Table 2
PACS 160 μm photometry.
| Source ID | RA (J2000) | Dec (J2000) | Flux | Comments |
| (deg) | (deg) | (Jy) | ||
|
|
||||
| S CrA | 285.285790 | −36.955485 | 13.6 ± 2.7 | |
| G-122 | 285.421180 | −36.953821 | 2.2 ± 0.4 | Sicilia-Aguilar et al. (2008) |
| IRS 2 | 285.422310 | −36.974903 | 61 ± 12 | |
| IRS 2+ring | 285.422310 | −36.974903 | 103 ± 20 | Including ring-like structure |
| IRS 5a+b + FP-25 | 285.451320 | −36.954874 | 23 ± 5 | Multiple system without spiral structure |
| IRS 5a+b/FP-25 + spiral | 285.451320 | −36.954874 | 131 ± 26 | Multiple system plus spiral structure |
| IRS 6a+b | 285.460040 | −36.943701 | 11 ± 2 | |
| V 710 | 285.461110 | −36.968953 | 70 ± 14 | IRS 1, extended? |
| SMM 1A s | 285.47914 | −36.97314 | 30 ± 7 | Groppi et al. (2007), extended? |
| IRS 7w+e | 285.4812 | −36.9564 | 880 ± 170 | Binary plus surrounding structure |
| SMM 2 | 285.49313 | −36.95201 | 25 ± 5 | |
| T CrA | 285.49493 | −36.96386 | 13 ± 3 | Uncertain due to proximity of IRS 7w/e |
| APEX 13+15 | 285.552040 | −37.008617 | 0.46 ± 0.10 | Sicilia-Aguilar (2011a), extended |
| APEX 6 | 285.577930 | −37.023607 | 0.40 ± 0.08 | Sicilia-Aguilar (2011a), extended |
| APEX 16 | 285.599610 | −36.942940 | 0.28 ± 0.06 | Sicilia-Aguilar (2011a), extended |
| APEX 19 | 285.635820 | −37.033284 | 0.12 ± 0.03 | Sicilia-Aguilar (2011a), extended |
| IRAS 18598 | 285.744070 | −37.126434 | 42 ± 3 | Extended? |
| APEX 7+10+24 | 285.770620 | −37.242373 | 0.24 ± 0.05 | Sicilia-Aguilar (2011a), extended |
| VV CrA | 285.778020 | −37.213602 | 66 ± 13 | |
| CrA-45 | 285.816670 | −37.235619 | 0.81 ± 0.16 | Peterson et al. (2011) |
| #19 North | 285.5520 | −36.9549 | 13 ± 3 | Part of source #19 from Chini et al. (2003), extended |
| #19 South | 285.5646 | −36.9631 | 2.4 ± 0.5 | Part of source #19 from Chini et al. (2003), extended |
Notes. Photometry of the known cluster members detected by Herschel/PACS at 160 μm. For extended sources, the photometry is obtained around the peak (or peaks), but the extended material results in a large uncertainty. In the “Comments” column we include the references of the source name and/or other naming conventions, and whether the source is extended or potentially contaminated.
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