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The matrix elements and energies needed to calculate vibrational-rotationalstate resolved cross sections and rate coefficients for radiative associationof H and p and for photodissociation of H${}_2^+$ are presented forapplications to simulations of chemistry in the early Universe and to stellaratmospheres.

State resolved data for radiative association of H and p and for photodissociation of H${}_2^+$