Spitzer/MIPS 70 μm sub-image centered on the ALMA source LB08 within B30. The white regions do not have data available. We overplotted the LABOCA contours (white), the ALMA detections (red), and the AKARI/FIS detection (magenta). The magenta circle represents the FWHM PSF of the AKARI FIS data at 65 μm (37′′ diameter). The source LB08 (red cross) is within a bright filamentary structure detected at 70 microns and extending from the northwest to the southeast. The MIPS/70 μm peak emission (green cross) is located at ~18 arcsec SW from the ALMA detection, and the green circle represents the FWHM of the PSF (18′′ diameter for MIPS).