diff --git a/src/engine/renderer/glsl_source/lightMapping_fp.glsl b/src/engine/renderer/glsl_source/lightMapping_fp.glsl
index 3aa2d234f5..ca9e255a09 100644
--- a/src/engine/renderer/glsl_source/lightMapping_fp.glsl
+++ b/src/engine/renderer/glsl_source/lightMapping_fp.glsl
@@ -118,32 +118,6 @@ void main()
 		// Compute light color from space lightmap.
 		vec3 lightColor = texture2D(u_LightMap, var_TexLight).rgb;
 
-		#if defined(USE_DELUXE_MAPPING)
-			/* Lightmaps generated by q3map2 don't store the raw light value, but
-			they store light premultiplied with the dot product of the light
-			direction and surface normal. The line is just an attempt to reverse
-			that and get the original light values.
-
-			The lightmap stores the light in this way because for the diffuse
-			lighting formula the outgoing light is equal to the incoming light
-			multiplied by the above dot product multiplied by the surface albedo.
-			So this premultiplication means that the diffuse lighting value can
-			be calculated with a single multiply operation.
-
-			But specular lighting and/or normal mapping formulas are more complex,
-			and so you need the true light value to get correct lighting.
-			Obviously the data is not good enough to recover the original color
-			in all cases. The lower bound was an arbitrary chose factor to
-			prevent too small divisors resulting in too bright lights.
-
-			Increasing the value should reduce these artifacts. -- gimhael
-			https://github.com/DaemonEngine/Daemon/issues/299#issuecomment-606186347
-			*/
-
-			// divide by cosine term to restore original light color
-			lightColor /= clamp(dot(normalize(var_Normal), lightDir), 0.3, 1.0);
-		#endif
-
 		color.rgb = vec3(0.0);
 	#else
 		// Compute light color from lightgrid.
@@ -153,6 +127,32 @@ void main()
 		color.rgb = ambientColor * r_AmbientScale * diffuse.rgb;
 	#endif
 
+	#if defined(USE_LIGHT_MAPPING)
+		/* Lightmaps generated by q3map2 don't store the raw light value, but
+		they store light premultiplied with the dot product of the light
+		direction and surface normal. The line is just an attempt to reverse
+		that and get the original light values.
+
+		The lightmap stores the light in this way because for the diffuse
+		lighting formula the outgoing light is equal to the incoming light
+		multiplied by the above dot product multiplied by the surface albedo.
+		So this premultiplication means that the diffuse lighting value can
+		be calculated with a single multiply operation.
+
+		But specular lighting and/or normal mapping formulas are more complex,
+		and so you need the true light value to get correct lighting.
+		Obviously the data is not good enough to recover the original color
+		in all cases. The lower bound was an arbitrary chose factor to
+		prevent too small divisors resulting in too bright lights.
+
+		Increasing the value should reduce these artifacts. -- gimhael
+		https://github.com/DaemonEngine/Daemon/issues/299#issuecomment-606186347
+		*/
+
+		// divide by cosine term to restore original light color
+		lightColor /= clamp(dot(normalize(var_Normal), lightDir), 0.3, 1.0);
+	#endif
+
 	// Blend static light.
 	computeLight(lightDir, normal, viewDir, lightColor, diffuse, material, color);