<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2015-05-06T12:38:50Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>A search for progenitors of short GRBs</title><shortName>J/ApJ/777/132</shortName><identifier>ivo://CDS.VizieR/J/ApJ/777/132</identifier><altIdentifier>doi:10.26093/cds/vizier.17770132</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Dichiara S.</name></creator><creator><name>Guidorzi C.</name></creator><creator><name>Frontera F.</name></creator><creator><name>Amati L.</name></creator><date role="Updated">2017-11-10T11:15:36Z</date><date role="Created">2015-05-06T12:38:50Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>gamma-ray-astronomy</subject><description>We searched for periodic and quasi-periodic signals in the prompt emission of a sample of 44 bright short gamma-ray bursts (GRBs) detected with Fermi/GBM, Swift/BAT, and CGRO/BATSE. The aim was to look for the observational signature of quasi-periodic jet precession, which is expected from black hole (BH)-neutron star (NS) mergers, but not from double NS systems. Thus, this kind of search holds the key to identifying the progenitor systems of short GRBs and, in the interim before gravitational wave detectors become on-lines, represents the only direct way to constrain the progenitors. We tailored our search to the nature of the expected signal by properly stretching the observed light curves by an increasing factor with time, after calibrating the technique with synthetic curves. None of our GRBs showed evidence for periodic or quasi-periodic signals. In particular, for the seven unambiguously short GRBs with the best signal-to-noise ratios, we obtained significant upper limits to the amplitude of the possible oscillations. This result suggests that BH-NS systems do not dominate the population of short GRB progenitors, as described by the kinematic model of Stone et al. (2013PhRvD..87h4053S).</description><source format="bibcode">2013ApJ...777..132D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/777/132</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/IX/20">IX/20 : The Fourth BATSE Burst Revised Catalog (Paciesas+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/216/32">J/ApJS/216/32 : Localizations of GRBs with Fermi GBM (Connaughton+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/211/13">J/ApJS/211/13 : The second Fermi/GBM GRB catalog (4yr) (von Kienlin+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/208/21">J/ApJS/208/21 : The BATSE 5B GRB spectral catalog (Goldstein+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/207/38">J/ApJS/207/38 : IPN localizations of Konus short GRBs (Pal'shin+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/431/3608">J/MNRAS/431/3608 : BeppoSAX/GRBM and Fermi/GBM long GRBs (Dichiara+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/207/39">J/ApJS/207/39 : IPN supplement to the Fermi GBM (Hurley+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/756/112">J/ApJ/756/112 : Fermi/GBM GRB time-resolved spectral analysis (Lu+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/748/134">J/ApJ/748/134 : Variability in BATSE GRB light curves (Gao+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/199/18">J/ApJS/199/18 : The Fermi GBM catalog (Paciesas+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/195/2">J/ApJS/195/2 : The second Swift BAT GRB catalog (BAT2) (Sakamoto+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/525/A53">J/A+A/525/A53 : GBM parameters for detected FERMI bursts (Guetta+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/740/104">J/ApJ/740/104 : BATSE GRB pulse catalog - preliminary data (Hakkila+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/711/495">J/ApJ/711/495 : Durations of Swift/BAT GRBs (Butler+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/134/385">J/ApJS/134/385 : Supplement to the BATSE GRB catalogs (Kommers+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/508/314">J/ApJ/508/314 : Gamma-ray bursts types (Mukherjee+, 1998)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/777/132</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/777/132</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/777/132</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/777/132</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/777/132</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/777/132</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/777/132/table1 (Best-fitting model and parameters for each 44 short duration gamma-ray burst (SGRB) of the total sample)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/777/132/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/777/132/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/777/132/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>328.7026</ra><dec>16.8909</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/390 866 3318 3706 4236 5371 6348 7519 7789 9675 12597 13411 13762 16672 18195 19529 20015 20191 20631 20800 20934 20935 21354 22216 22590 22916 23129 23329 27711 28234 29105 31342 32741 34917 35448 35574 35899 38723 39024 39463 44125 45180 47544 48666</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/777/132?format=ascii</footprint><waveband>Gamma-ray</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/777/132/table1</name><description>Best-fitting model and parameters for each 44 short duration gamma-ray burst (SGRB) of the total sample</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>GRB</name><description>Gamma-ray Burst identifier (YYMMDDA)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>r_GRB</name><description>[d-f] Detection origin (1)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Mod</name><description>Best PDS fit model: "pl" or "bpl" (2)</description><ucd>stat.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>logN</name><description>[0.9/5.3] Log of Power Density Spectrum (PDS) normalization (2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logN</name><description>[0.1/1.5] Lower 90% confidence level on logN</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_logN</name><description>[0.1/7.8] Upper 90% confidence level on logN</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logfb</name><description>[-0.8/1.5]? Log of PDS frequency break parameter f_b_ (2)</description><unit>log(Hz)</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logfb</name><description>[0.09/5]? Lower 90% confidence level on logfb</description><unit>log(Hz)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_logfb</name><description>[0.08/0.9]? Upper 90% confidence level on logfb</description><unit>log(Hz)</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>alpha</name><description>[0.8/6.8] PDS slope {alpha} (2)</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_alpha</name><description>[0.1/3] Lower 90% confidence level on alpha</description><ucd>stat.error;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_alpha</name><description>[0.1/7] Upper 90% confidence level on alpha</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B</name><description>[1.5/2.5] White (poissoinian) noise level parameter</description><ucd>instr.det.noise</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_B</name><description>[0.05/1.3] Lower 90% confidence level on B</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_B</name><description>[0.05/1] Upper 90% confidence level on B</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pTR</name><description>[0.01/1] Significance associated to T_R_ statistic</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pAD</name><description>[0.1/1] Significance of the Anderson-Darling test</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pKS</name><description>[0.1/1] Significance of the Kolmogorov-Smirnov test</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ratio</name><description>[0.006/0.6] Ratio of Pulse amplitude A_2{sigma}_/A_peak_</description><ucd>src.var.pulse</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>T90</name><description>[0.1/2.7] Burst duration</description><unit>s</unit><ucd>time.duration</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>t0</name><description>[-3/0.03] Start time t_0_</description><unit>s</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>t1</name><description>[0.1/3] Stop time t_1_</description><unit>s</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>f_HR</name><description>[h] ODS extraction &gt; T_5{sigma}_ (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>HR</name><description>[0.6/10.8] Hardness ratio (4)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_HR</name><description>[0.07/1.1] The 1{sigma} confidence level in HR</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pSh</name><description>[0.006/1] Probability of belonging to short class of GRB</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BATSE</name><description>Display sources within 60" from BATSE 4B (IX/20)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>GCat</name><description>Display the data from Fermi/GBM (4yr) (J/ApJS/211/13) and Swift/BAT (BAT2, J/ApJS/195/2) for this GRB identifier</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>NED</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>