A ~5 sigma cross-power signal between Spitzer infrared and Chandra X-ray background fluctuations is detected at large angular scales, and its soft X-ray spectrum is consistent with a power-law produced by accreting compact objects.
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Spectral Properties Of Populations Behind The Coherence In Spitzer Near-Infrared And Chandra X-Ray Backgrounds
A ~5 sigma cross-power signal between Spitzer infrared and Chandra X-ray background fluctuations is detected at large angular scales, and its soft X-ray spectrum is consistent with a power-law produced by accreting compact objects.