On the shape of the mass-function of dense clumps in the Hi-GAL fields - I. Spectral energy distribution determination and global properties of the mass-functions

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Table 2

Number of sources selected in the two SDP fields.

Region	All	Pre-stellar	Proto-stellar

ℓ = 30°	1950	929	1021
ℓ = 59°	3402	3079	323

Notes. The original sample of sources found during the source extraction and flux estimation procedure (Sect. 3.1) has been further filtered during the SED fitting procedure (Sect. 4).

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