Sep 2026· Research in Astronomy and Astrophysics· 0 citations
Abstract
Pulsar observations require backend systems capable of converting telescope signals into data products suitable for scientific analysis while supporting high time resolution, coherent dedispersion, and multiple observing modes. We present the development and performance evaluation of the Tianma Pulsar Observation Backend (TMPOB), a heterogeneous RFSoC-CPU-GPU system that supports fold, search, and baseband modes. In fold and search modes, TMPOB provides a maximum observing bandwidth of 512 MHz, with data streams processed at an aggregate payload rate of up to 32.8 Gb s
-1
. A unified control framework enables automated operation, remote management, and real-time monitoring. We evaluated TMPOB using S- and X-band observations conducted with the Tianma Radio Telescope (TMRT) between February and September 2025. In fold mode, TMPOB maintained a stable 10 s output cadence during long-duration observations, with a mean end-to-end latency of 8.638 s in short-term tests. Repeated observations conducted over a three-month campaign demonstrated reproducible short-term timing-residual performance, and an X-band observation successfully detected pulsars across the full bandwidth. Search and baseband data were further verified using standard pulsar processing software. These results demonstrate that TMPOB is a robust digital backend for broadband pulsar observations with the TMRT.
Data rates from current radio telescopes are of $\sim$O(10)PB/y and we expect a growth of an order of magnitude for future radio telescopes, e.g. SKA. Coping with these data flows requires a paradigm change in data management: building pipelines with intense I/O between their modules (offline mode) is becoming unsustai...
Valentina Cesare, G. Naldi, F. Fiori et al.· 0 citations
Current operational tests show that Py7DT can process a typical nightly survey volume within the daily time budget while producing prompt ToO products on an approximately one-hour end-to-end timescale when the target is immediately observable.
Donghwan Hyun, D. Tak, G. Paek et al.· Astronomical Telescopes + In...· 0 citations
In this contribution, we present the current status and recent advances in the Real-Time Analysis (RTA) framework being developed for the Cherenkov Telescope Array Observatory (CTAO). Rapidly variable and short-lived gamma ray phenomena, such as gamma ray bursts and flaring active galactic nuclei, require low-latency r...
P. Aubert, S. Caroff, T. Oprinsen et al.· Astronomical Telescopes + In...· 0 citations
We present a reconfigurable, real-time GPU FX correlator for the four-antenna commissioning configuration of QUEST (Qilu University Explorer Survey Telescope). Deterministic RFSoC/FPGA acquisition is paired with a software-defined Python/CuPy correlator on a commodity GPU server: a custom InfiniBand RDMA receiver deliv...
Jia-Lang Ding, Jun-Hua Gu, Guan-Hong Lin et al.· Publications of the Astronom...· 0 citations
Modern digital radio astronomy receivers produce increasingly wide-bandwidth, high bit-rate data streams that necessitate the development of flexible, scalable, and maintainable backend processing and recording systems. Historically, such backend instrumentation has been tightly coupled to telescope observing modes, li...
Ewan D. Barr, Amit Bansod, Jan Behrend et al.· 0 citations
The Multi-mode Autonomous Terminal for Compatible Hybrid-optics (MATCH), operated by Wuhan University and located at Lenghu, is a 1-m Ritchey--Chr\'etien telescope equipped with imaging and spectroscopic instruments. MATCH has been in trial operation since October 2025. In this work, we present the telescope and instru...
Sai-En Xu, Bei You, Han He et al.· 0 citations
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