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      \field{eprinttype}{arXiv}
      \field{journaltitle}{aj}
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      \field{title}{{The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package}}
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      \keyw{methods: data analysis,methods: miscellaneous,methods: statistical,reference systems,Astrophysics - Instrumentation and Methods for Astrophysics}
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      \field{title}{{Searching for flaring star-planet interactions in AU Mic TESS observations}}
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      \field{abstract}{Numerical simulations using a resistive MHD code are performed in order to investigate the interaction of the magnetospheres of hot Jupiters (or close-in extrasolar giant planets) with the central host stars. Because of the sub-Alfvénic nature of the stellar wind outflow at the orbital positions of these close-in exoplanets, no bow shock would form. When the orientation of the stellar coronal magnetic field is favorable to strong coupling with magnetic reconnection, the power (~1027 ergs s-1) generated could reach the level of a typical solar flare. As a particular type of star-planet atmospheric interaction, as investigated by Cuntz, Saar, &amp; Musielak, magnetospheric interaction as studied in this Letter could lead to extensive energy injection into the auroral zones of the exoplanets, producing massive atmospheric escape process as recently detected.}
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      \field{title}{On the Star-Magnetosphere Interaction of Close-in Exoplanets}
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