Open Access
Table D.1
eRASS1 catalogs column desciption. All errors are provided as 68% confidence intervals (1 − σ).
Column | Units | Description |
---|---|---|
IAUNAME | String containing the official IAU name of the source | |
DETUID | String unique detection ID | |
SKYTILE | Sky tile ID | |
ID_SRC | Source ID in each sky tile. Use SKYTILE+ID_SRC to identify the corresponding source products | |
UID | Integer unique detection ID. It equals CatID×1011 +SKYTILE×105+ID_SRC, where CatID is 1 for the 1B detected Main and Supp catalogs and 2 for the 3B detected Hard catalog. | |
UID_Hard | 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. Only in the 1B Main and Supp catalogs | |
UID_1B | Main or Supp catalog UID of the source with a strong association, or -UID if the association is weak. 0 means no counterpart found in the 1B catalogs. Only in the Hard catalog | |
ID_CLUSTER | Group ID of simultaneously fitted sources | |
RA | deg | Right ascension (ICRS), corrected |
DEC | deg | Declination (ICRS), corrected |
RA_RAW | deg | Right ascension (ICRS), uncorrected |
DEC_RAW | deg | Declination (ICRS), uncorrected |
RA_LOWERR | arcsec | 1-σ lower error of RA |
RA_UPERR | arcsec | 1-σ upper error of RA |
DEC_LOWERR | arcsec | 1-σ lower error of DEC |
DEC_UPERR | arcsec | 1-σ upper error of DEC |
RADEC_ERR | arcsec | Combined positional error, raw output from PSF fitting |
POS_ERR | arcsec | 1-σ position uncertainty |
LII | deg | Galactic longitude |
BII | deg | Galactic latitude |
ELON | deg | Ecliptic longitude |
ELAT | deg | Ecliptic latitude |
MJD | Modified Julian Date of the observation of the source nearest to the optical axis of the telescope | |
MJD_MIN | Modified Julian Date of the first observation of a source | |
MJD_MAX | Modified Julian Date of the last observation of a source | |
EXT | arcsec | Source extent parameter |
EXT_ERR | arcsec | 1-σ error of EXT |
EXT_LOWERR | arcsec | 1-σ lower error of EXT |
EXT_UPERR | arcsec | 1-σ upper error of EXT |
EXT_LIKE | Extent likelihood | |
DET_LIKE_n | Detection likelihood. 1B: n=0; 3B: n=0,1,2,3 | |
ML_CTS_n | cts | Source net counts. 1B: n=1,P[1-9]; 3B: n=0,1,2,3 |
ML_CTS_ERR_n | cts | 1-σ combined counts error. 1B: n=1,P[1-9]; 3B: n=0,1,2,3 |
ML_CTS_LOWERR_n | cts | 1-σ lower counts error. 1B: n=1,P[1-9]; 3B: n=1,2,3 |
ML_CTS_UPERR_n | cts | 1-σ upper counts error. 1B: n=1,P[1-9]; 3B: n=1,2,3 |
ML_RATE_n | cts/s | Source count rate. 1B: n=1,P[1-9]; 3B: n=0,1,2,3 |
ML_RATE_ERR_n | cts/s | 1-σ combined count rate error. 1B: n=1,P[1-9]; 3B: n=0,1,2,3 |
ML_RATE_LOWERR_n | cts/s | 1-σ lower count rate error. 1B: n=1,P[1-9]; 3B: n=1,2,3 |
ML_RATE_UPERR_n | cts/s | 1-σ upper count rate error. 1B: n=1,P[1-9]; 3B: n=1,2,3 |
ML_FLUX_n | erg/cm2/s | Source flux. 1B: n=1,P[1-9]; 3B: n=0,1,2,3 |
ML_FLUX_ERR_n | erg/cm2/s | 1-σ combined flux error. 1B: n=1,P[1-9]; 3B: n=0,1,2,3 |
ML_FLUX_LOWERR_n | erg/cm2/s | 1-σ lower flux error. 1B: n=1,P[1-9]; 3B: n=1,2,3 |
ML_FLUX_UPERR_n | erg/cm2/s | 1-σ upper flux error. 1B: n=1,P[1-9]; 3B: n=1,2,3 |
ML_EXP_n | s | Vignetted exposure time at the source position. 1B: n=1,P[1-9]; 3B: n=1,2,3 |
ML_BKG_n | cts/arcmin2 | Background at the source position. 1B: n=1,P[1-9]; 3B: n=0,1,2,3 |
ML_EEF_n | Encloded energy fraction. 1B: n=1,P[1-9]; 3B: n=1,2,3 | |
APE_CTS_n | cts | Total counts extracted within the aperture. 1B: n=1,P[1-9],S; 3B: n=1,2,3 |
APE_EXP_n | s | Exposure map value at the given position. 1B: n=1,P[1-9],S; 3B: n=1,2,3 |
APE_BKG_n | cts | Background counts extracted within the aperture, excluding nearby sources using the source map. 1B: n=1,P[1-9],S; 3B: n=1,2,3 |
APE_RADIUS_n | pixels | Extraction radius in pixels (4"). 1B: n=1,P[1-9]; 3B: n=1,2,3 |
APE_POIS_n | Poisson probability that the extracted counts (APE_CTS) are a background fluctuation. 1B: n=1,P[1-9],S; 3B: n=1,2,3 | |
FLAG_SP_SNR | Source may lie within an overdense region near a supernova remnant | |
FLAG_SP_BPS | Source may lie within an overdense region near a bright point source | |
FLAG_SP_SCL | Source may lie within an overdense region near a stellar cluster | |
FLAG_SP_LGA | Source may lie within an overdense region near a local large galaxy | |
FLAG_SP_GC_CONS | Source may lie within an overdense region near a galaxy cluster | |
FLAG_NO_RADEC_ERR | Source contained no RA_DEC_ERR in the pre-processed version of the catalogue | |
FLAG_NO_CTS_ERR | Source contained no ML_CTS_0_ERR in the pre-processed version of the catalogue | |
FLAG_NO_EXT_ERR | Source contained no EXT_ERR in the pre-processed version of the catalogue | |
FLAG_OPT | Source matched within 15″ with a bright optical star, likely contaminated by optical loading |
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