Table 2
Flux densities of CRBR 2422.8-34236 as shown in Fig. 2.
| λ [μm] | Flux density [mJy] | Instrument | Reference |
|
|
|||
| 1.6 | 0.07 ± 0.03 | VLT/ISAAC | (1) |
| 2.16 | 2.26 ± 0.24 | 2MASS facility | (2) |
| 3.6 | 54 | SST/IRAC | (3) |
| 4.5 | 131 | SST/IRAC | (3) |
| 5.8 | 191 | SST/IRAC | (3) |
| 8.0 | 198 | SST/IRAC | (3) |
| 9.0 | 140 ± 25 | AKARI | (4) |
| 10.5 | 130 ± 14 | VLT/VISIR | (5) |
| 18.0 | 645 ± 88 | AKARI | (4) |
| 18.7 | 858 ± 109 | VLT/VISIR | (5) |
| 24 | 1340 | SST/MIPS | (3) |
| 70 | 9800 | SST/MIPS | (3) |
| 850 | 1300 ± 260 | JCMT/SCUBA | (3) |
| 1300 | 150 | IRAM 30 m | (6) |
| 3300 | 1.5 ± 0.3 | ATCA | (7) |
Notes. ISAAC: Infrared Spectrometer And Array Camera; JCMT: James Clerk Maxwell Telescope; SCUBA: Submillimetre Common-User Bolometer Array; IRAM: Institut de Radioastronomie Millimétrique. In addition to the flux densities listed above there is also a K-band spectrum (Brandner et al. 2000), a M-band spectrum (Thi et al. 2002), and a SST/IRS spectrum (Pontoppidan et al. 2005) available in the literature.
Reference. (1) Brandner et al. (2000); (2) 2MASS All-Sky Catalog of Point Sources; (3) van Kempen et al. (2009); (4) AKARI Point Source Catalogs; (5) this work; (6) Motte et al. (1998); (7) Ricci et al. (2010).
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