Open Access
Table 1.
An example of entry to the GOSXMM catalog and column descriptions.
| Column Name | Explanation | ||
|---|---|---|---|
| GOSS | 006.01–01.20_01 | Name in the GOSS catalogue | |
| NAME | 9 Sgr | Alternative name | |
| XMM-NAME | 3XMM J180352.4–242138 | 3XMM Name as in DR7 | |
| GaiaDR2_source_id | 4066022591147527552 | Gaia source identifier, identical to the Gaia-DR2 source_id. | |
| RA | 18 03 52.446 | RAJ2000 | |
| Dec | −24 21 38.64 | DecJ2000 | |
| MV | (mag) | −5.5 | Absolute magnitude from Martins et al. (2005a) |
| error_MV | (mag) | 0.29 | Absolute magnitude error |
| Mbol | (mag) | −9.41 | Bolometric magnitude from Martins et al. (2005a) |
| e_Mbol | (mag) | 0.43 | Bolometric magnitude error |
| Teff | (K) | 43 000 | Effective temperature from Martins et al. (2005a) |
| e_Teff | (K) | 2000 | Effective temperature error |
| logg | 3.92 | Effective gravity from Martins et al. (2005a) | |
| e_logg | 0.1 | Effective gravity error | |
| logLbol, S | (erg s−1) | 5.66 | Bolometric luminosity derived from spectrophotometric distance |
| v∞ | (km s−1) | 2750 | Terminal wind velocity from Prinja et al. (1990) |
| log ṀVink | (M⊙ yr−1) | −5.62 | Mass-loss rate from the Vink et al. (2000) recipe |
| log Ṁ | (M⊙ yr−1) | −6.32 | Mass-loss rate from this work |
| distance_Gaia | (kpc) | 1.2 | Parallactic distance from Bailer-Jones et al. (2018) |
| min_distance_Gaia | (kpc) | 1.1 | Minimum parallactic distance from Bailer-Jones et al. (2018) |
| max_distance_Gaia | (kpc) | 1.3 | Maximum parallactic distance from Bailer-Jones et al. (2018) |
| distance_MV | (kpc) | 1.4 | Spectrophotometric distance |
| error_distance_MV | (kpc) | 0.1 | Error on the spectrophotometric distance |
| B | (mag) | 5.94 | B magnitude |
| e_B | (mag) | 0.01 | B magnitude error |
| V | (mag) | 5.96 | V magnitude |
| e_V | (mag) | 0.01 | V magnitude error |
| EB − V | (mag) | 0.26 | Color excess |
| e_EB − V | (mag) | 0.02 | Color excess error |
| AV | (mag) | 0.81 | Extinction in the V band |
| e_AV | (mag) | 0.08 | Error in the extinction in the V band |
| NH | (cm−2) | 1.5E21 | Hydrogen column density |
| PN count_rate | (s−1) | 1.284 | PN Count rate (0.2–12 keV) |
| error_count_rate | (s−1) | 0.017 | PN Count rate error (0.2–12 keV) |
| fX | (erg s−1 cm−2) | 4.4E−12 | Unabsorbed X-ray flux (0.2–12 keV) |
| fX, min | (erg s−1 cm−2) | 4.3E−12 | Minimum X-ray flux (0.2–12 keV) |
| fX, max | (erg s−1 cm−2) | 4.4E−12 | Maximum X-ray flux (0.2–12 keV) |
| log(fbol) | (erg s−1 cm−2) | −5.098 | Bolometric flux |
| e_log(fbol) | (erg s−1 cm−2) | 0.032 | Bolometric flux error |
| log(fX/fbol) | −6.26 | X-ray to bolometric flux ratio | |
| min_log(fX/fbol) | −6.30 | Minimum X-ray to bolometric flux ratio | |
| max_log(fX/fbol) | −6.22 | Maximum X-ray to bolometric flux ratio | |
| logLX | (erg s−1) | 32.84 | X-ray luminosity (0.2–12 keV) |
| logLX, min | (erg s−1) | 32.74 | minimum X-ray luminosity (0.2–12 keV) |
| logLX, max | (erg s−1) | 32.95 | maximum X-ray luminosity (0.2–12 keV) |
| logLbol, P | (erg s−1) | 39.10 | Bolometric luminosity derived from parallactic distance |
| min_logLbol, P | (erg s−1) | 38.98 | Minimum bolometric luminosity |
| max_logLbol, P | (erg s−1) | 39.24 | Maximum bolometric luminosity |
| HR2 | −0.493 | Hardness ratio HR2 | |
| error_HR2 | 0.013 | Error on the hardness ratio HR2 | |
| HR3 | −0.814 | Hardness ratio HR3 | |
| error_HR3 | 0.017 | Error on the hardness ratio HR3 |
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