Abstract
We use FRIIb radio galaxy redshift-angular size data to constrain cosmological parameters in a dark energy scalar field model. The derived constraints are consistent with, but weaker than, those determined using Type Ia supernova redshift-magnitude data.
Original language | English (US) |
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Pages (from-to) | 577-579 |
Number of pages | 3 |
Journal | Astrophysical Journal |
Volume | 584 |
Issue number | 2 I |
DOIs | |
State | Published - Feb 20 2003 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science