Pith Number
pith:DDQVZAJ2
pith:2016:DDQVZAJ2QR362M7BTLX4PKORBT
not attested
not anchored
not stored
refs pending
System mass constraints for the accreting millisecond pulsar XTE J1814-338 using Bowen fluorescence
arxiv:1612.06430 v1 · 2016-12-19 · astro-ph.HE · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{DDQVZAJ2QR362M7BTLX4PKORBT}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more · Embed verified badge
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 | 2026-05-18T00:52:37.139134Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
18e15c813a8477ed33e19aefc7a9d10cfa674a2eacb72dd5ea139e4317206cbc
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/DDQVZAJ2QR362M7BTLX4PKORBT \
| 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: 18e15c813a8477ed33e19aefc7a9d10cfa674a2eacb72dd5ea139e4317206cbc
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "e1a9a32cd8cff59e9645d926a4c8d4e05972f3a98ca7294ce2618491ec21898d",
"cross_cats_sorted": [
"astro-ph.SR"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2016-12-19T21:51:54Z",
"title_canon_sha256": "fdacff366d4fc0e999ec9d9c5dfa766a89e850f08fe37f1830082b0132f361c9"
},
"schema_version": "1.0",
"source": {
"id": "1612.06430",
"kind": "arxiv",
"version": 1
}
}