State resolved data for radiative association of H and p and for
  photodissociation of H${}_2^+$
  The matrix elements and energies needed to calculate vibrational-rotational
state resolved cross sections and rate coefficients for radiative association
of H and p and for photodissociation of H${}_2^+$ are presented for
applications to simulations of chemistry in the early Universe and to stellar
atmospheres.
