Tracing the formation and migration history: molecular signatures in the atmosphere of misaligned hot Jupiter WASP-94 A b using JWST NIRSpec/G395H

Acknowledgements: This work is based on observations made with the NASA/ESA/CSA JWST. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with program #3154. E-MA is grateful to L. Welbanks for providing details about the Na/H calculations following Welbanks et al. (2019) and P. Mollière for prt support. JK acknowledges financial support from Imperial College London through an Imperial College Research Fellowship grant. Support for program #3154 was provided to JT by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-03127. CHM gratefully acknowledges the Leverhulme Centre for Life in the Universe at the University of Cambridge for support through the Joint Collaborations Research Project Grant GAG/382. RN acknowledges funding from the UK Research and Innovation (UKRI)/Engineering and Physical Sciences Research Council (EPSRC) through a Stephen Hawking Fellowship (EP/T017287/1). PJW acknowledges support from the Science and Technology Facilities Council (STFC) through consolidated grant ST/X001121/1. MZ acknowledges support from a UKRI Future Leaders Fellowship (Grant MR/T040866/1), a STFC Funding Nucleus Award (Grant ST/T000082/1), and the Leverhulme Trust through a research project grant (RPG-2020-82). VP acknowledges support from the UKRI Future Leaders Fellowship grants (MR/S035214/1 and MR/Y011759/1) and UKRI STFC through the consolidated grant ST/X001121/1. We thank the anonymous referee for their time and valuable feedback which improved the paper.