Gaia Data Release 3
Open Access

Table 12.

Links to the Gaia archive table to retrieve pulsation characteristics, metallicity, and absorption in the G band computed by the SOS Cep&RRL pipeline for 270 891 confirmed RR Lyrae stars (and for 888 rejected sources listed in Table 9) that are released in Gaia DR3.

Table URL https://gea.esac.esa.int/archive/
RR Lyrae main parameters computed by the SOS Cep&RRL pipeline
Table name gaiadr3.vari_rrlyrae
Source ID source_id
Type best_classification (one of RRc, RRab or RRd)
Pf, P1O p_f, p1_o
σ(Pf, P1O) pf_error, p1_o_error
E (a)(G, GBP, GRP, RV) epoch_g, epoch_bp, epoch_rp, epoch_rv
σE(G, GBP, GRP, RV) epoch_g_error, epoch_bp_error, epoch_rp_error, epoch_rv_error
G⟩,⟨GBP⟩,⟨GRP⟩, ⟨RV⟩ int_average_g, int_average_bp, int_average_rp, average_rv
σG⟩, σGBP⟩, σGRP⟩, σ⟨RV⟩ int_average_g_error, int_average_bp_error, int_average_rp_error, average_rv_error
Amp(G, GBP, GRP, RV) peak_to_peak_g, peak_to_peak_bp, peak_to_peak_rp, peak_to_peak_rv
σ[Amp(G)], σ[Amp(GBP],σ[Amp(GRP],σ[Amp(RV)] peak_to_peak_g_error, peak_to_peak_bp_error, peak_to_peak_rp_error, peak_to_peak_rv_error
ϕ21(G) phi21_g
σ[ϕ21(G)] phi21_g_error
R21(G) r21_g
σ[R21(G)] r21_g_error
ϕ31(G) phi31_g
σ[ϕ31(G)] phi31_g_error
R31 r31_g
σ[R31(G)] r31_g_error
[Fe/H] (b) metallicity
σ ([Fe/H]) metallicity_error
A(G) (c) g_absorption
σ A(G) g_absorption_error
Nobs(G band) num_clean_epochs_g
Nobs(GBP band) num_clean_epochs_bp
Nobs(GRP band) num_clean_epochs_rp
Nobs(RV) num_clean_epochs_rv

Notes. Pulsation characteristics include period(s), epochs of maximum light and minimum radial velocity (E), peak-to-peak amplitudes, intensity-averaged mean magnitudes, mean radial velocity, ϕ21, R21, ϕ31, R31 Fourier parameters with related uncertainties. To facilitate access to the table, we also provide the correspondence between parameter [period(s), E, etc.] and the name of the parameter in the Gaia archive table.

(a)

E corresponds to the time of maximum in the light curve and the time of minimum in the RV curve. The BJD of all epochs is offset by JD 2455197.5 d (= J2010.0).

(b)

Photometric metal abundance derived from the period and the ϕ31 Fourier parameter of the G light curve of RR Lyrae stars (see Sects. 5.1 and 7).

(c)

Absorption in the G band computed from a relation that links the star intrinsic colour to the period and the amplitude of the G-band light variation of fundamental-mode RR Lyrae stars (see Sects. 5.3 and 7).

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