The deconvolved distribution estimator: enhancing reionization-era CO line-intensity mapping analyses with a cross-correlation analogue for one-point statistics

Author:

Chung Dongwoo T12ORCID,Bangari Ishika3,Breysse Patrick C4ORCID,Ihle Håvard T5,Bond J Richard1,Dunne Delaney A6,Padmanabhan Hamsa7ORCID,Philip Liju6,Rennie Thomas J8,Viero Marco P6ORCID,

Affiliation:

1. Canadian Institute for Theoretical Astrophysics, University of Toronto , 60 St. George Street, Toronto, ON M5S 3H8, Canada

2. Dunlap Institute for Astronomy and Astrophysics, University of Toronto , 50 St. George Street, Toronto, ON M5S 3H4, Canada

3. David A. Dunlap Department of Astronomy and Astrophysics, University of Toronto , 50 St. George Street, Toronto, ON M5S 3H4, Canada

4. Center for Cosmology and Particle Physics, Department of Physics, New York University , 726 Broadway, New York, NY 10003, USA

5. Institute of Theoretical Astrophysics, University of Oslo , PO Box 1029 Blindern, N-0315 Oslo, Norway

6. California Institute of Technology , 1200 E. California Blvd., Pasadena, CA 91125, USA

7. Département de Physique Théorique, Université de Genève , 24 Quai Ernest-Ansermet, CH-1211 Genève 4, Switzerland

8. Jodrell Bank Centre for Astrophysics, Alan Turing Building, Department of Physics and Astronomy, The University of Manchester , Oxford Road, Manchester M13 9PL, UK

Abstract

ABSTRACT We present the deconvolved distribution estimator (DDE), an extension of the voxel intensity distribution (VID), in the context of future observations proposed as part of the CO Mapping Array Project (COMAP). The DDE exploits the fact that the observed VID is a convolution of correlated signal intensity distributions and uncorrelated noise or interloper intensity distributions. By deconvolving the individual VID of two observables away from their joint VID in a Fourier-space operation, the DDE suppresses sensitivity to interloper emission while maintaining sensitivity to correlated components. The DDE thus improves upon the VID by reducing the relative influence of uncorrelated noise and interloper biases, which is useful in the context of COMAP observations that observe different rotational transitions of CO from the same comoving volume in different observing frequency bands. Fisher forecasts suggest that the theoretical sensitivity in the DDE allows significant improvements in constraining power compared to either the cross power spectrum or the individual VID data, and matches the constraining power of the combination of all other one- and two-point summary statistics. Future work should further investigate the covariance and model-dependent behaviour of this novel one-point cross-correlation statistic.

Funder

NSERC

CIFAR

Canada Foundation for Innovation

University of Toronto

Research Council of Norway

European Research Council

National Science Foundation

Swiss National Science Foundation

STFC

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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