Abstract
Observations of the Chandra Deep Field South (CDF-S) with the bolometer array SIMBA on the SEST 15m telescope is presented. SIMBA operates at 1250 μm and uses a fast-scanning observing technique suitable for large fields. An effective area of 110 sq arcmin was observed to a homogeneous noise level of 1.5 mJy.
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Wiklind, T. et al. The CDF-S Viewed with SIMBA. In: Renzini, A., Bender, R. (eds) Multiwavelength Mapping of Galaxy Formation and Evolution. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10995020_16
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DOI: https://doi.org/10.1007/10995020_16
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Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-25665-6
Online ISBN: 978-3-540-31641-1
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