Methodological refinement of the submillimeter galaxy magnification bias. II. Cosmological analysis with tomography

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This paper is the third in a series on submillimeter galaxy magnification bias, focusing on the tomographic scenario.

• It refines the methodology used to constrain the halo occupation distribution model and cosmological parameters within a flat $\Lambda$CDM model, using updated data.
• The study aims to optimize CPU time, explore strategies for analyzing different redshift bins, and assess the impact of excluding the GAMA15 field.
• The tomographic approach involves dividing the redshift range into bins and analyzing cross-correlation measurements between submillimeter and foreground galaxies.