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Data Model: eRASS1_Hard

General description
Hard eRASS1 X-ray catalogue from the 3B (2.3-5 keV) eSASS source detection run, as described in Merloni et al. (2024)


Filename:
eRASS1_Hard.v1.0.fits

Approximate size
2 MB

File type
FITS

Generated by product
eSASS

Sections

Content of the page.

HDU0: PRIMARY

HDU Type
IMAGE
HDU Size
0 bytes

HDU1: CATALOGUE

Catalogue table

HDU Type
BINARY TABLE
HDU Size
2 MB
Binary Table Caption for HDU1
NameTypeUnitDescription
IAUNAME char[23] None String containing the official IAU name of the source
DETUID char[32] None String unique detection ID
SKYTILE int32 None Sky tile ID
ID_SRC int32 None Source ID in each sky tile. Use SKYTILE+ID_SRC to identify the corresponding source products
UID int64 None Integer unique detection ID. It equals CatID*10^11+SKYTILE*10^5+ID_SRC, where catID is 1 for the 1B detected Main and Supp catalogs and 2 for the 3B detected Hard catalog
UID_1B int64 None 1B catalog UID of the source with a strong association, or -UID if the association is weak
ID_CLUSTER int32 None Group ID of simultaneously fitted sources
RA float64 deg Right ascension (ICRS), corrected
DEC float64 deg Declination (ICRS), corrected
RA_RAW float64 deg Right ascension (ICRS), uncorrected
DEC_RAW float64 deg Declination (ICRS), uncorrected
RA_LOWERR float32 arcsec 1-sigma lower error on RA
RA_UPERR float32 arcsec 1-sigma upper error on RA
DEC_LOWERR float32 arcsec 1-sigma lower error on DEC
DEC_UPERR float32 arcsec 1-sigma upper error on DEC
POS_ERR float32 arcsec 1-sigma positional uncertainty
RADEC_ERR float32 arcsec Combined positional error, raw output from PSF fitting
LII[1] float64 deg Galactic longitude
BII[1] float64 deg Galactic latitude
ELON float64 deg Ecliptic longitude
ELAT float64 deg Ecliptic latitude
MJD float32 d Modified Julian Date of the observation of the source nearest to the optical axis of the telescope
MJD_MIN float32 d Modified Julian Date of the first observation of the source
MJD_MAX float32 d Modified Julian Date of the last observation of the source
EXT float32 arcsec Source Extent Parameter
EXT_ERR float32 arcsec 1-sigma error on EXT
EXT_LOWERR float32 arcsec 1-sigma lower error on EXT
EXT_UPERR float32 arcsec 1-sigma upper error on EXT
EXT_LIKE float32 None Extent likelihood
ML_CTS_0 float32 count Source net counts in 0.2-5.0 keV band
ML_CTS_ERR_0 float32 count 1-sigma combined counts error in 0.2-5.0 keV band
ML_RATE_0 float32 count s-1 Source count rate in 0.2-5.0 keV band
ML_RATE_ERR_0 float32 count s-1 1-sigma combined count rate error in 0.2-5.0 keV band
ML_FLUX_0 float32 erg s-1 cm-2 Source flux in 2.3-5.0 keV band
ML_FLUX_ERR_0 float32 erg s-1 cm-2 1-sigma combined error on flux in 0.2-5.0 keV band
DET_LIKE_0 float32 None Detection likelihood in 0.2-5.0 keV band
ML_BKG_0 float32 arcmin-2 Background at the source position in the 0.2-5.0 keV band
ML_CTS_1 float32 count Source net counts in 0.2-0.6 keV band
ML_CTS_ERR_1 float32 count 1-sigma combined counts error in 0.2-0.6 keV band
ML_CTS_LOWERR_1 float32 count 1-sigma lower counts error in 0.2-0.6 keV band
ML_CTS_UPERR_1 float32 count 1-sigma upper counts error in 0.2-0.6 keV band
ML_RATE_1 float32 count s-1 Source count rate in 0.2-0.6 keV band
ML_RATE_ERR_1 float32 count s-1 1-sigma combined count rate error in 0.2-0.6 keV band
ML_RATE_LOWERR_1 float32 count s-1 1-sigma lower count rate error in 0.2-0.6 keV band
ML_RATE_UPERR_1 float32 count s-1 1-sigma upper count rate error in 0.2-0.6 keV band
ML_FLUX_1 float32 erg s-1 cm-2 Source flux in 0.2-0.6 keV band
ML_FLUX_ERR_1 float32 erg s-1 cm-2 1-sigma combined error on flux in 0.2-0.6 keV band
ML_FLUX_LOWERR_1 float32 erg s-1 cm-2 1-sigma lower error on flux in 0.2-0.6 keV band
ML_FLUX_UPERR_1 float32 erg s-1 cm-2 1-sigma upper error on flux in 0.2-0.6 keV band
DET_LIKE_1 float32 None Detection likelihood in 0.2-0.6 keV band
ML_BKG_1 float32 arcmin-2 Background at the source position in the 0.2-0.6 keV band
ML_EXP_1 float32 s Vignetted exposure time at the source position in 0.2-0.6 keV band
ML_EEF_1 float32 None Enclosed energy fraction in 0.2-0.6 keV band
APE_CTS_1 int32 count Total counts extracted within the aperture in 0.2-0.6 keV band
APE_BKG_1 float32 count Background counts extracted within the aperture in 0.2-0.6 keV band, excluding nearby sources using the source map
APE_EXP_1 float32 s Exposure map value in 0.2-0.6 keV band at the given position
APE_RADIUS_1 float32 pix Extraction radius in pixels (4'') in the 0.2-0.6 keV band
APE_POIS_1 float32 None Poisson probability that the extracted counts (APE_CTS_1) are a background fluctuation
ML_CTS_2 float32 count Source net counts in 0.6-2.3 keV band
ML_CTS_ERR_2 float32 count 1-sigma combined counts error in 0.6-2.3 keV band
ML_CTS_LOWERR_2 float32 count 1-sigma lower counts error in 0.6-2.3 keV band
ML_CTS_UPERR_2 float32 count 1-sigma upper counts error in 0.6-2.3 keV band
ML_RATE_2 float32 count s-1 Source count rate in 0.6-2.3 keV band
ML_RATE_ERR_2 float32 count s-1 1-sigma combined count rate error in 0.6-2.3 keV band
ML_RATE_LOWERR_2 float32 count s-1 1-sigma lower count rate error in 0.6-2.3 keV band
ML_RATE_UPERR_2 float32 count s-1 1-sigma upper count rate error in 0.6-2.3 keV band
ML_FLUX_2 float32 erg s-1 cm-2 Source flux in 0.6-2.3 keV band
ML_FLUX_ERR_2 float32 erg s-1 cm-2 1-sigma combined error on flux in 0.6-2.3 keV band
ML_FLUX_LOWERR_2 float32 erg s-1 cm-2 1-sigma lower error on flux in 0.6-2.3 keV band
ML_FLUX_UPERR_2 float32 erg s-1 cm-2 1-sigma upper error on flux in 0.6-2.3 keV band
DET_LIKE_2 float32 None Detection likelihood in 0.6-2.3 keV band
ML_BKG_2 float32 arcmin-2 Background at the source position in the 0.6-2.3 keV band
ML_EXP_2 float32 s Vignetted exposure time at the source position in 0.6-2.3 keV band
ML_EEF_2 float32 None Enclosed energy fraction in 0.6-2.3 keV band
APE_CTS_2 int32 count Total counts extracted within the aperture in 0.6-2.3 keV band
APE_BKG_2 float32 count Background counts extracted within the aperture in 0.6-2.3 keV band, excluding nearby sources using the source map
APE_EXP_2 float32 s Exposure map value in 0.6-2.3 keV band at the given position
APE_RADIUS_2 float32 pix Extraction radius in pixels (4'') in the 0.6-2.3 keV band
APE_POIS_2 float32 None Poisson probability that the extracted counts (APE_CTS_2) are a background fluctuation
ML_CTS_3 float32 count Source net counts in 2.3-5.0 keV band
ML_CTS_ERR_3 float32 count 1-sigma combined counts error in 2.3-5.0 keV band
ML_CTS_LOWERR_3 float32 count 1-sigma lower counts error in 2.3-5.0 keV band
ML_CTS_UPERR_3 float32 count 1-sigma upper counts error in 2.3-5.0 keV band
ML_RATE_3 float32 count s-1 Source count rate in 2.3-5.0 keV band
ML_RATE_ERR_3 float32 count s-1 1-sigma combined count rate error in 2.3-5.0 keV band
ML_RATE_LOWERR_3 float32 count s-1 1-sigma lower count rate error in 2.3-5.0 keV band
ML_RATE_UPERR_3 float32 count s-1 1-sigma upper count rate error in 2.3-5.0 keV band
ML_FLUX_3 float32 erg s-1 cm-2 Source flux in 2.3-5.0 keV band
ML_FLUX_ERR_3 float32 erg s-1 cm-2 1-sigma combined error on flux in 2.3-5.0 keV band
ML_FLUX_LOWERR_3 float32 erg s-1 cm-2 1-sigma lower error on flux in 2.3-5.0 keV band
ML_FLUX_UPERR_3 float32 erg s-1 cm-2 1-sigma upper error on flux in 2.3-5.0 keV band
DET_LIKE_3 float32 None Detection likelihood in 2.3-5.0 keV band
ML_BKG_3 float32 arcmin-2 Background at the source position in the 2.3-5.0 keV band
ML_EXP_3 float32 s Vignetted exposure time at the source position in 2.3-5.0 keV band
ML_EEF_3 float32 None Enclosed energy fraction in 2.3-5.0 keV band
APE_CTS_3 int32 count Total counts extracted within the aperture in 2.3-5.0 keV band
APE_BKG_3 float32 count Background counts extracted within the aperture in 2.3-5.0 keV band, excluding nearby sources using the source map
APE_EXP_3 float32 s Exposure map value in 2.3-5.0 keV band at the given position
APE_RADIUS_3 float32 pix Extraction radius in pixels (4'') in the 2.3-5.0 keV band
APE_POIS_3 float32 None Poisson probability that the extracted counts (APE_CTS_3) are a background fluctuation
FLAG_SP_SNR int16 None Source may lie within an overdense region near a supernova remnant
FLAG_SP_BPS int16 None Source may lie within an overdense region near a bright point source
FLAG_SP_SCL int16 None Source may lie within an overdense region near a stellar cluste
FLAG_SP_LGA int16 None Source may lie within an overdense region near a local large galaxy
FLAG_SP_GC_CONS int16 None Source may lie within an overdense region near a galaxy cluster
FLAG_NO_RADEC_ERR int16 None Source contained no RADEC_ERR in the pre-processed version of the catalogue
FLAG_NO_EXT_ERR int16 None Source contained no EXT_ERR in the pre-processed version of the catalogue
FLAG_NO_CTS_ERR int16 None Source contained no CTS_ERR in the pre-processed version of the catalogue
FLAG_OPT int16 None Source matched within 15'' with a bright optical star, likely contaminated by optical loading

[1] The Galactic coordinates (LII and BII) are based on the raw right ascension and declination coordinates (RA_RAW and DEC_RAW). The routine used for such conversion has been found to be faulty, and therefore, the Galactic coordinates displayed in the catalogs need to be corrected by a few arcseconds. Users are encouraged to use their own coordinate conversion tools to extract corrected Galactic coordinates based on the right ascension and declination coordinates (RA and DEC), which are correct.

References

Merloni, A., et al., The SRG/eROSITA all-sky survey First X-ray catalogues and data release of the western Galactic hemisphere, A&A, 682, A34 (2024)

Acknowledgement

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