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With the recently discovered formula, which relates the off shell Euclidean one loop determinant to the on shell quantities such as normal and quasinormal modes in real spacetime, we work out the one loop partition function for $\mathcal{N}=1$ supergravity in AdS$_3$ from scratch.
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Cited in the paper.
H. Zhang, SL(2, R R ) symmetry and quasi-normal modes in the BTZ black hole
2011
Later among the works it cites.
T. Creutzig, Y. Hikida and P. B. Ronne, Higher spin AdS 3 supergravity and its dual CFT
2012
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2012
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