Table 3: Differential reddening $(\Delta\mbox{$E(B-V)$ })$ in NGC 3960.
$\Delta Y (\hbox{$^\prime$ })$ $\Leftarrow\Delta X (\hbox{$^\prime$ })\Rightarrow$  
$\Downarrow$ +15.0 +10.0 +5.0 0.0 -5.0 -10.0 -15.0 $\overline{\Delta\mbox{$E(B-V)$ }}$
+15.0 -0.10 +0.06 +0.05 +0.16 -0.03 -0.02 +0.16 $0.04\pm0.10$
+10.0 +0.06 +0.11  0.00 +0.03 +0.14 +0.16 +0.05 $0.08\pm0.06$
+5.0 +0.03  0.00 +0.03 +0.02 -0.06 +0.08 +0.21 $0.04\pm0.08$
 0.0 +0.02 -0.02 -0.06  0.00 -0.10 +0.08 +0.18 $0.01\pm0.09$
-5.0 +0.14 +0.03 -0.03 +0.02 +0.05 +0.13 +0.05 $0.06\pm0.06$
-10.0 +0.16 +0.03 -0.06 +0.14 +0.08 +0.16 +0.03 $0.08\pm0.08$
-15.0 -0.08 +0.02 +0.21 +0.14  0.00 +0.11 +0.18 $0.08\pm0.10$

$\overline{\Delta\mbox{$E(B-V)$ }}$		 $0.03\pm0.10$ $0.03\pm0.04$ $0.02\pm0.09$ $0.07\pm0.07$ $0.01\pm0.08$ $0.10\pm0.06$ $0.12\pm0.08$  


Notes. Uncertainties in $\Delta\mbox{$E(B-V)$ }$ are of the order of $\pm0.05$. For absolute values: $\mbox{$E(B-V)$ }=0.13+\Delta\mbox{$E(B-V)$ }$.


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