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Table 2.
Wavelength coverage for KINGFISH SEDs.
Filter | Wavelength | Number |
---|---|---|
(μm) | galaxiesa | |
GALEX_FUV | 0.152 | 57 |
GALEX_NUV | 0.227 | 58 |
SDSS_u | 0.354 | 40 |
B_Bessel | 0.440 | 61 |
SDSS_g | 0.477 | 40 |
V_Bessel | 0.550 | 59 |
SDSS_r | 0.623 | 40 |
R_Cousins | 0.640 | 56 |
SDSS_i | 0.762 | 40 |
I_Cousins | 0.790 | 56 |
SDSS_z | 0.913 | 40 |
2MASS_J | 1.235 | 61 |
2MASS_H | 1.662 | 61 |
2MASS_Ks | 2.159 | 61 |
WISE_W1 | 3.353 | 59 |
IRAC_CH1 | 3.550 | 61 |
IRAC_CH2 | 4.490 | 61 |
WISE_W2 | 4.603 | 57 |
IRAC_CH3 | 5.730 | 61 |
IRAC_CH4 | 7.870 | 61 |
WISE_W3 | 11.561 | 61 |
WISE_W4b | 22.088 | 54 |
MIPS_24 | 23.70 | 61 |
PACS_70 | 71.11 | 61 |
MIPS_70 | 71.42 | 61 |
PACS_100 | 101.20 | 61 |
MIPS_160 | 155.90 | 61 |
PACS_160 | 162.70 | 61 |
SPIRE_250 | 249.40 | 61 |
SPIRE_350 | 349.90 | 61 |
SPIRE_500 | 503.70 | 61 |
SCUBA_850 | 850.0 | 21 |
Notes.
(b)
Shifting this effective wavelength to the modified value given by Brown et al. (2014a) would bring the WISE W4 and MIPS 24 μm fluxes into closer agreement.
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