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Table 2
Mean levels of CIB from different instruments at different frequencies with the corresponding colour corrections used to convert themto the Planck and IRAS bandpasses.
Instrument | Freq | νIν | Colour |
---|---|---|---|
GHz | nWm−2sr−1 | correction | |
Herschel/PACS | 3000 | ![]() |
0.9996 |
Berta et al. (2011) | |||
Herschel/PACS | 1875 | ![]() |
0.9713 |
Berta et al. (2011) | |||
Herschel/SPIRE | 1200 | ![]() |
0.9880 |
Béthermin et al. (2012b) | |||
Herschel/SPIRE | 857 | ![]() |
0.9887 |
Béthermin et al. (2012b) | |||
JCMT/SCUBA2 | 667 | ![]() |
1.0057 |
Wang et al. (2017) | |||
Herschel/SPIRE | 600 | ![]() |
0.9739 |
Béthermin et al. (2012b) | |||
JCMT/SCUBA2 | 353 | ![]() |
0.9595 |
Zavala et al. (2017) | |||
ALMA | 250 | >0.08 | – |
Aravena et al. (2016) |
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