A high angular resolution view of the PAH emission in Seyfert galaxies using JWST/MRS data
I. García-Bernete(University of Oxford), C. Packham(The University of Texas at San Antonio), D. J. Rosario(Max Planck Society), A. Alonso‐Herrero(Instituto de Física de Cantabria), C. Ramos Almeida(Universidad de La Laguna), Á. Labiano(ETH Zurich), E. K. S. Hicks(University of Alaska Anchorage), S. García‐Burillo(Spanish National Observatory), P. F. Roche(University of Oxford), M. J. Ward(University of Leicester), L. Peralta de Arriba(Centro de Astrobiología), Thomas Shimizu(Max Planck Institute for Extraterrestrial Physics), D. Rigopoulou(University of Oxford), M. Pereira-Santaella(Instituto de Física Fundamental), Fergus R. Donnan(University of Oxford), E. Bellocchi(Universidad Complutense de Madrid), Takuma Izumi(National Institutes of Natural Sciences), S. F. Hönig(University of Southampton), Lindsay Fuller(The University of Texas at San Antonio)
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