Published March 10, 2026 | Version v1
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Atlas of magnetic white dwarf spectra in LAMOST DR10

Authors/Creators

  • 1. ROR icon University of Oulu
  • 2. ROR icon National Astronomical Observatories
  • 3. ROR icon University of Helsinki
  • 4. National Astronomical Observatories, Chinese Academy of Sciences

Description

In this appendix, we present the full sample of MWDs discovered in this work. For DA MWDs, the rest-frame positions of the Balmer series (Hα, Hβ, and Hγ) are indicated by red dashed vertical lines. For helium-rich (DB) MWDs, blue dotted lines indicate the rest-frame positions of prominent He I transitions. In cases where the spectrum is dominated by carbon features (DQ MWDs), no reference lines are plotted. The mean surface magnetic field (Bmean ) is provided for confirmed targets alongside the LAMOST designation.

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