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The frequency resolution is chosen such that the frequency bin size is less than (2/3) × T coh, where T coh is the coherent integration time. In case of a 5 ms integration time, the frequency bin size should be less than or equal to 133.33 Hz. The efficiency of the orbit solutions is evaluated as a ratio between the number of successful SLR solutions to the number of determined orbit solutions using microwave observations at CODE for the same period. Cheng M, Ries J (2017) The unexpected signal in GRACE estimates of C20. J Geod 97(8):897–914. https://doi.org/10.1007/s00190-016-0995-5 Huang G, Yan X, Zhang Q (2018b) Estimation of antenna phase center offset for BDS IGSO and MEO satellites. In: Proceedings of IGS Workshop 2018, Oct 28–Nov 2, Wuhan, China

Seepersad, G. Reduction of Initial Convergence Period in GPS PPP Data Processing. Ph.D. Thesis, York University, Toronto, ON, Canada, 2012. [ Google Scholar]Klus, R.; Talvitie, J.; Valkama, M. Neural network fingerprinting and GNSS data fusion for improved localization in 5G. In Proceedings of the 2021 International Conference on Localization and GNSS (ICL-GNSS), Tampere, Finland, 1–3 June 2021; pp. 1–6. [ Google Scholar] How many SLR observations are necessary to determine precise multi-GNSS orbits using SLR data only? Kouba, J. Notes on December 2017 Version of the ECLIPS Subroutine. Available online: http://acc.igs.org/orbits/eclips_Dec_2017.tar (accessed on 10 November 2020).

The frequency resolution is chosen such that the frequency bin size is less than (2/3) × T coh, where T coh is the coherent integration time. In case of a 4 ms integration time, the frequency bin size should be less than or equal to 166.67 Hz. Xia L, Lin B, Liu Y, Xiong S, Bai T (2018) Satellite geometry and attitude mode of BDS-3 MEO satellites developed by SECM. In: Proceedings of ION GNSS 2018, Institute of Navigation, Miami, Florida, USA, Sep 24–28, pp 1268–1289 Duan B, Hugentobler U, Selmke I (2018) The adjusted optical properties for Galileo/BeiDou-2/QZS-1 satellites and initial results on BeiDou-3e and QZS-2 satellites. Adv Space Res 63(5):1803–1812. https://doi.org/10.1016/j.asr.2018.11.007Shang, P.; Wang, X.; Zou, D.; Chu, Z.; Guo, Y. Acquisition performance of B1I abounding with 5G signals. J. Syst. Eng. Electron. 2022, 33, 563–574. [ Google Scholar] [ CrossRef] Alghisi, M.; Biagi, L. Positioning with GNSS and 5G: Analysis of Geometric Accuracy in Urban Scenarios. Sensors 2023, 23, 2181. [ Google Scholar] [ CrossRef] [ PubMed] Wübbena G, Schmitz M, Boettcher G, Schumann C (2006) Absolute GNSS antenna calibration with a robot: repeatability of phase variations, calibration of GLONASS and determination of carrier-to-noise pattern. In: Proceedings of the IGS workshop 2006 perspectives and visions for 2010 and beyond, May 8–12, Darmstadt, Germany Shamaei, K.; Kassas, Z.M. Receiver design and time of arrival estimation for opportunistic localization with 5G signals. IEEE Trans. Wirel. Commun. 2021, 20, 4716–4731. [ Google Scholar] [ CrossRef] Drewes H, Kuglitsch F, Adám J, Szabolcs R (2016) The geodesist’s handbook 2016. J Geod 90(10):907–1205. https://doi.org/10.1007/s00190-016-0948-z

The skill description is somewhat misleading. The Press skill has the same functionality as the Hold skill (including the shield and energy storing), but only during a very brief window. Destino, G.; Saloranta, J.; Seco-Granados, G.; Wymeersch, H. Performance analysis of hybrid 5G-GNSS localization. In Proceedings of the 2018 52nd Asilomar Conference on Signals,Systems, and Computers, Pacific Grove, CA, USA, 28–31 October 2018; pp. 8–12. [ Google Scholar] Wang, C.; Guo, J.; Zhao, Q.; Liu, J. Empirically derivedmodel of solar radiation pressure for BeiDou GEO satellites. J. Geod. 2018, 93, 791–807. [ Google Scholar] [ CrossRef] Jin, C.; Tay, W.P.; Zhao, K.; Ling, K.V.; Sin, K.K. A 5G/GNSS Integrated Positioning Method. In Proceedings of the 35th International Technical Meeting of the Satellite Division of The Institute of Navigation (ION GNSS+ 2022), Denver, CO, USA, 19–23 September 2022; pp. 2429–2443. [ Google Scholar] Springer T, Beutler G, Rothacher M (1999) A new solar radiation pressure model for GPS satellites. GPS Solut 3(2):50–62. https://doi.org/10.1007/PL00012757

Constellation Level 5, Crimson Tidewalker: Increases this talent's level by 3, up to a maximum of 15. Cai, C.; Gao, Y.; Pan, L.; Zhu, J. Precise point positioning with quad-constellations: GPS, BeiDou, GLONASS and Galileo. Adv. Space Res. 2015, 56, 133–143. [ Google Scholar] [ CrossRef]