Pith Number
pith:PDQQ3GZP
pith:2011:PDQQ3GZPMXCIQ3JNTUSFMPKTJN
not attested
not anchored
not stored
refs pending
Why Supersoft X-ray Fluxes are So Weak in Early-type Galaxies? -- A Clue to Type Ia SN Progenitors --
arxiv:1110.0056 v1 · 2011-10-01 · astro-ph.SR
Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
Author claim
· sign in to
claim
4
Citations
5
Replications
✓
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 | 2026-05-18T04:11:50.826468Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
78e10d9b2f65c4886d2d9d24563d534b6171b8ac4dfc73fbd07fc31ef7f1ebc7
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/PDQQ3GZPMXCIQ3JNTUSFMPKTJN \
| 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: 78e10d9b2f65c4886d2d9d24563d534b6171b8ac4dfc73fbd07fc31ef7f1ebc7
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "80fd8c4d4978ad797474d128c652a286493de50a2981ca805daea4dd00db4bac",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2011-10-01T00:25:04Z",
"title_canon_sha256": "4808e88c3c5faf6731ad0c42b4d20c7792262bc14e81ee4c37aa0573e116db68"
},
"schema_version": "1.0",
"source": {
"id": "1110.0056",
"kind": "arxiv",
"version": 1
}
}