellite galaxies. The spectra have wider wavelength coverage (3300 to 9050 Å) and higher spectral resolution (R = 6800) than existing spectral libraries of Milky Way globular clusters. By including Large and Small Magellanic Cloud star clusters, we extend the coverage of parameter space of existing libraries towards young and intermediate ages. While testing stellar population synthesis models and analysis techniques is the main aim of this library, the observations may also further our understanding of the stellar populations of Local Group globular clusters and make possible the direct comparison of extragalactic globular cluster integrated light observations with well understood globular clusters in the Milky Way. The integrated spectra are publicly available via the project website.
KW - astro-ph.GA
KW - globular clusters: general
KW - galaxies: abundances
KW - Local Group
KW - galaxies: stellar content
U2 - 10.1093/mnras/stx713
DO - 10.1093/mnras/stx713
M3 - Article
SN - 0035-8711
VL - 468
SP - 3828
EP - 3849
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 4
ER -