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27 results on '"Contaldi C."'

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1. A Simulation-based Method for Correcting Mode Coupling in CMB Angular Power Spectra

2. A Constraint on Primordial B-modes from the First Flight of the Spider Balloon-borne Telescope

3. The XFaster Power Spectrum and Likelihood Estimator for the Analysis of Cosmic Microwave Background Maps

4. A New Limit on CMB Circular Polarization from SPIDER

5. The Anisotropy of the Microwave Background tol= 3500: Mosaic Observations with the Cosmic Background Imager

6. SPIDER OPTIMIZATION. II. OPTICAL, MAGNETIC, AND FOREGROUND EFFECTS

7. SUBDEGREE SUNYAEV-ZEL'DOVICH SIGNAL FROM MULTIFREQUENCY BOOMERANG OBSERVATIONS

8. HIGH-RESOLUTION CMB POWER SPECTRUM FROM THE COMPLETE ACBAR DATA SET

9. SpiderOptimization: Probing the Systematics of a Large‐ScaleB‐Mode Experiment

10. Searching for Non-Gaussian Signals in the BOOMERANG 2003 CMB Maps

11. Improved Measurements of the CMB Power Spectrum with ACBAR

12. Implications of the Cosmic Background Imager Polarization Data

13. Cosmological Parameters from the 2003 Flight of BOOMERANG

14. A Measurement of the Polarization‐Temperature Angular Cross‐Power Spectrum of the Cosmic Microwave Background from the 2003 Flight of BOOMERANG

15. A Measurement of the CMB 〈EE〉 Spectrum from the 2003 Flight of BOOMERANG

16. A Measurement of the Angular Power Spectrum of the CMB Temperature Anisotropy from the 2003 Flight of BOOMERANG

17. The Sunyaev‐Zel'dovich Effect in CMB‐calibrated Theories Applied to the Cosmic Background Imager Anisotropy Power atl> 2000

18. Extended Mosaic Observations with the Cosmic Background Imager

19. Estimates of Cosmological Parameters Using the Cosmic Microwave Background Angular Power Spectrum of ACBAR

20. Improved Measurement of the Angular Power Spectrum of Temperature Anisotropy in the Cosmic Microwave Background from Two New Analyses of BOOMERANG Observations

21. A Fast Gridded Method for the Estimation of the Power Spectrum of the Cosmic Microwave Background from Interferometer Data with Application to the Cosmic Background Imager

22. The Anisotropy of the Microwave Background tol= 3500: Deep Field Observations with the Cosmic Background Imager

23. Cosmological Parameters from Cosmic Background Imager Observations and Comparisons with BOOMERANG, DASI, and MAXIMA

24. Search for Non-Gaussian Signals in the BOOMERANG Maps: Pixel-Space Analysis

25. A Measurement by BOOMERANG of Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background

26. Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background: Significance and Consequences for Cosmology

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