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We present 2000 mock galaxy catalogs for the analysis of baryon acousticoscillations in the Emission Line Galaxy (ELG) sample of the Extended BaryonOscillation Spectroscopic Survey Data Release 16 (eBOSS DR16). Each mockcatalog has a number density of $6.7 \times 10^{-4} h^3 \rm Mpc^{-3}$, coveringa redshift range from 0.6 to 1.1. The mocks are calibrated to small-scale eBOSSELG clustering measurements at scales of around 10 $h^{-1}$Mpc. The mockcatalogs are generated using a combination of GaLAxy Mocks (GLAM) simulationsand the Quick Particle-Mesh (QPM) method. GLAM simulations are used to generatethe density field, which is then assigned dark matter halos using the QPMmethod. Halos are populated with galaxies using a halo occupation distribution(HOD). The resulting mocks match the survey geometry and selection function ofthe data, and have slightly higher number density which allows room forsystematic analysis. The large-scale clustering of mocks at the baryon acousticoscillation (BAO) scale is consistent with data and we present the correlationmatrix of the mocks.

The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogs for the Emission Line Galaxy Sample