1 INTRODUCTION  
2 METHODS  
2.1 Modeling the $L_{\mathrm{H}\alpha}–L_{\mathrm{UV}}$ joint distribution  
2.2 Relationship between the real-space zero-lag cross-correlation and the Fourier-space cross-bispectrum  
2.3 The EBL–galaxy cross-correlation: signals and errors  
3 RESULTS  
3.1 Detectability of cross-correlation signals  
3.2 Constraints on BCLF model parameters  
4 DISCUSSION  
4.1 Ambiguity associated with dust attenuation  
4.2 Limitations and implications of the presented method  
5 CONCLUSIONS