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Astron. Astrophys. 324, L5-L8 (1997)

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2. Observations

The observations presented here have been collected as part of the DENIS survey between January and May 1996 at La Silla (Chile) using the ESO 1 meter telescope equipped with the specially designed 3-channel camera (Copet, 1996). They cover an area of [FORMULA] centered at [FORMULA] (J2000) in three bands, namely I (0.8 [FORMULA]), J (1.25 [FORMULA]) and [FORMULA] (2.15 [FORMULA]). They consist of 13 strips each involving 180 images of [FORMULA] taken at constant RA along an arc of [FORMULA] in declination. The overlap between two adjacent strips reaches [FORMULA] in the Cham I cloud because of the proximity of the south pole. Wherever a star is picked up in two adjacent strips, position and flux values are averaged. Limiting magnitudes are 18, 16 and 14 at [FORMULA] in I, J and [FORMULA] bands, respectively, and position accuracy is [FORMULA] in both directions.

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© European Southern Observatory (ESO) 1997

Online publication: May 26, 1998

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