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   * Denevi, B. W., et al., MESSENGER global color observations: Implications for the composition and evolution of Mercury’s crust. In Lunar and Planetary Science Conference, pages 1–2, 2009.
   * Hamilton et al., Mineralogy of Martian atmospheric dust inferred from thermal infrared spectra of aerosols. Journal of Geophysical Research, 110(E12), E12006, 2005. doi: 10.1029/2005JE002501.
-  * Helbert et al., Visible and near-infrared reflectance spectra of thermally processed synthetic sulfides as a potential analog for the hollow forming materials on Mercury. Earth and Planetary Science Letters, 369-370:233–238, May 2013. ISSN 0012821X. doi: 10/gbddt9.
+  * Helbert et al., Visible and near-infrared reflectance spectra of thermally processed synthetic sulfides as a potential analog for the hollow forming materials on Mercury. Earth and Planetary Science Letters, 369-370:233–238, 2013. doi:10.1016/j.epsl.2013.03.045.
   * Kerr, R. A. Who Can Read the Martian Clock? Science, 312(5777):1132–1133, May 2006. ISSN 0036-8075, 1095-9203. doi: 10/b6v8tt.
   * McClintock, W. E. and Lankton, M. R. The mercury atmospheric and surface composition spectrometer for the MESSENGER mission. Space Science Reviews, 131(1-4):481–521, 2007. ISSN 00386308. doi: 10/btc6f6.