Relativistic effects of our galaxy's motion on circles-in-the-sky in CMB maps
- 6 May 2005
- journal article
- Published by IOP Publishing in Classical and Quantum Gravity
- Vol. 22 (11) , 1991-1999
- https://doi.org/10.1088/0264-9381/22/11/005
Abstract
No abstract availableAll Related Versions
This publication has 19 references indexed in Scilit:
- A hint of Poincaré dodecahedral topology in the WMAP first year sky mapAstronomy & Astrophysics, 2004
- Constraining the Topology of the UniversePhysical Review Letters, 2004
- Significance of the largest scale CMB fluctuations in WMAPPhysical Review D, 2004
- Dodecahedral space topology as an explanation for weak wide-angle temperature correlations in the cosmic microwave backgroundNature, 2003
- First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Preliminary Maps and Basic ResultsThe Astrophysical Journal Supplement Series, 2003
- First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Determination of Cosmological ParametersThe Astrophysical Journal Supplement Series, 2003
- First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: The Angular Power SpectrumThe Astrophysical Journal Supplement Series, 2003
- TheMicrowave Anisotropy ProbeMissionThe Astrophysical Journal, 2003
- Detectability of cosmic topology in almost flat universesClassical and Quantum Gravity, 2001
- Are small hyperbolic universes observationally detectable?Classical and Quantum Gravity, 2001