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Table 3.
Models assigned component to each photometric band for MRC 0114−211.
Photometric band | Assigned model | Fitted model |
---|---|---|
IRS (16 μm) | AGN, BB1, BB2 | AGN |
MIPS (24 μm) | AGN, BB1, BB2 | AGN |
PACS (70 μm) | AGN, BB1, BB2 | AGN, BB2 |
PACS (160 μm) | AGN, BB1, BB2 | AGN, BB2 |
SPIRE (250 μm) | AGN, BB1, BB2 | AGN, BB2 |
SPIRE (350 μm) | AGN, BB1, BB2 | BB2 |
SPIRE (500 μm) | AGN, BB1, BB2 | BB2 |
LABOCA (870 μm) | AGN, BB1, BB2 | BB2 |
ALMA 6 east comp. | BB1, Sync2 | Sync2 |
ALMA 6 west comp. | BB2, Sync1 | BB2 |
ALMA 3 | BB1, BB2, Sync1, Sync2 | Sync1, Sync2 |
ATCA (7 mm) | Sync1, Sync2 | Sync1, Sync2 |
VLA X west comp. | Sync2 | Sync2 |
VLA X east comp. | Sync1 | Sync1 |
VLA C west comp. | Sync2 | Sync2 |
VLA C east comp. | Sync1 | Sync1 |
VLA L | Sync1, Sync2 | Sync1, Sync2 |
Notes. The last column lists the model components that dominate each band as determined through SED fitting with MR-MOOSE. Models that contribute less than 1% to the total flux in a particular band for the best fitting model are not listed.
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