Table 1.
Host galaxy photometry used for SED fitting.
| Filter | Source | m | err | λeff [Å] | A(λ) |
|---|---|---|---|---|---|
| FUV | GALEX | 20.93 | 0.31 | 1548.85 | 0.20 |
| NUV | GALEX | 20.74 | 0.25 | 2303.37 | 0.22 |
| F225W | HST | 20.60 | 0.07 | 2358.70 | 0.20 |
| F336W | HST | 20.40 | 0.03 | 3359.11 | 0.13 |
| g | PS | 19.70 | 0.01 | 4810.00 | 0.09 |
| F555W | HST | 19.34 | 0.01 | 5235.33 | 0.08 |
| r | PS | 19.17 | 0.01 | 6170.00 | 0.07 |
| i | PS | 18.93 | 0.01 | 7520.00 | 0.05 |
| F763M | HST | 18.93 | 0.01 | 7602.85 | 0.05 |
| F814W | HST | 18.84 | 0.01 | 7954.84 | 0.04 |
| F845M | HST | 18.68 | 0.02 | 8430.20 | 0.04 |
| W1 | WISE | 18.91 | 0.07 | 33 526.00 | 0.00 |
| W2 | WISE | 18.82 | 0.13 | 46 028.00 | 0.00 |
| W3 | WISE | 16.92 | 0.38 | 115 608.00 | 0.00 |
Notes. All magnitudes are in the AB system, and before Galactic extinction correction. The filter effective wavelengths and Galactic extinction at that wavelength – assuming E(B − V) = 0.0254, RV = 3.1 and a Fitzpatrick (1999) extinction law – are also listed. We increase the PanSTARRS fluxes by 10% over the values below, as described in the text.
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