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Table B.1

Photometry used to construct the SEDs

Filters Instrument Reference Remark
UV GALEX Bianchi et al. (2017)
V, I OGLE Shallow Survey Ulaczyk et al. (2012, 2013) LMC
V, I OGLE-IV Soszyński et al. (2019, 2017, 2020); Udalski et al. (2018)
Bp, G, Rp
U,B,V,R,I
U,B,V
U,B,V
Gaia Gaia Collaboration (2023); Ripepi et al. (2023)
Berdnikov (2008); Berdnikov et al. (2015)
Szabados (1977, 1980, 1981, 1991)
Madore (1975); Eggen (1977); Martin & Warren (1979)
VBLUW Walraven Pel (1976); Groenewegen & Lub (2023)
u, g, r, i VPHAS+ DR2 Drew et al. (2014, 2016)
u, g, r, i, z SMASH DR2 Nidever et al. (2021) SMC
g, r, i, z Pan-STARRS DR1 Chambers et al. (2016)
g, r ZTF Chen et al. (2020)
B, V,g,r,i APASS DR9 Henden et al. (2015)
i AST survey Ma et al. (2018)
U,B,V,R,I Massey et al. (2016) M31, M33
B, V, I Pellerin & Macri (2011) M33
F555W, F814W, F160W HST Riess et al. (2019, 2021)
a HST/PHAT Williams et al. (2014) M31
a HST/PHATTER Williams et al. (2021) M33
Y, J, K VMC Cioni et al. (2011); Ripepi et al. (2016, 2022)
Z, Y, J, H, K VVV DR5 Minniti et al. (2010)
Y, J, H, K VHS DR6 McMahon et al. (2013)
J, H, K
J, H, K
2MASS, 2MASS-6X Cutri et al. (2003, 2012)
Laney & Stobie (1992); Monson & Pierce (2011)
I, J, K DENIS Denis (2005)
J, K Neugent et al. (2020) M31
J, H, K Javadi et al. (2011) M33
S7, S11, L15b Akari Ita et al. (2010); Kato et al. (2012)
9, 18 μm Akari Ishihara et al. (2010)
W1, W2 CatWISE Marocco et al. (2021)
W3, W4 c AllWISE Cutri & et al. (2014)
3.6, 4.5 μm Spitzer IRAC Chown et al. (2021)
5.8, 8.5 μm Spitzer IRAC IPAC d
IRAC, MIPS 24 μm Khan et al. (2015); Khan (2017) M31, M33
IRAC, MIPS 24 μm GLIMPSE, MIPSGAL Spitzer Science (2009); Gutermuth & Heyer (2015)
24 μm MIPS IRSA e MCs
A,C,D MSX Egan et al. (2003)
12 μm IRAS PSC Beichmann (1985)
70 μm Herschel PACS Herschel PSC Working Group et al. (2020)

Notes. (a)F275W, F336W, F475W, F814W, F110W, and F160W; (b) For the S7, S11, and L15 filters only errors in the magnitudes were accepted of <0.15, <0.20, and <0.20 mag, respectively; (c)In the W3 and W4 filters only errors in the magnitudes were accepted of <0.30, and <0.25 mag, respectively; (d) VizieR catalog II/305/catalog; (e)https://irsa.ipac.caltech.edu/applications/Gator/, the "SAGE MIPS 24 um Epoch 1 and Epoch 2 Full List".

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