# Digital receivers for low-frequency radio telescopes UTR-2, URAN, GURT

**Authors:** V. Zakharenko, A. Konovalenko, P. Zarka, O. Ulyanov, M. Sidorchuk, S., Stepkin, V. Koliadin, N. Kalinichenko, A. Stanislavsky, V. Dorovskyy, V., Shepelev, I. Bubnov, S. Yerin, V. Melnik, A. Koval, N. Shevchuk, I., Vasylieva, K. Mylostna, A. Shevtsova, A. Skoryk, I. Kravtsov, Y. Volvach, M., Plakhov, N. Vasilenko, Y. Vasylkivskyi, D. Vavriv, V. Vinogradov, R. Kozhin,, A. Kravtsov, E. Bulakh, A. Kuzin, A. Vasilyev, V. Ryabov, A. Reznichenko, V., Bortsov, V. Lisachenko, G. Kvasov, D. Mukha, G. Litvinenko, A. Brazhenko, R., Vashchishin, O. Pylaev, V. Koshovyy, A. Lozinsky, O. Ivantyshin, H. O., Rucker, M. Panchenko, G. Fischer, A. Lecacheux, L. Denis, A. Coffre, and, J.-M. Grie{\ss}meier

arXiv: 1703.04384 · 2017-03-14

## TL;DR

This paper discusses the development and deployment of digital radio receivers for low-frequency radio telescopes, highlighting their capabilities in dynamic spectrum analysis and data recording amidst interference, leading to new astronomical discoveries.

## Contribution

Introduces advanced digital receivers for low-frequency radio telescopes that operate in interference-rich environments and enable new astronomical observations.

## Key findings

- Successful detection of numerous low-frequency radio sources
- Effective operation in high-interference conditions
- Enhanced data collection for astronomical research

## Abstract

This paper describes digital radio astronomical receivers used for decameter and meter wavelength observations. This paper describes digital radio astronomical receivers used for decameter and meter wavelength observations. Since 1998, digital receivers performing on-the-fly dynamic spectrum calculations or waveform data recording without data loss have been used at the UTR-2 radio telescope, the URAN VLBI system, and the GURT new generation radio telescope. Here we detail these receivers developed for operation in the strong interference environment that prevails in the decameter wavelength range. Data collected with these receivers allowed us to discover numerous radio astronomical objects and phenomena at low frequencies, a summary of which is also presented.

## Full text

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## Figures

15 figures with captions in the complete paper: https://tomesphere.com/paper/1703.04384/full.md

## References

45 references — full list in the complete paper: https://tomesphere.com/paper/1703.04384/full.md

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Source: https://tomesphere.com/paper/1703.04384