diff --git a/CITATION.cff b/CITATION.cff
index 7f4fc95..ad16594 100644
--- a/CITATION.cff
+++ b/CITATION.cff
@@ -44,8 +44,8 @@ keywords:
   - earth sciences
   - marine sciences
 license: GPL-3.0-or-later
-version: 3.9.1
-date-released: '2024-03-04'
+version: 3.9.3
+date-released: '2024-04-24'
 references:
 - authors:
   - family-names: Zeebe
diff --git a/inst/CITATION b/inst/CITATION
index 429796e..bcb19d5 100644
--- a/inst/CITATION
+++ b/inst/CITATION
@@ -10,8 +10,8 @@ bibentry(
              ),
   ## journal = "CRAN / JOSS??",
   year = "2023",
-  abstract = "Easily calculate precession and obliquity from an astronomical solution (defaults to ZB18a from Zeebe and Lourens (2019)) and assumed or reconstructed values for tidal dissipation (Td) and dynamical ellipticity (Ed). This is a translation and adaptation of the C-code in the supplementary material to Zeebe and Lourens (2022), with further details on the methodology described in Zeebe (2022). The name of the C-routine is snvec, which refers to the key units of computation: spin vector s and orbit normal vector n.",
-  version = "3.9.2",
+  abstract = "Easily calculate precession and obliquity from an astronomical solution (defaults to ZB18a from Zeebe and Lourens (2019)) and assumed or reconstructed values for tidal dissipation (Td) and dynamical ellipticity (Ed). This is a translation and adaptation of the 'C'-code in the supplementary material to Zeebe and Lourens (2022), with further details on the methodology described in Zeebe (2022). The name of the 'C'-routine is 'snvec', which refers to the key units of computation: spin vector s and orbit normal vector n.",
+  version = "3.9.3",
   ## volume = {n/a},
   ## number = {n/a},
   ## pages = {},