Paper

{
  "raw_xml": "<entry>\n    <id>http://arxiv.org/abs/2603.11004v1</id>\n    <title>Searching for Magnetic White Dwarfs in LAMOST DR10</title>\n    <updated>2026-03-11T17:27:12Z</updated>\n    <link href='https://arxiv.org/abs/2603.11004v1' rel='alternate' type='text/html'/>\n    <link href='https://arxiv.org/pdf/2603.11004v1' rel='related' title='pdf' type='application/pdf'/>\n    <summary>Magnetic white dwarfs (MWDs) are key to understanding the origin and evolution of magnetic fields in compact stars. While large spectroscopic surveys such as SDSS have greatly expanded the known sample, the potential of LAMOST has not yet been fully explored. Our aim is to identify and characterize isolated MWDs in the LAMOST DR10 database. We cross-matched LAMOST DR10 spectra with white dwarf candidates from Gaia EDR3 and with recent SDSS-based catalogs of MWDs. Zeeman splitting in Balmer and helium absorption lines was used as the primary diagnostic to identify magnetic fields and to estimate their strengths. Reference objects from SDSS catalogs were used to test the detectability of MWDs in LAMOST low-resolution spectra. We identified 63 isolated MWDs in LAMOST DR10, of which 32 are new discoveries. Surface magnetic field strengths were measured from Zeeman splitting, covering a range from a few MG up to several tens of MG. For previously known SDSS MWDs, our LAMOST-based field measurements show mostly agreement with published values. This work demonstrates the capability of LAMOST low-resolution spectroscopy to identify and characterize isolated MWDs. The newly discovered objects expand the known population and provide valuable targets for future high-resolution spectroscopic and polarimetric follow-up studies. Our results highlight the potential of combining LAMOST with Gaia and other large surveys to build a more complete census of MWDs.</summary>\n    <category scheme='http://arxiv.org/schemas/atom' term='astro-ph.SR'/>\n    <category scheme='http://arxiv.org/schemas/atom' term='astro-ph.GA'/>\n    <published>2026-03-11T17:27:12Z</published>\n    <arxiv:comment>Accepted for publication in A&amp;A on March 8, 2026. 5 pages + 12 pages in Appendices</arxiv:comment>\n    <arxiv:primary_category term='astro-ph.SR'/>\n    <author>\n      <name>Si-Cheng Yu</name>\n    </author>\n    <author>\n      <name>Juan-Juan Ren</name>\n    </author>\n    <author>\n      <name>Vitaly V. Neustroev</name>\n    </author>\n    <author>\n      <name>Thomas Hackman</name>\n    </author>\n    <author>\n      <name>Hao-Tong Zhang</name>\n    </author>\n    <author>\n      <name>Yi-Qiao Dong</name>\n    </author>\n    <author>\n      <name>Zhong-Rui Bai</name>\n    </author>\n    <author>\n      <name>Hai-Long Yuan</name>\n    </author>\n    <author>\n      <name>Mengxin Wang</name>\n    </author>\n    <author>\n      <name>Ming Zhou</name>\n    </author>\n  </entry>"
}