Table A.1
Overview of filter bands and instruments considered in this study.
| Instrument | Band | λ(μm) | Reference |
|---|---|---|---|
| WISE | 3 | 12 | Wright et al. (2010) |
| WISE | 4 | 22 | Wright et al. (2010) |
| MSX/SPIRIT-III | 2 | 12.13 | Egan et al. (1999) |
| MSX/SPIRIT-III | 3 | 14.65 | Egan et al. (1999) |
| MSX/SPIRIT-III | 4 | 21.34 | Egan et al. (1999) |
| Spitzer | MIPS | 24 | Table 1, Dole et al. (2003) |
| SOFIA / HAWC+ | A | 53 | Harper et al. (2018) |
| SOFIA / HAWC+ | B | 63 | Harper et al. (2018) |
| SOFIA / HAWC+ | C | 89 | Harper et al. (2018) |
| SOFIA / HAWC+ | D | 154 | Harper et al. (2018) |
| SOFIA / HAWC+ | E | 214 | Harper et al. (2018) |
| Herschel | PACS 1 | 70 | PACS Photometer Quickstart Guide, Exter (2017) |
| Herschel | PACS 2 | 100 | PACS Photometer Quickstart Guide, Exter (2017) |
| Herschel | PACS 3 | 160 | PACS Photometer Quickstart Guide, Exter (2017) |
| Herschel | SPIRE 1 | 250 | Table 5.2, SPIRE Handbook, Valtchanov (2018) |
| Herschel | SPIRE 2 | 350 | Table 5.2, SPIRE Handbook, Valtchanov (2018) |
| Herschel | SPIRE 3 | 500 | Table 5.2, SPIRE Handbook, Valtchanov (2018) |
| ALMA | Band 10 | 350 | Table 7.1, Cortes et al. (2022) |
| Table 7.1, Cortes et al. (2022) | |||
| ALMA | Band 9 | 460 | Table 7.1, Cortes et al. (2022) |
| Table 7.1, Cortes et al. (2022) | |||
| ALMA | Band 8 | 690 | Table 7.1, Cortes et al. (2022) |
| Table 7.1, Cortes et al. (2022) | |||
| ALMA | Band 7 | 945 | Table 7.1, Cortes et al. (2022) |
| Table 7.1, Cortes et al. (2022) | |||
| ALMA | Band 6 | 1300 | Table 7.1, Cortes et al. (2022) |
| Table 7.1, Cortes et al. (2022) | |||
| APEX | LABOCA | 870 | APEX LABOCA website |
| (https://www.apex-telescope.org/ns/laboca-calibration/) | |||
| CSO | Bolocam | 1100 | Bolocam website |
| (http://www.cso.caltech.edu/bolocam/ProposerInfo.html) |
Notes. For each instrument and band, we list the central wavelength λ and the literature reference for the quoted values. We note that we treat ALMA Band 10 and Herschel SPIRE 2 as one band in our analysis, because they share the same central wavelength and we are not considering any instrument related effects. Consequently, there is no difference in the corresponding synthetic dust emission maps between SPIRE 2 and ALMA Band 10 in our analysis.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.