Citation ======== If you have used data from the **Kun** simulation suite, you may consider citing the `CSST Emulator paper `_: .. code-block:: bibtex @ARTICLE{2025SCPMA..6889512C, author = {{Chen}, Zhao and {Yu}, Yu and {Han}, Jiaxin and {Jing}, Yipeng}, title = "{CSST cosmological emulator I: Matter power spectrum emulation with one percent accuracy to k = 10h Mpc$^{{\ensuremath{-}}1}$}", journal = {Science China Physics, Mechanics, and Astronomy}, keywords = {simulation, large-scale structure of the Universe, cosmology, Cosmology and Nongalactic Astrophysics}, year = 2025, month = aug, volume = {68}, number = {8}, eid = {289512}, pages = {289512}, doi = {10.1007/s11433-025-2671-0}, archivePrefix = {arXiv}, eprint = {2502.11160}, primaryClass = {astro-ph.CO}, adsurl = {https://ui.adsabs.harvard.edu/abs/2025SCPMA..6889512C}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} } If you have used the particle lightcone data, you may consider citing the `Box replication effect paper `_ for the special line-of-sight directions: .. code-block:: bibtex @ARTICLE{2024MNRAS.534.1205C, author = {{Chen}, Zhao and {Yu}, Yu}, title = "{Box replication effects in weak lensing light-cone construction}", journal = {\mnras}, keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics}, year = 2024, month = oct, volume = {534}, number = {2}, pages = {1205-1216}, doi = {10.1093/mnras/stae2150}, archivePrefix = {arXiv}, eprint = {2312.05117}, primaryClass = {astro-ph.CO}, adsurl = {https://ui.adsabs.harvard.edu/abs/2024MNRAS.534.1205C}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} }