{
  "abstract": "Star formation and associated feedback processes play a key role in galaxy evolution. Astrochemistry is a powerful tool for characterising the physical conditions of dense star-forming gas and understanding the reciprocal relation between stellar feedback and the interstellar medium (ISM): from the way feedback influences the ISM to how the ISM conditions regulate the formation of new stars. The advent of large spectral surveys of a few individual galaxy centres have demonstrated the potential of molecular gas inventories to reveal the physical conditions of star-forming gas in great detail. A next-generation (sub)mm facility in the 2040s would extend this science to the local star-forming galaxy population, providing for the first time a comprehensive view of the physical and chemical conditions of the molecular ISM in the local universe.",
  "abstract_shown": true,
  "affiliations": [],
  "article_type": null,
  "arxiv": "2610.21687",
  "author_total": 24,
  "authors": [
    {
      "name": "Mathilde Bouvier"
    },
    {
      "name": "Erica Behrens"
    },
    {
      "name": "Laura Colzi"
    },
    {
      "name": "Ana Duarte-Cabral"
    },
    {
      "name": "Minou Greve"
    },
    {
      "name": "Jeff Mangum"
    },
    {
      "name": "Sébastien Muller"
    },
    {
      "name": "Miguel Querejeta"
    },
    {
      "name": "Víctor M. Rivilla"
    },
    {
      "name": "Francesco Salvestrini"
    },
    {
      "name": "Thomas G. Williams"
    },
    {
      "name": "Cecilia Bacchini"
    },
    {
      "name": "Viviana Casasola"
    },
    {
      "name": "Timothy A. Davis"
    },
    {
      "name": "Jakob den Brok"
    },
    {
      "name": "Cosima Eibensteiner"
    },
    {
      "name": "Daniel Espada"
    },
    {
      "name": "Sergio Martín"
    },
    {
      "name": "Frédérique Motte"
    },
    {
      "name": "Rosita Paladino"
    },
    {
      "name": "Miguel Pereira-Santaella"
    },
    {
      "name": "Ilaria Ruffa"
    },
    {
      "name": "Sabine Thater"
    },
    {
      "name": "Katarzyna M. Dutkowska"
    }
  ],
  "bibtex": "https://research.draconitic.com/paper/5r7a591t0r9gz.bib",
  "cited_by": 0,
  "doi": "10.48550/arxiv.2610.21687",
  "fulltext_url": null,
  "id": "5r7a591t0r9gz",
  "issns": [],
  "landing_url": "https://arxiv.org/abs/2610.21687",
  "language": null,
  "licence": "LicenseRef-arXiv-nonexclusive-1.0",
  "licence_label": "arXiv licence",
  "licence_source": "article",
  "licence_url": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
  "metadata_licence": "CC0-1.0",
  "native_subjects": [
    [
      "arxiv",
      "astro-ph.GA"
    ],
    [
      "arxiv",
      "astro-ph.IM"
    ],
    [
      "openalex",
      "3103|Astrophysics and Star Formation Studies"
    ]
  ],
  "openalex": "W7222642334",
  "pdf_url": "https://arxiv.org/pdf/2610.21687",
  "pmcid": null,
  "pmid": null,
  "published": "2026-10-15",
  "publisher": null,
  "ris": "https://research.draconitic.com/paper/5r7a591t0r9gz.ris",
  "sources": [
    {
      "first_seen": "2026-10-30T12:29:50Z",
      "native_id": "2610.21687",
      "source": "arxiv",
      "url": "https://arxiv.org/abs/2610.21687"
    }
  ],
  "subjects": [
    {
      "field": "astronomy",
      "origin": "arxiv:astro-ph.GA",
      "subfield": "galaxies"
    },
    {
      "field": "astronomy",
      "origin": "arxiv:astro-ph.IM",
      "subfield": "instrumentation-methods"
    }
  ],
  "title": "Molecular atlas of nearby galaxies through sensitive high-resolution multi-band molecular line surveys",
  "title_text": "Molecular atlas of nearby galaxies through sensitive high-resolution multi-band molecular line surveys",
  "type": "preprint",
  "updated_at": "2026-10-30T12:29:50Z",
  "url": "https://research.draconitic.com/paper/5r7a591t0r9gz",
  "venue": "arXiv",
  "versions": []
}