Open Access
Table 2
ESMORGA catalogue content, column by column.
| 1. Gaia DR3 source identifier, gaia_id. |
| 2. Solution type: Orbital, Orbital*3 and Orbital**4 for astrometric orbits, and AstroSpectroSB1 for astrospectroscopic solutions. |
| 3. Right Ascensión for J2016.0, RA (°). |
| 4. Declination for J2016.0, Dec (°). |
5. Parallax,  to (mas). |
| 6. Apparent combined magnitude in the G-band, mG (mag). |
| 7. Absolute combined magnitude in the G-band, MG (mag). |
| 8. Magnitude difference, ∆mG (mag). |
| 9. Primary absolute magnitude in the G-band, MG, A (mag). |
| 10. Secondary absolute magnitude in the G-band, MG, B (mag). |
| 11. Mass of the primary, ℳA (ℳ⊙). |
| 12. Mass of the secondary, ℳA (ℳ⊙). |
| 13. Effective temperature of the primary, interpolated by cubic splines from Pecaut & Mamajek (2013), TeffA (K). |
| 14. Effective temperature of the secondary, interpolated by cubic splines from Pecaut & Mamajek (2013), Teffb (K). |
| 15. Period, P (yr). |
| 16. Time of periastron, T (Fractional decimal year). |
| 17. Eccentricity, e. |
| 18. Semi-major axis, a″ (″). |
| 19. Inclination, I (°). |
| 20. Longitude of the node, Ω (°). |
| 21. Argument of the periastron, ω (°). |
22. Maximum angular separation of the apparent orbit,  |
23. Date of  (Fractional decimal year). |
24. Minimum angular separation of the apparent orbit,  . |
25. Date of  (Fractional decimal year). |
26. Degree of consonance between algorithmic (ℳA, ℳ⊙.) and Gaia  masses, grade, expressed as the grades defined in Sect. 2.3. An asterisk * is added next to the grade if the binary mass function test in Eq. (8) is also passed. |
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