Table 3
Photometric IRAC and MIPS points for Yggdrasil, Thor, and Loke after de-blending.
| Instrument | Wavelength | SYggdrasil | SThor | SLoke |
| μm | μJy | μJy | μJy | |
|
|
||||
| IRAC 1 | 3.6 | 21.9 | 9.02 | <2.10 |
| IRAC 2 | 4.5 | 36.1 | 21.0 | <1.32 |
| IRAC 3 | 5.8 | − | − | − |
| IRAC 4 | 8.0 | 30.2 | < 21.4 | − |
| MIPS | 24 | 468 ± 40 | 180 ± 40 | − |
Notes. Thor is not detected in the IRAC 3 image, however the flux at the position is influenced by an image artefact from a nearby star in the field. Extracting even an upper limit at this position is therefore not possible. Loke is not detected in any of the IRAC images; we quote the 3σ upper limits (Wylezalek et al. 2013).
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