Image Details

Choose export citation format:

No Evidence for a Supermassive Black Hole Binary in GSN 069

  • Authors: Yuhe Zeng, Zhen Pan, Bin Liu, Cong Zhou

Yuhe Zeng et al 2026 The Astrophysical Journal Letters 1011 .

  • Provider: AAS Journals

Caption: Figure A1.

Corner plot of the posterior distributions inferred from the GSN 069 QPE timing data. The sampled parameters are ﹩p[{M}_{\bullet }],\,e,\,\cos {\theta }_{{\rm{\min }}},\,{q}_{r,{\rm{ini}}},\,{q}_{z,{\rm{ini}}},\,{q}_{\phi ,{\rm{ini}}},\,{T}_{{\rm{obt}}}[{\rm{\sec }}],﹩ a, ﹩{\dot{T}}_{{\rm{obt}}},\,{{ \mathcal A }}_{0}[{M}_{\bullet }],\,\omega [{M}_{\bullet }^{-1}],\,{\rm{\Delta }}{{\rm{\Phi }}}_{0},\,{\theta }_{{\rm{obs}},{\rm{eff}}},\,{\sigma }_{{\rm{sys}}}[{\rm{\sec }}]﹩. The parameters ﹩{{ \mathcal A }}_{0}﹩, ω, and ΔΦ0 characterize the SMBHB-induced time modulation.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse