Table C.1.
Spatially integrated Brδλ1.944 μm, ro-vibrational H2(1–0)S(3)λ1.957 μm, H2(1–0)S(2)λ2.033 μm, H2(1–0)S(1)λ2.122 μm, and HeIλ2.058 μm fluxes relative to the Paα emission line flux.
| HATLAS090750 | HATLAS114625 | HATLAS121446 | |
|---|---|---|---|
| Brδ/Paα | 0.055 ± 0.002 | < 0.12 | < 0.08 |
| H2(1–0)S(3)/Paα | 0.063 ± 0.005 | 0.107 ± 0.006 | < 0.08 |
| H2(1–0)S(2)/Paα | 0.028 ± 0.006 | < 0.17 | < 0.33 |
| H2(1–0)S(1)/Paα | 0.072 ± 0.016 | – | – |
| HeI/Paα | 0.051 ± 0.006 | < 0.27 | < 0.29 |
Notes. We note that the H2(1–0)S(1) emission is redshifted out of the SINFONI K-band wavelength range for the later two galaxies. The upper emission line flux limits are calculated as rms × σPaα, ch, where the rms values are estimated within a 30 channel spectral window width centred at the expected emission line location in the spectra, and σPaα, ch is the Paα emission line width.
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