J/ApJS/232/18/3fhlLAT point source catalogrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint3FHL3FHL name (JHHMM.m+DDMMe) (Source_Name)meta.id;meta.maincharprimaryRAJ2000Right ascension; J2000 (RAJ2000)degpos.eq.ra;meta.mainDEJ2000Declination; J2000 (DEJ2000)degpos.eq.dec;meta.mainGLONGalactic longitude (GLON)degpos.galactic.lonGLATGalactic latitude (GLAT)degpos.galactic.latdoubleC95amaj[0.008/0.2]? Error radius at 95% confidence (Conf_95_SemiMajor)degstat.errorfloatnullableC95bmin[0.008/0.2]? Conf_95_SemiMajor in 3FHL (Conf_95_SemiMinor)degstat.errorfloatnullableC95PA[-1e+38]? error circle; NULL in 3FHL (Conf_95_PosAng)degstat.errordoublenullableROI[1/728] ROI number (ROI_num)meta.idintSig[4/169] Source significance in {sigma} units over the 10GeV to 2TeV band (Signif_Avg)stat.fit.goodness;arith.ratiofloatEPvt[11/195] Energy at which error on differential flux is minimal (Pivot_Energy)GeVphys.energyfloatSDifferential flux at Pivot_Energy (Flux_Density)ph.cm**-2.GeV**-1.s**-1phot.flux;arith.ratiodoublee_S1{sigma} error on S (Unc_Flux_Density)ph.cm**-2.GeV**-1.s**-1stat.errordoubleFluxIntegral photon flux from 10GeV to 1TeV obtained by spectral fitting (Flux)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_Flux1{sigma} error on Flux (Unc_Flux)ph.cm**-2.s**-1stat.error;phot.fluxdoubleEFlxEnergy flux from 10GeV to 1TeV obtained by spectral fitting; in erg/cm^2^/s (Energy_Flux)0.001W.m**-2phot.flux.density;em.gamma.harddoublee_EFlx1{sigma} error on EFlx (Unc_Energy_Flux)0.001W.m**-2stat.errordoubleSigCve[0/6] Significance (in {sigma} units) of the fit improvement between power-law and LogParabola (Signif_Curve) (1)stat.fit.goodnessfloatSpTSpectral type (PowerLaw or LogParabola); see section 2.4 (SpectrumType)src.spTypecharSInd[0.9/9.1] Best-fit photon number index at Pivot_Energy when fitting with LogParabola (Spectral_Index)spect.indexfloate_SInd[0.04/4.1] 1{sigma} error on SInd (Unc_Spectral_Index)spect.indexfloatbeta[-0.8/1] Curvature parameter {beta} when fitting with LogParabola (beta)stat.fit.paramfloate_beta[0.001/9.3] 1{sigma} error on beta (Unc_beta)stat.errorfloatPLInd[1/9.1] Best-fit photon number index when fitting with power law (PowerLaw_Index)spect.indexfloate_PLInd[0.02/4] 1{sigma} error on PLInd (Unc_PowerLaw_Index)spect.indexfloatF1Integral photon flux in 10-20GeV spectral band (Flux_Band1)ph.cm**-2.s**-1phot.fluxdoubleE_F1? 1{sigma} upper error on F1 (Low_Unc_Flux_Band2) (2)ph.cm**-2.s**-1stat.error;stat.maxdoublenullablee_F1? 1{sigma} lower error on F1 (Low_Unc_Flux_Band1) (2)ph.cm**-2.s**-1stat.errordoublenullableF2Integral photon flux in 20-50GeV spectral band (Flux_Band2)ph.cm**-2.s**-1phot.fluxdoubleE_F2? 1{sigma} upper error on F2 (Low_Unc_Flux_Band4) (2)ph.cm**-2.s**-1stat.error;stat.maxdoublenullablee_F2? 1{sigma} lower error on F2 (Low_Unc_Flux_Band3) (2)ph.cm**-2.s**-1stat.errordoublenullableF3[0/] Integral photon flux in 50-150GeV spectral band (Flux_Band3)ph.cm**-2.s**-1phot.fluxdoubleE_F3? 1{sigma} upper error on F3 (Up_Unc_Flux_Band1) (2)ph.cm**-2.s**-1stat.error;stat.maxdoublenullablee_F3? 1{sigma} lower error on F3 (Low_Unc_Flux_Band5) (2)ph.cm**-2.s**-1stat.errordoublenullableF4[0/] Integral photon flux in 150-500GeV spectral band (Flux_Band4)ph.cm**-2.s**-1phot.fluxdoubleE_F4? 1{sigma} upper error on F4 (Up_Unc_Flux_Band3) (2)ph.cm**-2.s**-1stat.error;stat.maxdoublenullablee_F4? 1{sigma} lower error on F4 (Up_Unc_Flux_Band2) (2)ph.cm**-2.s**-1stat.errordoublenullableF5[0/] Integral photon flux in 500-2000GeV spectral band (Flux_Band5)ph.cm**-2.s**-1phot.fluxdoubleE_F5? 1{sigma} upper error on F5 (Up_Unc_Flux_Band5) (2)ph.cm**-2.s**-1stat.error;stat.maxdoublenullablee_F5? 1{sigma} lower error on F5 (Up_Unc_Flux_Band4) (2)ph.cm**-2.s**-1stat.errordoublenullablenuFnu1Spectral energy distribution in 10-20GeV, in erg/cm^2^/s (nuFnu1)0.001W.m**-2phot.fluxdoublenuFnu2Spectral energy distribution in 20-50GeV, in erg/cm^2^/s (nuFnu2)0.001W.m**-2phot.fluxdoublenuFnu3[0/] Spectral energy distribution in 50-150GeV, in erg/cm^2^/s (nuFnu3)0.001W.m**-2phot.fluxdoublenuFnu4[0/] Spectral energy distribution in 150-500GeV, in erg/cm^2^/s (nuFnu4)0.001W.m**-2phot.fluxdoublenuFnu5[0/] Spectral energy distribution in 500-2000GeV, in erg/cm^2^/s (nuFnu5)0.001W.m**-2phot.fluxdoubleTS1[0/134] Square root of the Test Statistic in 10-20GeV (Sqrt_TS_Band1)stat.fit.goodnessfloatTS2[0/89] Square root of the Test Statistic in 20-50GeV (Sqrt_TS_Band2)stat.fit.goodnessfloatTS3[0/60] Square root of the Test Statistic in 50-150GeV (Sqrt_TS_Band3)stat.fit.goodnessfloatTS4[0/34] Square root of the Test Statistic in 150-500GeV (Sqrt_TS_Band4)stat.fit.goodnessfloatTS5[0/16] Square root of the Test Statistic in 500-2000GeV (Sqrt_TS_Band5)stat.fit.goodnessfloatNpred[4/3734] Predicted number of events in the model (Npred)meta.numberfloatHEPE[11.9/1997] Highest energy among events probably coming from the source (HEP_Energy)GeVphys.energy;stat.maxfloatHEPPProbability of that event to come from the source (HEP_Prob)stat.fit.goodnessfloatVar[1/15]? Number of Bayesian blocks from variability analysis (1=not variable) (Variability_BayesBlocks)meta.numberintnullableExNameCross-reference to the ExtendedSources extension (Extended_Source_Name)meta.id.assoccharAssocCorrespondence to previous {gamma}-ray source catalog (ASSOC_GAM) (3)meta.id.assoccharf_TNameTeVCat flag (TEVCAT_FLAG) (4)meta.codecharTNameName of likely corresponding TeV source from TeVCat, if any (ASSOC_TEV)meta.id.assoccharClClass designation for associated source see Table 2 (CLASS) (5)meta.code.classcharAssoc1Name of identified or likely associated source (ASSOC1)meta.id.assoccharAssoc2Alternate name or indicates whether the source is inside an extended sourcemeta.id.assoccharPBay? Probability of association according to the Bayesian method (ASSOC_PROB_BAY)stat.fit.goodnessfloatnullablePLR? Probability of association according to the Likelihood-Ratio method (ASSOC_PROB_LR)stat.fit.goodnessfloatnullablez[0.003/2.6]? Redshift of counterpart, if known (Redshift)src.redshiftfloatnullableNuPk? Frequency of the synchrotron peak of counterpart, if known (NuPeak_obs)Hzem.freqdoublenullable
J/ApJS/232/18/roiRegions Of Interest (ROI) over which the analysis ranrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintROI[1/741] Running sequence number of the ROI (ROI_num)meta.numberintRAJ2000Right ascension; J2000 (RAJ2000)degpos.eq.ra;meta.mainDEJ2000Declination; J2000 (DEJ2000)degpos.eq.dec;meta.mainGLONGalactic longitudedegpos.galactic.lonGLATGalactic latitudedegpos.galactic.latfloatRad[2.5/9] Radius (RADIUS)degphys.angSizefloatPar1[0.5/1.4] iso_P8V3_Source Normalization (PARNAM1)stat.fit.paramfloate_Par1[0.03/0.2]? Par1 uncertainty (Unc_PARNAM1)stat.errorfloatnullablePar2[0.8/1.7] gal_4yearP8V6_v3 Prefactor (PARNAM2)stat.fit.paramfloate_Par2[0.01/0.2]? Par2 uncertainty (Unc_PARNAM2)stat.errorfloatnullable
J/ApJS/232/18/table1Extended sources modeled in the 3FHL analysis (only 48 were detected)ModSpatial modelstat.param;meta.modelledcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint3FHL3FHL name (1)meta.id;meta.maincharNameName of the source that has been modeled as spatially extendedmeta.idcharChangesName of the source in previous catalog in case of a changemeta.idcharf_Mod[a]meta.codecharExt[0.1/3] Radius (or semimajor axis) (Extent) (2)degphys.angSizefloatbmin? Semiminor axis (3)degphys.angSize.sminAxisfloatnullablef_bminElliptical 2D shapes (3)meta.codecharRefReferencemeta.ref;pos.framechar