Table 2
Top section: emissivities of AME at 22.8 GHz (μK) relative to the Commander thermal dust amplitude at 545 GHz (MJy sr-1), the IRAS map at 100 μm (MJy sr-1), and the optical depth at 353 GHz, τ353, for the regions shown in Figs. 10 and 13. Bottom part: emissivities from Davies et al. (2006, D06; whole sky and region mean) and Planck Collaboration Int. XV (2014, XV; Perseus, ρ for comparison.
| Region ................. | AME/545 GHz | AME/100 μm | AME/τ353 |
| [μK (MJy sr-1)-1] | [μK (MJy sr-1)-1] | [μK 10-6] | |
|
|
|||
| R1: Perseus ................. | 24 ± 7 | 12.3 ± 1.9 | 1.5 ± 0.9 |
| R2: Plume ................. | 47 ± 6 | 18 ± 2 | 7.7 ± 1.0 |
| R3: R CrA ................. | 36 ± 14 | 50 ± 12 | 4.1 ± 1.8 |
| R4: ρ Oph ................. | 40 ± 9 | 4.6 ± 0.9 | 2.2 ± 1.2 |
| R5: Musca ................. | 59 ± 8 | 26 ± 3 | 6.9 ± 1.0 |
| Chamaeleon | 74 ± 8 | 22 ± 2 | 11 ± 1.1 |
| R6: Orion ................. | 47 ± 5 | 20 ± 2 | 4.7 ± 0.6 |
| R7: λ Orionis ................. | 104 ± 11 | 25 ± 3 | 15 ± 1.8 |
| LMC ................. | 56 ± 6 | 8.5 ± 1.0 | 7.9 ± 0.9 |
| SMC ................. | 30 ± 9 | 4.7 ± 1.5 | 3.3 ± 1.0 |
| Entire sky ................. | 65 ± 7 | 22 ± 2 | 8.3 ± 0.8 |
| | b | > 10deg ............. | 70 ± 7 | 21 ± 2 | 9.7 ± 1.0 |
|
|
|||
| XV: Perseus ................. | ... | 24 ± 4 | ... |
| XV: ρ Oph ................. | ... | 8.3 ± 1.1 | ... |
| XV: Mean ................. | ... | 32 ± 4 | ... |
| D06: Kp2 mask ................. | ... | 21.8 ± 1.0 | ... |
| D06: Region mean .............. | ... | 25.7 ± 1.3 | ... |
Notes. We also include emissivities for the LMC and SMC, discussed in Sect. 4.5.
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