BlazEr1_catalog.fitsContent of the page (HDU means "Header Data Unit" of a fits file).
BlazEr1 catalog
| Key | Value | Type | Comment |
|---|
| Name | Type | Unit | Description |
|---|---|---|---|
| SRC_NAME | char[29] | None | Common name of the source |
| RAJ2000 | float64 | deg | Right ascension from input catalog |
| DECJ2000 | float64 | deg | Declination from input catalog |
| BLAZAR_CLASS | char[5] | None | Blazar classification given by the input catalog |
| CONF_BLAZAR | float64 | None | 1 for confirmed blazars and 0 for candidates |
| FGL_SRC_NAME | char[32] | None | Name of source if listed in 4FGL (4FGL-DR4, Abdollahi+2022) |
| BZCAT_SRC_NAME | char[15] | None | Name of source if listed in BZCAT (Massaro+2015) |
| HSP_SRC_NAME | char[21] | None | Name of source if listed in 3HSP (Chang+2019) |
| HIGHZ_SRC_NAME | char[20] | None | Name of source if listed in the HighZ sample (Sbarrato+2026,Marcotulli+2025) |
| MILLIQUAS_SRC_NAME | char[26] | None | Name of source if listed in Milliquas (Flesch+2023) |
| KDEBLLACS_SRC_NAME | char[29] | None | Name of source if listed in KDEBLLACS (Dabrusco+2019) |
| WIBRALS2_SRC_NAME | char[28] | None | Name of source if listed in WIBRaLS2 (Dabrusco+2019) |
| ABC_SRC_NAME | char[14] | None | Name of source if listed in ABC (Paggi+2020) |
| BROS_SRC_NAME | char[17] | None | Name of source if listed in BROS (Itoh+2020) |
| ANGSEP | float64 | deg | Angular separation between catalog and eROSITA position |
| DETUID | char[32] | None | eROSITA unique detection ID |
| IAUNAME | char[23] | None | Official IAU name of the eROSITA source |
| SKYTILE | int32 | None | eROSITA sky tile ID |
| ID_SRC | int32 | None | eROSITA source ID in each sky tile |
| UID | int64 | None | Integer unique detection ID. See Merloni+2024 for details |
| UID_HARD | int64 | None | Hard catalog UID of the source with a strong association, or -UID if the association is weak. 0 means no counterpart found in the Hard catalog |
| ID_CLUSTER | int32 | None | Group ID of sources simultaneously modeled during source detection |
| RA | float64 | deg | Right ascension of eROSITA source |
| RA_ERR | float32[1PE(2)] | arcsec | Uncertainties of RA |
| DEC | float64 | deg | Declination of eROSITA source |
| DEC_ERR | float32[1PE(2)] | arcsec | Uncertainties of DEC |
| RA_RAW | float64 | deg | Right ascension of eROSITA source without applying the eROSITA aspect correction |
| DEC_RAW | float64 | deg | Declination of eROSITA source without applying the eROSITA aspect correction |
| POS_ERR | float64 | arcsec | 1sigma position uncertainty |
| RADEC_ERR | float64 | arcsec | Combined positional error, raw output from PSF fitting |
| LII | float64 | deg | Galactic longitude of eROSITA source with applied position correction (not identical to the coordinates listed by Merloni+2024) |
| BII | float64 | deg | Galactic latitude of eROSITA source with applied position correction (not identical to the coordinates listed by Merloni+2024) |
| ELON | float64 | deg | Equatorial longitude of eROSITA source |
| ELAT | float64 | deg | Equatorial latitude of eROSITA source |
| MJD | float32 | d | Modified Julian Date of the observation of the source nearest to the optical axis of eROSITA |
| MJD_MIN | float32 | d | Modified Julian Date of the sources' first eROSITA observation |
| MJD_MAX | float32 | d | Modified Julian Date of the sources' last eROSITA observation |
| EXT | float32 | arcsec | Source extent parameter and associated uncertainty |
| EXT_ERR | float32 | arcsec | Uncertainty of EXT |
| EXT_ASYM_ERR | float32[1PE(2)] | arcsec | Uncertainties of EXT |
| EXT_LIKE | float32 | None | Extent likelihood |
| DET_LIKE_0 | float32 | None | Detection likelihood in 0.2-2.3 keV band |
| ML_CTS_1 | float32 | count | ML source net counts in 0.2-2.3 keV band |
| ML_CTS_1_ERR | float32 | count | Uncertainty of ML_CTS_1 |
| ML_CTS_1_ASYM_ERR | float32[1PE(2)] | count | Uncertainties of ML_CTS_1 |
| ML_RATE_1 | float32 | count*s^(-1) | ML source count rate in 0.2-2.3 keV band |
| ML_RATE_1_ERR | float32 | count*s^(-1) | Uncertainty of ML_RATE_1 |
| ML_RATE_1_ASYM_ERR | float32[1PE(2)] | count*s^(-1) | Uncertainties of ML_RATE_1 |
| ML_FLUX_1 | float32 | erg*cm^(-2)*s^(-1) | ML source flux in 0.2-2.3 keV band |
| ML_FLUX_1_ERR | float32 | erg*cm^(-2)*s^(-1) | Uncertainty of ML_FLUX_1 |
| ML_FLUX_1_ASYM_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of ML_FLUX_1 |
| ML_BKG_1 | float32 | arcmin^(-2) | ML background counts at the source position in 0.2-2.3 keV band |
| ML_EXP_1 | float32 | s | ML vignetted exposure time at the source position in 0.2-2.3 keV band |
| ML_EEF_1 | float32 | None | ML enclosed energy fraction in 0.2-2.3 keV band |
| APE_CTS_1 | int32 | count | Total counts extracted within the aperture in 0.2-2.3 keV band |
| APE_BKG_1 | float32 | count | Background counts extracted within the aperture, excluding nearby sources using the source map in 0.2-2.3 keV band |
| APE_EXP_1 | float32 | s | Exposure map value at the given position in 0.2-2.3 keV band |
| APE_RADIUS_1 | float32 | pix | Extraction radius in 0.2-2.3 keV band |
| APE_POIS_1 | float32 | None | Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 0.2-2.3 keV band |
| DET_LIKE_P1 | float32 | None | Detection likelihood in 0.2-0.5 keV band |
| ML_CTS_P1 | float32 | count | ML source net counts in 0.2-0.5 keV keV band |
| ML_CTS_P1_ERR | float32 | count | Uncertainty of ML_CTS_P1 |
| ML_CTS_P1_ASYM_ERR | float32[1PE(2)] | count | Uncertainties of ML_CTS_P1 |
| ML_RATE_P1 | float32 | count*s^(-1) | ML source count rate in 0.2-0.5 keV band |
| ML_RATE_P1_ERR | float32 | count*s^(-1) | Uncertainty of ML_RATE_P1 |
| ML_RATE_P1_ASYM_ERR | float32[1PE(2)] | count*s^(-1) | Uncertainties of ML_RATE_P1 |
| ML_FLUX_P1 | float32 | erg*cm^(-2)*s^(-1) | ML source flux in 0.2-0.5 keV keV band |
| ML_FLUX_P1_ERR | float32 | erg*cm^(-2)*s^(-1) | Uncertainty of ML_FLUX_P1 |
| ML_FLUX_P1_ASYM_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of ML_FLUX_P1 |
| ML_BKG_P1 | float32 | arcmin^(-2) | ML background counts at the source position in 0.2-0.5 keV band |
| ML_EXP_P1 | float32 | s | ML vignetted exposure time at the source position in 0.2-0.5 keV band |
| ML_EEF_P1 | float32 | None | ML enclosed energy fraction in 0.2-0.5 keV band |
| APE_CTS_P1 | int32 | count | Total counts extracted within the aperture in 0.2-0.5 keV band |
| APE_BKG_P1 | float32 | count | Background counts extracted within the aperture, excluding nearby sources using the source map in 0.2-0.5 keV band |
| APE_EXP_P1 | float32 | s | Exposure map value at the given position in 0.2-0.5 keV band |
| APE_RADIUS_P1 | float32 | pix | Extraction radius in 0.2-0.5 keV band |
| APE_POIS_P1 | float32 | None | Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 0.2-0.5 keV band |
| DET_LIKE_P2 | float32 | None | Detection likelihood in 0.5-1.0 keV band |
| ML_CTS_P2 | float32 | count | ML source net counts in 0.5-1.0 keV keV band |
| ML_CTS_P2_ERR | float32 | count | Uncertainty of ML_CTS_P2 |
| ML_CTS_P2_ASYM_ERR | float32[1PE(2)] | count | Uncertainties of ML_CTS_P2 |
| ML_RATE_P2 | float32 | count*s^(-1) | ML source count rate in 0.5-1.0 keV band |
| ML_RATE_P2_ERR | float32 | count*s^(-1) | Uncertainty of ML_RATE_P2 |
| ML_RATE_P2_ASYM_ERR | float32[1PE(2)] | count*s^(-1) | Uncertainties of ML_RATE_P2 |
| ML_FLUX_P2 | float32 | erg*cm^(-2)*s^(-1) | ML source flux in 0.5-1.0 keV keV band |
| ML_FLUX_P2_ERR | float32 | erg*cm^(-2)*s^(-1) | Uncertainty of ML_FLUX_P2 |
| ML_FLUX_P2_ASYM_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of ML_FLUX_P2 |
| ML_BKG_P2 | float32 | arcmin^(-2) | ML background counts at the source position in 0.5-1.0 keV band |
| ML_EXP_P2 | float32 | s | ML vignetted exposure time at the source position in 0.5-1.0 keV band |
| ML_EEF_P2 | float32 | None | ML enclosed energy fraction in 0.5-1.0 keV band |
| APE_CTS_P2 | int32 | count | Total counts extracted within the aperture in 0.5-1.0 keV band |
| APE_BKG_P2 | float32 | count | Background counts extracted within the aperture, excluding nearby sources using the source map in 0.5-1.0 keV band |
| APE_EXP_P2 | float32 | s | Exposure map value at the given position in 0.5-1.0 keV band |
| APE_RADIUS_P2 | float32 | pix | Extraction radius in 0.5-1.0 keV band |
| APE_POIS_P2 | float32 | None | Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 0.5-1.0 keV band |
| DET_LIKE_P3 | float32 | None | Detection likelihood in 1.0-2.0 keV band |
| ML_CTS_P3 | float32 | count | ML source net counts in 1.0-2.0 keV keV band |
| ML_CTS_P3_ERR | float32 | count | Uncertainty of ML_CTS_P3 |
| ML_CTS_P3_ASYM_ERR | float32[1PE(2)] | count | Uncertainties of ML_CTS_P3 |
| ML_RATE_P3 | float32 | count*s^(-1) | ML source count rate in 1.0-2.0 keV band |
| ML_RATE_P3_ERR | float32 | count*s^(-1) | Uncertainty of ML_RATE_P3 |
| ML_RATE_P3_ASYM_ERR | float32[1PE(2)] | count*s^(-1) | Uncertainties of ML_RATE_P3 |
| ML_FLUX_P3 | float32 | erg*cm^(-2)*s^(-1) | ML source flux in 1.0-2.0 keV keV band |
| ML_FLUX_P3_ERR | float32 | erg*cm^(-2)*s^(-1) | Uncertainty of ML_FLUX_P3 |
| ML_FLUX_P3_ASYM_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of ML_FLUX_P3 |
| ML_BKG_P3 | float32 | arcmin^(-2) | ML background counts at the source position in 1.0-2.0 keV band |
| ML_EXP_P3 | float32 | s | ML vignetted exposure time at the source position in 1.0-2.0 keV band |
| ML_EEF_P3 | float32 | None | ML enclosed energy fraction in 1.0-2.0 keV band |
| APE_CTS_P3 | int32 | count | Total counts extracted within the aperture in 1.0-2.0 keV band |
| APE_BKG_P3 | float32 | count | Background counts extracted within the aperture, excluding nearby sources using the source map in 1.0-2.0 keV band |
| APE_EXP_P3 | float32 | s | Exposure map value at the given position in 1.0-2.0 keV band |
| APE_RADIUS_P3 | float32 | pix | Extraction radius in 1.0-2.0 keV band |
| APE_POIS_P3 | float32 | None | Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 1.0-2.0 keV band |
| DET_LIKE_P4 | float32 | None | Detection likelihood in 2.0-5.0 keV band |
| ML_CTS_P4 | float32 | count | ML source net counts in 2.0-5.0 keV keV band |
| ML_CTS_P4_ERR | float32 | count | Uncertainty of ML_CTS_P4 |
| ML_CTS_P4_ASYM_ERR | float32[1PE(2)] | count | Uncertainties of ML_CTS_P4 |
| ML_RATE_P4 | float32 | count*s^(-1) | ML source count rate in 2.0-5.0 keV band |
| ML_RATE_P4_ERR | float32 | count*s^(-1) | Uncertainty of ML_RATE_P4 |
| ML_RATE_P4_ASYM_ERR | float32[1PE(2)] | count*s^(-1) | Uncertainties of ML_RATE_P4 |
| ML_FLUX_P4 | float32 | erg*cm^(-2)*s^(-1) | ML source flux in 2.0-5.0 keV keV band |
| ML_FLUX_P4_ERR | float32 | erg*cm^(-2)*s^(-1) | Uncertainty of ML_FLUX_P4 |
| ML_FLUX_P4_ASYM_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of ML_FLUX_P4 |
| ML_BKG_P4 | float32 | arcmin^(-2) | ML background counts at the source position in 2.0-5.0 keV band |
| ML_EXP_P4 | float32 | s | ML vignetted exposure time at the source position in 2.0-5.0 keV band |
| ML_EEF_P4 | float32 | None | ML enclosed energy fraction in 2.0-5.0 keV band |
| APE_CTS_P4 | int32 | count | Total counts extracted within the aperture in 2.0-5.0 keV band |
| APE_BKG_P4 | float32 | count | Background counts extracted within the aperture, excluding nearby sources using the source map in 2.0-5.0 keV band |
| APE_EXP_P4 | float32 | s | Exposure map value at the given position in 2.0-5.0 keV band |
| APE_RADIUS_P4 | float32 | pix | Extraction radius in 2.0-5.0 keV band |
| APE_POIS_P4 | float32 | None | Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 2.0-5.0 keV band |
| DET_LIKE_P5 | float32 | None | Detection likelihood in 5.0-8.0 keV band |
| ML_CTS_P5 | float32 | count | ML source net counts in 5.0-8.0 keV keV band |
| ML_CTS_P5_ERR | float32 | count | Uncertainty of ML_CTS_P5 |
| ML_CTS_P5_ASYM_ERR | float32[1PE(2)] | count | Uncertainties of ML_CTS_P5 |
| ML_RATE_P5 | float32 | count*s^(-1) | ML source count rate in 5.0-8.0 keV band |
| ML_RATE_P5_ERR | float32 | count*s^(-1) | Uncertainty of ML_RATE_P5 |
| ML_RATE_P5_ASYM_ERR | float32[1PE(2)] | count*s^(-1) | Uncertainties of ML_RATE_P5 |
| ML_FLUX_P5 | float32 | erg*cm^(-2)*s^(-1) | ML source flux in 5.0-8.0 keV keV band |
| ML_FLUX_P5_ERR | float32 | erg*cm^(-2)*s^(-1) | Uncertainty of ML_FLUX_P5 |
| ML_FLUX_P5_ASYM_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of ML_FLUX_P5 |
| ML_BKG_P5 | float32 | arcmin^(-2) | ML background counts at the source position in 5.0-8.0 keV band |
| ML_EXP_P5 | float32 | s | ML vignetted exposure time at the source position in 5.0-8.0 keV band |
| ML_EEF_P5 | float32 | None | ML enclosed energy fraction in 5.0-8.0 keV band |
| APE_CTS_P5 | int32 | count | Total counts extracted within the aperture in 5.0-8.0 keV band |
| APE_BKG_P5 | float32 | count | Background counts extracted within the aperture, excluding nearby sources using the source map in 5.0-8.0 keV band |
| APE_EXP_P5 | float32 | s | Exposure map value at the given position in 5.0-8.0 keV band |
| APE_RADIUS_P5 | float32 | pix | Extraction radius in 5.0-8.0 keV band |
| APE_POIS_P5 | float32 | None | Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 5.0-8.0 keV band |
| DET_LIKE_P6 | float32 | None | Detection likelihood in 4.0-10.0 keV band |
| ML_CTS_P6 | float32 | count | ML source net counts in 4.0-10.0 keV keV band |
| ML_CTS_P6_ERR | float32 | count | Uncertainty of ML_CTS_P6 |
| ML_CTS_P6_ASYM_ERR | float32[1PE(2)] | count | Uncertainties of ML_CTS_P6 |
| ML_RATE_P6 | float32 | count*s^(-1) | ML source count rate in 4.0-10.0 keV band |
| ML_RATE_P6_ERR | float32 | count*s^(-1) | Uncertainty of ML_RATE_P6 |
| ML_RATE_P6_ASYM_ERR | float32[1PE(2)] | count*s^(-1) | Uncertainties of ML_RATE_P6 |
| ML_FLUX_P6 | float32 | erg*cm^(-2)*s^(-1) | ML source flux in 4.0-10.0 keV keV band |
| ML_FLUX_P6_ERR | float32 | erg*cm^(-2)*s^(-1) | Uncertainty of ML_FLUX_P6 |
| ML_FLUX_P6_ASYM_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of ML_FLUX_P6 |
| ML_BKG_P6 | float32 | arcmin^(-2) | ML background counts at the source position in 4.0-10.0 keV band |
| ML_EXP_P6 | float32 | s | ML vignetted exposure time at the source position in 4.0-10.0 keV band |
| ML_EEF_P6 | float32 | None | ML enclosed energy fraction in 4.0-10.0 keV band |
| APE_CTS_P6 | int32 | count | Total counts extracted within the aperture in 4.0-10.0 keV band |
| APE_BKG_P6 | float32 | count | Background counts extracted within the aperture, excluding nearby sources using the source map in 4.0-10.0 keV band |
| APE_EXP_P6 | float32 | s | Exposure map value at the given position in 4.0-10.0 keV band |
| APE_RADIUS_P6 | float32 | pix | Extraction radius in 4.0-10.0 keV band |
| APE_POIS_P6 | float32 | None | Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 4.0-10.0 keV band |
| DET_LIKE_P7 | float32 | None | Detection likelihood in 5.1-6.1 keV band |
| ML_CTS_P7 | float32 | count | ML source net counts in 5.1-6.1 keV keV band |
| ML_CTS_P7_ERR | float32 | count | Uncertainty of ML_CTS_P7 |
| ML_CTS_P7_ASYM_ERR | float32[1PE(2)] | count | Uncertainties of ML_CTS_P7 |
| ML_RATE_P7 | float32 | count*s^(-1) | ML source count rate in 5.1-6.1 keV band |
| ML_RATE_P7_ERR | float32 | count*s^(-1) | Uncertainty of ML_RATE_P7 |
| ML_RATE_P7_ASYM_ERR | float32[1PE(2)] | count*s^(-1) | Uncertainties of ML_RATE_P7 |
| ML_FLUX_P7 | float32 | erg*cm^(-2)*s^(-1) | ML source flux in 5.1-6.1 keV keV band |
| ML_FLUX_P7_ERR | float32 | erg*cm^(-2)*s^(-1) | Uncertainty of ML_FLUX_P7 |
| ML_FLUX_P7_ASYM_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of ML_FLUX_P7 |
| ML_BKG_P7 | float32 | arcmin^(-2) | ML background counts at the source position in 5.1-6.1 keV band |
| ML_EXP_P7 | float32 | s | ML vignetted exposure time at the source position in 5.1-6.1 keV band |
| ML_EEF_P7 | float32 | None | ML enclosed energy fraction in 5.1-6.1 keV band |
| APE_CTS_P7 | int32 | count | Total counts extracted within the aperture in 5.1-6.1 keV band |
| APE_BKG_P7 | float32 | count | Background counts extracted within the aperture, excluding nearby sources using the source map in 5.1-6.1 keV band |
| APE_EXP_P7 | float32 | s | Exposure map value at the given position in 5.1-6.1 keV band |
| APE_RADIUS_P7 | float32 | pix | Extraction radius in 5.1-6.1 keV band |
| APE_POIS_P7 | float32 | None | Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 5.1-6.1 keV band |
| DET_LIKE_P8 | float32 | None | Detection likelihood in 6.2-7.1 keV band |
| ML_CTS_P8 | float32 | count | ML source net counts in 6.2-7.1 keV keV band |
| ML_CTS_P8_ERR | float32 | count | Uncertainty of ML_CTS_P8 |
| ML_CTS_P8_ASYM_ERR | float32[1PE(2)] | count | Uncertainties of ML_CTS_P8 |
| ML_RATE_P8 | float32 | count*s^(-1) | ML source count rate in 6.2-7.1 keV band |
| ML_RATE_P8_ERR | float32 | count*s^(-1) | Uncertainty of ML_RATE_P8 |
| ML_RATE_P8_ASYM_ERR | float32[1PE(2)] | count*s^(-1) | Uncertainties of ML_RATE_P8 |
| ML_FLUX_P8 | float32 | erg*cm^(-2)*s^(-1) | ML source flux in 6.2-7.1 keV keV band |
| ML_FLUX_P8_ERR | float32 | erg*cm^(-2)*s^(-1) | Uncertainty of ML_FLUX_P8 |
| ML_FLUX_P8_ASYM_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of ML_FLUX_P8 |
| ML_BKG_P8 | float32 | arcmin^(-2) | ML background counts at the source position in 6.2-7.1 keV band |
| ML_EXP_P8 | float32 | s | ML vignetted exposure time at the source position in 6.2-7.1 keV band |
| ML_EEF_P8 | float32 | None | ML enclosed energy fraction in 6.2-7.1 keV band |
| APE_CTS_P8 | int32 | count | Total counts extracted within the aperture in 6.2-7.1 keV band |
| APE_BKG_P8 | float32 | count | Background counts extracted within the aperture, excluding nearby sources using the source map in 6.2-7.1 keV band |
| APE_EXP_P8 | float32 | s | Exposure map value at the given position in 6.2-7.1 keV band |
| APE_RADIUS_P8 | float32 | pix | Extraction radius in 6.2-7.1 keV band |
| APE_POIS_P8 | float32 | None | Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 6.2-7.1 keV band |
| DET_LIKE_P9 | float32 | None | Detection likelihood in 7.2-8.2 keV band |
| ML_CTS_P9 | float32 | count | ML source net counts in 7.2-8.2 keV keV band |
| ML_CTS_P9_ERR | float32 | count | Uncertainty of ML_CTS_P9 |
| ML_CTS_P9_ASYM_ERR | float32[1PE(2)] | count | Uncertainties of ML_CTS_P9 |
| ML_RATE_P9 | float32 | count*s^(-1) | ML source count rate in 7.2-8.2 keV band |
| ML_RATE_P9_ERR | float32 | count*s^(-1) | Uncertainty of ML_RATE_P9 |
| ML_RATE_P9_ASYM_ERR | float32[1PE(2)] | count*s^(-1) | Uncertainties of ML_RATE_P9 |
| ML_FLUX_P9 | float32 | erg*cm^(-2)*s^(-1) | ML source flux in 7.2-8.2 keV keV band |
| ML_FLUX_P9_ERR | float32 | erg*cm^(-2)*s^(-1) | Uncertainty of ML_FLUX_P9 |
| ML_FLUX_P9_ASYM_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of ML_FLUX_P9 |
| ML_BKG_P9 | float32 | arcmin^(-2) | ML background counts at the source position in 7.2-8.2 keV band |
| ML_EXP_P9 | float32 | s | ML vignetted exposure time at the source position in 7.2-8.2 keV band |
| ML_EEF_P9 | float32 | None | ML enclosed energy fraction in 7.2-8.2 keV band |
| APE_CTS_P9 | int32 | count | Total counts extracted within the aperture in 7.2-8.2 keV band |
| APE_BKG_P9 | float32 | count | Background counts extracted within the aperture, excluding nearby sources using the source map in 7.2-8.2 keV band |
| APE_EXP_P9 | float32 | s | Exposure map value at the given position in 7.2-8.2 keV band |
| APE_RADIUS_P9 | float32 | pix | Extraction radius in 7.2-8.2 keV band |
| APE_POIS_P9 | float32 | None | Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 7.2-8.2 keV band |
| APE_CTS_S | int32 | count | Total counts extracted within the aperture in 0.5-2.0 keV band |
| APE_BKG_S | float32 | count | Background counts extracted within the aperture, excluding nearby sources using the source map in 0.5-2.0 keV band |
| APE_EXP_S | float32 | s | Exposure map value at the given position in 0.5-2.0 keV band |
| APE_POIS_S | float32 | None | Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 0.5-2.0 keV band |
| FLAG_SP_SNR | int16 | None | If 1, source may lie within an overdense region near a supernova remnant |
| FLAG_SP_BPS | int16 | None | If 1, source may lie within an overdense region near a bright point source |
| FLAG_SP_SCL | int16 | None | If 1, source may lie within an overdense region near a stellar cluster |
| FLAG_SP_LGA | int16 | None | If 1, source may lie within an overdense region near a local large galaxy |
| FLAG_SP_GC_CONS | int16 | None | If 1, source may lie within an overdense region near a galaxy cluster |
| FLAG_NO_RADEC_ERR | int16 | None | If 1, source contained no RA_DEC_ERR in the preprocessed version of the catalog |
| FLAG_NO_EXT_ERR | int16 | None | If 1, source contained no EXT_ERR in the preprocessed version of the catalog |
| FLAG_NO_CTS_ERR | int16 | None | If 1, source contained no ML_CTS_0_ERR in the preprocessed version of the catalog |
| FLAG_OPT | int16 | None | If 1, source matched within 15arcsec with a bright optical star, likely contaminated by optical loading |
| CTS_1 | float64 | count | Counts from spectrum in 0.2-2.3 keV band |
| CTS_1_ERR | float32[1PE(2)] | count | Uncertainties of CTS_1 |
| CTS_T | float64 | count | Counts from spectrum in 0.2-10.0 keV band |
| CTS_T_ERR | float32[1PE(2)] | count | Uncertainties of CTS_T |
| SPEC_EXPOTIME | float64 | s | Exposure time as given in the spectrum |
| EXPOTIME | float64 | s | Exposure time from the eROSITA exposure map in 0.2-2.3 keV band |
| MIN_FLUX_95 | float64 | erg*cm^(-2)*s^(-1) | Minimum detectable flux at source position to guarantee 95% detection rate with a DET_LIKE_0 of 10 or greater in the 0.2-2.3 keV band |
| AVERAGE_NH | float64 | cm^(-2) | Average N_H from the Hi4picollaboration+2016 |
| WE_AVERAGE_NH | float64 | cm^(-2) | Weighted average N_H from the Hi4picollaboration+2016 |
| HR12 | float64 | None | Hardness ratio between 0.2-0.7 keV and 0.7-1.2 keV |
| HR12_ERR | float32[1PE(2)] | None | Uncertainties of HR12 |
| HR23 | float64 | None | Hardness ratio between 0.7-1.2 keV and 1.2-2.3 keV |
| HR23_ERR | float32[1PE(2)] | None | Uncertainties of HR23 |
| HR13 | float64 | None | Hardness ratio between 0.2-0.7 keV and 1.2-2.3 keV |
| HR13_ERR | float32[1PE(2)] | None | Uncertainties of HR13 |
| PWL15_NORM | float64 | ph*keV^(-1)*cm^(-2)*s^(-1) | Power law norm using a fixed N_H and an index of 1.5 at 1 keV |
| PWL15_NORM_ERR | float32[1PE(2)] | ph*keV^(-1)*cm^(-2)*s^(-1) | Uncertainties of PWL15_NORM |
| PWL15_FLUX_UNABS_0 | float64 | erg*cm^(-2)*s^(-1) | Fitted unabsorbed flux using a fixed N_H and fixed power law index 1.5 |
| PWL15_FLUX_UNABS_0_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of PWL15_FLUX_UNABS_0 |
| PWL15_FLUX_ABS_0 | float64 | erg*cm^(-2)*s^(-1) | Fitted observed flux using a fixed N_H and fixed power law index 1.5 |
| PWL15_FLUX_ABS_0_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of PWL15_FLUX_ABS_0 |
| PWL15_C_VARIANCE | float64 | None | Variance of Cash statistics of fixed N_H and fixed power law index 1.5 fit according to Kaastra+2017 |
| PWL15_CASH | float64 | None | Cash statistics of fixed N_H and fixed power law index 1.5 fit |
| PWL15_CSTAT_THEORY | float64 | None | Theoretical Cash statistics while using a fixed N_H and fixed power law index 1.5 fit according to Kaastra+2017 |
| PWL15_REDCASH | float64 | None | Reduced Cash statistics from fit with fixed N_H and fixed power law index 1.5 |
| PWL15_CASHBINS | int32 | None | Number of bins used during the fixed N_H and fixed power law index 1.5 fit |
| PWL15_CASHPAR | int32 | None | Number of parameters used during the fixed N_H and fixed power law index 1.5 fit |
| PWL15_NUM_BINS | int32 | None | Number of bins used to calculate Kaastra+2017 values of fixed N_H and fixed power law index 1.5 |
| PWL17_NORM | float64 | ph*keV^(-1)*cm^(-2)*s^(-1) | Power law norm using a fixed N_H and an index of 1.7 at 1 keV |
| PWL17_NORM_ERR | float32[1PE(2)] | ph*keV^(-1)*cm^(-2)*s^(-1) | Uncertainties of PWL17_NORM |
| PWL17_FLUX_UNABS_0 | float64 | erg*cm^(-2)*s^(-1) | Fitted unabsorbed flux using a fixed N_H and fixed power law index 1.7 |
| PWL17_FLUX_UNABS_0_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of PWL17_FLUX_UNABS_0 |
| PWL17_FLUX_ABS_0 | float64 | erg*cm^(-2)*s^(-1) | Fitted observed flux using a fixed N_H and fixed power law index 1.7 |
| PWL17_FLUX_ABS_0_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of PWL17_FLUX_ABS_0 |
| PWL17_C_VARIANCE | float64 | None | Variance of Cash statistics of fixed N_H and fixed power law index 1.7 fit according to Kaastra+2017 |
| PWL17_CASH | float64 | None | Cash statistics of fixed N_H and fixed power law index 1.7 fit |
| PWL17_CSTAT_THEORY | float64 | None | Theoretical Cash statistics while using a fixed N_H and fixed power law index 1.7 fit according to Kaastra+2017 |
| PWL17_REDCASH | float64 | None | Reduced Cash statistics from fit with fixed N_H and fixed power law index 1.7 |
| PWL17_CASHBINS | int32 | None | Number of bins used during the fixed N_H and fixed power law index 1.7 fit |
| PWL17_CASHPAR | int32 | None | Number of parameters used during the fixed N_H and fixed power law index 1.7 fit |
| PWL17_NUM_BINS | int32 | None | Number of bins used to calculate Kaastra+2017 values of fixed N_H and fixed power law index 1.7 |
| PWL20_NORM | float64 | ph*keV^(-1)*cm^(-2)*s^(-1) | Power law norm using a fixed N_H and an index of 2.0 at 1 keV |
| PWL20_NORM_ERR | float32[1PE(2)] | ph*keV^(-1)*cm^(-2)*s^(-1) | Uncertainties of PWL20_NORM |
| PWL20_FLUX_UNABS_0 | float64 | erg*cm^(-2)*s^(-1) | Fitted unabsorbed flux using a fixed N_H and fixed power law index 2.0 |
| PWL20_FLUX_UNABS_0_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of PWL20_FLUX_UNABS_0 |
| PWL20_FLUX_ABS_0 | float64 | erg*cm^(-2)*s^(-1) | Fitted observed flux using a fixed N_H and fixed power law index 2.0 |
| PWL20_FLUX_ABS_0_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of PWL20_FLUX_ABS_0 |
| PWL20_C_VARIANCE | float64 | None | Variance of Cash statistics of fixed N_H and fixed power law index 2.0 fit according to Kaastra+2017 |
| PWL20_CASH | float64 | None | Cash statistics of fixed N_H and fixed power law index 2.0 fit |
| PWL20_CSTAT_THEORY | float64 | None | Theoretical Cash statistics while using a fixed N_H and fixed power law index 2.0 fit according to Kaastra+2017 |
| PWL20_REDCASH | float64 | None | Reduced Cash statistics from fit with fixed N_H and fixed power law index 2.0 |
| PWL20_CASHBINS | int32 | None | Number of bins used during the fixed N_H and fixed power law index 2.0 fit |
| PWL20_CASHPAR | int32 | None | Number of parameters used during the fixed N_H and fixed power law index 2.0 fit |
| PWL20_NUM_BINS | int32 | None | Number of bins used to calculate Kaastra+2017 values of fixed N_H and fixed power law index 2.0 |
| PWL23_NORM | float64 | ph*keV^(-1)*cm^(-2)*s^(-1) | Power law norm using a fixed N_H and an index of 2.3 at 1 keV |
| PWL23_NORM_ERR | float32[1PE(2)] | ph*keV^(-1)*cm^(-2)*s^(-1) | Uncertainties of PWL23_NORM |
| PWL23_FLUX_UNABS_0 | float64 | erg*cm^(-2)*s^(-1) | Fitted unabsorbed flux using a fixed N_H and fixed power law index 2.3 |
| PWL23_FLUX_UNABS_0_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of PWL23_FLUX_UNABS_0 |
| PWL23_FLUX_ABS_0 | float64 | erg*cm^(-2)*s^(-1) | Fitted observed flux using a fixed N_H and fixed power law index 2.3 |
| PWL23_FLUX_ABS_0_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of PWL23_FLUX_ABS_0 |
| PWL23_C_VARIANCE | float64 | None | Variance of Cash statistics of fixed N_H and fixed power law index 2.3 fit according to Kaastra+2017 |
| PWL23_CASH | float64 | None | Cash statistics of fixed N_H and fixed power law index 2.3 fit |
| PWL23_CSTAT_THEORY | float64 | None | Theoretical Cash statistics while using a fixed N_H and fixed power law index 2.3 fit according to Kaastra+2017 |
| PWL23_REDCASH | float64 | None | Reduced Cash statistics from fit with fixed N_H and fixed power law index 2.3 |
| PWL23_CASHBINS | int32 | None | Number of bins used during the fixed N_H and fixed power law index 2.3 fit |
| PWL23_CASHPAR | int32 | None | Number of parameters used during the fixed N_H and fixed power law index 2.3 fit |
| PWL23_NUM_BINS | int32 | None | Number of bins used to calculate Kaastra+2017 values of fixed N_H and fixed power law index 2.3 |
| FLUX_JY | float64 | Jy | Flux density at 1 keV derived from the norm of the fixed Gamma_X=2.0 fit |
| FLUX_JY_ERR | float64 | Jy | Uncertainty of FLUX_JY |
| FREE_NH | float64 | cm^(-2) | Freely fitted N_H |
| FREE_NH_ERR | float32[1PE(2)] | cm^(-2) | Uncertainties of FREE_NH |
| FREE_GAMMA | float64 | None | Power law photon index using a free N_H |
| FREE_GAMMA_ERR | float32[1PE(2)] | None | Uncertainties of FREE_GAMMA |
| FREE_NORM | float64 | ph*keV^(-1)*cm^(-2)*s^(-1) | Power law norm using a free N_H at 1 keV |
| FREE_NORM_ERR | float32[1PE(2)] | ph*keV^(-1)*cm^(-2)*s^(-1) | Uncertainties of FREE_NORM |
| FREE_FLUX_UNABS_0 | float64 | erg*cm^(-2)*s^(-1) | Fitted unabsorbed flux for a free N_H power law fit in 0.2-2.3 keV band |
| FREE_FLUX_UNABS_0_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of FREE_FLUX_UNABS_0 |
| FREE_FLUX_ABS_0 | float64 | erg*cm^(-2)*s^(-1) | Fitted observed flux for a free N_H power law fit in 0.2-2.3 keV band |
| FREE_FLUX_ABS_0_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of FREE_FLUX_ABS_0 |
| FREE_C_VARIANCE | float64 | None | Variance of Cash statistics of free N_H power law fit according to Kaastra+2017 |
| FREE_CASH | float64 | None | Cash statistics of free N_H power law fit |
| FREE_CSTAT_THEORY | float64 | None | Theoretical Cash statistics while using a free N_H power law fit according to Kaastra+2017 |
| FREE_REDCASH | float64 | None | Reduced Cash statistics from fit with free N_H |
| FREE_CASHBINS | int32 | None | Number of bins used during the free N_H power law fit |
| FREE_CASHPAR | int32 | None | Number of parameters used during the free N_H power law fit |
| FREE_NUM_BINS | int32 | None | Number of bins used to calculate Kaastra+2017 values of free N_H power law fit |
| FIXED_NH | float64 | cm^(-2) | Fixed N_H |
| FIXED_GAMMA | float64 | None | Power law photon index using a fixed N_H |
| FIXED_GAMMA_ERR | float32[1PE(2)] | None | Uncertainties of FIXED_GAMMA |
| FIXED_NORM | float64 | ph*keV^(-1)*cm^(-2)*s^(-1) | Power law norm using a fixed N_H at 1 keV |
| FIXED_NORM_ERR | float32[1PE(2)] | ph*keV^(-1)*cm^(-2)*s^(-1) | Uncertainties of FIXED_NORM |
| FIXED_FLUX_UNABS_0 | float64 | erg*cm^(-2)*s^(-1) | Fitted unabsorbed flux for a fixed N_H power law fit in 0.2-2.3 keV band |
| FIXED_FLUX_UNABS_0_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of FIXED_FLUX_UNABS_0 |
| FIXED_FLUX_ABS_0 | float64 | erg*cm^(-2)*s^(-1) | Fitted observed flux for a fixed N_H power law fit in 0.2-2.3 keV band |
| FIXED_FLUX_ABS_0_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of FIXED_FLUX_ABS_0 |
| FIXED_C_VARIANCE | float64 | None | Variance of Cash statistics of fixed N_H power law fit according to Kaastra+2017 |
| FIXED_CASH | float64 | None | Cash statistics of fixed N_H power law fit |
| FIXED_CSTAT_THEORY | float64 | None | Theoretical Cash statistics while using a fixed N_H power law fit according to Kaastra+2017 |
| FIXED_REDCASH | float64 | None | Reduced Cash statistics from fit with fixed N_H |
| FIXED_CASHBINS | int32 | None | Number of bins used during the fixed N_H power law fit |
| FIXED_CASHPAR | int32 | None | Number of parameters used during the fixed N_H power law fit |
| FIXED_NUM_BINS | int32 | None | Number of bins used to calculate Kaastra+2017 values of fixed N_H power law fit |
| RXS_RA | float64 | deg | Right ascension of 2RXS source Boller+2016 |
| RXS_DEC | float64 | deg | Declination of 2RXS source Boller+2016 |
| RXS_NH_GAL | float64 | cm^(-2) | Galactic N_H assumed by Boller+2016 |
| RXS_NH | float64 | cm^(-2) | N_H derived from fit by Boller+2016 |
| RXS_GAMMA | float64 | None | Gamma_X from fit by Boller+2016 |
| RXS_GAMMA_ERR | float64 | None | Uncertainty of RXS_GAMMA |
| RXS_FLUX_U | float64 | erg*cm^(-2)*s^(-1) | Flux from power law fit by Boller+2016 in 0.1-2.4 keV band |
| XRT_SRC_NAME | char[22] | None | Name given in Evans+2020 |
| XRT_RA | float64 | deg | Right ascension from Evans+2020 |
| XRT_DEC | float64 | deg | Declination from Evans+2020 |
| XRT_ANGSEP | float64 | arcsec | Angular separation between blazar catalog source and closest source in Evans+2020 |
| XRT_FLAG | float64 | None | If 1 the blazar and the source listed by Evans+2020 are located within 8 arcsec of each other |
| XRT_NH | float64 | cm^(-2) | Galactic N_H and associated uncertainty from Evans+2020 |
| XRT_NH_ERR | float32[1PE(2)] | cm^(-2) | Uncertainties of XRT_NH |
| XRT_GAMMA | float64 | None | Power law photon index from Evans+2020 |
| XRT_GAMMA_ERR | float32[1PE(2)] | None | Uncertainties of XRT_GAMMA |
| XRT_ABS_FLUX_V | float64 | erg*cm^(-2)*s^(-1) | Observed flux from Evans+2020 in 0.3-10.0 keV band |
| XRT_ABS_FLUX_V_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of XRT_ABS_FLUX_V |
| XRT_UNABS_FLUX_V | float64 | erg*cm^(-2)*s^(-1) | Unabsorbed flux from Evans+2020 in 0.3-10.0 keV band |
| XRT_UNABS_FLUX_V_ERR | float32[1PE(2)] | erg*cm^(-2)*s^(-1) | Uncertainties of XRT_UNABS_FLUX_V |
| OUSXB_RA | float64 | deg | Right ascension of Swift-XRT sources from Giommi+2019 |
| OUSXB_DEC | float64 | deg | Declination of Swift-XRT sources from Giommi+2019 |
| OUSXB_MIN_FLUX_V | float64 | erg*cm^(-2)*s^(-1) | Minimum sources flux from Giommi+2019 in 0.3-10.0 keV band |
| OUSXB_MAX_FLUX_V | float64 | erg*cm^(-2)*s^(-1) | Maximum sources flux from Giommi+2019 in 0.3-10.0 keV band |
| OUSXB_MEAN_FLUX_V | float64 | erg*cm^(-2)*s^(-1) | Mean sources flux from Giommi+2019 in 0.3-10.0 keV band |
| OUSXB_MEDIAN_FLUX_V | float64 | erg*cm^(-2)*s^(-1) | Median sources flux from Giommi+2019 in 0.3-10.0 keV band |
| OUSXB_N_FLUX_V | float64 | erg*cm^(-2)*s^(-1) | Number of observations of source in Giommi+2019 with a flux in 0.3-10.0 keV band |
| OUSXB_MIN_GAMMA | float64 | erg*cm^(-2)*s^(-1) | Minimum power law photon index Giommi+2019 |
| OUSXB_MAX_GAMMA | float64 | erg*cm^(-2)*s^(-1) | Maximum power law photon index Giommi+2019 |
| OUSXB_MEAN_GAMMA | float64 | erg*cm^(-2)*s^(-1) | Mean power law photon index Giommi+2019 |
| OUSXB_MEDIAN_GAMMA | float64 | erg*cm^(-2)*s^(-1) | Median power law photon index Giommi+2019 |
| OUSXB_N_GAMMA | float64 | erg*cm^(-2)*s^(-1) | Number of observations of source in Giommi+2019 with a power law photon index |
| NUSTAR_RA | float64 | deg | Right ascension of NuSTAR sources from Middei+2022 |
| NUSTAR_DEC | float64 | deg | Declination of NuSTAR sources from Middei+2022 |
| NUSTAR_GAMMA | float64 | None | Photon index of NuSTAR sources from Middei+2022 |
| NUSTAR_GAMMA_ERR | float64 | None | Uncertainty of NUSTAR_GAMMA |
| NUSTAR_FLUX_X | float64 | erg*cm^(-2)*s^(-1) | Flux of extit{NuSTAR} sources from Middei+2022 in 3.0-10.0 keV band |
| NUSTAR_FLUX_X_ERR | float64 | erg*cm^(-2)*s^(-1) | Uncertainty of NUSTAR_FLUX_X |
| NUSTAR_FLUX_Y | float64 | erg*cm^(-2)*s^(-1) | Flux of extit{NuSTAR} sources from Middei+2022 in 10.0-30.0 keV band |
| NUSTAR_FLUX_Y_ERR | float64 | erg*cm^(-2)*s^(-1) | Uncertainty of NUSTAR_FLUX_Y |
| BAT_SRC_NAME | char[18] | None | Name of source given by Lien+2025 |
| BAT_RA | float64 | deg | Right ascension of Swift-BAT sources from Lien+2025 |
| BAT_DEC | float64 | deg | Declination of Swift-BAT sources from Lien+2025 |
| BAT_TYPE | char[17] | None | Source type provided by Lien+2025 |
| BAT_FLUX_Z | float64 | erg*cm^(-2)*s^(-1) | Flux of Swift-BAT sources from Lien+2025 in 14-195 keV band |
| BAT_MIN_FLUX_Z | float64 | erg*cm^(-2)*s^(-1) | Minimum flux of Swift-BAT sources from Lien+2025 in 14-195 keV band |
| BAT_MAX_FLUX_Z | float64 | erg*cm^(-2)*s^(-1) | Maximum flux of Swift-BAT sources from Lien+2025 in 14-195 keV band |
| BAT_GAMMA | float64 | None | Photon index of Swift-BAT sources from Lien+2025 |
| BAT_MIN_GAMMA | float64 | None | Minimum photon index of Swift-BAT sources from Lien+2025 |
| BAT_MAX_GAMMA | float64 | None | Maximum photon index of Swift-BAT sources from Lien+2025 |
| ASCAMASTER_EXPOTIME | float64 | s | ASCA exposure time according to Heasarc's ascamaster table |
| CHANMASTER_EXPOTIME | float64 | s | Chandra exposure time according to Heasarc's chanmaster table |
| NUMASTER_EXPOTIME | float64 | s | NuSTAR exposure time according to Heasarc's numaster table |
| SUZAMASTER_EXPOTIME | float64 | s | Suzaku exposure time according to Heasarc's suzamaster table |
| XMMMASTER_EXPOTIME | float64 | s | XMM-Newton exposure time according to Heasarc's xmmmaster table |
| SWIFTMASTR_EXPOTIME | float64 | s | Swift-XRT exposure time according to Heasarc's swiftmastr table |
| ROSMASTER_EXPOTIME | float64 | s | ROSAT exposure time according to Heasarc's rosmaster table |
| FGL_COMMON_SRC_NAME | char[32] | None | Name of identified or likely associated source from the 4FGL-DR4 catalog Abdollahi+2022 |
| FGL_FLUX_B | float64 | ph*cm^(-2)*s^(-1) | Integral photon flux in 1.0-100.0 GeV Abdollahi+2022 |
| FGL_FLUX_B_ERR | float64 | ph*cm^(-2)*s^(-1) | Uncertainty of FGL_FLUX_B |
| FGL_FLUX_A | float64 | erg*cm^(-2)*s^(-1) | Integral photon flux in 0.1-100.0 GeV Abdollahi+2022 |
| FGL_FLUX_A_ERR | float64 | erg*cm^(-2)*s^(-1) | Uncertainty of FGL_FLUX_A |
| FGL_SPEC_TYPE | char[32] | None | Spectral type in the global model (Power Law, LogParabola, PLSuperExpCutoff) Abdollahi+2022 |
| FGL_PL_FLUXDEN | float64 | cm^(-2)*MeV^(-1)*s^(-1) | Differential flux at pivot energy of the power law fit Abdollahi+2022 |
| FGL_PL_FLUXDEN_ERR | float64 | cm^(-2)*MeV^(-1)*s^(-1) | Uncertainty of FGL_PL_FLUXDEN |
| FGL_PL_INDEX | float64 | None | Photon index of power law fit Abdollahi+2022 |
| FGL_PL_INDEX_ERR | float64 | None | Uncertainty of FGL_PL_INDEX |
| FGL_LP_FLUXDEN | float64 | cm^(-2)*MeV^(-1)*s^(-1) | Differential flux at pivot energy of the LogPar fit Abdollahi+2022 |
| FGL_LP_FLUXDEN_ERR | float64 | cm^(-2)*MeV^(-1)*s^(-1) | Uncertainty of FGL_LP_FLUXDEN |
| FGL_LP_INDEX | float64 | None | hoton index at pivot energy for LogPar fit Abdollahi+2022 |
| FGL_LP_INDEX_ERR | float64 | None | Uncertainty of FGL_LP_INDEX |
| FGL_LP_BETA | float64 | None | Curvature parameter of LogPar fit Abdollahi+2022. |
| FGL_LP_BETA_ERR | float64 | None | Uncertainty of FGL_LP_BETA |
| FGL_LP_EPEAK | float64 | MeV | Peak energy of LogPar fit Abdollahi+2022 |
| FGL_LP_EPEAK_ERR | float64 | MeV | Uncertainty of FGL_LP_EPEAK |
| FGL_LP_SIGCURV | float64 | sigma | Significance of fit improvement between Power Law Abdollahi+2022 |
| FGL_PLEC_FLUXDEN | float64 | cm^(-2)*MeV^(-1)*s^(-1) | Differential flux at pivot energy of the PLSuperExpCutoff fit Abdollahi+2022 |
| FGL_PLEC_FLUXDEN_ERR | float64 | cm^(-2)*MeV^(-1)*s^(-1) | Uncertainty of FGL_PLEC_FLUXDEN |
| FGL_PLEC_INDEX | float64 | None | Photon index at pivot energy for PLSuperExpCutoff fit Abdollahi+2022 |
| FGL_PLEC_INDEX_ERR | float64 | None | Uncertainty of FGL_PLEC_INDEX |
| FGL_PLEC_EXPFACTOR | float64 | None | Spectral curvature at pivot energy for PLSuperExpCutoff fit Abdollahi+2022 |
| FGL_PLEC_EXPFACTOR_ERR | float64 | None | Uncertainty of FGL_PLEC_EXPFACTOR |
| FGL_PLEC_EXPINDEX | float64 | None | Exponential index of PLSuperExpCutoff Abdollahi+2022 |
| FGL_PLEC_EXPINDEX_ERR | float64 | None | Uncertainty of FGL_PLEC_EXPINDEX |
| FGL_PLEC_EPEAK | float64 | MeV | Peak energy of PLSuperExpCutoff fit Abdollahi+2022 |
| FGL_PLEC_EPEAK_ERR | float64 | MeV | Uncertainty of FGL_PLEC_EPEAK |
| FGL_PLEC_SIGCURV | float64 | sigma | Significance of fit improvement between Power Law and PLSuperExpCutoff Abdollahi+2022 |
| LAC_SED_CLASS | char[32] | None | SED classes listed in the 4LAC catalog by Ajello+2022 |
| LAC_HE_EPEAK | float64 | MeV | High-energy peak position listed in the 4LAC catalog by Ajello+2022 |
| LAC_HE_EPEAK_ERR | float64 | MeV | Uncertainty of LAC_HE_EPEAK |
| LAC_HE_NUFNU | float64 | MeV*cm^(-2)*s^(-1) | High-energy peak flux listed in the 4LAC catalog by Ajello+2022 |
| LAC_HE_NUFNU_ERR | float64 | MeV*cm^(-2)*s^(-1) | Uncertainty of LAC_HE_NUFNU |
| LAC_LE_FREQ | float64 | Hz | Low-energy peak position listed in the 4LAC catalog by Ajello+2022 |
| LAC_LE_NUFNU | float64 | erg*cm^(-2)*s^(-1) | Low-energy peak flux listed in the 4LAC catalog by Ajello+2022 |
| RFC_SRC_NAME | char[32] | None | Name of source in exttt{RFC} catalog Petrov+2025 |
| RFC_SBAND_RES | float64 | Jy | Total S-band flux density integrated over entire map Petrov+2025 |
| RFC_SUPPER_RES | char[32] | None | Blank for valid RFC_SBAND_RES values, - for invalid and < for upper limits Petrov+2025 |
| RFC_SBAND_UNRES | float64 | Jy | Unresolved S-band flux density at long VLBA baselines Petrov+2025 |
| RFC_SUPPER_UNRES | char[32] | None | Blank for valid RFC_SBAND_UNRES values, - for invalid and < for upper limits Petrov+2025 |
| RFC_CBAND_RES | float64 | Jy | Total C-band flux density integrated over entire map Petrov+2025 |
| RFC_CUPPER_RES | char[32] | None | Blank for valid RFC_CBAND_RES values, - for invalid and < for upper limits Petrov+2025 |
| RFC_CBAND_UNRES | float64 | Jy | Unresolved C-band flux density at long VLBA baselines Petrov+2025 |
| RFC_CUPPER_UNRES | char[32] | None | Blank for valid RFC_CBAND_UNRES values, - for invalid and < for upper limits Petrov+2025 |
| RFC_XBAND_RES | float64 | Jy | Total X-band flux density integrated over entire map Petrov+2025 |
| RFC_XUPPER_RES | char[32] | None | Blank for valid RFC_XBAND_RES values, - for invalid and < for upper limits Petrov+2025 |
| RFC_XBAND_UNRES | float64 | Jy | Unresolved X-band flux density at long VLBA baselines Petrov+2025 |
| RFC_XUPPER_UNRES | char[32] | None | Blank for valid RFC_XBAND_UNRES values, - for invalid and < for upper limits Petrov+2025 |
| RFC_UBAND_RES | float64 | Jy | Total U-band flux density integrated over entire map Petrov+2025 |
| RFC_UUPPER_RES | char[32] | None | Blank for valid RFC_UBAND_RES values, - for invalid and < for upper limits Petrov+2025 |
| RFC_UBAND_UNRES | float64 | Jy | Unresolved U-band flux density at long VLBA baselines Petrov+2025 |
| RFC_UUPPER_UNRES | char[32] | None | Blank for valid RFC_UBAND_UNRES values, - for invalid and < for upper limits Petrov+2025 |
| RFC_KBAND_RES | float64 | Jy | Total K-band flux density integrated over entire map Petrov+2025 |
| RFC_KUPPER_RES | char[32] | None | Blank for valid RFC_KBAND_RES values, - for invalid and < for upper limits Petrov+2025 |
| RFC_KBAND_UNRES | float64 | Jy | Unresolved K-band flux density at long VLBA baselines Petrov+2025 |
| RFC_KUPPER_UNRES | char[32] | None | Blank for valid RFC_KBAND_UNRES values, - for invalid and < for upper limits Petrov+2025 |
| TANAMI_SRC_NAME | char[32] | None | Name within TANAMI program Ojha+2010, Mueller+2018 |
| TANAMI_CLASS | char[32] | None | Class given by TANAMI program Ojha+2010, Mueller+2018 |
| TANAMI_FLUX | float64 | Jy | Flux density at 8.4 GHz from TANAMI program Ojha+2010, Mueller+2018 |
| MOJAVE_SRC_NAME | char[32] | None | Name of source in the MOJAVE program Lister+2021, Homan+2021 |
| MOJAVE_CLASS | char[32] | None | Class as listed by MOJAVE Lister+2021, Homan+2021 |
| MOJAVE_FLUX | float64 | mJy | Flux density at 15 GHz from MOJAVE Lister+2021, Homan+2021 |
| N_MATCH | float64 | None | Number of potential counterparts Salvato+2025 |
| LS10_SEP | float64 | arcsec | Angular separation between BLAZE catalog and LS10 source |
| LS10_USE | float64 | None | 1 for agreement on the counterpart with Salvato+2025, 0 otherwise |
| LS10_RELEASE | float64 | None | LS10 release of counterpart Salvato+2025 |
| LS10_BRICKID | float64 | None | LS10 brick ID of counterpart Salvato+2025 |
| LS10_OBJID | float64 | None | LS10 object ID of counterpart Salvato+2025 |
| LS10_RA | float64 | deg | Right ascension of LS10 counterpart Salvato+2025 |
| LS10_DEC | float64 | deg | Declination of LS10 counterpart Salvato+2025 |
| LS10_Xray_proba | float64 | None | Probability of LS10 counterpart being an X-ray emitter Salvato+2025 |
| LS10_FULLID | char[18] | None | LS10 catalog ID Salvato+2025 |
| ERO_LS10_FULLID | char[48] | None | Combined eROSITA and LS10 catalog ID Salvato+2025 |
| LS10_RA_IVAR | float32 | deg^(-2) | Inverse variance of LS10_RA |
| LS10_DEC_IVAR | float32 | deg^(-2) | Inverse variance of LS10_DEC |
| SEPARATION_LS10_ERO | float32 | arcsec | Separation between LS10 counterpart and eROSITA position Salvato+2025 |
| NCAT | float64 | None | Number of catalogs matched Salvato+2025 |
| DIST_BAYESFACTOR | float32 | None | Logarithm of ratio from prior and posterior distance matching Salvato+2025 |
| DIST_POST | float32 | None | Distance between posterior probability of a match compared to no matches Salvato+2025 |
| BIAS_LS10_XRAY_PROBA | float32 | None | Probability of counterpart being an X-ray emitter Salvato+2025 |
| P_SINGLE | float32 | None | Similar to DIST_POST including weighting by prior Salvato+2025 |
| P_ANY | float32 | None | Probability of any found match being correct Salvato+2025 |
| P_I | float32 | None | Match probability Salvato+2025 |
| MATCH_FLAG | float64 | None | Set to 1 for most probable match, 2 for other matches Salvato+2025 |
| TYPE | char[3] | None | LS10 morphology model given by S26 |
| LS10_DCHISQ | char[62] | None | Difference in chi^2 between successively more-complex model fits separated by '_' Salvato+2025 |
| EBV | float32 | mag | E(B-V) at source position Salvato+2025 |
| FLUX_G | float32 | nanomaggy | LS10 band G flux Salvato+2025 |
| FLUX_IVAR_G | float32 | nanomaggy^(-2) | Inverse variance of FLUX_G |
| MW_TRANSMISSION_G | float32 | None | LS10 Galactic transmission at position of source in band G Salvato+2025 |
| FLUX_R | float32 | nanomaggy | LS10 band R flux Salvato+2025 |
| FLUX_IVAR_R | float32 | nanomaggy^(-2) | Inverse variance of FLUX_R |
| MW_TRANSMISSION_R | float32 | None | LS10 Galactic transmission at position of source in band R Salvato+2025 |
| FLUX_I | float32 | nanomaggy | LS10 band I flux Salvato+2025 |
| FLUX_IVAR_I | float32 | nanomaggy^(-2) | Inverse variance of FLUX_I |
| MW_TRANSMISSION_I | float32 | None | LS10 Galactic transmission at position of source in band I Salvato+2025 |
| FLUX_Z | float32 | nanomaggy | LS10 band Z flux Salvato+2025 |
| FLUX_IVAR_Z | float32 | nanomaggy^(-2) | Inverse variance of FLUX_Z |
| MW_TRANSMISSION_Z | float32 | None | LS10 Galactic transmission at position of source in band Z Salvato+2025 |
| FLUX_W1 | float32 | nanomaggy | LS10 band W1 flux Salvato+2025 |
| FLUX_IVAR_W1 | float32 | nanomaggy^(-2) | Inverse variance of FLUX_W1 |
| MW_TRANSMISSION_W1 | float32 | None | LS10 Galactic transmission at position of source in band W1 Salvato+2025 |
| FLUX_W2 | float32 | nanomaggy | LS10 band W2 flux Salvato+2025 |
| FLUX_IVAR_W2 | float32 | nanomaggy^(-2) | Inverse variance of FLUX_W2 |
| MW_TRANSMISSION_W2 | float32 | None | LS10 Galactic transmission at position of source in band W2 Salvato+2025 |
| FLUX_W3 | float32 | nanomaggy | LS10 band W3 flux Salvato+2025 |
| FLUX_IVAR_W3 | float32 | nanomaggy^(-2) | Inverse variance of FLUX_W3 |
| MW_TRANSMISSION_W3 | float32 | None | LS10 Galactic transmission at position of source in band W3 Salvato+2025 |
| FLUX_W4 | float32 | nanomaggy | LS10 band W4 flux Salvato+2025 |
| FLUX_IVAR_W4 | float32 | nanomaggy^(-2) | Inverse variance of FLUX_W4 |
| MW_TRANSMISSION_W4 | float32 | None | LS10 Galactic transmission at position of source in band W4 Salvato+2025 |
| ANYMASK_G | int16 | None | Bitmask information if in any image of band G the central pixel satisfies the LS10 catalog criteria Salvato+2025 |
| ALLMASK_G | int16 | None | Bitmask information if in all image of band G the central pixel satisfies the LS10 catalog criteria Salvato+2025 |
| PSFSIZE_G | float32 | arcsec | Size of FWHM of the LS10 PSF in band G Salvato+2025 |
| PSFDEPTH_G | float32 | nanomaggy^(-2) | LS10 5sigma detection limit for band G Salvato+2025 |
| GALDEPTH_G | float32 | nanomaggy^(-2) | Same as PSFSIZE_G assuming a galaxy Salvato+2025 |
| ANYMASK_R | int16 | None | Bitmask information if in any image of band R the central pixel satisfies the LS10 catalog criteria Salvato+2025 |
| ALLMASK_R | int16 | None | Bitmask information if in all image of band R the central pixel satisfies the LS10 catalog criteria Salvato+2025 |
| PSFSIZE_R | float32 | arcsec | Size of FWHM of the LS10 PSF in band R Salvato+2025 |
| PSFDEPTH_R | float32 | nanomaggy^(-2) | LS10 5sigma detection limit for band R Salvato+2025 |
| GALDEPTH_R | float32 | nanomaggy^(-2) | Same as PSFSIZE_R assuming a galaxy Salvato+2025 |
| ANYMASK_I | int16 | None | Bitmask information if in any image of band I the central pixel satisfies the LS10 catalog criteria Salvato+2025 |
| ALLMASK_I | int16 | None | Bitmask information if in all image of band I the central pixel satisfies the LS10 catalog criteria Salvato+2025 |
| PSFSIZE_I | float32 | arcsec | Size of FWHM of the LS10 PSF in band I Salvato+2025 |
| PSFDEPTH_I | float32 | nanomaggy^(-2) | LS10 5sigma detection limit for band I Salvato+2025 |
| GALDEPTH_I | float32 | nanomaggy^(-2) | Same as PSFSIZE_I assuming a galaxy Salvato+2025 |
| ANYMASK_Z | int16 | None | Bitmask information if in any image of band Z the central pixel satisfies the LS10 catalog criteria Salvato+2025 |
| ALLMASK_Z | int16 | None | Bitmask information if in all image of band Z the central pixel satisfies the LS10 catalog criteria Salvato+2025 |
| PSFSIZE_Z | float32 | arcsec | Size of FWHM of the LS10 PSF in band Z Salvato+2025 |
| PSFDEPTH_Z | float32 | nanomaggy^(-2) | LS10 5sigma detection limit for band Z Salvato+2025 |
| GALDEPTH_Z | float32 | nanomaggy^(-2) | Same as PSFSIZE_Z assuming a galaxy Salvato+2025 |
| WISEMASK_W1 | bool | None | Bitmask information for band W1 Salvato+2025 |
| PSFDEPTH_W1 | float32 | nanomaggy^(-2) | LS10 5sigma detection limit for band W1 Salvato+2025 |
| W1_MAG_AB | float32 | mag | WISE W1 magnitude in AB system calculated from FLUX_W1 using MW_TRANSMISSION_W1 |
| W1_MAG | float32 | mag | WISE W1 magnitude in the Vega system calculated from FLUX_W1 using MW_TRANSMISSION_W1 |
| WISEMASK_W2 | bool | None | Bitmask information for band W2 Salvato+2025 |
| PSFDEPTH_W2 | float32 | nanomaggy^(-2) | LS10 5sigma detection limit for band W2 Salvato+2025 |
| W2_MAG_AB | float32 | mag | WISE W2 magnitude in AB system calculated from FLUX_W2 using MW_TRANSMISSION_W2 |
| W2_MAG | float32 | mag | WISE W2 magnitude in the Vega system calculated from FLUX_W2 using MW_TRANSMISSION_W2 |
| W3_MAG_AB | float32 | mag | WISE W3 magnitude in AB system calculated from FLUX_W3 using MW_TRANSMISSION_W3 |
| W3_MAG | float32 | mag | WISE W3 magnitude in the Vega system calculated from FLUX_W3 using MW_TRANSMISSION_W3 |
| W4_MAG_AB | float32 | mag | WISE W4 magnitude in AB system calculated from FLUX_W4 using MW_TRANSMISSION_W4 |
| W4_MAG | float32 | mag | WISE W4 magnitude in the Vega system calculated from FLUX_W4 using MW_TRANSMISSION_W4 |
| SHAPE_R | float32 | arcsec | LS10 half-light radius for given TYPE Salvato+2025 |
| SHAPE_R_IVAR | float32 | arcsec^(-2) | Inverse variance of SHAPE_R |
| SHAPE_E1 | float32 | arcsec | LS10 ellipticity component E1 of galaxy Salvato+2025 |
| SHAPE_E1_IVAR | float32 | arcsec^(-2) | Inverse variance of SHAPE_E1 |
| SHAPE_E2 | float32 | arcsec | LS10 ellipticity component E2 of galaxy Salvato+2025 |
| SHAPE_E2_IVAR | float32 | arcsec^(-2) | Inverse variance of SHAPE_E2 |
| SERSIC | float32 | None | LS10 power law index of Sersic profile and associated inverse variance Salvato+2025 |
| SERSIC_IVAR | float32 | None | Inverse variance of SERSIC |
| REF_CAT | char[2] | None | LS10 reference catalog for stars Salvato+2025 |
| REF_ID | int64 | None | LS10 reference catalog id for star Salvato+2025 |
| REF_EPOCH | float32 | a | LS10 reference epoch of REF_CAT Salvato+2025 |
| GAIA_PHOT_G_MEAN_MAG | float32 | mag | LS10 Gaia G band magnitude Salvato+2025 |
| GAIA_PHOT_G_MEAN_FLUX_OVER_ERROR | float32 | None | LS10 Gaia G band signal-to-noise ratio Salvato+2025 |
| GAIA_PHOT_BP_MEAN_MAG | float32 | mag | LS10 Gaia BP band magnitude Salvato+2025 |
| GAIA_PHOT_BP_MEAN_FLUX_OVER_ERROR | float32 | None | LS10 Gaia BP band signal-to-noise ratio Salvato+2025 |
| GAIA_PHOT_RP_MEAN_MAG | float32 | mag | LS10 Gaia RP band magnitude Salvato+2025 |
| GAIA_PHOT_RP_MEAN_FLUX_OVER_ERROR | float32 | None | LS10 Gaia RP band signal-to-noise ratio Salvato+2025 |
| GAIA_ASTROMETRIC_EXCESS_NOISE | float32 | None | LS10 Gaia astrometric excess noise Salvato+2025 |
| GAIA_PHOT_BP_RP_EXCESS_FACTOR | float32 | None | LS10 Gaia BP/RP excess factor Salvato+2025 |
| GAIA_ASTROMETRIC_SIGMA5D_MAX | float32 | arcsec | LS10 Gaia longest semi-major axis of the 5-d error ellipsoid Salvato+2025 |
| GAIA_DUPLICATED_SOURCE | char[5] | None | LS10 Gaia duplicate source flag Salvato+2025 |
| INALLLS10 | float64 | None | Nominal LS10 survey depth reached in all bands Salvato+2025 |
| INANYLS10 | float64 | None | Nominal LS10 survey depth reached in one band Salvato+2025 |
| DERED_MAG_W1 | float64 | mag | Dereddend magnitude of W1 band Salvato+2025 |
| DERED_MAG_W2 | float64 | mag | Dereddend magnitude of W2 band Salvato+2025 |
| DERED_MAG_G | float64 | mag | Dereddend magnitude of G band Salvato+2025 |
| DERED_MAG_R | float64 | mag | Dereddend magnitude of R band Salvato+2025 |
| DERED_MAG_Z | float64 | mag | Dereddend magnitude of Z band Salvato+2025 |
| SOFTFLUX_S | float64 | erg*cm^(-2)*s^(-1) | eROSITA flux in 0.5-2.0 keV band Salvato+2025 |
| SALVATO18_W1_X_LINEDISTANCE | float64 | None | Distance from separation line between Galactic and extra-galactic sources in the W1-X-ray plane Salvato+2025 |
| SALVATO22_ZW1_GR_LINEDISTANCE | float64 | None | Distance from separation line between Galactic and extra-galactic sources in the ZW1-GR plane Salvato+2025 |
| G_MINUS_R | float64 | mag | G-R color Salvato+2025 |
| Z_MINUS_W1 | float64 | mag | Z-W1 color Salvato+2025 |
| W1_MINUS_W2 | float64 | mag | W1-W2 color Salvato+2025 |
| HAS_SALVATO18_AGN_COLORS | char[5] | None | Information if source has colors consistent with being an AGN based on Salvato+2018, from S26 |
| GAIA_MOVING_5SIGMA | char[5] | None | Information if source shows movement at 5sigma significance in Gaia Salvato+2025 |
| HAS_SALVATO22_AGN_COLORS | char[5] | None | Information if source has colors consistent with being an AGN based on Salvato+2022, from S26. |
| SALVATO_MAIN_ID_SIMBAD | char[31] | None | SIMBAD ID Salvato+2025 |
| SALVATO_RA_SIMBAD | float64 | deg | Right ascension from SIMBAD Salvato+2025 |
| SALVATO_DEC_SIMBAD | float64 | deg | Declination from SIMBAD Salvato+2025 |
| EXGAL_PROB_GAIA_STAREX | float64 | None | Probability of source being extra-galactic by STAREX with Gaia data Salvato+2025 |
| EXGAL_PROB_STAREX | float64 | None | Probability of source being extra-galactic by STAREX without Gaia data Salvato+2025 |
| CLASS_GAL_EXGAL | float64 | None | Galactic/extra-galactic class assigned by S26 |
| SALVATO_HECATE | float64 | None | 1 for sources within HECATE source Salvato+2025 |
| SALVATO_HEC_OBJNAME | char[30] | None | Name of HECATE source Salvato+2025 |
| SALVATO_HEC_RA | float64 | deg | Right ascension of HECATE source Salvato+2025 |
| SALVATO_HEC_DEC | float64 | deg | Declination of HECATE source Salvato+2025 |
| SALVATO_HEC_R1 | float32 | arcmin | Semi major axis of HECATE source Salvato+2025 |
| SALVATO_HEC_R2 | float32 | arcmin | Semi minor axis of HECATE source Salvato+2025 |
| SALVATO_HEC_PA | float32 | deg | Position angle of HECATE source Salvato+2025 |
| PURITY6 | float64 | None | Purity obtained for DET_LIKE_0> at source position Salvato+2025 |
| COMPLETENESS6 | float64 | None | Purity obtained for DET_LIKE_0> at source position Salvato+2025 |
| COMPUR6 | float64 | None | Purity obtained for DET_LIKE_0> at source position Salvato+2025 |
| THRESHOLD6 | float64 | None | Purity obtained for DET_LIKE_0> at source position Salvato+2025 |
| PURITY7 | float64 | None | Completeness obtained for DET_LIKE_0> at source position Salvato+2025 |
| COMPLETENESS7 | float64 | None | Completeness obtained for DET_LIKE_0> at source position Salvato+2025 |
| COMPUR7 | float64 | None | Completeness obtained for DET_LIKE_0> at source position Salvato+2025 |
| THRESHOLD7 | float64 | None | Completeness obtained for DET_LIKE_0> at source position Salvato+2025 |
| PURITY8 | float64 | None | Intersection between completeness and purity obtained for DET_LIKE_0> at source position Salvato+2025 |
| COMPLETENESS8 | float64 | None | Intersection between completeness and purity obtained for DET_LIKE_0> at source position Salvato+2025 |
| COMPUR8 | float64 | None | Intersection between completeness and purity obtained for DET_LIKE_0> at source position Salvato+2025 |
| THRESHOLD8 | float64 | None | Intersection between completeness and purity obtained for DET_LIKE_0> at source position Salvato+2025 |
| Z_PHOTO_S3L | float64 | None | 3 sigma lower value of photometric redshift Salvato+2025 |
| Z_PHOTO_S3U | float64 | None | 3 sigma upper value of photometric redshift Salvato+2025 |
| Z_PHOTO_S1L | float64 | None | 1 sigma lower value of photometric redshift Salvato+2025 |
| Z_PHOTO_S1U | float64 | None | 1 sigma upper value of photometric redshift Salvato+2025 |
| Z_PHOTO | float64 | None | Value of photometric redshift Salvato+2025 |
| Z_SPEC | float64 | None | Spectroscopic redshift from Kluge+2024 provided by S26 |
| Z_SPEC_REF | char[38] | None | Source with Z_SPEC from Kluge+2024 provided by S26 |
| Z_ABC | float64 | None | Redshift listed in the ABC catalog Paggi+2020 |
| Z_3HSP | float64 | None | Redshift listed in the 3HSP catalog Chang+2019 |
| Z_F_3HSP | float64 | None | Redshift flag listed in the 3HSP catalog Chang+2019 |
| Z_MILLIQUAS | float64 | None | Redshift listed in the Milliquas catalog Flesch+2023 |
| Z_HIGHZ | float64 | None | Redshift listed in the HighZ sample |
| Z_HIGHZ_REF | char[56] | None | Paper reference for high-redshift sources |
| Z_MOJAVE | float64 | None | Redshift listed in MOJAVE |
| Z_4LAC | float64 | None | Redshift listed in the 4LAC catalog Ajello+2022 |
| Z_BZCAT | float64 | None | Redshift listed from the BZCAT catalog Massaro+2015 |
| Z_U_BZCAT | char[32] | None | Redshift flag from the BZCAT catalog Massaro+2015 |
| Z_CGRABS | float64 | None | Redshift listed in the CGRaBS catalog Healey+2008 |
| Z_F_CGRABS | char[32] | None | Redshift flag listed in CGRaBS catalog Healey+2008 |
| Z_VERONCAT | float64 | None | Redshift listed in the VERONCAT catalog Veron-Cetty+2010 |
| Z_VERONCAT_QSO | float64 | None | Redshift listed in the VERONCAT QSO catalog Veron-Cetty+2010 |
| Z_SIMBAD | float64 | None | Redshift listed on SIMBAD |
| Z_MASTER | float64 | None | Reliable redshift adopted for population studies |
| Z_MASTER_REF | char[13] | None | Source of Z_MASTER |
| Z_MASTER_PHOTO | float64 | None | Reliable redshift including the photometric ones from Salvato+2025 |
| Z_MASTER_PHOTO_REF | char[13] | None | Source where Z_MASTER_PHOTO was taken from |
| XRAY_LUM_PHOTO_1 | float64 | erg*s^(-1) | X-ray luminosity calculated from the fixed Gamma_X=2.0 fit and Z_MASTER_PHOTO in 0.2-2.3 keV band |
| XRAY_LUM_PHOTO_1_ERR | float32[1PE(2)] | erg*s^(-1) | Uncertainties of XRAY_LUM_PHOTO_1 |
| XRAY_LUM_1 | float64 | erg*s^(-1) | X-ray luminosity calculated from the fixed Gamma_X=2.0 fit and Z_MASTER in 0.2-2.3 keV band |
| XRAY_LUM_1_ERR | float32[1PE(2)] | erg*s^(-1) | Uncertainties of XRAY_LUM_1 |
| ALPHA_XG | float64 | None | alpha_XGamma using PWL20_FLUX_UNABS_0 and FGL_FLUX_A |
| ALPHA_XG_ERR | float64 | None | Uncertainty of ALPHA_XG |
| ALPHA_IRX | float64 | None | alpha_IRX using PWL20_FLUX_UNABS_0 and FLUX_W1 combined with MW_TRANSMISSION_W1 |
| ALPHA_IRX_ERR | float64 | None | Uncertainty, including a systematic uncertainty, of ALPHA_IRX |
| ALPHA_OX | float64 | None | alpha_OX using PWL20_FLUX_UNABS_0 and FLUX_R combined with MW_TRANSMISSION_R |
| ALPHA_OX_ERR | float64 | None | Uncertainty, including a systematic uncertainty, of ALPHA_OX |
| ALPHA_RX | float64 | None | alpha_RX using PWL20_FLUX_UNABS_0 and RFC_XBAND_RES |
| ALPHA_RX_ERR | float64 | None | Uncertainty of ALPHA_RX |
| ALPHA_TANAMI | float64 | None | alpha_TANAMI using PWL20_FLUX_UNABS_0 and TANAMI_FLUX |
| ALPHA_TANAMI_ERR | float64 | None | Uncertainty of ALPHA_TANAMI |
| ALPHA_MOJAVE | float64 | None | alpha_MOJAVE using PWL20_FLUX_UNABS_0 and MOJAVE_FLUX |
| ALPHA_MOJAVE_ERR | float64 | None | Uncertainty of ALPHA_MOJAVE |
| SIMBAD_SRC_NAME | char[35] | None | Name of closest source match on SIMBAD |
| SIMBAD_TYPE | char[19] | None | Type of source, if a blazar or AGN classification or a more precise type is listed as alternative, this one is selected |
| SIMBAD_ALT_TYPES | char[133] | None | All alternate types as listed in SIMBAD |
| SIMBAD_TYPE2 | char[19] | None | Type of source as listed by SIMBAD |
| SIMBAD_ANGSEP | float64 | arcsec | Angular separation between BLAZE catalog source and SIMBAD source |
| CAMBRIDGE_SRC_NAME | char[6] | None | Name in Third Cambridge catalog of radio sources as listed in SIMBAD |
| PARKS_SRC_NAME | char[14] | None | Name in Parkes catalog of radio sources as listed in SIMBAD |
| TEXAS_SRC_NAME | char[12] | None | Name in Texas survey of radio sources as listed in SIMBAD |
| EINSTEIN_SRC_NAME | char[7] | None | Name in Einstein 2E catalog of IPC X-Ray sources as listed in SIMBAD |
| COMMON_SRC_NAME | char[14] | None | Most commonly used source name from the above as listed in SIMBAD |
| BZCAT_RMAG | float64 | mag | R-band magnitude from the BZCAT catalog Massaro+2015 |
| BZCAT_FR | float64 | mJy | Radio flux density at 1.4 GHz or if unknown at 0.843 GHz from the BZCAT catalog Massaro+2015 |
| BZCAT_F143 | float64 | mJy | Flux density at 143 GHz from the Planck Compact Source Catalog Public Release 1 from the BZCAT catalog Massaro+2015 |
| BZCAT_FLUX_U | float64 | fW*m^(-2) | X-ray flux in the 0.1-2.4 keV band from the BZCAT catalog Massaro+2015 |
| BZCAT_FLUX_B | float64 | ph*cm^(-2)*s^(-1) | gamma-ray flux in the 1-100 GeV band from the BZCAT catalog Massaro+2015 |
| BZCAT_ALPHA_RO | float64 | None | The radio-to-optical spectral index of the blazar from the BZCAT catalog Massaro+2015 |
| XIE_MORPH_BZCAT | char[32] | None | Radio morphology for BZCAT sources as listed in Xie+2024 |
| XIE_MORPH_KDEBLLACS | char[32] | None | Radio morphology for KDEBLLACS sources as listed in Xie+2024 |
| XIE_MORPH_WIBRALS | char[32] | None | Radio morphology for WIBRALS sources as listed in Xie+2024 |
Haemmerich et al., A&A, 2026, accepted
Abdollahi et al. 2022, ApJS, 260, 53
Ajello et al. 2022, ApJS, 263, 24
Boller et al. 2016, A&A, 588, A103
Chang et al. 2019, A&A,632, A77
D’Abrusco et al. 2019, ApJS, 242, 4
Evans et al. 2020, ApJS, 247, 54
Flesch 2023, OJAp, 6, 49
Giommi et al. 2019, A&A, 631, A116
Healey et al. 2008, ApJS, 175, 97
HI4PI Collaboration. 2016, A&A, 594, A116
Homan et al. 2021, ApJ, 923, 67
Itoh et al. 2020, ApJ, 901, 3
Kaastra 2017, A&A, 605, A51
Kluge et al. 2024, A&A, 688, A210
Lien et al. 2025, ApJ, 989, 161
Lister et al. 2021, ApJ, 923, 30
Marcotulli et al. 2025, ApJ, 979, L6
Massaro et al. 2015, Ap&SS, 357, 75
Merloni et al. 2024, A&A, 682, A34
Middei et al. 2022, MNRAS, 514, 3179
Müller et al. 2018, A&A, 610, A1
Ojha et al. 2010, A&A, 519, A45
Paggi et al. 2020, A&A, 641, A62
Petrov 2025, ApJS, 276, 38
Salvato et al. 2018, MNRAS, 473, 4937
Salvato et al. 2022, A&A, 661, A3
Salvato et al. 2026, A&A, 704, A344
Sbarrato et al. 2026, A&A, submitted (arXiv:2603.24659)
Véron-Cetty et al. 2010, A&A, 518, A10
Xie et al. 2024, ApJ, 964, 98
This work is based on data from eROSITA, the soft X-ray instrument aboard SRG, a joint Russian-German science mission supported by the Russian Space Agency (Roskosmos), in the interests of the Russian Academy of Sciences represented by its Space Research Institute (IKI), and the Deutsches Zentrum für Luft- und Raumfahrt (DLR). The SRG spacecraft was built by Lavochkin Association (NPOL) and its subcontractors, and is operated by NPOL with support from the Max Planck Institute for Extraterrestrial Physics (MPE). The development and construction of the eROSITA X-ray instrument was led by MPE, with contributions from the Dr. Karl Remeis Observatory Bamberg & ECAP (FAU Erlangen-Nuernberg), the University of Hamburg Observatory, the Leibniz Institute for Astrophysics Potsdam (AIP), and the Institute for Astronomy and Astrophysics of the University of Tübingen, with the support of DLR and the Max Planck Society. The Argelander Institute for Astronomy of the University of Bonn and the Ludwig Maximilians Universität Munich also participated in the science preparation for eROSITA.The eROSITA data shown here were processed using the eSASS/NRTA software system developed by the German eROSITA consortium.