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Number of items: 4.

C

CHAPLIN, W. J., SERENELLI, A. M., BASU, S., ELSWORTH, Y., NEW, R. and VERNER, G. A. (2007). Solar heavy-element abundance: Constraints from frequency separation ratios of low-degree p-modes. The Astrophysical Journal, 670 (1), 872-884. [Article]

H

HOWE, R., CHAPLIN, W. J., ELSWORTH, Y. P., HILL, F., KOMM, R., ISAAK, G. R. and NEW, R. (2003). A comparison of low-degree solar p-mode parameters from BiSON and GONG: Underlying values and temporal variations. The Astrophysical Journal, 588 (2), 1204-1212. [Article]

S

SIMONIELLO, R., CHAPLIN, W. J., ELSWORTH, Y., ISAAK, G. R. and NEW, R. (2004). Phase variation as a new tool in the investigation of the excitation and damping of solar p-modes. The Astrophysical Journal, 616 (1), 594-599. [Article]

STELLO, D., CHAPLIN, W. J., BRUNTT, H., CREEVEY, O. L., GARCIA-HERNANDEZ, A., MONTEIRO, Mjpfg, MOYA, A., QUIRION, P. O., SOUSA, S. G., SUAREZ, J. C., APPOURCHAUX, T., ARENTOFT, T., BALLOT, J., BEDDING, T. R., CHRISTENSEN-DALSGAARD, J., ELSWORTH, Y., FLETCHER, S. T., GARCIA, R. A., HOUDEK, G., JIMENEZ-REYES, S. J., KJELDSEN, H., NEW, R., REGULO, C., SALABERT, D. and TOUTAIN, T. (2009). Radius determination of solar-type stars using asteroseismology: what to expect from the Kepler mission. The Astrophysical Journal, 700 (2), 1589-1602. [Article]

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