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Table 1:

The two H-ATLAS blazars found by cross-matching with the FIRST catalog.
H-ATLAS $\Delta$ $S_{1.4~{\rm GHz}}$ $S_{500~\mu{\rm m}}$ $S_{350~\mu{\rm m}}$ $S_{250~\mu{\rm m}}$ $S_{170~\mu{\rm m}}$ $S_{100~\mu{\rm m}}$
name arcsec mJy mJy mJy mJy mJy mJy
J090910.1+012135a 0.3 571.7 $265.8 \pm 8.9$ $193.8\pm 7.2$ $159.6\pm 6.4$ $105.4\pm 26.5$ $137.3\pm 26.5$
J090940.3+015957b 10.3 317.5 $68.2\pm 9.1$ $55.0\pm 7.2$ $35.5\pm 6.4$ <76.2 <79.5

Notes. Coordinates (RA and Dec) refer to the H-ATLAS source. $\Delta$ (arcsec) is the angular separation between FIRST and Herschel positions. The quoted errors in Herschel fluxes are statistical only. Calibration errors are estimated to be $\sim $15% for SPIRE (Swinyard et al. 2010), $\sim $10% at $100~\mu$m, and $\sim $20% at $160~\mu$m. Upper limits are at the 3$\sigma$ level.(a) [HB89] 0906+015, (b) PKS 0907+022.


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