{
  "abstract": "In this work, we present a systematic X-ray study of 85 TeV-detected blazars based on archival \\emph{Swift}-XRT and \\emph{NuSTAR} observations available up to May 2024. We derive unabsorbed X-ray fluxes and photon indices through spectral fitting, and investigate their light curves, spectral energy distributions, flux distributions, power spectral densities, and flux-index correlations. Using the fractional variability method, we identify 78 sources as variable in the soft X-ray band and 14 sources as variable in the hard X-ray band. For well-sampled soft X-ray light curves, the flux distributions are generally better described by log-normal functions, while the PSD slopes span $β_{\\rm PSD}=0.1$--$1.6$, with most values between 1.0 and 1.6, where the PSD is defined as $P(f)\\propto f^{-β_{\\rm PSD}}$. We find positive correlations between TeV and X-ray luminosities, supporting a leptonic emission scenario. We also find a correlation between X-ray and disk luminosities, whereas no significant correlation is found between X-ray luminosity and black hole mass.",
  "abstract_shown": true,
  "affiliations": [],
  "article_type": null,
  "arxiv": "2610.37114",
  "author_total": 10,
  "authors": [
    {
      "name": "Zhihao Ouyang"
    },
    {
      "name": "Hubing Xiao"
    },
    {
      "name": "Shangchun Xie"
    },
    {
      "name": "Jingyu Wu"
    },
    {
      "name": "Xuhong Ye"
    },
    {
      "name": "Junhang Liu"
    },
    {
      "name": "Lili Yang"
    },
    {
      "name": "Marina Manganaro"
    },
    {
      "name": "Jianzhen Chen"
    },
    {
      "name": "Junhui Fan"
    }
  ],
  "bibtex": "https://research.draconitic.com/paper/26wj6vxsbt58t.bib",
  "cited_by": 0,
  "doi": "10.48550/arxiv.2610.37114",
  "fulltext_url": null,
  "id": "26wj6vxsbt58t",
  "issns": [],
  "landing_url": "https://arxiv.org/abs/2610.37114",
  "language": null,
  "licence": "CC-BY-4.0",
  "licence_label": "CC BY 4.0",
  "licence_source": "article",
  "licence_url": "http://creativecommons.org/licenses/by/4.0/",
  "metadata_licence": "CC0-1.0",
  "native_subjects": [
    [
      "arxiv",
      "astro-ph.GA"
    ],
    [
      "arxiv",
      "astro-ph.HE"
    ],
    [
      "openalex",
      "3106|Astrophysics and Cosmic Phenomena"
    ]
  ],
  "openalex": "W7224107631",
  "pdf_url": "https://arxiv.org/pdf/2610.37114",
  "pmcid": null,
  "pmid": null,
  "published": "2026-10-27",
  "publisher": null,
  "ris": "https://research.draconitic.com/paper/26wj6vxsbt58t.ris",
  "sources": [
    {
      "first_seen": "2026-10-30T12:35:50Z",
      "native_id": "2610.37114",
      "source": "arxiv",
      "url": "https://arxiv.org/abs/2610.37114"
    }
  ],
  "subjects": [
    {
      "field": "astronomy",
      "origin": "arxiv:astro-ph.GA",
      "subfield": "galaxies"
    },
    {
      "field": "astronomy",
      "origin": "arxiv:astro-ph.HE",
      "subfield": "high-energy-astrophysics"
    }
  ],
  "title": "X-ray Emission Study of TeV Blazars",
  "title_text": "X-ray Emission Study of TeV Blazars",
  "type": "preprint",
  "updated_at": "2026-10-30T12:35:50Z",
  "url": "https://research.draconitic.com/paper/26wj6vxsbt58t",
  "venue": "arXiv",
  "versions": []
}