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mips 24 mu m observations of the hubble deep field south: probing the ir radio correlation of galaxies at z > 1

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Academic year: 2020

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Figure 1. Left: the MIPS 24 μm image of the HDF-S region. The green chevron figure marks the area covered by the original HST WFPC2 deep field, the squares to the east and south are the HST STIS and NICMOS deep fields, respectively
Figure 2. Left: completeness as a function of input flux density, as derived from the Monte Carlo simulations
Figure 4. Euclidean normalized differential 24 μm source counts in the HDF-S (black squares)
Figure 5. Left: histogram of the total offsets between the MUSYC optical candidate and the 24 μm source
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