Substellar objects in star formation regions: A deep near infrared study in the Serpens cloud
We present near infrared (J, H and Ks) observations of a 5'× 10' sample field in the Serpens Star Formation region obtained with SOFI at the NTT. These observations are sensitive enough to detect a 20 MJup brown dwarf through an extinction of AV˜ 16 and are used to build an infrared census of this field in the cluster. From photometry and mass
Klotz, A. et al.
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2004