E-tables for the manuscript "A Multi-band Photometric Selection of Period Bouncer Candidates in the Solar Neighborhood with Gaia, Galex, WISE, eROSITA and XMM-Newton Data"

430_BC1_finaltable_v5.csv is table 2, and table3.csv is table 3 in the manuscript. Notes on 430_BC1_finaltable_v5.csv: This is the table summarizing the sources within 500pc that shares similar GALEX FUV and WISE W1 absolute magnitudes with confirmed bouncers. Source marked with * or #: Confirmed bouncers or candidates from Mun ̃oz-Giraldo et al. (2024).Gaia3 ID: Gaia DR3 source ID. RA & Dec: Source coordinates. Bp − Rp: Gaia DR3 GBP − GRP color. MG: Absolute Gaia DR3 G-band magnitude. MW1: Absolute WISE W1 band magnitude. mg − mFUV: Gaia G−Galex FUV color. MFUV: Absolute Galex FUV magnitude. Porb: Orbital period (if available) in minutes. TWD: WD effective temperature from SED fitting. Tc: Companion effective temperature from SED fitting. Notes on table3.csv: This is the table summarizing the sources in 430_BC1_finaltable_v5.csv that were detected by eROSITA-eRASS1 DE or 4XMM DR14. Source marked with *: Sources included by (Mun ̃oz-Giraldo et al. 2024) as confirmed bouncers so that their likelihood to be bouncers are not discussed. Source marked with #: Sources classified as WDs in the Simbad.Simbad ID: Simbad source ID. FX: X-ray flux in units of 10−13erg s−1cm−2 (0.2-2.3 keV for BC2, 0.2-12 keV for BC1-XMM sources). LX: X-ray luminosity in units of 1030erg s−1 (0.2-2.3 keV for BC2, 0.2-12 keV for BC1-XMM sources). TWD & Tc: WD and companion temperatures in K from SED fitting, respectively. S Type: Scores assigned to the source according to its companion type, the non-zero value within parentheses are calculated assuming the companion type by the SED fitted temperatures. S m, S p, S Twd, S Gv, S Gc, S SDSS, S UV, S IR, & S E: Scores assigned to the source according to its companion mass, orbital period, WD temperature, Gaia variance, Gaia color, SDSS color, UV color, IR color and IR excess (Mun ̃oz-Giraldo et al. 2024). S t and %: total score and final score, where Final% = St/36 × 100. Ref: Referenced articles, 1: Ritter & Kolb (2003); 2: Inight et al. (2023); 3: Abril et al. (2020); 4: Gentile Fusillo et al. (2021); 5: Rodriguez et al. (2025).