WHAT ASTEROSEISMOLOGY CAN DO FOR EXOPLANETS: KEPLER-410A b IS A SMALL NEPTUNE AROUND A BRIGHT STAR, IN AN ECCENTRIC ORBIT CONSISTENT WITH LOW OBLIQUITY by Van Eylen, V., Lund, Mikkel N., Aguirre, V. Silva, Arentoft, T., Kjeldsen, H., Albrecht, Simon H., Chaplin, William J., Isaacson, Howard, Pedersen, M. G., Jessen-Hansen, J., Tingley, B., Christensen-Dalsgaard, J., Aerts, C., Campante, T. L., Bryson, Stephen T.

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