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. 
James F. Babb
physics.atom-ph astro-ph.CO astro-ph.SR