Notes. Fluxes are in Jy. IRAS fluxes at 12, 25, 60 and 100 μm are from SIMBAD (http://simbad.u-strasbg.fr/simbad/) by default, and from the IRAS Faint Source Reject Catalog (IPAC 1992) for AS 442, IRAS Faint Source Catalog,  | b |  > 10, Version 2.0 for BH Cep and BO Cep, and from Casey & Harper (1990) for VY Mon. AKARI fluxes at 9, 18, 65, 90, 140 and 160 μm are from AKARI/IRC All-Sky Survey Point Source Catalogue (Version 1.0) and AKARI/FIS All-Sky Survey Bright Source Catalogue (Version 1.0). Additional references are given in Col. 12 for photometry in the following wavelengths: (1): 10.7 μm from Monnier et al. (2009); (2): 10.5(N) and 20.1(Q) μm from Hillenbrand et al. (1992); (3): Spitzer IRAC 5.8 μm from the GLIMPSE catalogue; (4): Spitzer IRAC 3.6, 4.5, 5.8 and 8.0 μm from the “Spitzer survey of young stellar clusters” (Gutermuth et al. 2009); (5): 10.5(N) and 20.1(Q) μm from Herbst et al. (1982); (6): ISO photometry at 6.9, 9.6, 17, and 28.2 μm from Thi et al. (2001); (7): Spitzer IRAC 5.8, 8.0 and MIPs 24 μm from Hernández et al. (2006); (8, 9): Spitzer IRAC 3.6, 4.5, 5.8, 8.0 and MIPs 24, 70 μm from the “Spitzer survey of Serpens YSO population” (Harvey et al. 2007) and from Robitaille et al. (2007), respectively. Photometry extracted from ISO data is available in Merín (2004) for the stars indicated in Col. 2. The typical uncertainty is  ≲ 10% for IRAS and  ≲ 5% for AKARI data.