pith:EYGFAWTL
Systematic Spectral Distortion from Digital Whitening in Radio Telescopes and Implications for 21 cm Cosmology
Digital whitening of radio signals followed by re-quantization introduces systematic spectral distortions at levels problematic for 21 cm cosmology.
arxiv:2605.05489 v2 · 2026-05-06 · astro-ph.IM · astro-ph.CO
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\pithnumber{EYGFAWTLZJWNUM5EQL6VNKPQTY}
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Record completeness
Claims
Although the effect can be small so that it has heretofore been unrecognized, we demonstrate that it produces distortion of the spectrum at a level that is problematic for some science, in particular 21 cm cosmology.
That the observed distortion in OVRO-LWA data and the semi-analytic simulations arise specifically and solely from the whitening-plus-re-quantization sequence rather than from other unmodeled instrumental or environmental effects.
Digital spectrum whitening followed by re-quantization introduces a previously unrecognized systematic distortion in the gain-versus-frequency response of radio telescopes, reaching levels problematic for 21 cm cosmology.
Receipt and verification
| First computed | 2026-06-23T02:13:24.736672Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
260c505a6bca6cda33a482fd56a9f09e29fde115653399af517c2787b2656d85
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/EYGFAWTLZJWNUM5EQL6VNKPQTY \
| jq -c '.canonical_record' \
| python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: 260c505a6bca6cda33a482fd56a9f09e29fde115653399af517c2787b2656d85
Canonical record JSON
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"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
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"submitted_at": "2026-05-06T22:24:31Z",
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