17The Rhizaria is a super-group of ameoboid protists with ubiquitous distributions, from the 18 euphotic zone to the twilight zone and beyond. While rhizarians have been recently described as 19 important contributors to both silica and carbon fluxes, we lack the most basic information about 20 their ecological preferences. Here, using the in situ imaging (Underwater Vision Profiler 5), we 21 characterize the vertical ecological niches of different test-bearing rhizarian taxa in the southern 22California Current Ecosystem. We define three vertical layers between 0-500 m occupied, 23 respectively, by 1) surface dwelling and mostly symbiont-bearing rhizarians (Acantharia and 24 Collodaria), 2) flux-feeding phaeodarians in the lower epipelagic (100-200 m), and 3) 25Foraminifera and Phaeodaria populations adjacent to the Oxygen Minimum Zone. We then use 26Generalized Additive Models to analyze the response of each rhizarian category to a suite of 27 environmental variables. The models explain between 13 and 93% of the total variance observed 28 for the different groups. While temperature and the depth of the deep chlorophyll maximum, 29 appear as the main factors influencing populations in the upper 200 m, silicic acid concentration 30 is the most important variable related to the abundance of mesopelagic phaeodarians. The relative 31 importance of biotic interactions (e.g., predation, parasitism) is still to be considered, in order to 32 fully incorporate the dynamics of test-bearing pelagic rhizarians in ecological and 33 biogeochemical models. 34 35