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Pith Number

pith:KOXLGCBV

pith:2026:KOXLGCBVTDIXT7L3WC6EGSYEY3
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Rapid and robust simulation-based inference for kilonovae

Daniel Mortlock, Gurjeet Jagwani, Hiranya V. Peiris, Mattia Bulla, Nikhil Sarin, Samaya Nissanke, Stephanie M. Brown, Stephan Rosswog, Stephen Thorp

Simulation-based inference recovers kilonova parameters rapidly from light curves without the biases that affect MCMC fits to emulator outputs.

arxiv:2605.13983 v1 · 2026-05-13 · astro-ph.IM · astro-ph.HE · hep-ph

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\usepackage{pith}
\pithnumber{KOXLGCBVTDIXT7L3WC6EGSYEY3}

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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
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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

SBI provides a rapid alternative to MCMC for inference with emulators or approximate likelihoods that is robust to emulator uncertainty and likelihood misspecification.

C2weakest assumption

The Gaussian process emulator trained on the ~1300 POSSIS simulations fully captures the non-Gaussian, correlated structure of the predictive uncertainty, and the simulations themselves are sufficiently representative of real kilonova physics.

C3one line summary

Simulation-based inference with a Gaussian process emulator trained on ~1300 POSSIS simulations enables rapid, robust kilonova parameter estimation that avoids MCMC biases from likelihood misspecification.

References

184 extracted · 184 resolved · 26 Pith anchors

[1] Setzer , isbn =
[2] B. P. Abbott and R. Abbott and T. D. Abbott and F. Acernese and K. Ackley and C. Adams and T. Adams and P. Addesso and R. X. Adhikari and V. B. Adya and others , doi =. GW170817: Observation of Gravit
[3] B. P. Abbott and R. Abbott and T. D. Abbott and F. Acernese and K. Ackley and C. Adams and T. Adams and P. Addesso and R. X. Adhikari and V. B. Adya and others , doi =. Gravitational Waves and Gamma-R
[4] B. P. Abbott and R. Abbott and T. D. Abbott and F. Acernese and K. Ackley and C. Adams and T. Adams and P. Addesso and R. X. Adhikari and V. B. Adya and others , doi =. Multi-messenger Observations of
[5] B. P. Abbott and R. Abbott and T. D. Abbott and F. Acernese and K. Ackley and C. Adams and T. Adams and P. Addesso and R. X. Adhikari and V. B. Adya and others , doi =. A gravitational-wave standard s

Formal links

2 machine-checked theorem links

Receipt and verification
First computed 2026-05-17T23:39:13.355377Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

53aeb3083598d179fd7bb0bc434b04c6e646c5ffac1ff9b8ec913ed16d0fef40

Aliases

arxiv: 2605.13983 · arxiv_version: 2605.13983v1 · doi: 10.48550/arxiv.2605.13983 · pith_short_12: KOXLGCBVTDIX · pith_short_16: KOXLGCBVTDIXT7L3 · pith_short_8: KOXLGCBV
Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/KOXLGCBVTDIXT7L3WC6EGSYEY3 \
  | 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: 53aeb3083598d179fd7bb0bc434b04c6e646c5ffac1ff9b8ec913ed16d0fef40
Canonical record JSON
{
  "metadata": {
    "abstract_canon_sha256": "1b6a8fb660802ea3d5ed6baacf8992c5b4829306fc2df5cd5c917289536c51bf",
    "cross_cats_sorted": [
      "astro-ph.HE",
      "hep-ph"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.IM",
    "submitted_at": "2026-05-13T18:01:32Z",
    "title_canon_sha256": "8ee3665e8c1de7c900de362e45886344bc6e9a2632a4548efb2bfa6507adcfdd"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2605.13983",
    "kind": "arxiv",
    "version": 1
  }
}