We present an attempt to measure the large angular scale fluctuations in the X-Ray Background (XRB) from the HEAO1 A2 data, expressed in terms of spherical harmonics. We model the harmonic coefficients assuming a power spectrum and an epoch-dependent bias parameter, and using a phenomenological scenario describing the evolution of the X-ray sources. From the few low-order multipoles detected (l<10), we estimate the power-spectrum normalisation on scales intermediate between those explored by local galaxy redshift surveys (~ 100 Mpc) and by the COBE Microwave Background measurements (~ 1000 Mpc). We find that the HEAO1 harmonics are consistent with present epoch rms fluctuations of the X-ray sources bx(0)sigma8 ~ 1-2 in 8 Mpc spheres. Theref...
Although COBE's detection of large angle microwave background anisotropies fixes the amplitude of de...
Recent deep X-ray surveys combined with spectroscopic identification of the sources have allowed the...
The advent of high signal-to-noise cosmic microwave background (CMB) anisotropy experiments now allo...
The precision of intensity measurements of the extragalactic X-ray background (XRB) on an angular sc...
In universes with significant curvature or cosmological constant, cosmic microwave background (CMB) ...
The hard X-ray (>2 keV) emission of the local and distant Universe as observed with the HEAO1-A2 exp...
We have studied the fluctuations of the soft (0.9-2 keV) X-ray background intensity for ~10 arcmin a...
We propose a new, simple, dedicated X-ray mission to measure the power spectrum of density fluctuati...
In this paper we discuss various possibilities of using X-ray observations to gain information about...
One of the most stringent constraints to date on the integrated Sachs-Wolfe effect, a critical test ...
We have studied the fluctuations of the soft (0.9-2 keV) X-ray background intensity for ∼10 and ∼2 a...
Using HEAO 1 A-2 all-sky survey data we have determined the amplitude of intensity fluctuations of t...
The shape of the primordial fluctuation spectrum is probed by cosmic microwave background fluctuatio...
Fluctuations of the surface brightness of cosmic X-ray background (CXB) carry unique information abo...
Cosmological theories for the origin and evolution of structure in the Universe are highly predictiv...
Although COBE's detection of large angle microwave background anisotropies fixes the amplitude of de...
Recent deep X-ray surveys combined with spectroscopic identification of the sources have allowed the...
The advent of high signal-to-noise cosmic microwave background (CMB) anisotropy experiments now allo...
The precision of intensity measurements of the extragalactic X-ray background (XRB) on an angular sc...
In universes with significant curvature or cosmological constant, cosmic microwave background (CMB) ...
The hard X-ray (>2 keV) emission of the local and distant Universe as observed with the HEAO1-A2 exp...
We have studied the fluctuations of the soft (0.9-2 keV) X-ray background intensity for ~10 arcmin a...
We propose a new, simple, dedicated X-ray mission to measure the power spectrum of density fluctuati...
In this paper we discuss various possibilities of using X-ray observations to gain information about...
One of the most stringent constraints to date on the integrated Sachs-Wolfe effect, a critical test ...
We have studied the fluctuations of the soft (0.9-2 keV) X-ray background intensity for ∼10 and ∼2 a...
Using HEAO 1 A-2 all-sky survey data we have determined the amplitude of intensity fluctuations of t...
The shape of the primordial fluctuation spectrum is probed by cosmic microwave background fluctuatio...
Fluctuations of the surface brightness of cosmic X-ray background (CXB) carry unique information abo...
Cosmological theories for the origin and evolution of structure in the Universe are highly predictiv...
Although COBE's detection of large angle microwave background anisotropies fixes the amplitude of de...
Recent deep X-ray surveys combined with spectroscopic identification of the sources have allowed the...
The advent of high signal-to-noise cosmic microwave background (CMB) anisotropy experiments now allo...