Published January 1989 | Version v1
Journal article

Autocorrelation properties of fluctuations in the cosmic X-ray background

  • 1. Padova Universita, Padua (Italy)
  • 2. Osservatorio Astronomico, Padua (Italy)
  • 3. Osservatorio Astronomico, Trieste (Italy)
  • 4. NASA, Goddard Space Flight Center, Greenbelt, MD (USA)

Description

The HEAO 1 A-2 all-sky survey data have been analyzed to investigate the autocorrelation function of the surface brightness fluctuations of the extragalactic 2-10 keV X-ray background on angular scales ranging from 3 to 27 deg. The derived upper limits are compatible with optical estimates of the spatial correlation function of Abell's clusters and set interesting constraints on possible AGN clustering. 25 references

Additional details

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
336
Series
Astrophys. J.
Journal Page Range
L47-L50
ISSN
0004-637X
CODEN
ASJOA