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EFEDSHARD - eROSITA eFEDS Hard X-Ray (2.3-5.0 keV) Source Catalog

HEASARC
Archive

Overview

The eROSITA X-ray telescope on board the Spectrum-Roentgen-Gamma (SRG) observatory combines a large field of view and collecting area in the energy range ~0.2 to ~8.0 keV with the capability to perform uniform scanning observations of large sky areas. SRG/eROSITA performed scanning observations of the ~140 square degrees eROSITA Final Equatorial Depth Survey (eFEDS) field as part of its performance verification phase. The observing time was chosen to slightly exceed the depth of equatorial fields after the completion of the eROSITA all-sky survey. The authors present a catalog of detected X-ray sources in the eFEDS field providing source positions and extent information, as well as fluxes in multiple energy bands and document a suite of tools and procedures developed for eROSITA data processing and analysis, validated and optimized by the eFEDS work.

A multi-stage source detection procedure was optimized and calibrated by performing realistic simulations of the eROSITA eFEDS observations. The authors cross-matched the eROSITA eFEDS source catalog with previous XMM-ATLAS observations, confirming excellent agreement of the eROSITA and XMM-ATLAS source fluxes.

This table presents the hard band sample of 246 sources detected in the energy range 2.3-5.0 keV above a detection likelihood of 10. These sources were detected in three bands (0.2-0.6, 0.6-2.3, and 2.3-5keV) with detect_likelihood >=5 and extent_likelihood = 0 (i.e. point sources). The linked EFEDSMAIN table presents the primary catalog of 27910 X-ray sources, including 542 with significant spatial extent, detected in the 0.2-2.3 keV energy range with detection likelihoods >=6 , corresponding to a (point source) flux limit of ~6.5 x 10-15 erg/cm2/s in the 0.5-2.0 keV energy band (80% completeness). A supplementary catalog contains 4774 low-significance source candidates with detection likelihoods between 5 and 6. The dedicated data analysis software package, calibration database, and calibrated data products are described in an appendix.

Additional information for the eROSITA early data release observations is available at the eROSITA-DE EDR website.


Catalog Bibcode

2022A&A...661A...1B

References

Brunner et al. (2022), "The eROSITA Final Equatorial Depth Survey (eFEDS):
      The X-ray catalog", <A&A, 661, 1 (2022)>
     =2022A&A...661A...1B

Provenance

This database table was ingested by the HEASARC in August 2022 and is based upon the "eROSITA/eFEDS hard catalogue" file downloaded from the eROSITA-DE Early Data Release catalogs web page. In some cases, the HEASARC has altered the original field names, as per HEASARC conventions, and provides the original field names in square brackets.

Parameters

Name
The eFEDS source designation in the form 'eFEDS JHHMMSS.S+DDMMSS', which uses the J2000.0 equatorial coordinates truncated to 0.1 arcseconds in RA and to 1 arcsecond in Declination. [NAME]

Source_Number
The unique identification number for each source in this catalog. [ID_SRC]

Main_Source_Number
The matching identification number for corresponding source in the main catalog, EFEDSMAIN. [ID_main]

RA
The uncorrected right ascension of the source in the selected equinox. This was given in J2000 decimal degree coordinates to an accuracy of 10-5 degrees (0.036 arcseconds) in the original reference. [RA]

Dec
The uncorrected declination of the source in the selected equinox. This was given in J2000 decimal degree coordinates to an accuracy of 10-6 degrees (0.0036 arcseconds) in the original reference. [DEC]

LII
The uncorrected Galactic longitude of the source.

BII
The uncorrected Galactic latitude of the source.

Error_Radius
The uncertainty in the uncorrected position, in arcseconds, based on the combined uncertainties in the ra and dec coordinates. [RADEC_ERR]

RA_Corr
The astrometrically-corrected right ascension of the source in the selected equinox, based on matches to Gaia un-WISE AGN catalog (Shu et al. 2019). The computed corrections follow Equation 1 given in the reference paper (see Section 3.3). These values were given in J2000 decimal degree coordinates to an accuracy of 10-5 degrees (0.036 arcseconds) in the original reference. [RA_CORR]

Dec_Corr
The astrometrically-corrected declination of the source in the selected equinox, based on matches to Gaia un-WISE AGN catalog (Shu et al. 2019). The computed corrections follow Equation 1 given in the reference paper (see Section 3.3). These values were given in J2000 decimal degree coordinates to an accuracy of 10-6 degrees (0.0036 arcseconds) in the original reference. [DEC_CORR]

Error_Radius_Corr
The uncertainty in the uncorrected position, in arcseconds, based on the combined uncertainties in the astrometrically-corrected RA and Dec coordinates. [RADEC_ERR_CORR]

Source_Extent
The extent of the source, given in arcseconds. Values of 0.0 indicate point sources. [EXT]

Source_Extent_Error
The uncertainty in the extent of the source, given in arcseconds. Values of 0.0 indicate point sources. [EXT_ERR]

Extent_Likelihood
The likelihood associated with the extent measurement. Values of 0.0 indicate point sources. [EXT_LIKE]

Detect_Likelihood
The detection likelihood based on the combined three-band analysis. This catalog includes sources that were detected in three bands (0.2-0.6, 0.6-2.3, and 2.3-5 keV) with detect_likelihood >=5 and with detect_likelihood >= 10 in the 2.3-5 keV band and extent_likelihood = 0 (i.e. point sources). [DET_LIKE_0]

Count_Rate
The net count rate for the source, based on PSF-fitting the three band (0.2-0.6, 0.6-2.3, and 2.3-5 keV) combined dataset. [ML_RATE_0]

Count_Rate_Error
The 1-sigma uncertainty in the net count rate for the three band (0.2-0.6, 0.6-2.3, and 2.3-5keV) combined dataset. [ML_RATE_ERR_0]

Counts
The background-subtracted net counts for the source, measured from the three band (0.2-0.6, 0.6-2.3, and 2.3-5keV) combined dataset count_rate. [ML_CTS_0]

Counts_Error
The 1-sigma uncertainty in the net counts for the three band (0.2-0.6, 0.6-2.3, and 2.3-5keV) combined dataset. [ML_CTS_ERR_0]

Flux
The flux of the source in the three band (0.2-0.6, 0.6-2.3, and 2.3-5keV) combined dataset, in units of erg/s/cm2. The energy conversion factor (ECF; listed in Table D.1 of the reference paper) between the count rates and fluxes is based on a power-law model with Gamma=2.0 and with Galactic absorption (NH=3 x 1020 cm-2). [ML_FLUX_0]

Flux_Error
The 1-sigma uncertainty in the three band (0.2-0.6, 0.6-2.3, and 2.3-5 keV) combined dataset flux, in units of erg/s/cm2. [ML_FLUX_ERR_0]

Bkg_Counts
The background counts, in units of counts/arcmin2, at the source position in the three band (0.2-0.6, 0.6-2.3, and 2.3-5keV) combined dataset. [ML_BKG_0]

Inarea90_Flag
The flag designating sources within the inner region of the eFEDS field, where the exposure times exceed 500s and which comprises 90% of the eFEDS field area. [inArea90]

Tb1_Detect_Likelihood
The detection likelihood based on forced PSF-fitting in the 0.2-0.6 keV band. [DET_LIKE_1]

Tb2_Detect_Likelihood
The detection likelihood based on forced PSF-fitting in the 0.6-2.3 keV band. [DET_LIKE_2]

Tb3_Detect_Likelihood
The detection likelihood based on forced PSF-fitting in the 2.3-5 keV band. [DET_LIKE_3]

Tb1_Count_Rate
The net count rate for the source in the 0.2-0.6 keV band, based on forced PSF-fitting, as described in Section 3.4 of the reference paper. [ML_RATE_1]

Tb2_Count_Rate
The net count rate for the source in the 0.6-2.3 keV band, based on forced PSF-fitting, as described in Section 3.4 of the reference paper. [ML_RATE_2]

Tb3_Count_Rate
The net count rate for the source in the 2.3-5 keV band, based on forced PSF-fitting, as described in Section 3.4 of the reference paper. [ML_RATE_3]

Tb1_Count_Rate_Error
The 1-sigma uncertainty in the 0.2-0.6 keV net count rate. [ML_RATE_ERR_1]

Tb2_Count_Rate_Error
The 1-sigma uncertainty in the 0.6-2.3 keV net count rate. [ML_RATE_ERR_2]

Tb3_Count_Rate_Error
The 1-sigma uncertainty in the 2.3-5 keV net count rate. [ML_RATE_ERR_3]

Tb1_Counts
The background-subtracted 0.2-0.6 keV net counts for the source, measured from the forced PSF-fitted count rate, e.g., b2_count_rate. [ML_CTS_1]

Tb2_Counts
The background-subtracted 0.6-2.3 keV net counts for the source, measured from the forced PSF-fitted count rate, e.g., b2_count_rate. [ML_CTS_2]

Tb3_Counts
The background-subtracted 2.3-5 keV net counts for the source, measured from the forced PSF-fitted count rate, e.g., b2_count_rate. [ML_CTS_3]

Tb1_Counts_Error
The 1-sigma uncertainty in the 0.2-0.6 keV net counts. [ML_CTS_ERR_1]

Tb2_Counts_Error
The 1-sigma uncertainty in the 0.6-2.3 keV net counts. [ML_CTS_ERR_2]

Tb3_Counts_Error
The 1-sigma uncertainty in the 2.3-5 keV net counts. [ML_CTS_ERR_3]

Tb1_Flux
The flux of the source in the 0.2-0.6 keV band, in units of erg/s/cm2, measured from the forced PSF-fitted count rate, e.g., b1_count_rate. The energy conversion factor (ECF; listed in Table D.1 of the reference paper) between the count rates and fluxes is based on a power-law model with Gamma=2.0 and with Galactic absorption (NH=3 x 1020 cm-2). [ML_FLUX_1]

Tb2_Flux
The flux of the source in the 0.6-2.3 keV band, in units of erg/s/cm2, measured from the forced PSF-fitted count rate, e.g., b1_count_rate. The energy conversion factor (ECF; listed in Table D.1 of the reference paper) between the count rates and fluxes is based on a power-law model with Gamma=2.0 and with Galactic absorption (NH=3 x 1020 cm-2). [ML_FLUX_2]

Tb3_Flux
The flux of the source in the 2.3-5 keV band, in units of erg/s/cm2, measured from the forced PSF-fitted count rate, e.g., b1_count_rate. The energy conversion factor (ECF; listed in Table D.1 of the reference paper) between the count rates and fluxes is based on a power-law model with Gamma=2.0 and with Galactic absorption (NH=3 x 1020 cm-2). [ML_FLUX_3]

Tb1_Flux_Error
The 1-sigma uncertainty in the 0.2-0.6 keV flux, in units of erg/s/cm2. [ML_FLUX_ERR_1]

Tb2_Flux_Error
The 1-sigma uncertainty in the 0.6-2.3 keV flux, in units of erg/s/cm2. [ML_FLUX_ERR_2]

Tb3_Flux_Error
The 1-sigma uncertainty in the 2.3-5 keV flux, in units of erg/s/cm2. [ML_FLUX_ERR_3]

Tb1_Exposure
The vignetting-corrected exposure, in seconds, at the source position for the 0.2-0.6 keV band. [ML_EXP_1]

Tb2_Exposure
The vignetting-corrected exposure, in seconds, at the source position for the 0.6-2.3 keV band. [ML_EXP_2]

Tb3_Exposure
The vignetting-corrected exposure, in seconds, at the source position for the 2.3-5 keV band. [ML_EXP_3]

Tb1_Bkg_Counts
The background counts, in units of counts/arcmin2, at the source position in the 0.2-0.6 keV band. [ML_BKG_1]

Tb2_Bkg_Counts
The background counts, in units of counts/arcmin2, at the source position in the 0.6-2.3 keV band. [ML_BKG_2]

Tb3_Bkg_Counts
The background counts, in units of counts/arcmin2, at the source position in the 2.3-5 keV band. [ML_BKG_3]

B1_Detect_Likelihood
The detection likelihood based on forced PSF-fitting in the 0.2-0.5 keV band. [DET_LIKE_b1]

B2_Detect_Likelihood
The detection likelihood based on forced PSF-fitting in the 0.5-1 keV band. [DET_LIKE_b2]

B3_Detect_Likelihood
The detection likelihood based on forced PSF-fitting in the 1-2 keV band. [DET_LIKE_b3]

B4_Detect_Likelihood
The detection likelihood based on forced PSF-fitting in the 2-4.5 keV band. [DET_LIKE_b4]

SB_Detect_Likelihood
The detection likelihood based on forced PSF-fitting in the 0.5-2.0 keV band. [DET_LIKE_s]

HB_Detect_Likelihood
The detection likelihood based on forced PSF-fitting in the 1.2-5 keV band. [DET_LIKE_h]

UB_Detect_Likelihood
The detection likelihood based on forced PSF-fitting in the 5-8 keV band. [DET_LIKE_u]

B1_Count_Rate
The net count rate for the source in the 0.2-0.5 keV band, based on forced PSF-fitting, as described in Section 3.4 of the reference paper. [ML_RATE_b1]

B2_Count_Rate
The net count rate for the source in the 0.5-1 keV band, based on forced PSF-fitting, as described in Section 3.4 of the reference paper. [ML_RATE_b2]

B3_Count_Rate
The net count rate for the source in the 1-2 keV band, based on forced PSF-fitting, as described in Section 3.4 of the reference paper. [ML_RATE_b3]

B4_Count_Rate
The net count rate for the source in the 2-4.5 keV band, based on forced PSF-fitting, as described in Section 3.4 of the reference paper. [ML_RATE_b4]

SB_Count_Rate
The net count rate for the source in the 0.5-2 keV band, based on forced PSF-fitting, as described in Section 3.4 of the reference paper. [ML_RATE_s]

HB_Count_Rate
The net count rate for the source in the 2.3-5 keV band, based on forced PSF-fitting, as described in Section 3.4 of the reference paper. [ML_RATE_h]

UB_Count_Rate
The net count rate for the source in the 5-8 keV band, based on forced PSF-fitting, as described in Section 3.4 of the reference paper. [ML_RATE_u]

B1_Count_Rate_Error
The 1-sigma uncertainty in the 0.2-0.5 keV net count rate. [ML_RATE_ERR_b1]

B2_Count_Rate_Error
The 1-sigma uncertainty in the 0.5-1 keV net count rate. [ML_RATE_ERR_b2]

B3_Count_Rate_Error
The 1-sigma uncertainty in the 1-2 keV net count rate. [ML_RATE_ERR_b3]

B4_Count_Rate_Error
The 1-sigma uncertainty in the 2-4.5 keV net count rate. [ML_RATE_ERR_b4]

SB_Count_Rate_Error
The 1-sigma uncertainty in the 0.5-2 keV net count rate. [ML_RATE_ERR_s]

HB_Count_Rate_Error
The 1-sigma uncertainty in the 2.3-5 keV net count rate. [ML_RATE_ERR_h]

UB_Count_Rate_Error
The 1-sigma uncertainty in the 5-8 keV net count rate. [ML_RATE_ERR_u]

B1_Count_Rate_Lower
The 1-sigma lower error value in the 0.2-0.5 keV net count rate. [ML_RATE_LOWERR_b1]

B2_Count_Rate_Lower
The 1-sigma lower error value in the 0.5-1 keV net count rate. [ML_RATE_LOWERR_b2]

B3_Count_Rate_Lower
The 1-sigma lower error value in the 1-2 keV net count rate. [ML_RATE_LOWERR_b3]

B4_Count_Rate_Lower
The 1-sigma lower error value in the 2-4.5 keV net count rate. [ML_RATE_LOWERR_b4]

SB_Count_Rate_Lower
The 1-sigma lower error value in the 0.5-2 keV net count rate. [ML_RATE_LOWERR_s]

HB_Count_Rate_Lower
The 1-sigma lower error value in the 2.3-5 keV net count rate. [ML_RATE_LOWERR_h]

UB_Count_Rate_Lower
The 1-sigma lower error value in the 5-8 keV net count rate. [ML_RATE_LOWERR_u]

B1_Count_Rate_Upper
The 1-sigma upper error value in the 0.2-0.5 keV net count rate. [ML_RATE_UPERR_b1]

B2_Count_Rate_Upper
The 1-sigma upper error value in the 0.5-1 keV net count rate. [ML_RATE_UPERR_b2]

B3_Count_Rate_Upper
The 1-sigma upper error value in the 1-2 keV net count rate. [ML_RATE_UPERR_b3]

B4_Count_Rate_Upper
The 1-sigma upper error value in the 2-4.5 keV net count rate. [ML_RATE_UPERR_b4]

SB_Count_Rate_Upper
The 1-sigma upper error value in the 0.5-2 keV net count rate. [ML_RATE_UPERR_s]

HB_Count_Rate_Upper
The 1-sigma upper error value in the 2.3-5 keV net count rate. [ML_RATE_UPERR_h]

UB_Count_Rate_Upper
The 1-sigma upper error value in the 5-8 keV net count rate. [ML_RATE_UPERR_u]

B1_Counts
The background-subtracted 0.2-0.5 keV net counts for the source, measured from the forced PSF-fitted count rate, e.g., b1_count_rate. [ML_CTS_b1]

B2_Counts
The background-subtracted 0.5-1 keV net counts for the source, measured from the forced PSF-fitted count rate, e.g., b2_count_rate. [ML_CTS_b2]

B3_Counts
The background-subtracted 1-2 keV net counts for the source, measured from the forced PSF-fitted count rate, e.g., b3_count_rate. [ML_CTS_b3]

B4_Counts
The background-subtracted 2-4.5 keV net counts for the source, measured from the forced PSF-fitted count rate, e.g., b4_count_rate. [ML_CTS_b4]

SB_Counts
The background-subtracted 0.5-2 keV net counts for the source, measured from the forced PSF-fitted count rate, e.g., sb_count_rate. [ML_CTS_s]

HB_Counts
The background-subtracted 2.3-5 keV net counts for the source, measured from the forced PSF-fitted count rate, e.g., hb_count_rate. [ML_CTS_h]

UB_Counts
The background-subtracted 5-8 keV net counts for the source, measured from the forced PSF-fitted count rate, e.g., ub_count_rate. [ML_CTS_u]

B1_Counts_Error
The 1-sigma uncertainty in the 0.2-0.5 keV net counts. [ML_CTS_ERR_b1]

B2_Counts_Error
The 1-sigma uncertainty in the 0.5-1 keV net counts. [ML_CTS_ERR_b2]

B3_Counts_Error
The 1-sigma uncertainty in the 1-2 keV net counts. [ML_CTS_ERR_b3]

B4_Counts_Error
The 1-sigma uncertainty in the 2-4.5 keV net counts. [ML_CTS_ERR_b4]

SB_Counts_Error
The 1-sigma uncertainty in the 0.5-2 keV net counts. [ML_CTS_ERR_s]

HB_Counts_Error
The 1-sigma uncertainty in the 2.3-5 keV net counts. [ML_CTS_ERR_h]

UB_Counts_Error
The 1-sigma uncertainty in the 5-8 keV net counts. [ML_CTS_ERR_u]

B1_Counts_Lower
The 1-sigma lower error in the 0.2-0.5 keV net counts. [ML_CTS_LOWERR_b1]

B2_Counts_Lower
The 1-sigma lower error in the 0.5-1 keV net counts. [ML_CTS_LOWERR_b2]

B3_Counts_Lower
The 1-sigma lower error in the 1-2 keV net counts. [ML_CTS_LOWERR_b3]

B4_Counts_Lower
The 1-sigma lower error in the 2-4.5 keV net counts. [ML_CTS_LOWERR_b4]

SB_Counts_Lower
The 1-sigma lower error in the 0.5-2 keV net counts. [ML_CTS_LOWERR_s]

HB_Counts_Lower
The 1-sigma lower error in the 2.3-5 keV net counts. [ML_CTS_LOWERR_h]

UB_Counts_Lower
The 1-sigma lower error in the 5-8 keV net counts. [ML_CTS_LOWERR_u]

B1_Counts_Upper
The 1-sigma upper error in the 0.2-0.5 keV net counts. [ML_CTS_UPERR_b1]

B2_Counts_Upper
The 1-sigma upper error in the 0.5-1 keV net counts. [ML_CTS_UPERR_b2]

B3_Counts_Upper
The 1-sigma upper error in the 1-2 keV net counts. [ML_CTS_UPERR_b3]

B4_Counts_Upper
The 1-sigma upper error in the 2-4.5 keV net counts. [ML_CTS_UPERR_b4]

SB_Counts_Upper
The 1-sigma upper error in the 0.5-2 keV net counts. [ML_CTS_UPERR_s]

HB_Counts_Upper
The 1-sigma upper error in the 2.3-5 keV net counts. [ML_CTS_UPERR_h]

UB_Counts_Upper
The 1-sigma upper error in the 5-8 keV net counts. [ML_CTS_UPERR_u]

B1_Flux
The flux of the source in the 0.2-0.5 keV band, in units of erg/s/cm2, measured from the forced PSF-fitted count rate, e.g., b1_count_rate. The energy conversion factor (ECF; listed in Table D.1 of the reference paper) between the count rates and fluxes is based on a power-law model with Gamma=2.0 and with Galactic absorption (NH=3 x 1020 cm-2). [ML_FLUX_b1]

B2_Flux
The flux of the source in the 0.5-1 keV band, in units of erg/s/cm2, measured from the forced PSF-fitted count rate, e.g., b1_count_rate. The energy conversion factor (ECF; listed in Table D.1 of the reference paper) between the count rates and fluxes is based on a power-law model with Gamma=2.0 and with Galactic absorption (NH=3 x 1020 cm-2). [ML_FLUX_b2]

B3_Flux
The flux of the source in the 1-2 keV band, in units of erg/s/cm2, measured from the forced PSF-fitted count rate, e.g., b1_count_rate. The energy conversion factor (ECF; listed in Table D.1 of the reference paper) between the count rates and fluxes is based on a power-law model with Gamma=2.0 and with Galactic absorption (NH=3 x 1020 cm-2). [ML_FLUX_b3]

B4_Flux
The flux of the source in the 2-4.5 keV band, in units of erg/s/cm2, measured from the forced PSF-fitted count rate, e.g., b1_count_rate. The energy conversion factor (ECF; listed in Table D.1 of the reference paper) between the count rates and fluxes is based on a power-law model with Gamma=2.0 and with Galactic absorption (NH=3 x 1020 cm-2). [ML_FLUX_b4]

SB_Flux
The flux of the source in the 0.5-2 keV band, in units of erg/s/cm2, measured from the forced PSF-fitted count rate, e.g., b1_count_rate. The energy conversion factor (ECF; listed in Table D.1 of the reference paper) between the count rates and fluxes is based on a power-law model with Gamma=2.0 and with Galactic absorption (NH=3 x 1020 cm-2). [ML_FLUX_s]

HB_Flux
The flux of the source in the 2.3-5 keV band, in units of erg/s/cm2, measured from the forced PSF-fitted count rate, e.g., b1_count_rate. The energy conversion factor (ECF; listed in Table D.1 of the reference paper) between the count rates and fluxes is based on a power-law model with Gamma=2.0 and with Galactic absorption (NH=3 x 1020 cm-2). [ML_FLUX_h]

UB_Flux
The flux of the source in the 5-8 keV band, in units of erg/s/cm2, measured from the forced PSF-fitted count rate, e.g., b1_count_rate. The energy conversion factor (ECF; listed in Table D.1 of the reference paper) between the count rates and fluxes is based on a power-law model with Gamma=2.0 and with Galactic absorption (NH=3 x 1020 cm-2). [ML_FLUX_u]

B1_Flux_Error
The 1-sigma uncertainty in the 0.2-0.5 keV flux, in units of erg/s/cm2. [ML_FLUX_ERR_b1]

B2_Flux_Error
The 1-sigma uncertainty in the 0.5-1 keV flux, in units of erg/s/cm2. [ML_FLUX_ERR_b2]

B3_Flux_Error
The 1-sigma uncertainty in the 1-2 keV flux, in units of erg/s/cm2. [ML_FLUX_ERR_b3]

B4_Flux_Error
The 1-sigma uncertainty in the 2-4.5 keV flux, in units of erg/s/cm2. [ML_FLUX_ERR_b4]

SB_Flux_Error
The 1-sigma uncertainty in the 0.5-2 keV flux, in units of erg/s/cm2. [ML_FLUX_ERR_s]

HB_Flux_Error
The 1-sigma uncertainty in the 2.3-5 keV flux, in units of erg/s/cm2. [ML_FLUX_ERR_h]

UB_Flux_Error
The 1-sigma uncertainty in the 5-8 keV flux, in units of erg/s/cm2. [ML_FLUX_ERR_u]

B1_Flux_Lower
The 1-sigma lower error value in the 0.2-0.5 keV flux, in units of erg/s/cm2. [ML_FLUX_LOWERR_b1]

B2_Flux_Lower
The 1-sigma lower error value in the 0.5-1 keV flux, in units of erg/s/cm2. [ML_FLUX_LOWERR_b2]

B3_Flux_Lower
The 1-sigma lower error value in the 1-2 keV flux, in units of erg/s/cm2. [ML_FLUX_LOWERR_b3]

B4_Flux_Lower
The 1-sigma lower error value in the 2-4.5 keV flux, in units of erg/s/cm2. [ML_FLUX_LOWERR_b4]

SB_Flux_Lower
The 1-sigma lower error value in the 0.5-2 keV flux, in units of erg/s/cm2. [ML_FLUX_LOWERR_s]

HB_Flux_Lower
The 1-sigma lower error value in the 2.3-5 keV flux, in units of erg/s/cm2. [ML_FLUX_LOWERR_h]

UB_Flux_Lower
The 1-sigma lower error value in the 5-8 keV flux, in units of erg/s/cm2. [ML_FLUX_LOWERR_u]

B1_Flux_Upper
The 1-sigma upper error value in the 0.2-5 keV flux, in units of erg/s/cm2. [ML_FLUX_UPERR_b1]

B2_Flux_Upper
The 1-sigma upper error value in the 0.5-1 keV flux, in units of erg/s/cm2. [ML_FLUX_UPERR_b2]

B3_Flux_Upper
The 1-sigma upper error value in the 1-2 keV flux, in units of erg/s/cm2. [ML_FLUX_UPERR_b3]

B4_Flux_Upper
The 1-sigma upper error value in the 2-4.5 keV flux, in units of erg/s/cm2. [ML_FLUX_UPERR_b4]

SB_Flux_Upper
The 1-sigma upper error value in the 0.5-2 keV flux, in units of erg/s/cm2. [ML_FLUX_UPERR_s]

HB_Flux_Upper
The 1-sigma upper error value in the 2.3-5 keV flux, in units of erg/s/cm2. [ML_FLUX_UPERR_h]

UB_Flux_Upper
The 1-sigma upper error value in the 5-8 keV flux, in units of erg/s/cm2. [ML_FLUX_UPERR_u]

B1_Exposure
The vignetting-corrected exposure, in seconds, at the source position for the 0.2-0.5 keV band. [ML_EXP_b1]

B2_Exposure
The vignetting-corrected exposure, in seconds, at the source position for the 0.5-1 keV band. [ML_EXP_b2]

B3_Exposure
The vignetting-corrected exposure, in seconds, at the source position for the 1-2 keV band. [ML_EXP_b3]

B4_Exposure
The vignetting-corrected exposure, in seconds, at the source position for the 2-4.5 keV band. [ML_EXP_b4]

SB_Exposure
The vignetting-corrected exposure, in seconds, at the source position for the 0.5-2 keV band. [ML_EXP_s]

HB_Exposure
The vignetting-corrected exposure, in seconds, at the source position for the 2.3-5 keV band. [ML_EXP_h]

UB_Exposure
The vignetting-corrected exposure, in seconds, at the source position for the 5-8 keV band. [ML_EXP_u]

B1_Bkg_Counts
The background counts, in units of counts/arcmin2, at the source position in the 0.2-0.5 keV band. [ML_BKG_b1]

B2_Bkg_Counts
The background counts, in units of counts/arcmin2, at the source position in the 0.5-1 keV band. [ML_BKG_b2]

B3_Bkg_Counts
The background counts, in units of counts/arcmin2, at the source position in the 1-2 keV band. [ML_BKG_b3]

B4_Bkg_Counts
The background counts, in units of counts/arcmin2, at the source position in the 2-4.5 keV band. [ML_BKG_b4]

SB_Bkg_Counts
The background counts, in units of counts/arcmin2, at the source position in the 0.5-2 keV band. [ML_BKG_s]

HB_Bkg_Counts
The background counts, in units of counts/arcmin2, at the source position in the 2.3-5 keV band. [ML_BKG_h]

UB_Bkg_Counts
The background counts, in units of counts/arcmin2, at the source position in the 5-8 keV band. [ML_BKG_u]

B1_Aperture_Counts
The background-subtracted 0.2-0.5 keV net counts for the source, measured from the aperture photometry methods described in Section 4.2 of the reference paper. [APE_CTS_b1]

B2_Aperture_Counts
The background-subtracted 0.5-1 keV net counts for the source, measured from the aperture photometry methods described in Section 4.2 of the reference paper. [APE_CTS_b2]

B3_Aperture_Counts
The background-subtracted 1-2 keV net counts for the source, measured from the aperture photometry methods described in Section 4.2 of the reference paper. [APE_CTS_b3]

B4_Aperture_Counts
The background-subtracted 2-4.5 keV net counts for the source, measured from the aperture photometry methods described in Section 4.2 of the reference paper. [APE_CTS_b4]

SB_Aperture_Counts
The background-subtracted 0.5-2 keV net counts for the source, measured from the aperture photometry methods described in Section 4.2 of the reference paper. [APE_CTS_s]

HB_Aperture_Counts
The background-subtracted 2.3-5 keV net counts for the source, measured from the aperture photometry methods described in Section 4.2 of the reference paper. [APE_CTS_h]

UB_Aperture_Counts
The background-subtracted 5-8 keV net counts for the source, measured from the aperture photometry methods described in Section 4.2 of the reference paper. [APE_CTS_u]

B1_Aperture_Exposure
The vignetting-corrected exposure, in seconds, at the source position for the 0.2-0.5 keV band. [APE_EXP_b1]

B2_Aperture_Exposure
The vignetting-corrected exposure, in seconds, at the source position for the 0.5-1 keV band. [APE_EXP_b2]

B3_Aperture_Exposure
The vignetting-corrected exposure, in seconds, at the source position for the 1-2 keV band. [APE_EXP_b3]

B4_Aperture_Exposure
The vignetting-corrected exposure, in seconds, at the source position for the 2-4.5 keV band. [APE_EXP_b4]

SB_Aperture_Exposure
The vignetting-corrected exposure, in seconds, at the source position for the 0.5-2 keV band. [APE_EXP_s]

HB_Aperture_Exposure
The vignetting-corrected exposure, in seconds, at the source position for the 2.3-5 keV band. [APE_EXP_h]

UB_Aperture_Exposure
The vignetting-corrected exposure, in seconds, at the source position for the 5-8 keV band. [APE_EXP_u]

B1_Aperture_Bkg_Counts
The background counts in the 0.2-0.5 keV, in units of counts/arcmin2, within the aperture and excluding nearby sources. [APE_BKG_b1]

B2_Aperture_Bkg_Counts
The background counts in the 0.5-1 keV, in units of counts/arcmin2, within the aperture and excluding nearby sources. [APE_BKG_b2]

B3_Aperture_Bkg_Counts
The background counts in the 1-2 keV, in units of counts/arcmin2, within the aperture and excluding nearby sources. [APE_BKG_b3]

B4_Aperture_Bkg_Counts
The background counts in the 2-4.5 keV, in units of counts/arcmin2, within the aperture and excluding nearby sources. [APE_BKG_b4]

SB_Aperture_Bkg_Counts
The background counts in the 0.5-2 keV, in units of counts/arcmin2, within the aperture and excluding nearby sources. [APE_BKG_s]

HB_Aperture_Bkg_Counts
The background counts in the 2.3-5 keV, in units of counts/arcmin2, within the aperture and excluding nearby sources. [APE_BKG_h]

UB_Aperture_Bkg_Counts
The background counts in the 5-8 keV, in units of counts/arcmin2, within the aperture and excluding nearby sources. [APE_BKG_u]

B1_Aperture_Radius
The aperture radius, in pixels, for the 0.2-0.5 keV band. [APE_RADIUS_b1]

B2_Aperture_Radius
The aperture radius, in pixels, for the 0.5-1 keV band. [APE_RADIUS_b2]

B3_Aperture_Radius
The aperture radius, in pixels, for the 1-2 keV band. [APE_RADIUS_b3]

B4_Aperture_Radius
The aperture radius, in pixels, for the 2-4.5 keV band. [APE_RADIUS_b4]

SB_Aperture_Radius
The aperture radius, in pixels, for the 0.5-2 keV band. [APE_RADIUS_s]

HB_Aperture_Radius
The aperture radius, in pixels, for the 2.3-5 keV band. [APE_RADIUS_h]

UB_Aperture_Radius
The aperture radius, in pixels, for the 5-8 keV band. [APE_RADIUS_u]

B1_Aperture_Prob
The Poisson probability that the source is generated by background fluctuations, based on the 0.2-0.5 keV band. [APE_POIS_b1]

B2_Aperture_Prob
The Poisson probability that the source is generated by background fluctuations, based on the 0.5-1 keV band. [APE_POIS_b2]

B3_Aperture_Prob
The Poisson probability that the source is generated by background fluctuations, based on the 1-2 keV band. [APE_POIS_b3]

B4_Aperture_Prob
The Poisson probability that the source is generated by background fluctuations, based on the 2-4.5 keV band. [APE_POIS_b4]

SB_Aperture_Prob
The Poisson probability that the source is generated by background fluctuations, based on the 0.5-2 keV band. [APE_POIS_s]

HB_Aperture_Prob
The Poisson probability that the source is generated by background fluctuations, based on the 2.3-5 keV band. [APE_POIS_h]

UB_Aperture_Prob
The Poisson probability that the source is generated by background fluctuations, based on the 5-8 keV band. [APE_POIS_u]


Contact Person

Questions regarding the EFEDSHARD database table can be addressed to the HEASARC Help Desk.
Page Author: Browse Software Development Team
Last Modified: Friday, 05-Aug-2022 17:13:31 EDT