Muestra métricas de impacto externas asociadas a la publicación. Para mayor detalle:
| Indexado |
|
||||
| DOI | 10.1093/MNRAS/STX713 | ||||
| Año | 2017 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
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 (3300-9050 angstrom) 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.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Usher, Christopher | Hombre |
Liverpool John Moores Univ - Reino Unido
Swinburne Univ Technol - Australia Liverpool John Moores University - Reino Unido Swinburne University of Technology - Australia |
| 2 | Pastorello, Nicola | Mujer |
Swinburne Univ Technol - Australia
Deakin Univ - Australia Swinburne University of Technology - Australia Deakin University - Australia |
| 3 | Bellstedt, Sabine | Mujer |
Swinburne Univ Technol - Australia
Swinburne University of Technology - Australia |
| 4 | Alabi, Adebusola | - |
Swinburne Univ Technol - Australia
Swinburne University of Technology - Australia |
| 5 | Espada, Daniel | Hombre |
Swinburne Univ Technol - Australia
Universidad de Concepción - Chile Swinburne University of Technology - Australia |
| 5 | Cerulo, Pierluigi | - |
Swinburne University of Technology - Australia
Universidad de Concepción - Chile |
| 6 | Chevalier, Leonie | Mujer |
Swinburne Univ Technol - Australia
Swinburne University of Technology - Australia |
| 7 | Fraser-Mckelvie, Amelia | Mujer |
MONASH UNIV - Australia
Monash University - Australia |
| 8 | Penny, Samantha | Mujer |
Univ Portsmouth - Reino Unido
University of Portsmouth - Reino Unido |
| 9 | Foster, Caroline | Mujer |
Australian Astron Observ - Australia
Australian Astronomical Observatory - Australia |
| 10 | McDermid, R. M. | Hombre |
Australian Astron Observ - Australia
Macquarie Univ - Australia Australian Astronomical Observatory - Australia Macquarie University - Australia |
| 11 | Schiavon, R. | Hombre |
Liverpool John Moores Univ - Reino Unido
Liverpool John Moores University - Reino Unido |
| 12 | Villaume, Alexa | Mujer |
Univ Calif Observ - Estados Unidos
University of California Observatories - Estados Unidos |
| Fuente |
|---|
| FONDECYT |
| National Science Foundation |
| European Research Council |
| National Aeronautics and Space Administration |
| California Institute of Technology |
| Horizon 2020 Framework Programme |
| FONDE-CYT |
| European Research Council (Multi-Pop) |
| AAO PhD Topup Scholarship |
| National Aeronautics and Space Administration’s Earth Science Technology Office |
| National Aeronautics and Space Administration's Earth Science Technology Office, Computational Technologies Project |
| American Academy of Ophthalmology |
| Swinburne Chancellor Research Scholarship |
| Agradecimiento |
|---|
| We thank the referee Soren Larsen for his useful comments and suggestions that helped to improve this paper. We also thank Nate Bastian, Joel Pfeffer and Thomas Beckwith for helpful discussions and useful suggestions. We are grateful to Paolo Bonfini, Martina Fagioli, Bililign Dullo, Elisa Boera, Srdan Kotus and Paul Frederic Robert for their assistance with the observations. We thank Simon O'Toole for his assistance with hosting the first WAGGS data release. We also wish to greatly thank the Siding Spring Observatory staff for their assistance with the ANU 2.3 m telescope and WiFeS instrument. We also wish to thank Jeremy Mould for originally suggesting the use of WiFeS to obtain integrated spectra of Local Group GCs. CU wishes to thank the University of Victoria's Department of Physics and Astronomy for their hospitality while a portion of this work was carried out. CU gratefully acknowledges financial support from the European Research Council (ERC-CoG-646928, Multi-Pop). PC acknowledges the support provided by FONDECYT postdoctoral research grant no. 3160375 and by the Swinburne Chancellor Research Scholarship and the AAO PhD Topup Scholarship during the 2015 observing runs. SB acknowledges the support of the AAO PhD Topup Scholarship. This work made use of NUMPY (van der Walt, Colbert & Varoquaux 2011), Scary (Jones et al. 2001) and MATPLOTLIB (Hunter 2007) as well as ASTROPY, a community-developed core PYTHON package for astronomy (Astropy Collaboration et al. 2013). Additionally, this work made use of TOPCAT (Taylor 2005) and ALADIN (Bonnarel et al. 2000). This work was partially performed on the swinSTAR supercomputer at Swinburne University of Technology. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. This research made use of Montage, funded by the National Aeronautics and Space Administration's Earth Science Technology Office, Computational Technologies Project, under Cooperative Agreement Number NCC5-626 between NASA and the California Institute of Technology. The code is maintained by the NASA/IPAC Infrared Science Archive. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This research is based on observations made with the NASA/ESA Hubble Space Telescope, and obtained from the Hubble Legacy Archive, which is a collaboration between the Space Telescope Science Institute (STScI/NASA), the Space Telescope European Coordinating Facility (ST-ECF/ESA) and the Canadian Astronomy Data Centre (CADC/NRC/CSA). |
| Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. This research made use of Montage, funded by the National Aeronautics and Space Administration’s Earth Science Technology Office, Computational Technologies Project, under Co-operative Agreement Number NCC5-626 between NASA and the California Institute of Technology. The code is maintained by the NASA/IPAC Infrared Science Archive. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This research is based on observations made with the NASA/ESA Hubble Space Telescope, and obtained from the Hubble Legacy Archive, which is a collaboration between the Space Telescope Science Institute (STScI/NASA), the Space Telescope European Coordinating Facility (ST-ECF/ESA) and the Canadian Astronomy Data Centre (CADC/NRC/CSA). |
| We thank the referee Søren Larsen for his useful comments and suggestions that helped to improve this paper. We also thank Nate Bastian, Joel Pfeffer and Thomas Beckwith for helpful discussions and useful suggestions. We are grateful to Paolo Bonfini, Martina Fagioli, Bililign Dullo, Elisa Boera, Srdan Kotus and Paul Frederic Robert for their assistance with the observations. We thank Simon O’Toole for his assistance with hosting the first WAGGS data release. We also wish to greatly thank the Siding Spring Observatory staff for their assistance with the ANU 2.3 m telescope and WiFeS instrument. We also wish to thank Jeremy Mould for originally suggesting the use of WiFeS to obtain integrated spectra of Local Group GCs. CU wishes to thank the University of Victoria’s Department of Physics and Astronomy for their hospitality while a portion of this work was carried out. CU gratefully acknowledges financial support from the European Research Council (ERC-CoG-646928, |
| Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. This research made use of Montage, funded by the National Aeronautics and Space Administration’s Earth Science Technology Office, Computational Technologies Project, under Co-operative Agreement Number NCC5-626 between NASA and the California Institute of Technology. The code is maintained by the NASA/IPAC Infrared Science Archive. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This research is based on observations made with the NASA/ESA Hubble Space Telescope, and obtained from the Hubble Legacy Archive, which is a collaboration between the Space Telescope Science Institute (STScI/NASA), the Space Telescope European Coordinating Facility (ST-ECF/ESA) and the Canadian Astronomy Data Centre (CADC/NRC/CSA). |