Pith Number
pith:4Y57ITID
pith:2018:4Y57ITIDVARACOBTSAK2DGN5IP
not attested
not anchored
not stored
refs pending
Nonthermal afterglow of the binary neutron star merger GW170817: a more natural modeling of electron energy distribution leads to a qualitatively different new solution
arxiv:1810.02587 v2 · 2018-10-05 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{4Y57ITIDVARACOBTSAK2DGN5IP}
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Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
Author claim
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claim
4
Citations
5
Replications
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Portable graph bundle live · download bundle · merged
state
The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same
current state with the deterministic merge algorithm.
Receipt and verification
| First computed | 2026-05-17T23:53:57.427407Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
e63bf44d03a8220138339015a199bd43cb791e7c1d6eac675eb35a3046140a9f
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/4Y57ITIDVARACOBTSAK2DGN5IP \
| 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: e63bf44d03a8220138339015a199bd43cb791e7c1d6eac675eb35a3046140a9f
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "8041e89f25bc0c30300cad3b7946003418ba9a2e19060b3b1e15008a0070cba0",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2018-10-05T09:47:01Z",
"title_canon_sha256": "405c680d665796f341d8b2a2c48b29cc248e242a73d8fb7744a1fceee8ae9afc"
},
"schema_version": "1.0",
"source": {
"id": "1810.02587",
"kind": "arxiv",
"version": 2
}
}