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.
Follow a real 21-cm H I waterfall with synchronized, data-driven sound.
Beam-centre coordinates are calculated from the Az/El values entered in the H I program. The dish has no mechanical encoder feedback.
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.
Data-driven auditory interpretations of measured ARAS radio-astronomy observations.
The moving scan line follows observation time across the measured H I waterfall. The audio carrier is an artistic sound texture whose loudness is driven by the measured H I intensity in the corresponding time slice: brighter H I structure produces a stronger sound.
Bu video, 12–13 Ağustos 2026 Az 0° / El 72° sabit-bakış 21-cm H I drift gözleminin gerçek waterfall verisini kullanır. Tarama çizgisi gözlem zamanını takip eder. Sesin taşıyıcısı sanatsal bir ses dokusudur; ses yüksekliği aynı zaman dilimindeki ölçülmüş H I yoğunluğuna bağlıdır. Sarı/parlak H I yapısı güçlendikçe ses de güçlenir. Bu ses hidrojenin fiziksel sesi değildir.
The scan line follows the measured full-drift waterfall. Brighter measured H I residuals produce louder audio. The two main complexes span the Cygnus–Vulpecula sector and the Galactic anticentre / Auriga–Taurus sector.