Pith Number
pith:XCGTAQSY
pith:2016:XCGTAQSY2RU7RTIF4FLJK7UOAV
not attested
not anchored
not stored
refs pending
MOA-II Galactic Microlensing Constraints: The Inner Milky Way has a Low Dark Matter Fraction and a Near Maximal Disk
arxiv:1607.06462 v1 · 2016-07-21 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{XCGTAQSY2RU7RTIF4FLJK7UOAV}
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
✓
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 | 2026-05-18T01:08:38.034646Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b88d304258d469f8cd05e156957e8e05473abdce4542a15b61605dcaf1c1d493
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/XCGTAQSY2RU7RTIF4FLJK7UOAV \
| 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: b88d304258d469f8cd05e156957e8e05473abdce4542a15b61605dcaf1c1d493
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "f1470097077cc584aafec3e9e90e114687c6333b4c3aaec604ee4c86b6633a4e",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2016-07-21T20:00:05Z",
"title_canon_sha256": "c2afb30f0c8077abf3cb11a180c046a7c362be075d9ee5520c355e8cbae8d267"
},
"schema_version": "1.0",
"source": {
"id": "1607.06462",
"kind": "arxiv",
"version": 1
}
}