Notes. All the NIKA2 flux densities are derived in this work.

^(a)Flux densities computed in this work from downloaded images at http://archives.esac.esa.int/hsa/whsa/

^(b)Flux densities computed in this work from downloaded images at http://www.vla.nrao.edu/astro/nvas/

References. (1) ESA (1997); (2) Paegert et al. (2022); (3) Lasker et al. (2008); (4) Chambers & Pan-STARRS Team (2018); (5) Gaia Collaboration (2022); (6) Skrutskie et al. (2006); (7) Cutri et al. (2012); (8) Cutri et al. (2013); (9) Schlafly et al. (2019); (10) Marocco et al. (2021); (11) Spitzer Science Center (SSC) & Infrared Science Archive (IRSA) (2021); (12) Spitzer Science Center (SSC) (2009); (13) Egan et al. (2003); (14) Arneson et al. (2018); (15) Ishihara et al. (2010); (16) Helou & Walker (1988); (17) Gutermuth & Heyer (2015); (18) Molinari et al. (2016); (19) Elia et al. (2017); (20) Mizuno et al. (2010); (21) Marocco et al. (2021); (22) Higgs et al. (1994); (23) Crossley et al. (2007); (24) Leitherer et al. (1995); (25) Agliozzo et al. (2014); (26) Purcell et al. (2013); (27) Ingallinera et al. (2014); (28) Gordon et al. (2021); (29) Wang et al. (2020); (30) Helfand et al. (2006); (31) Bordiu et al. (2025); (32) Hale et al. (2021); (33) Yang et al. (2023)