Detection of X-ray Emission from the Warm-Hot Intergalactic Medium through the Angular Autocorrelation Function with Chandra
M Galeazzi, A Gupta, K Huffenberger… - arXiv preprint arXiv …, 2012 - arxiv.org
M Galeazzi, A Gupta, K Huffenberger, E Ursino
arXiv preprint arXiv:1205.5753, 2012•arxiv.org[1205.5753] Detection of X-ray Emission from the Warm-Hot Intergalactic Medium through the
Angular Autocorrelation Function with Chandra Skip to main content Cornell University We
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Cosmology and Nongalactic Astrophysics arXiv:1205.5753 (astro-ph) This paper has been …
Angular Autocorrelation Function with Chandra Skip to main content Cornell University We
gratefully acknowledge support from the Simons Foundation, member institutions, and all
contributors. Donate arxiv logo > astro-ph > arXiv:1205.5753 Help | Advanced Search Search
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Cosmology and Nongalactic Astrophysics arXiv:1205.5753 (astro-ph) This paper has been …
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.
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