gdr3spec Webivo://org.gavo.dc/gaia/s3/webdoi:10.21938/W:hWbPah3wBabuqewQULTAThe GAVO DC teamDemleitner, M.Andrae, R.2022-11-07T08:46:33ZGAVO Data Centre Team

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gavo@ari.uni-heidelberg.de+49 6221 54 1837starssurveysspectroscopy This is a re-publication the Gaia DR3 RP/BP spectra in the IVOA Spectral Data Model. It presents the continous spectra in sampled form, using a Monte Carlo scheme to decorrelate errors, elaborated in this resource's reference URL. The underlying tables are also available for querying through TAP, which opens some powerful methods for mass-analysing the data.2022arXiv220800211Ghttps://dc.g-vo.org/gaia/s3/web/info This data is derived from public Gaia DR3 data. Please take note of `ESAC's guide`_ on how to acknowledge and cite Gaia results. .. _ESAC's guide: https://gea.esac.esa.int/archive/documentation/GDR3/Miscellaneous/sec_credit_and_citation_instructions/GaiaGaia BP/BP Spectrometer0/0-1156863 579011.986e-19 4.966e-19https://dc.g-vo.org/gaia/s3/web/coverageOpticalgdr3spec This is a re-publication the Gaia DR3 RP/BP spectra in the IVOA Spectral Data Model. It presents the continous spectra in sampled form, using a Monte Carlo scheme to decorrelate errors, elaborated in this resource's reference URL. The underlying tables are also available for querying through TAP, which opens some powerful methods for mass-analysing the data.output This is a re-publication the Gaia DR3 RP/BP spectra in the IVOA Spectral Data Model. It presents the continous spectra in sampled form, using a Monte Carlo scheme to decorrelate errors, elaborated in this resource's reference URL. The underlying tables are also available for querying through TAP, which opens some powerful methods for mass-analysing the data.spectrumMerged BP/RP spectrum from Gaia DR3, using a local Monte Carlo technique for conversion from the upstream continuous formfloatnullablelocation_radegpos.eq.ra;meta.mainssa:Char.SpatialAxis.Coverage.Location.Value.C1floatnullablelocation_decdegpos.eq.dec;meta.mainssa:Char.SpatialAxis.Coverage.Location.Value.C2floatnullablephot_g_mean_magMean magnitude in the G band. This is computed from the G-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_g_mean_flux_over_error.magphot.mag;em.opt;stat.mean1.7732815.506819.722921.033322.75070.996994floatnullablephot_bp_mean_magMean magnitude in the integrated BP band. This is computed from the BP-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_bp_mean_flux_over_error.magphot.mag;em.opt.B2.39815.891120.294321.856525.31610.851071floatnullablephot_rp_mean_magMean magnitude in the integrated RP band. This is computed from the RP-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_rp_mean_flux_over_error.magphot.mag;em.opt.R1.9687414.540418.604320.259924.64070.85822floatnullablesource_idGaia DR3 unique source identifier. Note that this *cannot* be matched against the DR1 or DR2 source_ids.meta.id;meta.main15118286476804.59792466834312e+174.280400489214347e+186.707472532802898e+1869175289932832044801.0longnullableraBarycentric Right Ascension in ICRS at epoch J2016.0degpos.eq.ra;meta.main1.63271e-0644.3559260.257327.9323601doublenullabledecBarycentric Declination in ICRS at epoch J2016.0degpos.eq.dec;meta.main-89.8559-69.306-25.65858.828789.80891doublenullable