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Title: On Estimation of Contamination from Hydrogen Cyanide in Carbon Monoxide Line-intensity Mapping

Journal Article · · The Astrophysical Journal (Online)

Here, 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%.

Research Organization:
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1394079
Journal Information:
The Astrophysical Journal (Online), Vol. 846, Issue 1; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 11 works
Citation information provided by
Web of Science

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Cited By (8)

Joint Power Spectrum and Voxel Intensity Distribution Forecast on the CO Luminosity Function with COMAP journal January 2019
Probing Cosmic Origins with CO and [C ii] Emission Lines journal January 2019
Line Intensity Mapping with [C ii] and CO(1-0) as Probes of Primordial Non-Gaussianity journal February 2019
Extracting Bias Using the Cross-bispectrum: An EoR and 21 cm–[C ii]–[C ii] Case Study journal October 2018
Measuring the EoR Power Spectrum without Measuring the EoR Power Spectrum journal April 2019
Probing Cosmic Origins with CO and [CII] Emission Lines text January 2018
Line intensity mapping with [CII] and CO(1-0) as probes of primordial non-Gaussianity text January 2018
Measuring the EoR Power Spectrum Without Measuring the EoR Power Spectrum text January 2018