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Table 1

Stellar basic properties and photometric data of the Sample B stars (portion).

Name SpT D Teff F12, obs F12, phot χ12 Fexcess/F12, phot Upper limits
(pc) (K) (mJy) (mJy)
(1) (2) (3) (4) (5) (6) (7) (8) (9)
Proxima Cen M5.5 1.3020±0.0001 3000 912.631±12.585 922.238±44.335 –0.156 –0.010 0.201
alf Cen A G2 1.3459±0.0024 5750 122965.068±44334.671 168116.304±31509.799 –0.826 –0.269 0.976
Barnard’s Star M3.5 1.8282±0.0001 3900 557.185±14.362 658.055±21.903 –2.782 –0.153 0.165
Luhman 16 A L7.5 1.9938±0.0003 1600 103.271±1.427 98.468±0.370 0.985 0.049 0.149
WISEA J085510.74-071442.5 Y2 2.2779±0.0124 550 1.090±0.127 1.009±0.017 0.596 0.081 0.645
Wolf 359 M6 2.4086±0.0004 3000 200.779±2.772 206.543±8.022 –0.465 –0.028 0.180
HD 95735 M1.5e 2.5461±0.0002 3200 1906.919±26.322 1916.526±133.532 –0.060 –0.005 0.252
alf CMa A A1 2.6371±0.0110 11 750 77813.832±23920.548 103271.444±12680.773 –0.933 –0.247 0.793
G 272-61 A M5 2.7195±0.0055 3000 388.108±5.380 396.754±12.441 –0.391 –0.022 0.167
Ross 154 M3.5e 2.9760±0.0003 3400 336.713±4.650 343.918±27.955 –0.224 –0.021 0.280

Notes. Column (1): name of Sample B objects. Col. (2): spectral type quoted from the Reylé sample. Col. (3): stellar distance from Earth quoted from the Reylé sample. Col. (4): effective temperature obtained from VOSA SED fitting. Col. (5): Observed data in the W3 band from ALLWISE. Col. (6): predicted photospheric data in the W3 band obtained from VOSA SED fitting. Col. (7): flux excess significance, χ12, in the W3 band. Col. (8): Fexcess/F12,phot at 12 μm. Col. (9): upper limit of Fexcess/F12,phot at 12 μm, taken as the larger value between 3σtot/F12,phot and 3σ. (A portion of the table is shown here for guidance regarding its form and content. The full version is available at the CDS.)

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