pith. sign in
Pith Number

pith:OMULMED6

pith:2026:OMULMED6UBOUJQ4MHAPNFOJBZ6
not attested not anchored not stored refs resolved

One Merge to Rule Them All: From Galaxy Interactions to Black Hole Mergers Using Horizon-AGN

Clotilde Laigle, Ecaterina Leonova, Marta Volonteri, Pascal A. Oesch, Samaya Nissanke, Yohan Dubois

Galaxy merger rates closely track supermassive black hole merger rates across cosmic time in simulations.

arxiv:2605.12599 v1 · 2026-05-12 · astro-ph.GA

Add to your LaTeX paper
\usepackage{pith}
\pithnumber{OMULMED6UBOUJQ4MHAPNFOJBZ6}

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 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.

Claims

C1strongest claim

Our results demonstrate a close correspondence between galaxy and BH cosmic histories. This work provides a comprehensive, simulation-based framework for linking galaxy and BH merger populations.

C2weakest assumption

That the Horizon-AGN simulation accurately reproduces the physical processes of galaxy mergers and black hole dynamics, and that the optimized MCC thresholds correctly isolate physically bound pairs without large projection contamination.

C3one line summary

Horizon-AGN shows galaxy and black hole merger rates both rise with stellar mass and fall with redshift, peaking near z=2-3, establishing a direct evolutionary link from galaxy interactions to black hole coalescences.

References

88 extracted · 88 resolved · 52 Pith anchors

[1] Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe · doi:10.1093/mnras/stu1536
[2] M., & Spurzem, R 2004 · doi:10.1111/j.1365-2966.2004.07883.x
[3] Building Merger Trees from Cosmological N-body Simulations · doi:10.1051/0004-6361/200911787
[4] Laser Interferometer Space Antenna · doi:10.48550/arxiv.1702.00786
[5] 9Ã uVBʧX˛=ұ K Td GjZoUU Ԫ[E>-uhc 7ch HεVS :SQ0<( ? 6v · doi:10.1093/mnras/183.3.341

Formal links

2 machine-checked theorem links

Receipt and verification
First computed 2026-05-18T03:10:01.013829Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

7328b6107ea05d44c38c381ed2b921cfa334398c1d3e6f603eeb525abe61c9fe

Aliases

arxiv: 2605.12599 · arxiv_version: 2605.12599v1 · doi: 10.48550/arxiv.2605.12599 · pith_short_12: OMULMED6UBOU · pith_short_16: OMULMED6UBOUJQ4M · pith_short_8: OMULMED6
Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/OMULMED6UBOUJQ4MHAPNFOJBZ6 \
  | 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: 7328b6107ea05d44c38c381ed2b921cfa334398c1d3e6f603eeb525abe61c9fe
Canonical record JSON
{
  "metadata": {
    "abstract_canon_sha256": "18ab02c4db5acc81a4db071b492b889019e424800e2d4d7dedc20e3eab246700",
    "cross_cats_sorted": [],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "astro-ph.GA",
    "submitted_at": "2026-05-12T18:00:03Z",
    "title_canon_sha256": "c3c6d3d4c66e01c47352462f14d0a14a47f0c0e734fc961694a524dd58068b01"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2605.12599",
    "kind": "arxiv",
    "version": 1
  }
}