pith:44Z4JOLU
Hamilton's Object Revisited: A challenging source redshift of a strong lensing configuration
Re-analysis of spectra confirms Hamilton's object has redshift 0.82 rather than 3.2
arxiv:2604.19867 v1 · 2026-04-21 · astro-ph.GA · astro-ph.CO
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\pithnumber{44Z4JOLUQSM3N2NGCNB6REHLMT}
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Record completeness
Claims
The re-evaluation confirms the previous result based on 6 absorption features, z=0.820 ± 0.001 and 4 emission features, z=0.821 ± 0.002. The alternative z=3.199± 0.003, based on 6 absorption and 2 emission lines is a worse fit, also compared to other spectra.
That the chosen line identifications at z=0.82 are the correct physical assignment and that the PypeIt pipeline plus custom Python fitting routines introduce no systematic wavelength or flux errors that would alter the relative goodness-of-fit between the two redshift solutions.
Re-analysis of KCWI spectra with PypeIt confirms Hamilton's object redshift at z=0.820, showing the MOIRCS z=3.2 fit is worse and the earlier data inconclusive due to slit coverage and calibration issues.
References
Receipt and verification
| First computed | 2026-06-10T14:10:50.518145Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
e733c4b9748499b6e9a61343e890eb64ded29b897e797b20c5f7768455337ff9
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/44Z4JOLUQSM3N2NGCNB6REHLMT \
| 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: e733c4b9748499b6e9a61343e890eb64ded29b897e797b20c5f7768455337ff9
Canonical record JSON
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"license": "http://creativecommons.org/licenses/by-nc-nd/4.0/",
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