389 citations
- Saha Institute of Nuclear PhysicsIN7 papers
- Virginia Commonwealth UniversityUS7 papers
- Variable Energy Cyclotron CentreIN5 papers
- CEA Paris-SaclayFR3 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR3 papers
- Institut de Recherche sur les Lois Fondamentales de l'UniversFR3 papers
- Massachusetts Institute of TechnologyUS3 papers
- Argonne National LaboratoryUS2 papers
- Arizona State UniversityUS2 papers
- California State University, Dominguez HillsUS2 papers
- Carnegie Mellon UniversityUS2 papers
- Catholic University of AmericaUS2 papers
6 papers · 1 filter
Phase Shift Sequences for an Adding Interferometer
Peter Hyland, Brent Follin, Emory F. Bunn
Cosmic microwave background (CMB) polarimetry has the potential to provide revolutionary advances in cosmology. Future experiments to detect the very weak B mode signal in CMB pola…
Contamination cannot explain the lack of large-scale power in the cosmic microwave background radiation
Emory F. Bunn, Austin Bourdon
Several anomalies appear to be present in the large-angle cosmic microwave background (CMB) anisotropy maps of WMAP. One of these is a lack of large-scale power. Because the data o…
Constraining f(R) Gravity as a Scalar Tensor Theory
Thomas Faulkner, Max Tegmark, Emory F. Bunn +1
We search for viable f(R) theories of gravity, making use of the equivalence between such theories and scalar-tensor gravity. We find that models can be made consistent with solar…
Systematic Errors in Cosmic Microwave Background Interferometry
Emory F. Bunn
Cosmic microwave background (CMB) polarization observations will require superb control of systematic errors in order to achieve their full scientific potential, particularly in th…
Mosaicking with cosmic microwave background interferometers
Emory F. Bunn, Martin White
Measurements of cosmic microwave background (CMB) anisotropies by interferometers offer several advantages over single-dish observations. The formalism for analyzing interferometer…
Probing the Universe on Gigaparsec Scales with Remote Cosmic Microwave Background Quadrupole Measurements
Emory F. Bunn
Scattering of cosmic microwave background (CMB) radiation in galaxy clusters induces a polarization signal proportional to the CMB quadrupole anisotropy at the cluster's location a…