Table C.7
DUNES_DB stars with d ≤ 20 pc: IRAS 12, 25, 60 μm and Spitzer/MIPS 24 and 70 μm fluxes.
HIP | IRAS | MIPS | ||||||||
|
||||||||||
|
||||||||||
12 μm | % | 25 μm | % | 60 μm | % | 24 μm | 70 μm | |||
(mJy) | (mJy) | (mJy) | (mJy) | (mJy) | ||||||
|
||||||||||
FGK stars (d ≤ 15 pc) | ||||||||||
|
||||||||||
1599 | 3.11 ×103 | 4 | 6.95 ×102 | 4 | 519 ± 11 | 82 ± 8 | ||||
3765 | 1.56 ×103 | 7 | 264 ± 5 | 26 ± 10 | ||||||
7751 | 2.70 ×103 | 5 | 6.55 ×102 | 7 | 231 ± 5 | 22 ± 4 | ||||
7918 | 1.67 ×103 | 5 | 3.87 ×102 | 8 | 289 ± 6 | 25 ± 11 | ||||
7981 | 1.87 ×103 | 7 | 6.38 ×102 | 10 | 334 ± 7 | 48 ± 9 | ||||
10644 | 2.11 ×103 | 5 | 4.97 ×102 | 6 | 359 ± 7 | 43 ± 5 | ||||
12114 | 1.83 ×103 | 5 | 3.47 ×102 | 14 | 311 ± 6 | 35 ± 6 | ||||
12843 | 1.93 ×103 | 6 | 346 ± 7 | 37 ± 13 | ||||||
14879 | 4.02 ×103 | 4 | 9.43 ×102 | 4 | 1.80 ×102 | 18 | 754 ± 15 | 105 ± 13 | ||
15457 | 2.05 ×103 | 4 | 4.67 ×102 | 8 | 340 ± 7 | 39 ± 8 | ||||
15510 | 4.27 ×103 | 4 | 9.50 ×102 | 5 | 1.89 ×102 | 17 | 722 ± 15 | 100 ± 8 | ||
16852 | 2.85 ×103 | 5 | 6.81 ×102 | 8 | 502 ± 10 | 106 ± 9 | ||||
22449 | 5.67 ×103 | 12 | 1.51 ×103 | 7 | 2.04 ×102 | 20 | 1020 ± 21 | 116 ± 9 | ||
23693 | 1.67 ×103 | 5 | 4.40 ×102 | 8 | 308 ± 6 | 6 ± 7 | ||||
27072 | 4.40 ×103 | 5 | 9.81 ×102 | 6 | 2.28 ×102 | 16 | 765 ± 16 | 56 ± 10 | ||
37279 | 8.29 ×104 | 4 | 1.87 ×104 | 5 | 3.00 ×103 | 6 | 1520 ± 103 | |||
47080 | 1.47 ×103 | 5 | 3.49 ×102 | 11 | 257 ± 5 | 581 ± 0 | ||||
56997 | 258 ± 5 | 30 ± 5 | ||||||||
57443 | 2.03 ×103 | 7 | 4.92 ×102 | 10 | 334 ± 7 | 32 ± 6 | ||||
57757 | 5.24 ×103 | 7 | 1.21 ×103 | 10 | 1.79 ×102 | 25 | 829 ± 17 | 114 ± 1 | ||
59199 | 2.45 ×103 | 7 | 5.52 ×102 | 9 | 368 ± 8 | 46 ± 6 | ||||
61317 | 3.49 ×103 | 5 | 7.29 ×102 | 6 | 557 ± 11 | 65 ± 1 | ||||
61941 | 7.67 ×103 | 6 | 1.70 ×103 | 7 | 2.91 ×102 | 20 | 1410 ± 29 | 238 ± 122 | ||
64394 | 2.98 ×103 | 7 | 6.46 ×102 | 8 | 489 ± 10 | 49 ± 6 | ||||
64924 | 2.56 ×103 | 6 | 5.80 ×102 | 12 | 443 ± 9 | 192 ± 16 | ||||
70497 | 3.08 ×103 | 4 | 7.24 ×102 | 5 | 1.09 ×102 | 28 | 540 ± 11 | 63 ± 8 | ||
72659 | 3.90 ×103 | 5 | 8.95 ×102 | 6 | 1.57 ×102 | 25 | 476 ± 10 | 53 ± 7 | ||
73695 | 2.50 ×103 | 4 | 5.88 ×102 | 5 | 468 ± 10 | 70 ± 12 | ||||
77257 | 2.46 ×103 | 4 | 5.91 ×102 | 7 | 433 ± 9 | 84 ± 15 | ||||
78072 | 3.82 ×103 | 5 | 8.82 ×102 | 5 | 3.32 ×102 | 12 | 630 ± 13 | 70 ± 17 | ||
80686 | 1.58 ×103 | 4 | 3.68 ×102 | 6 | 284 ± 6 | 21 ± 13 | ||||
89937 | 5.51 ×103 | 3 | 1.31 ×103 | 4 | 2.20 ×102 | 14 | 1050 ± 21 | 127 ± 10 | ||
93017 | 1.44 ×103 | 4 | 3.47 ×102 | 6 | 239 ± 5 | 25 ± 6 | ||||
99825 | 1.49 ×103 | 6 | 4.04 ×102 | 23 | 237 ± 5 | 22 ± 4 | ||||
102485 | 2.35 ×103 | 7 | 5.14 ×102 | 14 | 391 ± 8 | 44 ± 8 | ||||
105858 | 2.95 ×103 | 4 | 6.42 ×102 | 6 | 1.72 ×102 | 21 | 472 ± 10 | 44 ± 6 | ||
109176 | 3.70 ×103 | 7 | 8.55 ×102 | 11 | 667 ± 14 | 75 ± 7 | ||||
113283 | 1.27 ×103 | 6 | 3.45 ×102 | 13 | 213 ± 4 | 27 ± 4 | ||||
116771 | 2.97 ×103 | 6 | 7.37 ×102 | 15 | 511 ± 10 | 61 ± 8 | ||||
FGK stars (15 pc <d ≤ 20 pc) | ||||||||||
|
||||||||||
5862 | 1.44 ×103 | 7 | 3.45 ×102 | 14 | 246 ± 5 | 45 ± 5 | ||||
17651 | 2.19 ×103 | 5 | 4.76 ×102 | 7 | 366 ± 8 | 48 ± 5 | ||||
36366 | 2.01 ×103 | 5 | 4.82 ×102 | 21 | 356 ± 7 | 42 ± 7 | ||||
44248 | 2.94 ×103 | 5 | 7.41 ×102 | 7 | 518 ± 11 | |||||
46509 | 1.69 ×103 | 5 | 3.37 ×102 | 14 | 258 ± 5 | 31 ± 4 | ||||
48113 | 1.48 ×103 | 5 | 3.27 ×102 | 9 | 247 ± 5 | 33 ± 5 | ||||
61174 | 2.24 ×103 | 6 | 7.70 ×102 | 8 | 3.08 ×102 | 14 | 573 ± 12 | 20 ± 14 | ||
64241 | 2.19 ×103 | 6 | 5.11 ×102 | 13 | 385 ± 8 | 50 ± 11 | ||||
67153 | 1.93 ×103 | 5 | 4.22 ×102 | 10 | 332 ± 7 | 106 ± 76 | ||||
71284 | 1.61 ×103 | 5 | 4.13 ×102 | 7 | 1.40 ×102 | 25 | 302 ± 6 | 72 ± 11 | ||
75312 | 1.43 ×103 | 5 | 3.41 ×102 | 9 | 273 ± 6 | 70 ± 12 | ||||
77760 | 2.31 ×103 | 5 | 5.71 ×102 | 6 | 402 ± 8 | 40 ± 6 | ||||
88745 | 1.52 ×103 | 5 | 3.50 ×102 | 8 | 268 ± 6 | 107 ± 9 | ||||
104858 | 2.21 ×103 | 7 | 5.42 ×102 | 8 | 362 ± 7 | 43 ± 5 | ||||
112447 | 3.05 ×103 | 7 | 7.56 ×102 | 9 | 467 ± 10 | 50 ± 5 |
Notes. All IRAS fluxes are from the Faint Source Catalogue (II/156A in Vizier) except for HIP 3765, which is from the IRAS Catalogue of Point Sources (II/125). Upper limits to the fluxes are not given. Spitzer/MIPS fluxes at 24 and 70 μm were extracted by members of the DUNES team. See http://sdc.cab.inta-csic.es/dunes/HELP/DUNES_Archive_ReadMe.jsp or http://sdc.cab.inta-csic.es/dunes/HELP/DUNES_Archive_ReadMe.pdf for details.
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