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We consider two stable Interacting Dark Matter -- Dark Energy models and confront them against current Cosmic Microwave Background data from the \textit{Planck} satellite.
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G. Otalora, Scaling attractors in interacting teleparallel dark energy,
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A. Nishizawa, Measurement of Hubble constant with stellar-mass binary black holes,
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R. G. Cai, N. Tamanini and T. Yang, Reconstructing the dark sector interaction with LISA,
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