Bolometric luminosities and radii in solar units for a subset of ultracool dwarfs (gaiadr3.gold_sample_ucd)
The table has 21062 rows, 7 columns.
Description
The table contains the bolometric luminosities and radii in solar units for a subset of ultracool dwarfs from the Gaia DR3 catalogue, as well as some intermediate quantities used in the selection of sources and in the derivation of the luminosities and radii. For more details please refer to DR3-DPACP-123.
Attribution
If you have used Gaia data in your research, please use the following acknowledgement:
This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement.
More information can be found on the credit and citation instructions page.
Columns
Name | Type | UCD | Unit | Description |
---|---|---|---|---|
source_id | long |
meta.id meta.main meta.ref |
Unique source identifier (unique within a particular Data Release) |
|
ftot_fobs | float | arith.factor |
Correction factor applied to obtain the total SED flux |
|
lum | float | phys.luminosity | solLum |
Bolometric luminosity in solar units |
lum_uncertainty | float |
stat.error phys.luminosity |
solLum |
Uncertainty in bolometric luminosity |
radius | float | phys.size.radius | solRad |
Radius in solar unit |
radius_uncertainty | float |
stat.error phys.size.radius |
solRad |
Uncertainty in radius |
reduced_chi2 | float | stat.fit.chi2 |
Reduced chi-square of the SED fit |