EDP Sciences
The MUSE Hubble Ultra Deep Field Survey
Press Release
Free Access

Fig. 14

image

FSF Fitting results for all mosaic and udf-10 fields. For each field, 4 fit MOFFAT FWHMs corresponding to 4 HST filters (F606W, F775W, F814W, F850LP) are displayed, together with the linear fit. The UDF10-ALL is for the combined depth of the udf-10 field and its associated mosaic fields (1, 2 ,4 and 5).

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