{
  "annotation_id": "d0b3eab0-c952-4d74-9486-00c484604181",
  "date_created": "2026-02-17T05:53:19.282000Z",
  "date_modified": "2026-02-17T05:53:19.282000Z",
  "file_hash": "d400762999a945d1d7b058a697188f32be9012f67834ac04ee61dd0a8d68ed74",
  "private": false,
  "record": {
    "abstract": "Several papers have recently calculated the contribution to pulsar timing array overlap reduction functions (ORFs) induced by our peculiar velocity with respect to the rest frame of the stochastic gravitational-wave background. Here we show that a harmonic-space calculation confirms the most recent result. We note that, with the harmonic-space calculation, the ORFs for spin-1 GWs and the correlations with astrometry measurements are also easily obtained.",
    "arxiv_id": "2601.08915",
    "authors": [
      "Neha Anil Kumar",
      "Keisuke Inomata",
      "Marc Kamionkowski"
    ],
    "categories": [
      "astro-ph.CO",
      "gr-qc",
      "hep-ph"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "title": "Note on pulsar timing array correlation functions induced by peculiar velocities",
    "url": "https://arxiv.org/abs/2601.08915",
    "version": "v1"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "8c2d4474-ee39-4ee8-bd6a-061b9335a84e",
    "id": "arXiv Dataset",
    "type": "Model",
    "variant": "snapshot-2026-01-17",
    "version": "0.1.0"
  },
  "user_id": 1000002
}