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We have analysed the rest‐frame far‐infrared properties of a sample of massive  ( M  ★  &gt; 10 11  M ⊙ )  galaxies at  2 ≲ z ≲ 3  in the Great Observatories Origins Deep Survey‐North (GOODS‐N) field using the Spectral and Photometric Imaging Receiver (SPIRE) instrument aboard the  Herschel Space Observatory . To conduct this analysis we take advantage of the data from the  Herschel  Multi‐tiered Extragalactic Survey (HerMES) key programme. The sample comprises 45 massive galaxies with structural parameters characterized with  HST  NICMOS‐3. We study detections at submm  Herschel  bands, together with  Spitzer  24‐μm data, as a function of the morphological type, mass and size. We find that 26/45 sources are detected at MIPS 24 μm and 15/45 (all MIPS 24‐μm detections) are detected at SPIRE 250 μm, with disc‐like galaxies more easily detected. We derive star formation rates (SFRs) and specific star formation rates (sSFRs) by fitting the spectral energy distribution of our sources, taking into account non‐detections for SPIRE and systematic effects for MIPS derived quantities. We find that the mean SFR for the spheroidal galaxies  (∼50–100 M ⊙  yr −1 )  is substantially (a factor ∼3) lower than the mean value presented by disc‐like galaxies  (∼250–300 M ⊙  yr −1 ) .

HerMES: SPIRE detection of high‐redshift massive compact galaxies in GOODS‐N field