Pith Number
pith:MBTWHONF
pith:2017:MBTWHONFMK3GKXEV4AZPG4B7LV
not attested
not anchored
not stored
refs pending
Extreme radio flares and associated X-ray variability from young stellar objects in the Orion Nebula Cluster
arxiv:1706.05562 v1 · 2017-06-17 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{MBTWHONFMK3GKXEV4AZPG4B7LV}
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 | 2026-05-18T00:38:50.853017Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
606763b9a562b6655c95e032f3703f5d790ae4a273bc6027271f192decc7327d
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/MBTWHONFMK3GKXEV4AZPG4B7LV \
| 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: 606763b9a562b6655c95e032f3703f5d790ae4a273bc6027271f192decc7327d
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "6178453eee41e12d0ddaaf19e1b4bc258bf06fe6ced41441ca2e66d6718f26d4",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2017-06-17T16:42:13Z",
"title_canon_sha256": "684d43d4a1261b49ef37cda4091c5aa5a7870434cd53187440e6782f45b4e043"
},
"schema_version": "1.0",
"source": {
"id": "1706.05562",
"kind": "arxiv",
"version": 1
}
}