Published January 1989
| Version v1
Journal article
Autocorrelation properties of fluctuations in the cosmic X-ray background
Creators
- 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
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 20047631
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BACKGROUND RADIATION; CORRELATION FUNCTIONS; COSMIC PHOTONS; FLUCTUATIONS; GALAXY CLUSTERS; GALAXY NUCLEI; LIMITING VALUES
- Descriptors DEC
- BOSONS; COSMIC RADIATION; ELEMENTARY PARTICLES; FUNCTIONS; IONIZING RADIATIONS; MASSLESS PARTICLES; PHOTONS; RADIATIONS; VARIATIONS