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Dear Community,
I'd appreciate help on the following issue.
Im doing apperture photometry with direct local background subtraction using the code
flux_lcbkg, fluxerr_lcbkg, flag_lcbkg = sep.sum_circle(datac_c, posx, posy, R, bkgann=(R_in, R_out), subpix=0)
, with R = 6, R_in = 32., R_out = 46. (pixels)
However, when using 1-channel images (from a MUSE datacube) I get many NaNs for the estimated flux (see bottom image below).
On the contrary, when using coadded 3-channel images (ie adding three wavelength bins along the spectral dimension of thre datacube), I don´t get any NaNs.
Any suggestion why I'm getting NaNs when using the former??? Plots of both images shown below.
Txs vm in advance
Jose
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