Add to ORKGThe WMAP mission has produced sky maps from seven years of observations at L2. We present the angular power spectra derived from the seven-year maps and discuss the cosmological conclusions that can be inferred from WMAP data alone. With the seven-year data, the temperature (TT) spectrum measurement has a signal-to-noise ratio per multipole that exceeds unity for l < 919; and in band powers of width Δl = 10, the signal-to-noise rati
iPreface This document is a concise description of the delivered data sets for the nine years of sci...
We present new full-sky temperature and polarization maps in five frequency bands from 23 to 94 GHz,...
We present WMAP seven-year observations of bright sources which are often used as calibrators at mic...
The WMAP mission has produced sky maps from seven years of observations at L2. We present the angula...
The WMAP mission has produced sky maps from 7 years of observations at L2. We present the angular po...
The WMAP mission has produced sky maps from seven years of observations at L2. We present the angula...
New full-sky temperature and polarization maps based on seven years of data from WMAP are presented....
New full-sky temperature and polarization maps based on seven years of data from WMAP are presented....
New full-sky temperature and polarization maps based on seven years of data from WMAP are presented....
New full sky temperature and polarization maps based on seven years of data from WMAP are presented....
We present WMAP seven-year observations of bright sources which are often used as calibrators at mic...
The combination of 7-year data from WMAP and improved astrophysical data rigorously tests the standa...
The combination of seven-year data from WMAP and improved astrophysical data rigorously tests the st...
We present new full-sky temperature maps in five frequency bands from 23 to 94 GHz, based on the fir...
The combination of seven-year data from WMAP and improved astrophysical data rigorously tests the st...
iPreface This document is a concise description of the delivered data sets for the nine years of sci...
We present new full-sky temperature and polarization maps in five frequency bands from 23 to 94 GHz,...
We present WMAP seven-year observations of bright sources which are often used as calibrators at mic...
The WMAP mission has produced sky maps from seven years of observations at L2. We present the angula...
The WMAP mission has produced sky maps from 7 years of observations at L2. We present the angular po...
The WMAP mission has produced sky maps from seven years of observations at L2. We present the angula...
New full-sky temperature and polarization maps based on seven years of data from WMAP are presented....
New full-sky temperature and polarization maps based on seven years of data from WMAP are presented....
New full-sky temperature and polarization maps based on seven years of data from WMAP are presented....
New full sky temperature and polarization maps based on seven years of data from WMAP are presented....
We present WMAP seven-year observations of bright sources which are often used as calibrators at mic...
The combination of 7-year data from WMAP and improved astrophysical data rigorously tests the standa...
The combination of seven-year data from WMAP and improved astrophysical data rigorously tests the st...
We present new full-sky temperature maps in five frequency bands from 23 to 94 GHz, based on the fir...
The combination of seven-year data from WMAP and improved astrophysical data rigorously tests the st...
iPreface This document is a concise description of the delivered data sets for the nine years of sci...
We present new full-sky temperature and polarization maps in five frequency bands from 23 to 94 GHz,...
We present WMAP seven-year observations of bright sources which are often used as calibrators at mic...