• Open Access

Photometric redshifts and intrinsic alignments: Degeneracies and biases in the 3×2pt analysis

C. Danielle Leonard, Markus Michael Rau, and Rachel Mandelbaum
Phys. Rev. D 109, 083528 – Published 25 April 2024

Abstract

We present a systematic study of cosmological parameter bias in weak lensing and large-scale structure analyses for upcoming imaging surveys induced by the interplay of intrinsic alignments (IA) and photometric redshift (photo-z) model misspecification error. We first examine the degeneracies between the parameters of the tidal alignment–tidal torquing (TATT) model for IA and of a photo-z model including a mean shift (Δz¯) and variance (σz) for each tomographic bin of lenses and sources, under a variety of underlying true IA behaviors. We identify strong degeneracies between: (1) the redshift scaling of the tidal alignment amplitude and the mean shift and variances of source bins, (2) the redshift scaling of the tidal torquing amplitude and the variance of the lowest-z source bin, and (3) the IA source density weighting and the mean shift and variance of several source bins. We then use this information to guide our exploration of the level of cosmological parameter bias which can be induced given incorrect modeling of IA, photo-z, or both. We find that marginalizing over all the parameters of TATT is generally sufficient to preclude cosmological parameter bias in the scenarios we consider. However, this does not necessarily mean that IA and photo-z parameters are themselves unbiased, nor does it mean that the best-fit model is a good fit to the data. We also find scenarios where the inferred parameters produce χd.o.f.2 values indicative of a good fit but cosmological parameter bias is significant, particularly when the IA source density weighting parameter is not marginalized over.

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  • Received 12 January 2024
  • Accepted 28 March 2024

DOI:https://doi.org/10.1103/PhysRevD.109.083528

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

C. Danielle Leonard1,*, Markus Michael Rau1,2, and Rachel Mandelbaum3

  • 1School of Mathematics, Statistics and Physics, Newcastle University, Newcastle upon Tyne NE1 7RU, United Kingdom
  • 2High Energy Physics Division, Argonne National Laboratory, Lemont, Illinois 60439, USA
  • 3McWilliams Center for Cosmology, Department of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15213, USA

  • *danielle.leonard@newcastle.ac.uk

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Issue

Vol. 109, Iss. 8 — 15 April 2024

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