Clues from $\mathcal{Q}$--A null test designed for line intensity mapping cross-correlation studies
Debanjan Sarkar, Ella Iles, Adrian Liu

TL;DR
This paper introduces a new diagnostic statistic, al, for validating assumptions in cross-correlation based auto-spectrum estimation in line-intensity mapping, enhancing robustness against systematics.
Contribution
The al statistic is a novel, data-driven null test that assesses the validity of key assumptions in cross-spectrum auto-spectrum reconstruction using multiple spectral lines.
Findings
al reliably identifies regimes where assumptions hold
Deviations in al indicate violations of linear bias or correlation assumptions
Validated through analytic models and simulations across various redshifts and configurations
Abstract
Estimating the auto power spectrum of cosmological tracers from line-intensity mapping (LIM) data is often limited by instrumental noise, residual foregrounds, and systematics. Cross-power spectra between multiple lines offer a robust alternative, mitigating noise bias and systematics. However, inferring the auto spectrum from cross-correlations relies on two key assumptions: that all tracers are linearly biased with respect to the matter density field, and that they are strongly mutually correlated. In this work, we introduce a new diagnostic statistic, \(\mathcal{Q}\), which serves as a data-driven null test of these assumptions. Constructed from combinations of cross-spectra between four distinct spectral lines, \(\mathcal{Q}\) identifies regimes where cross-spectrum-based auto-spectrum reconstruction is unbiased. We validate its behavior using both analytic toy models and…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astrophysics and Star Formation Studies · Astronomy and Astrophysical Research
