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• W3103695338 abstract "Line-intensity mapping surveys probe large-scale structure through spatial variations in molecular line emission from a population of unresolved cosmological sources. Future such surveys of carbon monoxide line emission, specifically the CO(1-0) line, face potential contamination from a disjointed population of sources emitting in a hydrogen cyanide emission line, HCN(1-0). This paper explores the potential range of the strength of HCN emission and its effect on the CO auto power spectrum, using simulations with an empirical model of the CO/HCN–halo connection. We find that effects on the observed CO power spectrum depend on modeling assumptions but are very small for our fiducial model, which is based on current understanding of the galaxy–halo connection. Given the fiducial model, we expect the bias in overall CO detection significance due to HCN to be less than 1%." @default.
• W3103695338 created "2020-11-23" @default.
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• W3103695338 date "2017-08-31" @default.
• W3103695338 modified "2023-10-02" @default.
• W3103695338 title "On Estimation of Contamination from Hydrogen Cyanide in Carbon Monoxide Line-intensity Mapping" @default.
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• W3103695338 doi "https://doi.org/10.3847/1538-4357/aa8624" @default.
• W3103695338 hasPublicationYear "2017" @default.
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