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Table 2
Infrared photometry of the nucleus.
| Beam | Nuclear | |||||||||||
| Name | λ obs | f ν | FWHM | FWHM a | Ref. | |||||||
| ( μm) | (Jy) | (′′) | (′′) | |||||||||
|
|
||||||||||||
| MIPS | 24 | 1.72 ± 0.02 | 5.̋9 | 7.̋1 | 1 | |||||||
| PACS | 70 | 42.3 ± 0.2 | 5.̋6 | 6.̋4 | 2 | |||||||
| PACS | 100 | 48.6 ± 0.2 | 6.̋8 | 7.̋7 | 2 | |||||||
| PACS | 160 | 33.4 ± 0.1 | 11.̋4 | 12 | 2 | |||||||
| SPIRE | 250 | 11.7 ± 0.1 | 17.̋6 | 18 | 2 | |||||||
| SPIRE | 350 | 4.4 ± 0.1 | 23.̋9 | 26 | 2 | |||||||
| SPIRE | 500 | 1.42 ± 0.02 | 35.̋2 | 37 | 2 | |||||||
Notes. Nuclear fluxes of ESO 320-G030 from the Spitzer/MIPS, Herschel/PACS, and Herschel/SPIRE observations. In all these images, the integrated emission of ESO 320-G030 is dominated by a barely resolved nuclear source.
Reference. (1) Pereira-Santaella et al. (2011); (2) This work.
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