Mid-IR Luminosity Functions: Inferred Dusty Cosmic Star Formation and Black Hole Accretion Histories from the JWST SMILES

The authors are grateful to the anonymous referee for the valuable comments, which significantly improved the paper. This work is based on observations made with the NASA/E-SA/CSA JWST. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. This work utilized high-performance computing facilities operated by the Center for Informatics and Computation in Astronomy (CICA) at National Tsing Hua University, funded by the Ministry of Education of Taiwan, the National Science and Technology Council of Taiwan, and the National Tsing Hua University. T.G. acknowledges the support of the National Science and Technology Council of Taiwan through grants 113-2112-M-007-006, 113-2927-I-007-501, and 113-2123-M-001-008. T.H. acknowledges the support of the National Science and Technology Council of Taiwan through grants 113-2112-M-005-009-MY3, 113-2123-M-001-008-, and 111-2112-M-005-018-MY3 and the Ministry of Education of Taiwan through the grant 113RD109.