Seeing-Sorted Large Binocular Camera U-band Imaging of the Extended Groth Strip

Abstract We present the results of deep ground-based U -band imaging Extended Groth Strip (EGS) field, and creation a best resolution mosaic depth following seeing-sorted stacking method Ashcraft et al. The analysis uses 324 images taken from 2012 March to 2021 June using Large Binocular Camera. includes 16.4% with FWHM ≤ 0.″9, while 73.5% 1.″6. Each image’s zero-point was matched SDSS u , account for transparency variations. Images stellar ellipticity (1 − b / ) ≥ 0.08 were omitted. find that galaxy counts turn over at AB ∼ 25.75 mag in ∼26 mosaic. EGS field is final UVCANDELS analyzed method.