Catalogues containing photometry in 22 passbands for 603311 LMC stars and 124578 SMC stars from Bellazzini & Pascale 2024, A&A,

<p>Catalogues from the paper "The RGB Tip in the SDSS, PS1, JWST, NGRST and Euclid photometric systems. Calibration in optical passbands using Gaia DR3 synthetic photometry" by M. Bellazzini (INAF - OAS Bo) &amp; R. Pascale (INAF - OAS Bo), A&amp;A, in press, (<a href="https://arxiv.org/abs/2406.04781" target="_blank" rel="noopener">arXiv:2406.04781</a>). &nbsp;Stars have been selected from the Gaia DR3 dataset and the magnitudes has been obtained from the Gaia GSPC catalogue of from GaiaXPy as described in Gaia Collaboration 2023.</p> <div>Each catalogue contains:</div> <div>&nbsp;</div> <div> <ul> <li>Column 1-15, parameters directly extracted from the Gaia DR3 source catalogue, namely: source_id, ra, dec, parallax, parallax_error, pmra, pmra_error, pmdec, pmdec_error, ruwe, phot_variable_flag, and non_single_star.</li> <li>Column 16: C⋆, a parameter that is derived from phot_bp_rp_excess_factor (that, in turn, has been extracted from the Gaia DR3 source catalogue) following (Riello et al. 2021).</li> <li>Column 17: colour excess E(B-V), derived from Skowronet al. (2021) and Schlegel et al. (1998); Schlafly &amp; Finkbeiner (2011) as described in Sect. 2.</li> <li>Columns 18-27: standardised ugriz magnitudes in the SDSS system extracted from the Gaia DR3 GSPC (Gaia Collaboration et al. 2023a) and associated uncertainties.</li> <li>Columns 28-37: standardised UBVRI magnitudes in the JKCsystem extracted from the Gaia DR3 GSPC (Gaia Collaboration et al. 2023a) and associated uncertainties.</li> <li>Columns 38-47: standardised grizy magnitudes in the PS1 system computed with GaiaXPy and associated uncertainties.</li> <li>Columns 48-51: standardised F606W, F814W magnitudes in the HST ACS-WFC system extracted from the Gaia DR3 GSPC (Gaia Collaboration et al. 2023a) and associated uncertainties.</li> <li>Columns 52-55: non-standardised F070W and F090W magnitudes in the JWST-NIRCAM system computed with GaiaXPy and associated uncertainties.</li> <li>Columns 56-59: non-standardised R062 and Z087 magnitudes in the NGRST system computed with GaiaXPy and associated uncertainties .</li> <li>Columns 60-61: non-standardised I_E magnitude in the Euclid-VIS system computed with GaiaXPy and associated uncer-tainties (in this case, not corrected for the bias described in Sect. 2.1 of Gaia Collaboration et al. 2023a, hence slightly underestimated).</li> </ul> <p><strong>It is very important to remind </strong>that u_SDSS and U_JKC magnitudes from Gaia XPSP are significantly less accurate and pre-<br>cise than all the other magnitudes included in our catalogues (see Gaia Collaboration et al. 2023a, for detailed discussion).<br>Each star can lack some of the 22 magnitudes listed in the catalogues, depending on the signal-to-noise constraints applied to the original GSPC (S/N&gt; 30 Gaia Collaboration et al. 2023a). For example, of the 603311 stars listed in the LMC sample only 83229(85338) have valid u_SDSS (U_JKC ) magnitudes. See Bellazzini &amp; Pascale 2024 for further details and references.</p> </div> <p><strong>We cannot give any hint or guarantee on the behaviour of the completeness of the samples</strong> as a function of the various magnitudes and colours, as well as as a function of position in the sky (see Bellazzini &amp; Pascale 2024 for details on the selections applied).</p>