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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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