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Table 3
Photometric data HD 34282 (not corrected for extinction) used in this study.
| Band ID | λ [μm] | Fν [Jansky] | Reference | ||
|
|
|||||
| Walraven W | 0.32 | 0.09 | 0.00 | a | |
| Johnson U | 0.36 | 0.16 | 0.00 | b | |
| Walraven U | 0.36 | 0.12 | 0.00 | a | |
| Walraven L | 0.38 | 0.23 | 0.01 | a | |
| Walraven B | 0.43 | 0.39 | 0.01 | a | |
| Johnson B | 0.44 | 0.44 | 0.01 | b | |
| Walraven V | 0.54 | 0.41 | 0.00 | a | |
| Johnson V | 0.55 | 0.44 | 0.00 | b | |
| Cousins R | 0.64 | 0.36 | 0.01 | a | |
| Cousins I | 0.79 | 0.34 | 0.01 | a | |
| Near-IR J | 1.23 | 0.43 | 0.01 | b | |
| Near-IR H | 1.65 | 0.58 | 0.01 | b | |
| Near-IR K | 2.22 | 0.71 | 0.01 | b | |
| WISE 1 | 3.35 | 0.61 | 0.02 | c | |
| Near-IR L | 3.77 | 0.65 | 0.03 | b | |
| WISE 2 | 4.60 | 0.52 | 0.01 | c | |
| Near-IR M | 4.78 | 0.58 | 0.03 | b | |
| AKARI S09 | 9.00 | 0.74 | 0.04 | d | |
| WISE 3 | 11.60 | 0.54 | 0.01 | c | |
| IRAS 12 | 11.80 | 0.65 | 0.1 | e | |
| WISE 4 | 22.10 | 1.40 | 0.02 | c | |
| IRAS 25 | 25.00 | 1.58 | 0.23 | e | |
| IRAS 60 | 60.00 | 10.60 | 1.57 | e | |
| AKARI S65 | 65.00 | 10.04 | 0.73 | d | |
| AKARI S90 | 90.00 | 11.17 | 0.26 | d | |
| IRAS 100 | 100.00 | 10.58 | 1.85 | e | |
| AKARI S140 | 140.00 | 9.75 | 0.93 | d | |
| AKARI S160 | 160.00 | 9.35 | 0.19 | d | |
| 450 micron | 450.00 | 1.61 | 0.83 | b | |
| 800 micron | 800.00 | 0.41 | 0.32 | b | |
| 1100 micron | 1100.00 | 0.18 | 0.14 | b | |
| PDB 1.3 | 1300.00 | 0.10 | 0.02 | g | |
| 2600 micron | 2600.0 | 0.02 | 0.019 | f | |
| PDB 3.2 | 3200.00 | 0.01 | 0.00 | g | |
Reference. a) de Winter et al. (2001). b) Sylvester et al. (1996). c) WISE All-Sky Data Release. d) AKARI/IRC mid-IR all-sky Survey. e) IRAS Point-source catalogue. f) Mannings & Sargent (2000). g)Natta et al. (2004).
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