Table B.1
Columns of the mock input and output eFEDS catalogs
| Name | Description |
|---|---|
| For both input AGN and clusters | |
| SRC_ID | Source ID; always < 5 × 106 for AGN; always > 107 for clusters |
| RA | Right ascension (deg) |
| DEC | Declination (deg) |
| Z | redshift (in redshift space) |
| dL | luminosity distance (cm) in the cosmology adopted by Comparat et al. (2019, 2020) to create the mock catalogs |
| ID_Uniq | source ID in single-band catalog whose ID_Uniq is this source |
| ID_Any | source ID in single-band catalog whose ID_Any is this source |
| ID_Any2 | source ID in single-band catalog whose ID_Any2 is this source |
| ID_contam | ID of contaminating input source |
| ID_Uniq_T | source ID in three-band catalog whose ID_Uniq is this source |
| ID_Any_T | source ID in three-band catalog whose ID_Any is this source |
| ID_Any2_T | source ID in three-band catalog whose ID_Any2 is this source |
| Nreal | number of realization (1–18) |
| For input AGN only, see Comparat et al. (2019) for more details | |
| logNH | AGN column density (cm−2) |
| FLUX | 0.5−2 keV observed flux (erg cm−2 s−1); the input flux in simulation |
| FLUX_GalCorr | 0.5−2 keV flux corrected for Galactic absorption (erg cm−2 s−1) |
| Lx_hard | 2−10 keV intrinsic luminosity (erg/s) |
| agn_type | AGN type |
| galaxy_SMHMR_mass | Host galaxy stellar mass (M⊙) |
| For input cluster only, see Comparat et al. (2020) for more details | |
| kT | cluster tempeature (keV) |
| Lx_soft | rest-frame 0.5–2 keV luminosity within R500c (erg/s) |
| Lx_soft_2R500 | rest-frame 0.5–2 keV luminosity within twice R500c (erg/s) |
| Fx_soft | observed 0.5–2 keV flux within R500c |
| Fx_soft_2R500 | observed 0.5–2 keV flux within twice R500c; the input flux in simulation |
| M500c | halo mass within R500c (M⊙) |
| R500c_arcmin | apparent radius where the mass density is 500 times the universe critical density (arcmin) |
| R500c_kpc | physical radius where the mass density is 500 times the universe critical density (kpc, proper distance) |
| Pid | flag; a value of -1 means the halo is a distinct halo |
| Mvir | halo mass within the virial radius (M⊙) |
| Rvir | halo virial radius (kpc) |
| Xoff | halo offset parameter (kpc) |
| b_to_a_500c | halo ellipticity |
| Single-band and three-band detected output catalogs | |
| ID_SRC | source ID |
| RA | Right ascension (deg) |
| DEC | Declination (deg) |
| RADEC_ERR | combined positional error (arcsec) |
| EXT | source extent (arcsec) |
| EXT_ERR | extent error (arcsec) |
| EXT_LIKE | extent likelihood measured by PSF-fitting |
| ML_RATE_n | source count rate (cts/s) |
| ML_RATE_ERR_n | count rate error (cts/s) |
| DET_LIKE_n | detection likelihood measured by PSF-fitting |
| ML_BKG_n | background at source position (cts/arcmin2) |
| ML_EXP_n | vignetted exposure (s) at source position |
| ID_Uniq | ID of the unique input counterpart |
| ID_Any | ID of the brightest input counterpart, allowing duplicate |
| ID_Any2 | ID of the secondary input counterpart |
| ID_contam | ID of the input source contaminating the unique input counterpart |
| Nreal | number of realization (1–18) |
Notes. The input AGN and clusters catalogs have some columns in common. They are listed in the first section. Some exclusive columns are listed in the second and third sections. The output single-band-detected and three-band-detected catalogs share basically the same columns, except for a few columns from PSF fitting with an optional suffix _n in the name. The columns with n = 1, 2, or 3 correspond to the three individual energy bands 0.2–0.6, 0.6–2.3, and 2.3–5 keV used in the three-band detection; n =0 indicates the summary value in the three-band detection; if without the _n suffix, the column corresponds to the single-band detection.
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.