J/ApJ/794/82ivo://CDS.VizieR/J/ApJ/794/82doi:10.26093/cds/vizier.17940082CDSBartoli B.Bernardini P.Bi X.J.Branchini P.Budano A.Camarri P.,Cao Z.Cardarelli R.Catalanotti S.Chen S.Z.Chen T.L.Creti P.,Cui S.W.Dai B.Z.D'Amone A.DanzengluobuDe Mitri I.,D'Ettorre Piazzoli B.Di Girolamo T.Di Sciascio G.Feng C.F.Feng Z.,Feng Z.Gou Q.B.Guo Y.Q.He H.H.Hu H.Hu H.Iacovacci M.Iuppa R.,Jia H.Y.LabacirenLi H.J.Liguori G.Liu C.Liu J.Liu M.Y.Lu H.,Ma L.L.Ma X.H.Mancarella G.Mari S.M.Marsella G.Martello D.,Mastroianni S.Montini P.Ning C.C.Panareo M.Perrone L.Pistilli P.,Ruggieri F.Salvini P.Santonico R.Shen P.R.Sheng X.D.Shi F.,Surdo A.Tan Y.H.Vallania P.Vernetto S.Vigorito C.Wang H.,Wu C.Y.Wu H.R.Xue L.Yang Q.Y.Yang X.C.Yao Z.G.Yuan A.F.,Zha M.Zhang H.M.Zhang L.Zhang X.Y.Zhang Y.Zhao J.Zhaxiciren,ZhaxisangzhuZhou X.X.Zhu F.R.Zhu Q.Q.Zizzi G.,(the ARGO-YBJ Collaboration)2017-06-06T07:44:11Z2017-05-16T14:58:16ZCDS support team

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

cds-question@unistra.frgamma-ray-astronomystellar-spectral-typesThe search for gamma-ray burst (GRB) emission in the energy range of 1-100 GeV in coincidence with the satellite detection has been carried out using the Astrophysical Radiation with Ground-based Observatory at YangBaJing (ARGO-YBJ) experiment. The high-altitude location (4300 m a.s.l.), the large active surface (~6700 m^2^ of Resistive Plate Chambers), the wide field of view (~2 sr, limited only by the atmospheric absorption), and the high duty cycle (>86%) make the ARGO-YBJ experiment particularly suitable to detect short and unexpected events like GRBs. With the scaler mode technique, i.e., counting all the particles hitting the detector with no measurement of the primary energy and arrival direction, the minimum threshold of ~1 GeV can be reached, overlapping the direct measurements carried out by satellites. During the experiment lifetime from 2004 December 17 to 2013 February 7, a total of 206 GRBs occurring within the ARGO-YBJ field of view (zenith angle {theta}<=45{deg}) have been analyzed. This is the largest sample of GRBs investigated with a ground-based detector. Two light curve models have been assumed and since in both cases no significant excess has been found, the corresponding fluence upper limits in the 1-100 GeV energy region have been derived, with values as low as 10^-5^ erg/cm2. The analysis of a subset of 24 GRBs with known redshift has been used to constrain the fluence extrapolation to the GeV region together with possible cutoffs under different assumptions on the spectrum.2014ApJ...794...82Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/794/82CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toIX/36 : GRANAT/PHEBUS catalog of cosmic gamma-ray burstsJ/A+A/438/1175 : First INTEGRAL SPI-ACS Gamma-Ray Burst Catalogue (Rau+, 2005)J/ApJ/829/7 : The third Swift/BAT GRB catalog (past ~11yrs) (BAT3)J/ApJS/223/28 : The third Fermi/GBM GRB catalog (6yr) (Bhat+, 2016)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/794/82https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/794/82http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/794/82https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/794/82https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/794/82http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/794/82GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/794/82/table2 (GRBs with No Measured Redshift (z=2 and z=0.6 are Assumed for Long and Short GRBs, Respectively) Observed by ARGO-YBJ)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/794/82/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/794/82/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/794/82/table2?GETtext/xml+votable180.050000true336.655.050.0055555555555555566/146 210 398 877 1040 1049 1070 1507 1526 1532 1652 1827 1882 2296 2603 2683 2752 2875 3145 3164 3288 3289 3316 3354 3388 3399 3602 3659 3832 4140 4228 4741 4862 5153 5228 5323 5346 5650 5871 5907 5909 5945 6404 6439 6518 6576 6862 7043 7184 7300 7332 7390 7492 7747 7789 8617 8761 8966 9024 9215 9270 9298 9317 9330 9399 9536 9576 9636 9662 9827 10210 10247 10473 10529 10721 10723 10824 10994 11218 11482 11545 11640 12558 12565 12622 12726 12848 12893 13313 13363 13559 13574 13676 13767 13854 14404 14492 14555 14746 14781 14859 14967 14977 15292 15415 15513 15595 15683 15820 15995 16037 16137 17269 17561 17938 18081 18167 19060 19190 19237 19473 19544 19624 19991 21284 21495 21748 21766 22157 22580 22838 23637 24041 24113 24378 25529 26036 26084 26831 26999 27352 27566 27606 27964 28035 28361 28416 28578 30040 30137 30181 30595 30678 31092 31187 31241 31299 31526 31727 31730 31847 32055 32058 32183 32234 32484 32568 32744 36837 44918 44979 45246 49034https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/794/82?format=asciiGamma-rayOpticaldefaultJ/ApJ/794/82/table2GRBs with No Measured Redshift (z=2 and z=0.6 are Assumed for Long and Short GRBs, Respectively) Observed by ARGO-YBJSpTypeSpectral index (1)src.spTypecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGRBGRB name corresponding to the detection date in UT (YYMMDD)meta.id;time.epochcharSatelSatellite that detected the burstmeta.id;instrchart90Burst durationstime.durationfloattext90? Extended burst durationstime.durationfloatnullablethetaZenith angledegposfloatFSquare root of the Fano factor (Fano, 1947PhRv...72...26F)stat.fit.paramfloatf_SpType[*] Flag on SpType (2)meta.codecharAdetDetector active aream**2phys.area;instr.detintsigmaStatistical significance of the on-source counts over the background for standard burst durationstat.fit.goodnessfloatsigmaext? Statistical significance of the on-source counts over the background for extended burst durationinstr.backgroundfloatnullablefsat? 99% confidence upper limit on the fluence between 1 and 100 GeV for spectral index (in erg/cm^2^) (3)1e-07J.cm**-2phot.fluence;em.gamma.harddoublenullablef2.599% confidence upper limit on the fluence between 1 and 100 GeV for fixed value -2.5 (in erg/cm^2^) (4)1e-07J.cm**-2phot.fluence;em.gamma.harddoublel_Ecut[<] Limit flag on Ecutmeta.code.errorcharEcut? Cutoff upper limit (5)GeVem.energyintnullableSimbadSimbad column added by the CDSmeta.ref.urlchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.mainnullable_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainnullable