Notes. Only three sources are listed as example here, the complete catalogue is available at the CDS. For each of the three clouds, two tables are provided: one for the catalogue of the dense cores and one for the catalogue of YSOs/protostars. Catalogue entries are as follows: (1): source running number; (2): source name = HGBS_J prefix followed by a tag created from the J2000 sexagesimal coordinates; (3) and (4): right ascension and declination of source centre; (5), (15), (25), (35), and (45): detection significance from monochromatic single scales, in the 70, 160, 250, 350, and 500 μm maps, respectively (NB: the detection significance has the special value of 0.0 when the source is not visible in clean single scales); (6) ± (7), (16) ± (17), (26) ± (27), (36) ± (37), (46) ± (47): peak flux density and its error in Jy beam⁻¹ as estimated by getsources; (8), (18), (28), (38), (48): contrast over the local background, defined as the ratio of the background-subtracted peak intensity to the local background intensity; (9), (19), (29), (39): peak flux density measured after smoothing to a 36.3′′ beam; (10) ± (11), (20) ± (21), (30) ± (31), (40) ± (41), (49) ± (50): integrated flux density and its error in Jy as estimated by getsources; (12), (22), (32), (42), (51): major FWHM diameters of the source as estimated by getsources; (13), (23), (33), (43), (52): minor FWHM diameters of the source as estimated by getsources (NB: the special value of -1 means that no size measurement was possible); (14), (24), (34), (44), (53): position angle of the source major axis, measured east of north; (54): detection significance in the high-resolution column density image; (55): peak H₂ column density as estimated by getsources in the high-resolution column density image; (56): column density contrast over the local background, as estimated by getsources in the high-resolution column density image; (57): peak column density measured in a 36.3′′ beam; (58): local background H₂ column density as estimated by getsources in the high-resolution column density image; (59)–(61): major and minor FWHM diameters of the source, and position angle of the major axis, respectively, as measured in the high-resolution column density image; (62): number of Herschel bands in which the source is significant (Sig_λ > 5) and has a positive flux density, excluding the column density plane; (63): CuTEx flag: 1 if the getsources source has a counterpart detected with the CuTEx algorithm, 0 if no CuTEx counterpart exists; (64): source type: starless, prestellar, or protostellar; (65): comments, (66): closest counterpart found in SIMBAD within 6′′ from the Herschel position, (67): closest Spitzer counterpart within 6′′ from the Herschel position. When present, the Spitzer source name has the form of SSTc2d JHHMMSSs-DDMMSS; (68): closest WISE counterpart within 6′′ from the Herschel position. When present, the WISE source name has the form of JHHMMSS.ss-DDMMSS.s