We perform the statistics of temperature maxima and minima in COBE-DMR 2-year maps. For power-law spectra the surface distribution of peaks implies an amplitude consistent with more conventional analyses of COBE data (for instance, we get Q_{{\rm rms-PS}}=17\pm 3\ \mu K for a spectral index % n=1), but not with the measured quadrupole Q_{{\rm rms}}=6\pm 3\ \mu K. This provides further support for the existence an infrared cutoff in the cosmic spectrum
Fourier analysis and power spectrum estimation of the cosmic microwave background anisotropy on an i...
We compute the three-point temperature correlation function of the {\it COBE} Differential Microwave...
We investigate the effect of a putative X-ray emitting halo surrounding the Local Group of galaxies,...
The angular power spectra of the infrared maps obtained by the DIRBE (Diffuse InfraRed Background Ex...
Fourier analysis and power spectrum estimation of the cosmic microwave background anisotropy on an i...
Density perturbations at the decoupling epoch produce angular fluctuations in the temperature of the...
We discuss the problem of CMB spectrum corruption during Galactic emission removing. A new technique...
We extend a previous bispectrum analysis of the Cosmic Microwave Background temperature anisotropy, ...
We review our recent claim that there is evidence of non-Gaussianity in the 4 Year COBE DMR data. We...
As part of the work performed under this contract, we have computed the 3- and 4-point correlation f...
Results from a cross-correlation analysis between the COBE DMR 4 year, and ROSAT PSPC All-Sky Survey...
A new method for estimating the power spectrum C_l from cosmic microwave background (CMB) maps was r...
Density perturbations at the decoupling epoch produce angular uctuations in the temperature of the ...
As part of the work performed under NASA contract # NAS5-32648, we have computed the 3-point and 4-p...
We perform a discrete wavelet analysis of the COBE-DMR 4yr sky maps and find a significant scale-sca...
Fourier analysis and power spectrum estimation of the cosmic microwave background anisotropy on an i...
We compute the three-point temperature correlation function of the {\it COBE} Differential Microwave...
We investigate the effect of a putative X-ray emitting halo surrounding the Local Group of galaxies,...
The angular power spectra of the infrared maps obtained by the DIRBE (Diffuse InfraRed Background Ex...
Fourier analysis and power spectrum estimation of the cosmic microwave background anisotropy on an i...
Density perturbations at the decoupling epoch produce angular fluctuations in the temperature of the...
We discuss the problem of CMB spectrum corruption during Galactic emission removing. A new technique...
We extend a previous bispectrum analysis of the Cosmic Microwave Background temperature anisotropy, ...
We review our recent claim that there is evidence of non-Gaussianity in the 4 Year COBE DMR data. We...
As part of the work performed under this contract, we have computed the 3- and 4-point correlation f...
Results from a cross-correlation analysis between the COBE DMR 4 year, and ROSAT PSPC All-Sky Survey...
A new method for estimating the power spectrum C_l from cosmic microwave background (CMB) maps was r...
Density perturbations at the decoupling epoch produce angular uctuations in the temperature of the ...
As part of the work performed under NASA contract # NAS5-32648, we have computed the 3-point and 4-p...
We perform a discrete wavelet analysis of the COBE-DMR 4yr sky maps and find a significant scale-sca...
Fourier analysis and power spectrum estimation of the cosmic microwave background anisotropy on an i...
We compute the three-point temperature correlation function of the {\it COBE} Differential Microwave...
We investigate the effect of a putative X-ray emitting halo surrounding the Local Group of galaxies,...