pith:U5WP5GI2
Rapid-response 1.3 mm Observations of GRB 260127A with the Submillimeter Array
SMA observations indicate the 1.3 mm afterglow of GRB 260127A declined at least as fast as t^{-0.5} if the detection is associated.
arxiv:2604.14297 v2 · 2026-04-15 · astro-ph.HE · astro-ph.IM
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Claims
If the SMA detection is associated with GRB 260127A, we infer that the 1.3 mm light curve for GRB 260127A declined at least as fast as t^{-0.5}, suggesting that peak brightness of the event at this wavelength was reached in under a day.
The 6.9 mJy SMA source is physically associated with GRB 260127A despite the 2.7 arcsec offset from the optical afterglow position and the 0.9 arcsec radial uncertainty.
SMA detected a 6.9 mJy source at 1.3 mm from GRB 260127A 12.6 minutes post-trigger with a 2.7 arcsec offset from the optical position; no emission was seen 1.9 days later, implying a decline at least as steep as t to the -0.5.
Receipt and verification
| First computed | 2026-05-22T02:04:41.168689Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
a76cfe991af33b0b78580ccdcae0db360c2bb788326061f3a5b59883d968e366
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Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/U5WP5GI26M5QW6CYBTG4VYG3GY \
| 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: a76cfe991af33b0b78580ccdcae0db360c2bb788326061f3a5b59883d968e366
Canonical record JSON
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