gaia.dr2epochfluivo://org.gavo.dc/gaia/q2/dr2epochfluxThe GAVO DC teamGAIA Collaboration2022-01-26T13:38:59Z2018-12-05GAVO Data Centre Team

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gavo@ari.uni-heidelberg.de+49 6221 54 1837starssurveysastrometryproper-motionstime-domain-astronomy A table of the light curves released with Gaia DR2 (about half a million in total). In each Gaia band (G, BP, RP), we give epochs, fluxes and their errors in arrays. We do not include the quality flags (DR2: “may be safely ignored for many general purpose applications”). You can access them through the associated datalink service if you select source_id. You will usually join this table with gaia.dr2light. We have also removed all entries with NaN observation times; hence, the array lengths in the different bands can be significantly different, and the indices in transit_ids do not always correspond to the indices in the time series. Furthermore, we only give fluxes and their errors here rather than magnitudes. Fluxes can be turned into magnitude using:: mag = -2.5 log10(flux)+zero point, where the zero points assumed for Gaia DR2 are 25.6884±0.0018 in G, 25.3514±0.0014 in BP, and 24.7619±0.0019 in RP (VEGAMAG).http://dc.g-vo.org/tableinfo/gaia.dr2epochfluxIsServedByGAVO Data Center TAP servicehttp://dc.g-vo.org/taphttps://dc.g-vo.org/tapGaia0/0-1157174 571741.986e-19 4.966e-19Opticalgaia This schema contains data re-published from the official Gaia mirrors (such as ivo://uni-heidelberg.de/gaia/tap) either to support combining its data with local tables (the various Xlite tables) or to make the data more accessible to VO clients (e.g., epoch fluxes). Other Gaia-related data is found in, among others, the gdr2dist, gdr3mock, gdr3spec, gedr3auto, gedr3dist, gedr3mock, and gedr3spur schemas.gaia.dr2epochflux A table of the light curves released with Gaia DR2 (about half a million in total). In each Gaia band (G, BP, RP), we give epochs, fluxes and their errors in arrays. We do not include the quality flags (DR2: “may be safely ignored for many general purpose applications”). You can access them through the associated datalink service if you select source_id. You will usually join this table with gaia.dr2light. We have also removed all entries with NaN observation times; hence, the array lengths in the different bands can be significantly different, and the indices in transit_ids do not always correspond to the indices in the time series. Furthermore, we only give fluxes and their errors here rather than magnitudes. Fluxes can be turned into magnitude using:: mag = -2.5 log10(flux)+zero point, where the zero points assumed for Gaia DR2 are 25.6884±0.0018 in G, 25.3514±0.0014 in BP, and 24.7619±0.0019 in RP (VEGAMAG).550737source_idUnique source identifier. Note that this *cannot* be matched against the DR1 source_id.meta.id;meta.mainlongindexedprimarytransit_idTransit unique identifier. For a given object, a transit comprises the different Gaia observations (SM, AF, BP, RP and RVS) obtained for each focal plane crossing. NOTE: Where invalid observations have been removed, transit_id *cannot* be joined with times and fluxes.meta.versionlongnullableg_transit_timeThe field-of-view transit averaged observation times for the G-band observations. This is given for barycentric TCB in JD-2,455,197.5.dtime.epochdoublenullableg_transit_fluxG-band fluxes for the transit, for combination with g_transit_time_mjd. Here, this is a combination of individual SM-AF CCD fluxess**-1phot.flux;em.opt.Vfloatnullableg_transit_flux_errorThe error in G-band flux.s**-1stat.error;phot.flux;em.opt.Vfloatnullablerp_obs_timeThe observation time of the RP CCD transit. This is given for barycentric TCB in JD-2,455,197.5.dtime.epochdoublenullablerp_fluxRP-band integrated fluxes, for combination with rp_obs_times**-1phot.flux;em.opt.Rfloatnullablerp_flux_errorThe error in RP-band flux.s**-1stat.error;phot.flux;em.opt.Rfloatnullablebp_obs_timeThe observation time of the BP CCD transit. This is given for barycentric TCB in JD-2,455,197.5.dtime.epochdoublenullablebp_fluxBP-band integrated fluxes, for combination with bp_obs_times**-1phot.flux;em.opt.Bfloatnullablebp_flux_errorThe error in BP-band flux.s**-1stat.error;phot.flux;em.opt.Bfloatnullablesolution_idA DPAC id for the toolchain used to produce these particular time series. It is given to facilitate comparison with ESAC data products.meta.versionlonggaia.dr2lightsource_idsource_id