Open Access
Table F.1.
Content of the samples of this work, with the example of Proxima Centauri.
| Column name | Unit | Description | Example |
|---|---|---|---|
| CNS5_id | designation in CNS5 | 3591 | |
| gj_id | Gliese-Jahreiß number | 551 | |
| other_name | name of stars that do not have CNS5_id and gj_id | ||
| component_id | component in a multiple system | C | |
| RA | deg | right ascension (Gaia DR3) | 217.392321472009 |
| DEC | deg | declination (Gaia DR3) | -62.6760751167667 |
| GAIA_peculiar_color | flag for stars with peculiar Gaia colors | 0 | |
| SpT | SpT | M5.5 | |
| r_SpT | reference of SpT | 1995AJ....110.1838R | |
| Gaia_SpT | SpT according to MG which is different from literature SpT | ||
| distance | pc | Gaia DR3 distance to the Sun | 1.30 |
| Lx_eROSITA | erg s−1 | X-ray luminosity according to eROSITA | 6.86E+026 |
| Lx_eROSITA_uerr | erg s−1 | upper error of Lx_eROSITA | 3.09E+025 |
| Lx_eROSITA_lerr | erg s−1 | lower error of Lx_eROSITA | 3.02E+025 |
| eROSITA_upp_lim | flag for Lx_eROSITA as upper limit value | 0 | |
| Eband_Lx_eROSITA | keV | energy band of Lx_eROSITA and its errors | 0.2-2.3 |
| r_Lx_eROSITA | reference of Lx_eROSITA and its errors | eRASS1 | |
| Lx_ROSAT | erg s−1 | X-ray luminosity according to ROSAT | 6.58E+026 |
| Lx_ROSAT_uerr | erg s−1 | upper error of Lx_ROSAT | 6.91E+024 |
| Lx_ROSAT_lerr | erg s−1 | lower error of Lx_ROSAT | 6.91E+024 |
| eROSAT_upp_lim | flag for Lx_ROSAT as upper limit value | 0 | |
| Eband_Lx_ROSAT | keV | energy band of Lx_ROSAT and its errors | 0.1-2.4 |
| instrument_Lx_ROSAT | camera of ROSAT useda | PSPC | |
| r_Lx_ROSAT | reference of Lx_ROSAT and its errors | NEXXUS | |
| Lx_other | erg s−1 | X-ray luminosity according to other telescopes (Chandra or XMM-Newton) | 6.49E+026 |
| Lx_other_uerr | erg s−1 | upper error of Lx_other | |
| Lx_other_lerr | erg s−1 | lower error of Lx_other | |
| Lx_other_upp_lim | flag for Lx_other as upper limit value | 0 | |
| Eband_Lx_other | keV | energy band of Lx_other and its errors | 0.2-10 |
| instrument_Lx_other | camera of other telescopes used | EPIC | |
| r_Lx_other | reference of Lx_other and its errors | 2011A&A...534A.133F | |
| Lx_final | erg s−1 | X-ray luminosity used in the analysis, converted to ROSAT energy band | 8.32E+026 |
| Lx_final_uerr | erg s−1 | upper error of Lx_final | |
| Lx_final_lerr | erg s−1 | lower error of Lx_final | |
| Lx_final_upp_lim | flag for Lx_final as upper limit value | 0 | |
| L_bol | erg s−1 | bolometric luminosity | 5.83E+030 |
| r_L_bol | reference of L_bol | GAIAb | |
| Lx/L_bol | LX/Lbol used in the final analysis | 1.43E−04 | |
| Lx/L_bol_uerr | upper error of Lx/L_bol | ||
| Lx/L_bol_lerr | lower error of Lx/L_bol |
aROSAT all-sky survey also used PSPC, and we distinguish between RASS (survey) and PSPC (pointed observation). bThe references are the Gaia parameter catalog (GAIA), Lbol calculated with the Gaia BC routine (GAIA_EEM) and the Mamajek table (EEM).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.