publication . Article . Preprint . 2019

The morphology and structure of stellar populations in the Fornax dwarf spheroidal galaxy from Dark Energy Survey Data

Mei-Yu Wang; T. J. L. de Boer; A. Pieres; Ting Li; Alex Drlica-Wagner; Sergey E. Koposov; A. K. Vivas; Andrew B. Pace; Basilio X. Santiago; A. R. Walker; ...
Open Access English
  • Published: 21 Aug 2019
  • Publisher: HAL CCSD
Comment: 15 pages, 10 figures, 3 tables, submitted to ApJ
free text keywords: [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Matéria escura, Formacao de estrelas, Populacoes estelares, Galáxias anãs, dwarf [Galaxies], individual (Fornax) [galaxies], Local group, astro-ph.GA, Astrophysics - Astrophysics of Galaxies, Space and Planetary Science, Astronomy and Astrophysics, RCUK, STFC, /dk/atira/pure/subjectarea/asjc/3100/3103, Astronomy and Astrophysics, /dk/atira/pure/subjectarea/asjc/1900/1912, Space and Planetary Science, Local Group, Photometry (optics), Surface brightness, Galaxy, Stars, Stellar population, Dark energy, Astrophysics, Dwarf spheroidal galaxy, Physics
Related Organizations
Funded by
Capitalizing on Gravitational Shear
  • Funder: European Commission (EC)
  • Project Code: 240672
  • Funding stream: FP7 | SP2 | ERC
Understanding the Origin of Cosmic Structure
  • Funder: European Commission (EC)
  • Project Code: 306478
  • Funding stream: FP7 | SP2 | ERC
Galaxy formation through the eyes of globular clusters
  • Funder: European Commission (EC)
  • Project Code: 335936
  • Funding stream: FP7 | SP2 | ERC
Testing the Dark Energy Paradigm and Measuring Neutrino Mass with the Dark Energy Survey
  • Funder: European Commission (EC)
  • Project Code: 291329
  • Funding stream: FP7 | SP2 | ERC
NSF| Collaborative Research: The Dark Energy Survey Data Management Operations
  • Funder: National Science Foundation (NSF)
  • Project Code: 1138766
  • Funding stream: Directorate for Mathematical & Physical Sciences | Division of Astronomical Sciences
63 references, page 1 of 5

NGMIX CLASS = ((CM T + 5 CM T ERR) > 0.1)

+ ((CM T + CM T ERR) > 0.05)

+ ((CM T − CM T ERR) > 0.02).

Aihara, H., Arimoto, N., Armstrong, R., et al. 2018, PASJ, 70, S4

Amorisco, N. C., & Evans, N. W. 2012, ApJ, 756, L2

Astropy Collaboration, Robitaille, T. P., Tollerud, E. J., et al. 2013, A&A, 558, A33

Bate, N. F., McMonigal, B., Lewis, G. F., et al. 2015, MNRAS, 453, 690

Battaglia, G., Tolstoy, E., Helmi, A., et al. 2006, A&A, 459, 423

Bersier, D. 2000, ApJ, 543, L23

Bertin, E., & Arnouts, S. 1996, A&AS, 117, 393

Bertin, E., Mellier, Y., Radovich, M., et al. 2002, in Astronomical Society of the Pacific Conference Series, Vol. 281, Astronomical Data Analysis Software and Systems XI, ed. D. A. Bohlender, D. Durand, & T. H. Handley, 228

Choi, J., Dotter, A., Conroy, C., et al. 2016, ApJ, 823, 102

Coleman, M., Da Costa, G. S., Bland-Hawthorn, J., et al. 2004, AJ, 127, 832

Coleman, M. G., Da Costa, G. S., Bland-Hawthorn, J., & Freeman, K. C. 2005, AJ, 129, 1443

Coleman, M. G., & de Jong, J. T. A. 2008, ApJ, 685, 933

63 references, page 1 of 5
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