Table 1
Source photometry and integrated luminosities.
| Source name | RA (J2000) | Dec (J2000) | F70 μm (Jy) | F160 μm (Jy) | Lintegrated (L⊙) | Class | Other IDsc |
|
|
|||||||
| IC 1396 A-PACS-1 | 21:37:05.04 | +57:30:56.4 | 2.32 ± 0.23 | 25.5 ± 2.6 | 1.5 ± 0.1 | 0 | |
| 21364660+5729384 | 21:36:46.60 | +57:29:38.4 | 3.31 ± 0.33 | 3.2 ± 0.3 | 1.00 ± 0.08 | I | α |
| 21361942+5728385 | 21:36:19.42 | +57:28:38.5 | 0.97 ± 0.10 | 5.4 ± 1.1a | 0.22 ± 0.10b | I | ϵ |
| 21361836+5728316 | 21:36:18.36 | +57:28:31.6 | 1.49 ± 0.15 | 5.4 ± 1.1a | 0.26 ± 0.10b | I | δ |
Notes. Photometry of the known cluster members detected by Herschel/PACS in IC 1396 A, and their integrated luminosities (taking the ancillary data for the Class I sources into account, see Table 2). The 160 μm flux for 21361836+5728316 and 21361942+5728385 corresponds to both sources, which appear merged in the image, with the peak flux close to the position of 21361836+5728316.
Luminosities for these sources are very uncertain due to the lack of observations at longer and shorter wavelengths, and the fact that the 160 μm data point includes both objects.
Alternative IDs from Reach et al. (2004).
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