Pith Number

pith:FEY2BPYU

pith:2014:FEY2BPYUV3COEXWHVXNIPFOCSX

not attested not anchored not stored refs pending

Long way to go: how outflows from large galaxies propagate through the hot halo gas

Biman B. Nath, Kartick Chandra Sarkar, Prateek Sharma, Yuri Shchekinov

arxiv:1409.4874 v2 · 2014-09-17 · astro-ph.GA

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Record completeness

1 Bitcoin timestamp

2 Internet Archive

3 Author claim open · sign in to claim

4 Citations open

5 Replications open

Cited by

1 paper in Pith

Nested Fermi and eROSITA bubbles require very similar $\sim10^{56}$ erg collimated Galactic-center outbursts; their asymmetry indicates an eastern density gradient

Receipt and verification

First computed	2026-05-18T02:27:18.350359Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

2931a0bf14aec4e25ec7adda8795c295c84a8dbca7b92bc027eb4125584f1f19

Aliases

arxiv: 1409.4874 · arxiv_version: 1409.4874v2 · doi: 10.48550/arxiv.1409.4874

Agent API

Resolver JSON Graph JSON Events JSON Schema Signing key

Verify this Pith Number yourself

curl -sH 'Accept: application/ld+json' https://pith.science/pith/FEY2BPYUV3COEXWHVXNIPFOCSX \
  | 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: 2931a0bf14aec4e25ec7adda8795c295c84a8dbca7b92bc027eb4125584f1f19

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "b3ebd8601b34f71ea3616230cbb0ebacb6252986751509e8b8ec3b24edc5f783",
    "cross_cats_sorted": [],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.GA",
    "submitted_at": "2014-09-17T06:19:05Z",
    "title_canon_sha256": "bcbf4386411d51d11c4f83eadf73555a4a358387fd6e1a6a2bc60a9b0638be98"
  },
  "schema_version": "1.0",
  "source": {
    "id": "1409.4874",
    "kind": "arxiv",
    "version": 2
  }
}