Pith Number

pith:OFNDH5NS

pith:2009:OFNDH5NSRUNVRIJT5G3SDS7RU5

not attested not anchored not stored refs pending

The M-sigma and M-L Relations in Galactic Bulges and Determinations of their Intrinsic Scatter

(10) LBT Observatory, (11) Department of Physics, (13) Institut d'Astronomie et d'Astrophysique, (2) Department of Astronomy, (3) National Optical Astronomy Observatory, (4) School of Natural Sciences, (5) Department of Physics, (6) Universitaets-Sternwarte der Ludwig-Maximilians-Universit\"at, (7) Observatories of the Carnegie Institution of Washington, (8) University of California Observatories/Lick Observatory, (9) Department of Astronomy, Alan Dressler (7), Alexei V. Filippenko (9), Astronomy, Astrophysics, Berkeley, Board of Studies in Astronomy, Christos Siopis (13) ((1) Dept. of Astronomy, Douglas O. Richstone (1), ETH Zurich, Institute for Advanced Study, Institute of Astronomy, Jason Pinkney (12), John Kormendy (2), John Magorrian (11), Karl Gebhardt (2), Kayhan Gultekin (1), Luis C. Ho (7), M. C. Aller (5), Ohio Northern University, Ralf Bender (6), Richard Green (10), Santa Cruz, Scott Tremaine (4), S. M. Faber (8), Tod R. Lauer (3), Universit\'e Libre de Bruxelles), University of Arizona, University of California, University of Durham (12) Department of Physics, University of Michigan, University of Texas

arxiv:0903.4897 v1 · 2009-03-27 · astro-ph.GA · astro-ph.CO

Open paper page JSON Open Graph Bundle Merged state What is a Pith Number?

Record completeness

1 Bitcoin timestamp

2 Internet Archive

3 Author claim open · sign in to claim

4 Citations open

5 Replications open

✓ 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.

Cited by

6 papers in Pith

FLAMINGO: The thermal history of the Universe from tSZ effect cross-correlations and its dependencies on cosmology and baryon physics

Jet-driven shocks and turbulence in radio-loud Active Galactic Nuclei observed with JWST MIRI/MRS

FLAMINGO: The thermal history of the Universe from tSZ effect cross-correlations and its dependencies on cosmology and baryon physics

Optical Variability Structure Function of Low-Luminosity AGN using ATLAS Lightcurves

Massive black holes and their galaxies

Receipt and verification

First computed	2026-05-18T04:29:15.533364Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

715a33f5b28d1b58a133e9b721cbf1a7637e59e66862cf170b974d361810512a

Aliases

arxiv: 0903.4897 · arxiv_version: 0903.4897v1 · doi: 10.48550/arxiv.0903.4897 · pith_short_12: OFNDH5NSRUNV · pith_short_16: OFNDH5NSRUNVRIJT · pith_short_8: OFNDH5NS

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/OFNDH5NSRUNVRIJT5G3SDS7RU5 \
  | 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: 715a33f5b28d1b58a133e9b721cbf1a7637e59e66862cf170b974d361810512a

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "ad5661c22e337b955e2f6e78c28fcbc9191a0e0c77c65b8c7781ae3e249f7db8",
    "cross_cats_sorted": [
      "astro-ph.CO"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.GA",
    "submitted_at": "2009-03-27T20:05:09Z",
    "title_canon_sha256": "8c8eb8098317967f86bbee9d1f5fa34fa8eb48e1e1ec9ad40d35c609a97c7277"
  },
  "schema_version": "1.0",
  "source": {
    "id": "0903.4897",
    "kind": "arxiv",
    "version": 1
  }
}