CROSS-CORRELATIONS AS A COSMOLOGICAL CARBON MONOXIDE DETECTOR

We present a new procedure to measure the large-scale carbon monoxide (CO) emissions across cosmic history. As a tracer of large-scale structure (LSS), the CO gas content as a function of redshift can be quantified by its three-dimensional fluctuation power spectra. Furthermore, cross-correlating CO...

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Veröffentlicht in:The Astrophysical journal 2013-05, Vol.768 (1), p.1-15
Hauptverfasser: Pullen, Anthony R, Chang, Tzu-Ching, Dore, Olivier, Lidz, Adam
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Sprache:eng
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