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Spectral Energy Distribution and Galactic Kinematic Diagnostics for Dormant Black Hole–Neutron Star Binary Candidates

  • Authors: Qian-Yu An, Wei-Min Gu

Qian-Yu An and Wei-Min Gu 2026 The Astrophysical Journal Letters 1003 .

  • Provider: AAS Journals

Caption: Figure 2.

(a) SED example for a candidate with UV excess. (b) SED example for a candidate without UV excess. The optical-to-infrared SEDs of both sources can be well fitted by a single-star SED model. For each panel, red points show observed fluxes, open black squares show model-predicted fluxes, and the orange curve shows the best-fit spectrum.

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