IX/67/4fgldr3The incremental 4th Fermi LAT point source catalog, Data Release 3 (4FGL-DR3) -- 12 yearsROI[1/1988] ROI number (ROI_num)obs.fieldintLPEPk[0.03/1.2e+8]? Peak energy in nuFnu estimated from the LogParabola model (LP_EPeak)MeVphys.energy;stat.maxdoublenullablee_F10000[-4.4e-10/-1e-12]? Lower uncertainty on F10000 (LoUnc_Flux_Band6) (4)ph.cm**-2.s**-1stat.errordoublenullableFlags[0/14336] Source flags (binary coding as in Table 4) (10)meta.code.errorintFGLMost recent correspondence to FGL source catalogs prior to 4FGL, if any (ASSOC_FGL)meta.id.crosscharFHLMost recent correspondence to previous FHL source catalogs, if any (ASSOC_FHL)meta.id.crosscharAssoc1Name of identified or likely associated source (ASSOC1)meta.id.assoccharLC1-year light curve for this sourcemeta.ref.urlcharSimbadSimbad column added by the CDSmeta.ref.urlcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintDR[1/3] Data release number (DataRelease) (2)meta.codeintRAJ2000Right ascension in decimal degrees (J2000) (RAJ2000)degpos.eq.ra;meta.mainDEJ2000Declination in decimal degrees (J2000) (DEJ2000)degpos.eq.dec;meta.mainGLONGalactic longitudedegpos.galactic.lonGLAT[-88/88.7] Galactic latitudedegpos.galactic.latdoublee_LPEPk[0.5/1.1e+10]? LPEPk uncertainty (Unc_LP_EPeak)MeVstat.errordoublenullableamaj68[0.004/0.6]? Long radius of error ellipse at 68% confidence (Conf_68_SemiMajor) (3)degphys.angSize;pos.errorEllipsedoublenullablebmin68[0.004/0.4]? Short radius of error ellipse at 68% confidence (Conf_68_SemiMinor) (3)degphys.angSize;pos.errorEllipsedoublenullablePA68[-90/90]? Position angle of the 68% ellipse (Conf_68_PosAng) (3)degpos.posAng;pos.errorEllipsefloatnullableamaj95[0.007/0.9]? Long radius of error ellipse at 95% confidence (Conf_95_SemiMajor)degphys.angSize;pos.errorEllipsefloatnullablebmin95[0.007/0.7]? Short radius of error ellipse at 95% confidence (Conf_95_SemiMinor)degphys.angSize;pos.errorEllipsefloatnullablePA95[-90/90]? Position angle (eastward) of the long axis from celestial north (Conf_95_PosAng)degpos.posAng;pos.errorEllipsefloatnullableSig[1.6/885]? Source significance in {sigma} units over the 100MeV to 1TeV band (Signif_Avg)stat.fit.goodnessdoublenullableE0[49.6/195055] Energy at which error on differential flux is minimal (Pivot_Energy)MeVem.energydoubleF1000i[3.7e-13/1.4e-6] Integral photon flux from 1 to 100GeV (Flux1000)cm**-2.ph.s**-1phot.flux.density;em.gamma.harddoublee_F1000i[1.5e-13/4e-9]? F1000i uncertainty (Unc_Flux1000)cm**-2.ph.s**-1stat.errordoublenullableEF100[3.7e-13/9.3e-9] Energy flux from 100MeV to 100GeV obtained by spectral fitting in erg/cm^2^/s (Energy_Flux100)mW.m**-2phot.flux.density;em.gamma.harddoublee_EF100[1e-13/3.1e-11]? EF100 uncertainty (Unc_Energy_Flux100)mW.m**-2stat.errordoublenullableFpivPL[2.6e-17/2.4e-7]? Differential flux at Pivot Energy in PowerLaw fit (PL_Flux_Density)cm**-2.MeV**-1.ph.s**-1phot.flux;arith.ratiodoublenullablee_FpivPL[1e-17/1.8e-8]? FpivPL uncertainty (Unc_PL_Flux_Density)cm**-2.MeV**-1.ph.s**-1stat.errordoublenullablePLGam[1/3.4]? Photon index when fitting with PowerLaw (PL_Index)spect.indexdoublenullablee_PLGam[0.0005/0.6]? PLGam uncertainty (Unc_PL_Index)spect.indexdoublenullableFpivLP[3.6e-17/1.8e-7] Differential flux at Pivot Energy in LogParabola fit (LP_Flux_Density)cm**-2.MeV**-1.ph.s**-1phot.flux;arith.ratiodoublee_FpivLP[1.8e-17/9e-9]? FpivLP uncertainty (Unc_LP_Flux_Density)cm**-2.MeV**-1.ph.s**-1stat.errordoublenullableLPalpha[-0.05/3.5] Photon index at Pivot Energy ({alpha} of Eq. 1) when fitting with LogParabola (LP_Index)spect.indexdoublee_LPalpha[0.002/3]? LPalpha uncertainty (Unc_LP_Index)spect.indexdoublenullableLPbeta[-0.16/1] Curvature parameter ({beta} of Eq. 1) when fitting with LogParabola (LP_beta)stat.fit.paramdoublee_LPbeta[0.002/1.8]? LPbeta uncertainty (Unc_LP_beta)stat.fit.paramdoublenullableSigCurv1[0/240] Significance (in {sigma} units) of the fit improvement between PowerLaw and LogParabola (LP_SigCurv)stat.fit.goodnessdoubleFpivPLEC[4e-17/1.8e-7]? Differential flux at Pivot Energy in PLSuperExpCutoff fit (PLEC_Flux_Density)cm**-2.MeV**-1.ph.s**-1phot.flux;arith.ratiodoublenullablee_FpivPLEC[2e-17/1.2e-8]? FpivPLEC uncertainty (Unc_PLEC_Flux_Density)cm**-2.MeV**-1.ph.s**-1stat.errordoublenullablePLECGamS[-0.16/3.4]? Photon index at Pivot Energy ({Gamma}_S_ of Eq. 2) when fitting with PLSuperExpCutoff (PLEC_IndexS)spect.indexdoublenullablee_PLECGamS[0.004/4.7]? PLECGamS uncertainty (Unc_PLEC_IndexS)stat.errordoublenullablePLECCd[-0.4/5.5]? Spectral curvature at Pivot Energy (d of Eq. 2) when fitting with PLSuperExpCutoff (PLEC_ExpfactorS)stat.fit.paramdoublenullablee_PLECCd[0/9.7]? PLECCd uncertainty (Unc_PLEC_ExpfactorS)stat.errordoublenullablePLECCb[0.2/1]? Exponential index (b of Eq. 2) when fitting with PLSuperExpCutoff (PLEC_Exp_Index)stat.fit.paramdoublenullablee_PLECCb[0.01/0.15]? PLECCb uncertainty (Unc_PLEC_Exp_Index)stat.errordoublenullableSigCurv2[0/245] Significance (in {sigma} units) of the fit improvement between PowerLaw and PLSuperExpCutoff (PLEC_SigCurv)stat.fit.goodnessdoublePLECEPk[0.05/5e+6]? Peak energy in nuFnu estimated from the PLSuperExpCutoff model (PLEC_EPeak)MeVphys.energy;stat.maxdoublenullablee_PLECEPk[9.2/2.1e+8]? PLECEPk uncertainty (Unc_PLEC_EPeak)MeVstat.errordoublenullableNpred[5.9/261899] Predicted number of events in the modelmeta.numberdoubleF50[4.5e-19/5.4e-6] Integral photon flux in 50-100MeV (Band 1) (Flux_Band1)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_F50[-3.9e-7/-5.3e-9]? Lower uncertainty on F50 (LoUnc_Flux_Band1) (4)ph.cm**-2.s**-1stat.errordoublenullableE_F50? Upper uncertainty on F50 (UpUnc_Flux_Band1) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullableF100[7.6e-20/5.6e-6] Integral photon flux in 100-300MeV (Band 2) (Flux_Band2)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_F100[-5e-7/-5.3e-10]? Lower uncertainty on F100 (LoUnc_Flux_Band2) (4)ph.cm**-2.s**-1stat.errordoublenullableE_F100? Upper uncertainty on F100 (upUnc_Flux_Band2) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullableF300[5e-20/3.4e-6] Integral photon flux in 300MeV-1GeV (Band 3) (Flux_Band3)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_F300[-4.1e-8/-5.7e-11]? Lower uncertainty on F300 (LoUnc_Flux_Band3) (4)ph.cm**-2.s**-1stat.errordoublenullableE_F300? Upper uncertainty on F300 (upUnc_Flux_Band3) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullableF1000[7.3e-18/1.1e-6] Integral photon flux in 1-3GeV (Band 4) (Flux_Band4)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_F1000[-4.4e-9/-9.2e-12]? Lower uncertainty on F1000 (LoUnc_Flux_Band4) (4)ph.cm**-2.s**-1stat.errordoublenullableE_F1000? Upper uncertainty on F1000 (upUnc_Flux_Band4) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullableF3000[3.3e-20/2.3e-7] Integral photon flux in 3-10GeV (Band 5) (Flux_Band5)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_F3000[-1.1e-9/-2.7e-12]? Lower uncertainty on F3000 (LoUnc_Flux_Band5) (4)ph.cm**-2.s**-1stat.errordoublenullableE_F3000? Upper uncertainty on F3000 (upUnc_Flux_Band5) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullableF10000[2.7e-24/1.2e-8] Integral photon flux in 10-30GeV (Band 6) (Flux_Band6)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoubleE_F10000[1.9e-12/4.5e-10]? Upper uncertainty on F10000 (upUnc_Flux_Band6) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullableF30000[3.9e-26/4.7e-9] Integral photon flux in 30-100GeV (Band 7) (Flux_Band7)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_F30000[-1.7e-10/-8.9e-13]? Lower uncertainty on F30000 (LoUnc_Flux_Band7) (4)ph.cm**-2.s**-1stat.errordoublenullableE_F30000? Upper uncertainty on F30000 (upUnc_Flux_Band7) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullableF100000[0/1.7e-9] Integral photon flux in 100GeV-1TeV (Band 8) (Flux_Band8)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_F100000[-9.9e-11/-8.9e-13]? Lower uncertainty on F100000 (LoUnc_Flux_Band8) (4)ph.cm**-2.s**-1stat.errordoublenullableE_F100000[1.7e-12/9.9e-11]? Upper uncertainty on F100000 (upUnc_Flux_Band8) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullablenuFnu50[7.8e-23/8.9e-10] Spectral energy distribution over 50-100MeV in erg/cm2/s (nuFnu_Band1)mW.m**-2phot.fluxdoublenuFnu100[1.8e-23/1.5e-9] Spectral energy distribution over 100-300MeV in erg/cm2/s (nuFnu_Band2)mW.m**-2phot.fluxdoublenuFnu300[3.6e-23/2.5e-9] Spectral energy distribution over 300MeV-1GeV in erg/cm2/s (nuFnu_Band3)mW.m**-2phot.fluxdoublenuFnu1000[2e-20/2.6e-9] Spectral energy distribution over 1-3GeV in erg/cm2/s (nuFnu_Band4)mW.m**-2phot.fluxdoublenuFnu3000[1.7e-22/1.4e-9] Spectral energy distribution over 3-10GeV in erg/cm2/s (nuFnu_Band5)mW.m**-2phot.fluxdoublenuFnu10000[6e-26/2.3e-10] Spectral energy distribution over 10-30GeV in erg/cm2/s (nuFnu_Band6)mW.m**-2phot.fluxdoublenuFnu30000[2e-27/3.2e-10] Spectral energy distribution over 30-100GeV in erg/cm2/s (nuFnu_Band7)mW.m**-2phot.fluxdoublenuFnu100000[0/2.6e-10] Spectral energy distribution over 100GeV-1TeV in erg/cm2/s (nuFnu_Band8)mW.m**-2phot.fluxdoubleTS50[0/26]? Square root of the Test Statistic in 50-100MeV (Sqrt_TS_Band1)stat.likelihood;obsdoublenullableTS100[0/142]? Square root of the Test Statistic in 100-300MeV (Sqrt_TS_Band2)stat.likelihood;obsdoublenullableTS300[0/388]? Square root of the Test Statistic in 300MeV-1GeV (Sqrt_TS_Band3)stat.likelihood;obsdoublenullableTS1000[0/581]? Square root of the Test Statistic in 1-3GeV (Sqrt_TS_Band4)stat.likelihood;obsdoublenullableTS3000[0/498]? Square root of the Test Statistic in 3-10GeV (Sqrt_TS_Band5)stat.likelihood;obsdoublenullableTS10000[0/189]? Square root of the Test Statistic in 10-30GeV (Sqrt_TS_Band6)stat.likelihood;obsdoublenullableTS30000[0/107]? Square root of the Test Statistic in 30-100GeV (Sqrt_TS_Band7)stat.likelihood;obsdoublenullableTS100000[0/68]? Square root of the Test Statistic in 100GeV-1TeV (Sqrt_TS_Band8)stat.likelihood;obsdoublenullableVarInd[1.59/84341]? Variability (Variability_Index) (5)src.var.indexdoublenullablefVar[0/3]? Fractional variability computed from the fluxes in each year (Frac_Variability)phot.mag;arith.ratiodoublenullablee_fVar[0.003/10]? fVar uncertainty (Unc_Frac_Variability)stat.errordoublenullableSigPk[3.4/413]? Source significance in peak interval in {sigma} units (Signif_Peak)stat.fit.goodnessdoublenullableFPk[1.8e-10/5.1e-6]? Peak integral photon flux from 100MeV to 100GeV (Flux_Peak)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublenullablee_FPk[7e-11/3.4e-8]? FPk uncertainty (Unc_Flux_Peak)ph.cm**-2.s**-1stat.errordoublenullableTPk[255223712/602270016]? Time of center of interval in which peak flux was measured (Time_Peak)stime.epochlongnullableIntPk[3.1e+7/3.2e+7]? Length of interval in which peak flux was measured (Peak_Interval)stime.interval;phys.sizedoublenullableF100y1[1.7e-21/1.1e-5] Integral photon flux from 100 MeV to 100 GeV in year 1 (Flux_History1)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_F100y1[-6.4e-8/-1.7e-11]? Lower uncertainty on F100y1 (loUnc_Flux_History1) (4)ph.cm**-2.s**-1stat.errordoublenullableE_F100y1? Upper uncertainty on F100y1 (upUnc_Flux_History1) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullableF100y2Integral photon flux from 100 MeV to 100 GeV in year 2 (Flux_History2)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_F100y2[-6.3e-8/-1.4e-11]? Lower uncertainty on F100y2 (loUnc_Flux_History2) (4)ph.cm**-2.s**-1stat.errordoublenullableE_F100y2? Upper uncertainty on F100y2 (upUnc_Flux_History2) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullableF100y3Integral photon flux from 100 MeV to 100 GeV in year 3 (Flux_History3)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_F100y3[-6.3e-8/-1.4e-11]? Lower uncertainty on F100y3 (loUnc_Flux_History3) (4)ph.cm**-2.s**-1stat.errordoublenullableE_F100y3? Upper uncertainty on F100y3 (upUnc_Flux_History3) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullableF100y4Integral photon flux from 100 MeV to 100 GeV in year 4 (Flux_History4)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_F100y4[-6.3e-8/-1.3e-11]? Lower uncertainty on F100y4 (loUnc_Flux_History4) (4)ph.cm**-2.s**-1stat.errordoublenullableE_F100y4? Upper uncertainty on F100y4 (upUnc_Flux_History4) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullableF100y5Integral photon flux from 100 MeV to 100 GeV in year 5 (Flux_History5)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_F100y5[-6.4e-8/-1.7e-11]? Lower uncertainty on F100y5 (loUnc_Flux_History5) (4)ph.cm**-2.s**-1stat.errordoublenullableE_F100y5? Upper uncertainty on F100y5 (upUnc_Flux_History5) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullableF100y6Integral photon flux from 100 MeV to 100 GeV in year 6 (Flux_History6)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_F100y6[-6.5e-8/-1.4e-11]? Lower uncertainty on F100y6 (loUnc_Flux_History6) (4)ph.cm**-2.s**-1stat.errordoublenullableE_F100y6? Upper uncertainty on F100y6 (upUnc_Flux_History6) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullableF100y7Integral photon flux from 100 MeV to 100 GeV in year 7 (Flux_History7)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_F100y7[-6.5e-8/-1.5e-11]? Lower uncertainty on F100y7 (loUnc_Flux_History7) (4)ph.cm**-2.s**-1stat.errordoublenullableE_F100y7? Upper uncertainty on F100y7 (upUnc_Flux_History7) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullableF100y8[1.7e-22/1.1e-5] Integral photon flux from 100 MeV to 100 GeV in year 8 (Flux_History8)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_F100y8[-6.3e-8/-1.6e-11]? Lower uncertainty on F100y8 (loUnc_Flux_History8) (4)ph.cm**-2.s**-1stat.errordoublenullableE_F100y8? Upper uncertainty on F100y8 (upUnc_Flux_History8) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullableF100y9[3.2e-21/1.1e-5] Integral photon flux from 100 MeV to 100 GeV in year 9 (Flux_History9)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_F100y9[-6.3e-8/-1.8e-11]? Lower uncertainty on F100y9 (loUnc_Flux_History9) (4)ph.cm**-2.s**-1stat.errordoublenullableE_F100y9? Upper uncertainty on F100y9 (upUnc_Flux_History9) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullableF100y10Integral photon flux from 100 MeV to 100 GeV in year 10 (Flux_History10)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_F100y10[-5.9e-8/-1.8e-11]? Lower uncertainty on F100y10 (loUnc_Flux_History10) (4)ph.cm**-2.s**-1stat.errordoublenullableE_F100y10? Upper uncertainty on F100y10 (upUnc_Flux_History10) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullableF100y11Integral photon flux from 100 MeV to 100 GeV in year 11 (Flux_History11)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_F100y11[-6.2e-8/-1.7e-11]? Lower uncertainty on F100y11 (loUnc_Flux_History11) (4)ph.cm**-2.s**-1stat.errordoublenullableE_F100y11? Upper uncertainty on F100y11 (upUnc_Flux_History11) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullableF100y12[1e-22/1.1e-5] Integral photon flux from 100 MeV to 100 GeV in year 12 (Flux_History12)ph.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_F100y12[-5.8e-8/-1.3e-11]? Lower uncertainty on F100y12 (loUnc_Flux_History12) (4)ph.cm**-2.s**-1stat.errordoublenullableE_F100y12? Upper uncertainty on F100y12 (upUnc_Flux_History12) (4)ph.cm**-2.s**-1stat.error;stat.maxdoublenullableTS100y1[0/427] Square root of the Test Statistic in year 1 (Sqrt_TS_History1)stat.likelihood;obsdoubleTS100y2Square root of the Test Statistic in year 2 (Sqrt_TS_History2)stat.likelihood;obsdoubleTS100y3Square root of the Test Statistic in year 3 (Sqrt_TS_History3)stat.likelihood;obsdoubleTS100y4Square root of the Test Statistic in year 4 (Sqrt_TS_History4)stat.likelihood;obsdoubleTS100y5Square root of the Test Statistic in year 5 (Sqrt_TS_History5)stat.likelihood;obsdoubleTS100y6Square root of the Test Statistic in year 6 (Sqrt_TS_History6)stat.likelihood;obsdoubleTS100y7Square root of the Test Statistic in year 7 (Sqrt_TS_History7)stat.likelihood;obsdoubleTS100y8[0/390] Square root of the Test Statistic in year 8 (Sqrt_TS_History8)stat.likelihood;obsdoubleTS100y9Square root of the Test Statistic in year 9 (Sqrt_TS_History9)stat.likelihood;obsdoubleTS100y10Square root of the Test Statistic in year 10 (Sqrt_TS_History10)stat.likelihood;obsdoubleTS100y11Square root of the Test Statistic in year 11 (Sqrt_TS_History11)stat.likelihood;obsdoubleTS100y12[0/360] Square root of the Test Statistic in year 12 (Sqrt_TS_History12)stat.likelihood;obsdoublef_TeVCatFlag on TeVCat (TEVCAT_FLAG)meta.codecharAssoc2Name of low-confidence association or of enclosing extended source (ASSOC2)meta.id.assoccharProbBy[0/1]? Probability of association according to the Bayesian method (ASSOC_PROB_BAY) (7)stat.fit.goodnessdoublenullableProbLR[0/1]? Probability of association according to the Likelihood Ratio method (ASSOC_PROB_LR) (8)stat.likelihood;stat.probabilitydoublenullableRACdeg? Right ascension of the counterpart Assoc1 (J2000) (RA_Counterpart)degmeta.id.assoc;pos.eq.ranullableDECdeg? Declination of the counterpart Assoc2 (J2000) (DEC_Counterpart)degmeta.id.assoc;pos.eq.decnullableerrPos[3e-9/2.5]? 95% precision of the counterpart localization (Unc_Counterpart) (9)degmeta.code.qual;instr.precisiondoublenullable4FGLThe 4FGL name (JHHMM.m+DDMMa) (Source_Name) (1)meta.id;meta.maincharNameCross-reference to the ExtendedSources extension (Extended_Source_Name)meta.idcharModSpectral type in the global model (PowerLaw, LogParabola, PLSuperExpCutoff) (SpectrumType)src.spType;meta.modelledcharAsso4FGLCorrespondence to 4FGL source catalog, if any (ASSOC_4FGL)meta.id.crosschar2AGLName of likely corresponding 2AGL source, if any (ASSOC_GAM1)meta.id.crosschar3EGName of likely corresponding 3EG source, if any (ASSOC_GAM2)meta.id.crosscharEGRName of likely corresponding EGR source, if any (ASSOC_GAM3)meta.id.crosscharTeVCatName of likely corresponding TeV source from TeVCat, if any (ASSOC_TEV)meta.id.crosscharCl1Class designation for associated source; see Table 5 (CLASS1) (6)meta.code.classcharCl2Class designation for low-confidence association (CLASS2)meta.code.classchar