Notes. Catalog entries are as follows: (1) core running number; (2) core name = HGBS_J prefix directly followed by a tag created from the J2000 sexagesimal coordinates; (3) and (4): right ascension and declination of core center; (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 core is not visible in clean single scales); (6) ± (7), (16) ± (17) (26) ± (27) (36) ± (37) (46) ± (47): peak flux density and its errorin 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 (/S_bg); (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)–(13), (22)–(23), (32)–(33), (42)–(43), (51)–(52): major and minor FWHM diameters of the core (in arcsec), respectively, 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 core major axis, measured east of north, in degrees; (54) detection significance in the high-resolution column density image; (55) peak H₂ column density in units of 10²¹ cm⁻² 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)–(60)–(61): major and minor FWHM diameters of the core, 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 core is significant (Sig_λ > 5) and has a positive flux density, excluding the column density plane; (63) core type: 1-starless, 2-prestellar, 3-protostellar, or 0-tentative core. The latter is a likely extragalactic source; (64) 1 if a Spitzer-identified YSO (Megeath et al. 2012) is found within 6′′ of the Herschel peak position, 0 otherwise (see text for details); (65) SIMBAD counterparts, if any, up to 6′′ from the Herschel peak position; (66) comments: “N region”.