| Instrument . | Central . | FWHM . | Calibration . | Reference* . | Coverage . |
|---|---|---|---|---|---|
| . | wavelength . | . | uncertainty . | . | contribution . |
| AKARI/IRC | 9|$\, \mu$|m | ∼10″ | <10% | [1] | VSGs; 6.2, 7.7, 8.6 |
| and 11.2|$\, \mu$|m PAH | |||||
| AKARI/IRC | 18|$\, \mu$|m | ∼10″ | <10% | [1] | VSGs |
| AKARI/FIS | 65|$\, \mu$|m | 63″ | <10% | [2,3] | VSGs, TEGs† |
| AKARI/FIS | 90|$\, \mu$|m | 78″ | <10% | [2,3] | TEGs |
| AKARI/FIS | 140|$\, \mu$|m | 88″ | <10% | [2,3] | TEGs |
| AKARI/FIS | 160|$\, \mu$|m | 88″ | <10% | [2,3] | TEGs |
| COBE/DIRBE | 160|$\, \mu$|m | 88″ | <10% | [2,3] | TEGs |
| IRAS/IRIS | 12|$\, \mu$|m | |${4_{.}^{\prime}0}$| | <5.1% | [4] | VSGs, 8.6, 11.2, 12.7|$\, \mu$|m PAH features |
| IRAS/IRIS | 25|$\, \mu$|m | |${4_{.}^{\prime}0}$| | <15.1% | [4] | VSGs |
| IRAS/IRIS | 60|$\, \mu$|m | |${4_{.}^{\prime}2}$| | <10.4% | [4] | VSGs, TEGs |
| IRAS/IRIS | 100|$\, \mu$|m | |${4_{.}^{\prime}5}$| | <13.5% | [4] | TEGs |
| Planck/HFI | 345|$\, \mu$|m | |${4_{.}^{\prime}7}$| | [5] | TEGs | |
| Planck/HFI | 550|$\, \mu$|m | |${4_{.}^{\prime}3}$| | [5] | TEGs | |
| Hα | 658.5 nm | 36″ | [6] | Free–free tracer | |
| Planck |$\mathit {AME}{\rm var}$| (PR2) | 22.8 GHz | 60″ | [7] | Variable peak frequency AME | |
| Planck |$\mathit {AME}{\rm fix}$| (PR2) | 41.0 GHz | 60″ | [7] | Fixed peak frequency AME |
| Instrument . | Central . | FWHM . | Calibration . | Reference* . | Coverage . |
|---|---|---|---|---|---|
| . | wavelength . | . | uncertainty . | . | contribution . |
| AKARI/IRC | 9|$\, \mu$|m | ∼10″ | <10% | [1] | VSGs; 6.2, 7.7, 8.6 |
| and 11.2|$\, \mu$|m PAH | |||||
| AKARI/IRC | 18|$\, \mu$|m | ∼10″ | <10% | [1] | VSGs |
| AKARI/FIS | 65|$\, \mu$|m | 63″ | <10% | [2,3] | VSGs, TEGs† |
| AKARI/FIS | 90|$\, \mu$|m | 78″ | <10% | [2,3] | TEGs |
| AKARI/FIS | 140|$\, \mu$|m | 88″ | <10% | [2,3] | TEGs |
| AKARI/FIS | 160|$\, \mu$|m | 88″ | <10% | [2,3] | TEGs |
| COBE/DIRBE | 160|$\, \mu$|m | 88″ | <10% | [2,3] | TEGs |
| IRAS/IRIS | 12|$\, \mu$|m | |${4_{.}^{\prime}0}$| | <5.1% | [4] | VSGs, 8.6, 11.2, 12.7|$\, \mu$|m PAH features |
| IRAS/IRIS | 25|$\, \mu$|m | |${4_{.}^{\prime}0}$| | <15.1% | [4] | VSGs |
| IRAS/IRIS | 60|$\, \mu$|m | |${4_{.}^{\prime}2}$| | <10.4% | [4] | VSGs, TEGs |
| IRAS/IRIS | 100|$\, \mu$|m | |${4_{.}^{\prime}5}$| | <13.5% | [4] | TEGs |
| Planck/HFI | 345|$\, \mu$|m | |${4_{.}^{\prime}7}$| | [5] | TEGs | |
| Planck/HFI | 550|$\, \mu$|m | |${4_{.}^{\prime}3}$| | [5] | TEGs | |
| Hα | 658.5 nm | 36″ | [6] | Free–free tracer | |
| Planck |$\mathit {AME}{\rm var}$| (PR2) | 22.8 GHz | 60″ | [7] | Variable peak frequency AME | |
| Planck |$\mathit {AME}{\rm fix}$| (PR2) | 41.0 GHz | 60″ | [7] | Fixed peak frequency AME |
*References. [1] Ishihara et al. (2010); [2] Doi et al. (2015); [3] Takita et al. (2015); [4] Miville-Deschênes and Lagache (2005); [5] Planck Collaboration (2014c); [6] Finkbeiner (2003); [7] PC15X.
†Thermal equilibrium grains.
| Instrument . | Central . | FWHM . | Calibration . | Reference* . | Coverage . |
|---|---|---|---|---|---|
| . | wavelength . | . | uncertainty . | . | contribution . |
| AKARI/IRC | 9|$\, \mu$|m | ∼10″ | <10% | [1] | VSGs; 6.2, 7.7, 8.6 |
| and 11.2|$\, \mu$|m PAH | |||||
| AKARI/IRC | 18|$\, \mu$|m | ∼10″ | <10% | [1] | VSGs |
| AKARI/FIS | 65|$\, \mu$|m | 63″ | <10% | [2,3] | VSGs, TEGs† |
| AKARI/FIS | 90|$\, \mu$|m | 78″ | <10% | [2,3] | TEGs |
| AKARI/FIS | 140|$\, \mu$|m | 88″ | <10% | [2,3] | TEGs |
| AKARI/FIS | 160|$\, \mu$|m | 88″ | <10% | [2,3] | TEGs |
| COBE/DIRBE | 160|$\, \mu$|m | 88″ | <10% | [2,3] | TEGs |
| IRAS/IRIS | 12|$\, \mu$|m | |${4_{.}^{\prime}0}$| | <5.1% | [4] | VSGs, 8.6, 11.2, 12.7|$\, \mu$|m PAH features |
| IRAS/IRIS | 25|$\, \mu$|m | |${4_{.}^{\prime}0}$| | <15.1% | [4] | VSGs |
| IRAS/IRIS | 60|$\, \mu$|m | |${4_{.}^{\prime}2}$| | <10.4% | [4] | VSGs, TEGs |
| IRAS/IRIS | 100|$\, \mu$|m | |${4_{.}^{\prime}5}$| | <13.5% | [4] | TEGs |
| Planck/HFI | 345|$\, \mu$|m | |${4_{.}^{\prime}7}$| | [5] | TEGs | |
| Planck/HFI | 550|$\, \mu$|m | |${4_{.}^{\prime}3}$| | [5] | TEGs | |
| Hα | 658.5 nm | 36″ | [6] | Free–free tracer | |
| Planck |$\mathit {AME}{\rm var}$| (PR2) | 22.8 GHz | 60″ | [7] | Variable peak frequency AME | |
| Planck |$\mathit {AME}{\rm fix}$| (PR2) | 41.0 GHz | 60″ | [7] | Fixed peak frequency AME |
| Instrument . | Central . | FWHM . | Calibration . | Reference* . | Coverage . |
|---|---|---|---|---|---|
| . | wavelength . | . | uncertainty . | . | contribution . |
| AKARI/IRC | 9|$\, \mu$|m | ∼10″ | <10% | [1] | VSGs; 6.2, 7.7, 8.6 |
| and 11.2|$\, \mu$|m PAH | |||||
| AKARI/IRC | 18|$\, \mu$|m | ∼10″ | <10% | [1] | VSGs |
| AKARI/FIS | 65|$\, \mu$|m | 63″ | <10% | [2,3] | VSGs, TEGs† |
| AKARI/FIS | 90|$\, \mu$|m | 78″ | <10% | [2,3] | TEGs |
| AKARI/FIS | 140|$\, \mu$|m | 88″ | <10% | [2,3] | TEGs |
| AKARI/FIS | 160|$\, \mu$|m | 88″ | <10% | [2,3] | TEGs |
| COBE/DIRBE | 160|$\, \mu$|m | 88″ | <10% | [2,3] | TEGs |
| IRAS/IRIS | 12|$\, \mu$|m | |${4_{.}^{\prime}0}$| | <5.1% | [4] | VSGs, 8.6, 11.2, 12.7|$\, \mu$|m PAH features |
| IRAS/IRIS | 25|$\, \mu$|m | |${4_{.}^{\prime}0}$| | <15.1% | [4] | VSGs |
| IRAS/IRIS | 60|$\, \mu$|m | |${4_{.}^{\prime}2}$| | <10.4% | [4] | VSGs, TEGs |
| IRAS/IRIS | 100|$\, \mu$|m | |${4_{.}^{\prime}5}$| | <13.5% | [4] | TEGs |
| Planck/HFI | 345|$\, \mu$|m | |${4_{.}^{\prime}7}$| | [5] | TEGs | |
| Planck/HFI | 550|$\, \mu$|m | |${4_{.}^{\prime}3}$| | [5] | TEGs | |
| Hα | 658.5 nm | 36″ | [6] | Free–free tracer | |
| Planck |$\mathit {AME}{\rm var}$| (PR2) | 22.8 GHz | 60″ | [7] | Variable peak frequency AME | |
| Planck |$\mathit {AME}{\rm fix}$| (PR2) | 41.0 GHz | 60″ | [7] | Fixed peak frequency AME |
*References. [1] Ishihara et al. (2010); [2] Doi et al. (2015); [3] Takita et al. (2015); [4] Miville-Deschênes and Lagache (2005); [5] Planck Collaboration (2014c); [6] Finkbeiner (2003); [7] PC15X.
†Thermal equilibrium grains.
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