Comparative Measurements of Astrogeodetic Deflection of the Vertical by Latvian and Swiss Digital Zenith Cameras

Nowadays, zenith telescope-based digital zenith cameras (DZC), such as the COmpact DIgital Astrometric Camera (CODIAC) and VErtical by STArs (VESTA), are used to determine highly precise astrogeodetic deflections of the vertical (DoVs). The CODIAC and VESTA were developed by Eidgenossische Technische Hochschule (ETH) Zurich and University of Latvia, respectively, and only two CODIACs and four VESTAs were produced. The CODIAC has an established accuracy higher than 0.05 '', while the accuracy of VESTA is similar to 0.1 ''. These two DZCs, which are the most used DZCs of the last decade, were used effectively over many survey campaigns. In this study, we used both the CODIAC and VESTA to conduct simultaneous observations at the School of Management and Engineering Vaud (HEIG-VD) in Yverdon-les-Bains, Switzerland, over five nights in August 2021. Our DZC measurements with CODIAC and VESTA mark the second time that simultaneous parallel observations were made with two different DZCs. Additionally, the VESTA was never tested against another DZC through comparative simultaneous measurements. These comparative measurements between the VESTA and CODIAC allowed for VESTA precision validation and checking the agreement between the two DZCs. The results of repeated, comparative DoV observations over five nights at HEIG-VD revealed a DoV measurement precision of VESTA around 0.13-0.16 '' for 15 min long observation session and 0.10-0.13 '' for 50 min long observation session. Mean DoV differences between CODIAC and VESTA at HEIG-VD were 0.08 '' and -0.06 '' for the North-South and East-West components, respectively.

Automated summary

Nowadays, zenith telescope-based digital zenith cameras (DZC) are used to determine precise astrogeodetic deflections of the vertical (DoVs). CODIAC and VESTA, developed by ETH Zurich and University of Latvia respectively, are the most commonly used DZCs. This study conducted simultaneous observations using both CODIAC and VESTA at HEIG-VD in Yverdon-les-Bains, Switzerland, and revealed the precision and agreement between the two DZCs.