Astrophysical Data Pipelines
Observational spectra, orbital trajectories, and pulsar frequency archives processed by the node.
Survey Mirror
Deep Sky Radio Feeds
Telemetry collected by ground-based amateur and academic radio telescopes is staged on regional mirror nodes before deep archival indexing.
| Target Field | Frequency Band | Feed Resolution |
|---|---|---|
| Cygnus A / X-1 | 1420.4 MHz (H I) | 16-bit float / 250kHz |
| Crab Pulsar (B0531) | 432 MHz | High-rate time series |
| Cassiopeia A SNR | 1.4 – 2.2 GHz | FITS spectral cubes |
Transit Topology
Regional Mirror Ingestion
To reduce cross-border link congestion during seasonal observation campaigns, telemetry frames are cached across European research mirrors before being packed into archival HDF5 tables.
| Ingress Point | Channel Type | Status |
|---|---|---|
| FRA-Node-01 (Frankfurt) | Encrypted Tunnel (Origin CA) | Online |
| AMS-Relay (Amsterdam) | Transit Link (High SLA) | Syncing |
| Survey Calibration Feed | Multiplexed Stream | Calibration |
Notice & License
Data Availability & Access Rules
Direct live data streams from the primary sensor array are reserved for registered academic observatories. Public catalog snapshots are scheduled for release under the Open Science Data Commons license in Q4 2026. For automated ingestion integrations, contact the laboratory team through designated research channels.