Search for and analysis of eclipsing binaries in the LAMOST Medium-Resolution Survey field. I. RA: $\textbf{23}^h$$\textbf{01}^m$$\textbf{51}^s$, Dec: +34$^\circ$36$^\prime$45$^{\prime \prime}$

Similar Items

• Photometric and Spectroscopic analysis of eight totally eclipsing contact binaries with small mass ratios
  by: Wang, Li-Heng, et al.
  Published: (2024)
• The lattices $\textbf m\times\textbf 2$ and $\textbf m\times\textbf 3$ are not Schur positive
  by: Wang, David G. L., et al.
  Published: (2025)
• Finite axiomatization of $\textbf{GL}\times\textbf{S5}$ and $\textbf{Grz}\times\textbf{S5}$
  by: Bezhanishvili, Guram, et al.
  Published: (2025)
• D-Branes in $\textbf{AdS}_3\times \textbf{S}^3 \times \textbf{S}^3 \times \textbf{S}^1$
  by: Belleri, Giorgio, et al.
  Published: (2025)
• A Photometric and Spectroscopic investigation of 11 TESS eclipsing contact binaries
  by: Guo, Yani, et al.
  Published: (2026)