期刊
PHYSICS LETTERS B
卷 715, 期 1-3, 页码 9-14出版社
ELSEVIER SCIENCE BV
DOI: 10.1016/j.physletb.2012.07.011
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资金
- DOE grant [DEFG030-99EP41093]
- NSF grant [AST-1109275]
- SNSF (SCOPES grant) [128040]
- Direct For Mathematical & Physical Scien
- Division Of Astronomical Sciences [1109275] Funding Source: National Science Foundation
In this Letter we use H II starburst galaxy apparent magnitude versus redshift data from Siegel et al. (2005) [74] to constrain dark energy cosmological model parameters. These constraints are generally consistent with those derived using other data sets, but are not as restrictive as the tightest currently available constraints. (c) 2012 Elsevier B.V. All rights reserved.
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