J/ApJS/227/7ivo://CDS.VizieR/J/ApJS/227/7doi:10.26093/cds/vizier.22270007CDSLi Y.Zhang B.Lu H.-J.2017-09-22T16:15:52Z2017-01-27T09:34:43ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frgamma-ray-astronomyredshiftedastronomical-reference-materialsextinctionchemical-abundancesGamma-ray bursts (GRBs) are classified into long and short categories based on their durations. Broadband studies suggest that these two categories of objects roughly correspond to two different classes of progenitor systems, i.e., compact star mergers (Type I) versus massive star core collapse (Type II). However, the duration criterion sometimes leads to mis-identification of the progenitor systems. We perform a comprehensive multi-wavelength comparative study between duration-defined long GRBs and short GRBs as well as the so-called "consensus" long GRBs and short GRBs (which are believed to be more closely related to the two types of progenitor systems). The parameters we study include two parts: the prompt emission properties including duration (T_90_), spectral peak energy (E_p_), low energy photon index ({alpha}), isotropic {gamma}-ray energy (E_{gamma},iso_), isotropic peak luminosity (L_p,iso_), and the amplitude parameters (f and f_eff_); and the host galaxy properties including stellar mass (M_*_), star formation rate, metallicity ([X/H]), half light radius (R_50_), angular and physical (R_off_) offset of the afterglow from the center of the host galaxy, the normalized offset (r_off_=R_off_/R_50_), and the brightness fraction F_light_. For most parameters, we find interesting overlapping properties between the two populations in both one-dimensional (1D) and 2D distribution plots. The three best parameters for the purpose of classification are T_90_, f_eff_, and F_light_. However, no single parameter alone is good enough to place a particular burst into the right physical category, suggesting the need for multiple criteria for physical classification.2016ApJS..227....7Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/227/7CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toIX/20 : The Fourth BATSE Burst Revised Catalog (Paciesas+ 1999)J/ApJS/224/20 : 10yr of Swift/XRT obs. of GRBs (Yi+, 2016)J/ApJ/802/103 : Model predictions for GRB host galaxies (Trenti+, 2015)J/A+A/581/A125 : UV/Optical/NIR spectroscopy GRB hosts (Kruehler+, 2015)J/A+A/568/A19 : Photometry of 3 {gamma}-ray burst supernovae (Cano+, 2014)J/ApJS/211/13 : The second Fermi/GBM GRB catalog (4yr) (von Kienlin+, 2014)J/ApJ/778/128 : GRB-host galaxies photometry (Perley+, 2013)J/ApJS/208/21 : The BATSE 5B GRB spectral catalog (Goldstein+, 2013)J/ApJ/763/15 : Fermi GRB analysis. III. T_90_ distributions (Qin+, 2013)J/A+A/557/A100 : Fermi and Swift GRBs E_peak_-E_iso_ relation (Heussaff+, 2013)J/ApJS/199/18 : The Fermi GBM catalog (Paciesas+, 2012)J/ApJS/195/2 : The second Swift BAT GRB catalog (BAT2) (Sakamoto+, 2011)J/ApJ/731/103 : Redshift catalog for Swift long GRBs (Xiao+, 2011)J/ApJ/720/1513 : The afterglows of Swift-era GRBs. I. (Kann+, 2010)J/ApJS/180/192 : BeppoSAX/GRBM {gamma}-ray Burst Catalog (Frontera+, 2009)J/ApJ/609/935 : Gamma-ray burst formation rate (Yonetoku+, 2004)J/ApJS/126/19 : BATSE gamma-ray burst spectral catalog. I. (Preece+, 2000)http://swift.gsfc.nasa.gov/archive/grb_table/ : Swift GRBs at NASAhttp://www.mpe.mpg.de/~jcg/grbgen.html : List of GRBshttp://ibas.iasf-milano.inaf.it/IBAS_Results.html : GRBs localized with IBAShttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/227/7https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/227/7http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/227/7https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/227/7https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/227/7http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/227/7GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/227/7/table1 (Basic sample)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/227/7/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/227/7/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/227/7/table1?GETtext/xml+votable180.050000true328.12532.0145830.0055555555555555566/186 207 210 228 314 393 500 503 557 646 699 908 918 923 1087 2044 2315 2336 2357 2735 2948 2949 3059 3111 3536 3586 3700 3935 4312 4323 4341 4371 4397 4449 4450 4955 5051 5376 5455 5493 5625 5726 5745 5840 5941 6102 6141 6258 6261 6445 6448 6523 6729 7044 7182 7184 7227 7518 7532 7589 7650 8074 8103 8182 8318 8375 8425 8459 8641 8669 8733 8761 8798 8932 8954 9022 9100 9321 9363 9370 9431 9662 9682 9897 9910 9989 9998 10080 10094 10135 10400 10401 10407 10447 10519 10589 10666 10704 10723 10762 10852 10912 11008 11058 11220 11657 11673 11713 11756 11822 11905 12020 12134 12438 12597 13312 13331 13574 13694 13701 13720 13779 13828 13924 14259 14892 14967 14977 15004 15054 15214 15246 15295 15348 15530 15915 16057 16072 16212 16276 16282 16303 16489 16546 16661 16919 16991 17038 17316 17406 17411 17453 17561 17703 17721 17733 17749 17758 17814 17911 17980 17982 18030 18494 18681 18728 18777 18945 18978 19049 19164 19168 19194 19293 19519 19731 19864 19865 19890 19911 20030 20053 20191 20263 20346 20360 20372 20460 20655 20710 20753 21082 21137 21284 21498 21595 21688 21766 21962 22005 22008 22129 22422 22559 22580 22590 22619 22624 22916 23138 23413 24007 24072 24779 24926 24993 25061 25131 25146 25148 25174 25192 25248 25293 25394 25452 25761 25901 25946 26011 26036 26076 26365 26441 26503 26671 27085 27238 27289 27541 27566 27572 27810 27841 27906 27933 27961 27962 27983 28032 28058 28063 28071 28187 28202 28224 28234 28344 28467 28496 28497 28546 28555 28930 29019 29231 29731 30088 30557 31185 31281 31385 31494 31521 31583 31607 31700 31934 32110 32239 32310 32646 32713 32790 33004 33050 33146 33265 33278 33525 33617 33679 33735 33813 34147 34364 34435 34440 34465 34590 34605 34699 34788 34949 35045 35227 35330 35393 35427 35448 35569 35633 35844 36066 36297 36361 36460 36468 36528 37007 37123 37383 37391 37459 37505 37628 38280 38301 38926 39008 39024 39076 39327 39427 39553 39594 39993 40249 40273 40433 40560 40778 40784 41095 41285 42545 42892 42901 42914 42952 43193 43853 44022 44212 44436 44630 44857 45008 45081 45180 45205 45361 45401 45402 45409 45422 45469 45510 45561 45777 45828 45836 45938 46002 46022 46218 46250 46365 46395 46488 46510 46517 46594 46789 46989 47027 47031 47136 47148 47162 47217 47245 47251 47436 47459 47620 47991 48007 48054 48189 48371 48447 48458 48666 48804 49004https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/227/7?format=asciiGamma-rayOpticaldefaultJ/ApJS/227/7/table1Basic sampleSimbadNameSimbad column added by the CDSmeta.idcharl_T90Limit flag on T90meta.code.errorcharl_zLimit flag on zmeta.code.error;src.redshiftcharz[0.008/8.3]? Redshiftsrc.redshiftdoublenullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTypeType of GRB (L=long or S=short)meta.codecharGRBGRB identifiermeta.id;meta.maincharprimaryf_GRB[a] Flag on GRB (G1)meta.codecharE_z[0.001/0.6]? Upper uncertainty on zstat.error;stat.maxfloatnullablee_z[0.001/0.6]? Lower uncertainty in zstat.error;src.redshiftfloatnullablen_zMethod on z (1)meta.notecharr_z? Reference code for z (see refs.dat file)meta.ref;pos.frameintnullablen_T90Observatory used to obtain T90meta.notecharT90[0.02/25000] Timescale where 5-95% of total {gamma}-ray fluence is emittedstime.intervaldoublee_T90[0.05/23]? Uncertainty in T90sstat.errorfloatnullableT90ex[77/120]? T90 including the extended emission (2)stime.intervalintnullabler_T90Reference code for T90 (see refs.dat file)meta.ref;pos.frameintEg_iso? Isotropic 1-1e4keV energy; erg (3)1e-07Jphys.energydoublenullableLp_iso? Isotropic peak 1-1e4keV luminosity; erg/s (4)1e-07Wphys.luminositydoublenullablef[1/42.5]? Amplitude f parameter, F_p_/F_b_ (5)phot.flux;arith.ratiofloatnullablefeff[1/8]? Effective f parameter (6)phot.flux;arith.ratiofloatnullablee_feff[0.01/2]? Uncertainty in feffstat.errorfloatnullableNEDSimbad column added by the CDSmeta.ref.urlchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainJ/ApJS/227/7/table2Prompt emission properties sample (see section 2.1)l_EpLimit flag on EPmeta.code.errorcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTypeType of GRB (L=long or S=short)meta.codecharGRBGRB identifiermeta.id;meta.maincharprimaryDetDetector used to obtain the datainstr.setup;instr.detcharGamma[0.4/3.2]? Power law indexmeta.code;spect.indexfloatnullableE_Gamma[0/0.8]? Upper uncertainty in Gammastat.error;stat.maxfloatnullablee_Gamma[0/0.8]? Lower uncertainty in Gammastat.errorfloatnullablealpha[-1.9/-0.06]? Low energy photon indexspect.indexfloatnullableE_alpha[0/2.3]? Upper uncertainty in alphastat.error;stat.maxfloatnullablee_alpha[0/2.2]? Lower uncertainty in alphastat.error;pos.eq.rafloatnullablel_betaLimit flag on betameta.code.errorcharbeta[-22.1/-1.5]? High energy photon indexspect.indexfloatnullableE_beta[0/11.1]? Upper uncertainty in betastat.error;stat.maxfloatnullablee_beta[0/11.1]? Lower uncertainty in betastat.errorfloatnullableEp[2.6/4301]? Spectral peak energykeVem.energyfloatnullableE_Ep[1/2398]? Upper uncertainty in EpkeVstat.error;stat.maxfloatnullablee_Ep[0.8/901]? Lower uncertainty in EpkeVstat.errorfloatnullablel_SgLimit flag on Sgmeta.code.errorcharSg[0.07/24619] Energy fluence in SgBand; 1e-7erg/cm^2^1e-10J.m**-2phot.fluence;em.gamma.harddoubleE_Sg[0/610]? Upper uncertainty in Sg1e-10J.m**-2stat.error;stat.maxfloatnullablee_Sg[0/610]? Lower uncertainty in Sg1e-10J.m**-2stat.errorfloatnullableSgBandEnergy band range used for SgkeVinstr.bandpasscharKWFlag[1/8]? Konus-Wind flag (1)meta.codeintnullablel_FpLimit flag on Fpmeta.code.errorcharFp[0.02/8700]? The 1 second peak flux in FpBand; 1e-7erg/s/cm^2^1e-10W.m**-2phot.flux.density;em.gamma.harddoublenullableE_Fp[0/400]? Upper uncertainty in Fp1e-10W.m**-2stat.error;stat.maxfloatnullablee_Fp[0/430]? Lower uncertainty in Fp1e-10W.m**-2stat.errorfloatnullablef_Fp[p] p: Fp is a peak photon flux; ph/s/cm2meta.codecharFpBandEnergy band range used for FpkeVinstr.bandpasscharRefReference(s) (see refs.dat file)meta.ref;pos.framecharJ/ApJS/227/7/table3Star Formation Rate (SFR) of host galaxies (see section 2.2.1)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTypeType of GRB (L=long or S=short)meta.codecharGRBGRB identifiermeta.id;meta.maincharprimaryz[0.008/8.3]? Spectroscopic redshiftsrc.redshiftdoublenullableInstInstrument used to obtain the spectruminstr.setupcharl_logM*Limit flag on logM*meta.code.errorcharlogM*[7.7/12.3]? Log stellar masslog(solMass)phys.massfloatnullableE_logM*[0.01/1.5]? Upper uncertainty in logM*log(solMass)stat.error;stat.maxfloatnullablee_logM*[0.01/1.5]? Lower uncertainty in logM*log(solMass)stat.errorfloatnullablen_logM*Method used to derive logM* (SED, IR or line_width)meta.notecharl_SFRLimit flag on SFRmeta.code.error;phys.SFRcharSFR[0.01/280]? Star Formation RatesolMass/yrphys.SFRfloatnullableE_SFR[0.005/1563]? Upper uncertainty in SFRsolMass/yrstat.error;stat.maxdoublenullablee_SFR[0.005/174]? Lower uncertainty in methodsolMass/yrstat.error;phys.SFRfloatnullablen_SFRMethod used to derive SFRmeta.notesSFR[0.01/58]? Specific Star Formation RateGyr**-1meta.idfloatnullablel_[X/H]Limit flag on [X/H]meta.code.error;phys.abundchar[X/H][-2.2/0.7]? Metallicityphys.abundfloatnullable[X/H]up[-0.6/0.04]? Upper branch of R_23_-[X/H] relation (2)phys.abundfloatnullableE_[X/H][0.07/0.6]? Upper uncertainty in [X/H]stat.error;stat.maxfloatnullablee_[X/H][0.07/0.6]? Lower uncertainty in [X/H]stat.error;phys.abundfloatnullablen_[X/H]Method used to derive [X/H]meta.notecharl_AvLimit flag on Avmeta.code.errorcharAv[0/4.4]? Extinction in the V bandmagphys.absorption;em.opt.VdoublenullableE_Av[0/3]? Upper uncertainty in Avmagstat.error;stat.maxfloatnullablee_Av[0/2]? Lower uncertainty in Avmagstat.errorfloatnullablen_AvMethod used to derive Avmeta.notecharRefReference(s) (see refs.dat file)meta.ref;pos.framecharJ/ApJS/227/7/table4Offset of the GRB location from the center of host galaxy (see section 2.2.2)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTypeType of GRB (L=long or S=short)meta.codecharGRBGRB identifiermeta.id;meta.maincharprimaryf_GRB[a] Flag on GRB (G1)meta.codecharz[0.008/8.3]? Spectroscopic redshiftsrc.redshiftdoublenullableInstInstrument used to obtain the optical imageinstr.setup;obs.imagecharPcc[0/0.32]? Probability of chance coincidencestat.fit.goodnessfloatnullablel_R50aLimit flag on R50ameta.code.errorcharR50a[0.04/19]? Angular half light radiusarcsecphys.angSizefloatnullablef_R50a[*] Flag on R50a (1)meta.codecharE_R50a[0/0.8]? Upper uncertainty in R50aarcsecstat.error;stat.maxfloatnullablee_R50a[0/0.8]? Upper uncertainty in F50aarcsecstat.errorfloatnullablel_R50pLimit flag on R50pmeta.code.errorcharR50p[0.3/21]? Physical half light radiuskpcphysfloatnullableE_R50p[0/1.4]? Upper uncertainty in R50pkpcstat.error;stat.maxfloatnullablee_R50p[0/1.4]? Lower uncertainty in R50pkpcstat.errorfloatnullablen[0.3/5.6]? Sersic indexstat.fit.paramfloatnullablel_RoffaLimit flag on Roffameta.code.errorcharRoffa[0.01/18]? Angular GRB offset from host galaxy centerarcsecpos;arith.difffloatnullablef_Roffa[*] Flag on Roffa (1)meta.codecharE_Roffa[0/3.4]? Upper uncertainty in Roffaarcsecstat.error;stat.maxfloatnullablee_Roffa[0/3.4]? Lower uncertainty in Roffaarcsecstat.errorfloatnullablel_RoffpLimit flag on Roffpmeta.code.errorcharRoffp[0.07/86.2]? Physical GRB offset from host galaxy centerkpcpos;arith.difffloatnullableE_Roffp[0/18.1]? Upper uncertainty in Roffpkpcstat.error;stat.maxfloatnullablee_Roffp[0/18.1]? Lower uncertainty in Roffpkpcstat.errorfloatnullablel_roffLimit flag on roffmeta.code.errorcharroff[0.04/15.5]? Normalized offset (roff=Roff(a|p)/R50(a|p))pos;arith.difffloatnullableE_roff[0/5.2]? Upper uncertainty in roffstat.error;stat.maxfloatnullablee_roff[0/5.2]? Lower uncertainty in roffstat.errorfloatnullableFlight[0/1]? Fraction of host galaxy area brighter than GRB region (2)stat.fit.paramfloatnullableRefReference(s) (see refs.dat file)meta.ref;pos.framecharJ/ApJS/227/7/refsReferencesGCNLink to GCN circularmeta.ref.urlcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRefReference codemeta.noteintBibCodeBibcodemeta.bib.bibcodecharAuthFirst author's name(s)meta.bib.authorcharCommCommentmeta.notechar