{
  "annotation_id": "7eb12ced-ddf9-44e5-b1a6-4fe7a420886b",
  "date_created": "2026-02-17T05:53:08.616000Z",
  "date_modified": "2026-02-17T05:53:08.616000Z",
  "file_hash": "869915e8b751b86e0224d7063e49f9820914ef2b0b3ce2accaeddee8b7d01fff",
  "private": false,
  "record": {
    "abstract": "We investigate the impact of gravitational wave (GW) dephasing due to gas accretion on the subtraction of massive black hole (MBH) binary signals over 4 yr of LISA data in the context of the global-fit. Based on state of the art predictions for the population of merging MBHs, we show that imperfect subtraction with vacuum waveform templates leaves a GW residual with an SNR of $3.2^{+5.4}_{-1.9}\\times \\sqrt{f_{\\rm Edd} \\langle \\dot n \\rangle/(20\\, {\\rm yr}^{-1})}$, where $f_{\\rm Edd}$ is the typical Eddington ratio and $\\langle \\dot n \\rangle$ the mean merger rate of LISA MBH binaries. We characterize the dependence of the residual on key population hyper-parameters, provide a simple fitting function and discuss detection and mitigation strategies.",
    "arxiv_id": "2601.06684",
    "authors": [
      "Lorenz Zwick"
    ],
    "categories": [
      "gr-qc",
      "astro-ph.HE"
    ],
    "license": "http://creativecommons.org/publicdomain/zero/1.0/",
    "title": "Limits of vacuum-template subtraction for LISA massive black hole binary sources in realistic environments",
    "url": "https://arxiv.org/abs/2601.06684",
    "version": "v1"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "16ff7711-a4e8-4e90-81ea-af760a100a74",
    "id": "arXiv Dataset",
    "type": "Model",
    "variant": "snapshot-2026-01-17",
    "version": "0.1.0"
  },
  "user_id": 1000002
}