Properties derived from photometric measurements and parallaxes of the stars. The second column contains effective temperatures derived from all available standardized photometry. The third column temperatures are based on photometry exluding SkyMapper u and v. For comparison, temperatures in the fourth column are those expected from the MS spectral types (Pecaut & Mamajek 2013). Errors on Mbol are given in brackets. Bolometric magnitudes in column 6 are given for comparison: these are for main sequence dwarfs of the same spectral types.4 The last column shows the maximum number of photometric filters taken into account.
| Name . | Teff, 1 . | Teff, 2 . | Sp. Teff . | Mbol . | Dwarf Mbol . | n . |
|---|---|---|---|---|---|---|
| . | (K) . | (K) . | . | (mag) . | (mag) . | . |
| CD-36 3202 | 4900 | 4820 | 4760 | 5.94(0.02) | 5.02 | 20 |
| CD-49 1902 | 5430 | 5310 | 5290 | 5.07(0.02) | 5.88 | 16 |
| CD-56 1438 | 5190 | 5070 | 5030 | 4.81(0.04) | 5.54 | 20 |
| CD-66 395 | 5470 | 5310 | 5030 | 4.99(0.02) | 5.54 | 19 |
| CD-72 248 | 5040 | 4870 | 5030 | 4.84(0.03) | 5.54 | 18 |
| Name . | Teff, 1 . | Teff, 2 . | Sp. Teff . | Mbol . | Dwarf Mbol . | n . |
|---|---|---|---|---|---|---|
| . | (K) . | (K) . | . | (mag) . | (mag) . | . |
| CD-36 3202 | 4900 | 4820 | 4760 | 5.94(0.02) | 5.02 | 20 |
| CD-49 1902 | 5430 | 5310 | 5290 | 5.07(0.02) | 5.88 | 16 |
| CD-56 1438 | 5190 | 5070 | 5030 | 4.81(0.04) | 5.54 | 20 |
| CD-66 395 | 5470 | 5310 | 5030 | 4.99(0.02) | 5.54 | 19 |
| CD-72 248 | 5040 | 4870 | 5030 | 4.84(0.03) | 5.54 | 18 |
Properties derived from photometric measurements and parallaxes of the stars. The second column contains effective temperatures derived from all available standardized photometry. The third column temperatures are based on photometry exluding SkyMapper u and v. For comparison, temperatures in the fourth column are those expected from the MS spectral types (Pecaut & Mamajek 2013). Errors on Mbol are given in brackets. Bolometric magnitudes in column 6 are given for comparison: these are for main sequence dwarfs of the same spectral types.4 The last column shows the maximum number of photometric filters taken into account.
| Name . | Teff, 1 . | Teff, 2 . | Sp. Teff . | Mbol . | Dwarf Mbol . | n . |
|---|---|---|---|---|---|---|
| . | (K) . | (K) . | . | (mag) . | (mag) . | . |
| CD-36 3202 | 4900 | 4820 | 4760 | 5.94(0.02) | 5.02 | 20 |
| CD-49 1902 | 5430 | 5310 | 5290 | 5.07(0.02) | 5.88 | 16 |
| CD-56 1438 | 5190 | 5070 | 5030 | 4.81(0.04) | 5.54 | 20 |
| CD-66 395 | 5470 | 5310 | 5030 | 4.99(0.02) | 5.54 | 19 |
| CD-72 248 | 5040 | 4870 | 5030 | 4.84(0.03) | 5.54 | 18 |
| Name . | Teff, 1 . | Teff, 2 . | Sp. Teff . | Mbol . | Dwarf Mbol . | n . |
|---|---|---|---|---|---|---|
| . | (K) . | (K) . | . | (mag) . | (mag) . | . |
| CD-36 3202 | 4900 | 4820 | 4760 | 5.94(0.02) | 5.02 | 20 |
| CD-49 1902 | 5430 | 5310 | 5290 | 5.07(0.02) | 5.88 | 16 |
| CD-56 1438 | 5190 | 5070 | 5030 | 4.81(0.04) | 5.54 | 20 |
| CD-66 395 | 5470 | 5310 | 5030 | 4.99(0.02) | 5.54 | 19 |
| CD-72 248 | 5040 | 4870 | 5030 | 4.84(0.03) | 5.54 | 18 |
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