Detection of X-ray Emission from the Warm-Hot Intergalactic Medium through the Angular Autocorrelation Function with Chandra
Cosmology and Nongalactic Astrophysics
2012-09-28 v2
Abstract
We have used the angular Autocorrelation Function (AcF) in a pointing with Chandra's ACIS-S instrument. However, we determined that the contribution of Chandra's background below 1 keV is too high to achieve reasonable sensitivity.
Cite
@article{arxiv.1205.5753,
title = {Detection of X-ray Emission from the Warm-Hot Intergalactic Medium through the Angular Autocorrelation Function with Chandra},
author = {Massimiliano Galeazzi and Anjali Gupta and Kevin Huffenberger and Eugenio Ursino},
journal= {arXiv preprint arXiv:1205.5753},
year = {2012}
}
Comments
This paper has been withdrawn by the authors