Table D.1
Column names and description of the entries of the main results table.
| Column name | Description |
|---|---|
| Name | eROSITA source name |
| ID_SRC | Source ID of detection pipeline |
| RA_CORR | RA of the X-ray center |
| DEC_CORR | DEC of the X-ray center |
| EXT | Source extent in X-ray |
| EXT_ERR | Error in source extent |
| EXT_LIKE | Extent likelihood |
| DET_LIKE_0 | Detection likelihood |
| ML_RATE_0 | X-ray count rate |
| ML_RATE_ERR_0 | error on count rate |
| F_CONT_BEST_COMB | fcont of best optical counter part: −1, −2 for manually added systems |
| Z_BEST_COMB | Photometric redshift of best counter part |
| SIGMA_Z_BEST_COMB | Uncertainty of the photometric redshift |
| LAMBDA_BEST_COMB | Richness of best counter part |
| ELAMBDA_BEST_COMB | Uncertainty richness |
| SURV_BEST_COMB | Survey used: −1 group catalog, 1 LS, 2 HSC |
| RA_OPTCEN_BEST_COMB | Ra of optical center of best counter part |
| DEC_OPTCEN_BEST_COMB | Same but DEC |
| SPEC_Z_BEST_COMB | Spec-z |
| N_SPEC | Number of redshifts used for spec-z |
| MASSPROX_BEST_COMB | Approx. M500 used for richness estimate [1/h] |
| FLAG_OPTICAL_X_POS | Value of the optical footprint map at X-ray position |
| MASKFRAC_3_FOOT | Fraction of the area not int the optical footprint within a 3 arcmin radiuss |
| MASKFRAC_3_FLAGGED | Similar but including flagged area due to bright star masks |
| MASKFRAC_R500_FOOT_BEST_COMB | Same as MASKFRAC_3_FOOT but for a r_500 sized region |
| MASKFRAC_R500_FLAGGED_BEST_COMB | Same as MASKFRAC_3_FLAGGED but for a r_500 sized region |
| ALPHA | Dynamical state estimator alpha |
| BETA | Dynamical state estimator beta |
| DELTA | Dynamical state estimator delta |
| ELLIP | Dynamical state estimator: model ellipticity |
| CENTERSHIFT | Shift of the centre of the 2D density model with respect to X-ray position |
| DIST_NEXT_OPT | Distance to next optical structure in the galaxy density map |
| DIST_NEXT_XCLUST | Distance to next extent-selected eFEDS cluster |
| MCMF_NWAY_SECTOR | Sector in fcont- pany plane according to Sect. 5.4 |
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