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gaia data release 3 documentation

Gaia Data Release 3 Documentation release 1.3

Gaia Data Release 3 Documentation release 1.3

17.2 Catalogue plots 17.2.6 Astrometric correlations 17.2.8 Radial Velocity

17.2.7 Observations

Figure 17.28: HEALPix maps of the median of number of good astrometric observations AL (astrometric_n_good_obs_al) for all sources (large image), 5p (large image) and 6p (large image) solutions.

Figure 17.28: HEALPix maps of the median of number of good astrometric observations AL (astrometric_n_good_obs_al) for all sources (large image), 5p (large image) and 6p (large image) solutions.

Figure 17.29: HEALPix maps of the median of astrometric_matched_transits for all sources (large image), 5p (large image) and 6p (large image) solutions.

Figure 17.29: HEALPix maps of the median of astrometric_matched_transits for all sources (large image), 5p (large image) and 6p (large image) solutions.

Figure 17.30: Number of good astrometric observations AL (astrometric_n_good_obs_al) as a function of $G$ for all sources (large image), 5p (large image) and 6p (large image) solutions, in bins of 0.32 mag for $G$ and 5 for astrometric_n_good_obs_al.

Figure 17.30: Number of good astrometric observations AL (astrometric_n_good_obs_al) as a function of $G$ for all sources (large image), 5p (large image) and 6p (large image) solutions, in bins of 0.32 mag for $G$ and 5 for astrometric_n_good_obs_al.

Figure 17.31: Number of astrometric_matched_transits as a function of $G$ for all sources (large image), 5p (large image) and 6p (large image) solutions, in bins of 0.32 for $G$ and 1 for astrometric_matched_transits.

Figure 17.31: Number of astrometric_matched_transits as a function of $G$ for all sources (large image), 5p (large image) and 6p (large image) solutions, in bins of 0.32 for $G$ and 1 for astrometric_matched_transits.

Figure 17.32: Number of observations in $G$ magnitude (phot_g_n_obs) as a function of $G$ for all sources (large image), 5p (large image) and 6p (large image) solutions, in bins of 0.32 mag for $G$ and 5 for phot_g_n_obs.

Figure 17.32: Number of observations in $G$ magnitude (phot_g_n_obs) as a function of $G$ for all sources (large image), 5p (large image) and 6p (large image) solutions, in bins of 0.32 mag for $G$ and 5 for phot_g_n_obs.

Figure 17.33: Number of observations in $G_{\rm BP}$ magnitude (phot_bp_n_obs) as a function of $G$ for all sources (large image), 5p (large image) and 6p (large image) solutions, in bins of 0.32 mag for $G$ and 1 for phot_bp_n_obs.

Figure 17.33: Number of observations in $G_{\rm BP}$ magnitude (phot_bp_n_obs) as a function of $G$ for all sources (large image), 5p (large image) and 6p (large image) solutions, in bins of 0.32 mag for $G$ and 1 for phot_bp_n_obs.

Figure 17.34: Number of observations in $G_{\rm RP}$ magnitude (phot_rp_n_obs) as a function of $G$ for all sources (large image), 5p (large image) and 6p (large image) solutions, in bins of 0.32 mag for $G$ and 1 for phot_rp_n_obs.

Figure 17.34: Number of observations in $G_{\rm RP}$ magnitude (phot_rp_n_obs) as a function of $G$ for all sources (large image), 5p (large image) and 6p (large image) solutions, in bins of 0.32 mag for $G$ and 1 for phot_rp_n_obs.

Figure 17.35: Number of RVS transits (rv_nb_transits) as a function of $G$ for all sources (large image), 5p (large image) and 6p (large image) solutions, in bins of 0.32 mag for $G$ and 1 for rv_nb_transits.

Figure 17.35: Number of RVS transits (rv_nb_transits) as a function of $G$ for all sources (large image), 5p (large image) and 6p (large image) solutions, in bins of 0.32 mag for $G$ and 1 for rv_nb_transits.

17.2.6 Astrometric correlations Bibliography 17.2.8 Radial Velocity

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