“…11B), we assign the youngest (Bayona et al, 2006) Girón Formation (Bayona et al, 2006) Los Santos Formation Angostura del Río Lebrija Formation Girón Group Perijá Range (Gose et al, 2003) Perijá Range (Nova et al, 2012) Girón-Tibasosa Formation (Bayona et al, 2006 (Torsvik et al, 2012) Confidence interval (Kent and Irving, 2010) Unflattened paleolatitude Girón Group (7.0°N) Observed paleolatitude Girón Group (4.2°N) Perijá Range (Nova et al, 2012) Merida Andes (Castillo et al, 1991) Santa Marta Massif (Bayona et al, 2010) Bucaramanga (Bayona et al, 2006) Age (Ma) Berriasian Cumbre Fm (Cediel, 1968;Etayo-Serna and Rodriguez, 1985;Etayo-Serna, 1989) and concordant contact (Laverde and Clavijo, 1985;Osorio-Afanador, 2016) with Valanginian Rosablanca Fm (Etayo-Serna and Rodriguez, 1985;Etayo-Serna, 1989;Gomez-Cruz et al, 2015;Rojas and Sandy, 2019). possible age to the succession based on the Valanginian age for the Rosablanca Formation (Etayo-Serna and Rodriguez, 1985;Etayo-Serna, 1989;Cooper et al, 1995;Sarmiento-Rojas et al, 2006;Gómez-Cruz et al, 2015;Rojas and Sandy, 2019) and thus a Berriasian age for the Los Santos Formation (Cediel, 1968;Etayo-Serna and Rodriguez, 1985;Etayo-Serna, 1989). In doing so, the observed magnetic polarity stratigraphic record can be compared with the Geomagnetic Polarity Time Scale (GPTS) (Ogg et al, 2016) for this time interval.…”