Acquire
Timestamped HDF5 spectra remain the primary observational source.
A public archive of real measured data: neutral-hydrogen spectra, repeat observations, calibration history, waterfalls, animations, reports and ongoing experiments.
ARAS keeps reproducible Galactic H I observations, experimental datasets and ongoing extragalactic searches visibly distinct. Calibration faults, null results and revised analyses remain part of the record rather than being hidden.
Timestamped HDF5 spectra remain the primary observational source.
Warm-up intervals, hardware failures, RFI and bad channels are explicitly marked or excluded.
ON/OFF work is performed in linear power with pre/post or time-dependent reference regions.
Spectra are placed on a common LSRK velocity frame before scientific comparison or stacking.
Independent nights, jackknifes, broad-line tests and null-transit controls are used before stronger claims.
Spectra, waterfalls, reports, animations and limitations are kept together for inspection.
Fixed-pointing drift scans and repeated target crossings.
Externally powered 1420 MHz LNA/filter front end.
Timestamped spectral acquisition into the ARAS workflow.
Approx. 40.988° N, 29.028° E.
Independent recordings support the same astronomical structure or profile.
A real observational dataset or experiment exists, but the label does not automatically imply a source-detection claim.
A target is still being stacked, repeated or challenged with null/control tests.