Table 1
Flux densities of PDS 66 as shown in Fig. 1.
λ [μm] | Flux density [mJy] | Instrument | Reference |
|
|||
0.37 | 31 ± 3 | (1) | |
0.43 | 116 ± 15 | Hipparcos | (2) |
0.55 | 252 ± 19 | Hipparcos | (2) |
0.64 | 392 ± 11 | (1) | |
0.9 | 551 ± 30 | La Silla/ESO 1m | (3) |
1.25 | 779 ± 46 | 2MASS facility | (4) |
1.65 | 899 ± 39 | 2MASS facility | (4) |
2.16 | 807 ± 27 | 2MASS facility | (4) |
3.6 | 657 ± 14 | SST/IRAC | (5) |
4.5 | 521 ± 12 | SST/IRAC | (5) |
8.0 | 471 ± 10 | SST/IRAC | (5) |
9.0 | 544 ± 39 | AKARI | (6) |
10.5 | 599 ± 8 | VLT/VISIR | (7) |
11.6 | 730 ± 30 | La Silla/TIMMI2 | (8) |
12 | 882 ± 88 | IRAS | (9) |
18 | 1337 ± 27 | AKARI | (6) |
24 | 1874 ± 120 | SST/MIPS | (5) |
25 | 2070 ± 228 | IRAS | (9) |
60 | 2390 ± 335 | IRAS | (9) |
70 | 1672 ± 118 | SST/MIPS | (5) |
90 | 2126 ± 79 | AKARI | (6) |
160 | 2138 ± 290 | SST/MIPS | (5) |
1200 | 224 ± 8 | SEST/SIMBA | (8) |
3000 | 22 ± 3.3 | ATCA | (1) |
12 000 | 0.41 ± 0.06 | ATCA | (1) |
Notes. SST: Spitzer Space Telescope; IRAC: Infrared Array Camera; VLT: Very Large Telescope; VISIR: VLT spectrometer and imager for the mid-infrared; TIMMI2: Thermal Infrared MultiMode Instrument; IRAS: Infrared Astronomical Satellite; MIPS: Multiband Imaging Photometer for Spitzer; SEST: Swedish ESO Submillimeter Telescope; SIMBA: SEST IMaging Bolometer Array; ATCA: Australia Telescope Compact Array. In addition to the flux densities listed above there is also a TIMMI2 spectrum in the range [8, 13] μm (Schütz et al. 2005), a SST/Infrared Spectrograph low-resolution spectrum in the range [5, 35] μm (Silverstone et al. 2006; Bouwman et al. 2008), and a spectrum in the range [0.3, 1] μm obtained with the 4 m Cerro Tololo Inter-American Observatory (Pascucci et al. 2007) available in the literature.
Reference. (1) Cortes et al. (2009); (2) Tycho-2 Catalog; (3) DENIS database; (4) 2MASS All-Sky Catalog of Point Sources; (5) Hillenbrand et al. (2008); (6) AKARI Point Source Catalogs; (7) this work; (8) Schütz et al. (2005); (9) IRAS Catalog of Point Sources.
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