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Table 3.

Multicolor photometry of ExtEV used by us to perform the SED fitting described in Sect. 3.

Mission/survey Passband λeff (μm) ( * ) Magnitude Reference
Swift/UVOT UVW2 0.208 14.22(3) J21
UVM2 0.225 14.24(4) J21
UVW1 0.268 13.92(4) J21
GALEX NUV 0.230 15.62(5) This work
XMM/OM UVW1 0.268 13.3248(14) Page et al. (2021)
The Magellanic Clouds U 0.355 12.63(4) Zaritsky et al. (2004)
Photometric Survey B 0.437 13.62(11) Zaritsky et al. (2004)
I 0.857 13.28(8) Zaritsky et al. (2004)
UBVR CCD Survey of U 0.355 12.830(17) Massey (2002)
The Magellanic Clouds B 0.437 13.670(14) Massey (2002)
V 0.547 13.560(10) Massey (2002)
R 0.670 13.430(22) Massey (2002)
Gaia DR3 GBP 0.504 13.504(6) Gaia Collaboration (2022)
G 0.582 13.423(3) Gaia Collaboration (2022)
GRP 0.762 13.227(7) Gaia Collaboration (2022)
APASS DR10 B 0.437 13.678(9) Henden (2019)
g 0.472 13.542(7) Henden (2019)
V 0.547 13.530(13) Henden (2019)
r 0.620 13.568(21) Henden (2019)
i 0.767 13.604(22) Henden (2019)
OGLE V 0.547 13.7720(10) Wrona et al. (2022b)
IC 0.783 13.4730(10) Wrona et al. (2022b)
2MASS J 1.235 12.992(23) Cutri et al. (2012)
H 1.662 12.847(25) Cutri et al. (2012)
Ks 2.159 12.699(24) Cutri et al. (2012)
Spitzer/IRAC Ch1 3.508 12.41(3) Bonanos et al. (2009)
Ch2 4.437 12.30(3) Bonanos et al. (2009)
Ch3 5.628 12.14(7) Bonanos et al. (2009)
Ch4 7.589 11.87(9) Bonanos et al. (2009)
AllWISE W1 3.353 12.416(24) Cutri et al. (2021)
W2 4.603 12.377(22) Cutri et al. (2021)
W3 11.561 9.90(7) Cutri et al. (2021)
W4 22.088 6.20(9) Cutri et al. (2021)

Notes. ( * )Effective wavelengths of passbands as calculated by VOSA VO SED Analyzer (Bayo et al. 2008).

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