Variable stars: Long period variable (gaiafpr.vari_long_period_variable)
The table has 9614 rows, 11 columns.
Description
This table describes the Long Period Variable stars.Some entries can be NaN when absent.
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.
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Columns
| Name | Type | UCD | Unit | Description |
|---|---|---|---|---|
| solution_id | long | meta.version |
Solution Identifier |
|
| source_id | long |
meta.id meta.main |
Unique source identifier |
|
| frequency | double | src.var.pulse | d**-1 |
Frequency from G FoV time series |
| frequency_error | float |
stat.error src.var.pulse |
d**-1 |
Uncertainty on the frequency from G FoV time series |
| amplitude | float | src.var.amplitude | mag |
Variability amplitude based on the best-fit model to the G FoV time series |
| median_delta_wl_rp | float |
em.wl stat.median |
Median of the pseudo-wavelength separations between the two highest peaks in RP spectra |
|
| is_cstar | boolean | meta.code.class |
Flag to mark C-stars |
|
| frequency_rv | double | src.var.pulse | d**-1 |
Frequency from radial velocity time series |
| frequency_rv_error | float |
stat.error src.var.pulse |
d**-1 |
Uncertainty on the frequency from radial velocity time series |
| amplitude_rv | float | src.var.amplitude | km.s**-1 |
Variability amplitude based on the best-fit model to the radial velocity time series |
| flag_rv | boolean | meta.code.qual |
Flag identifying a top-quality subsample |