J/ApJS/280/34ivo://CDS.VizieR/J/ApJS/280/34CDSGuo X.Wang H.Xiao Y.Chen H.Ke Y.Miao C.Wang P.Li DiJin C.,He L.Feng YiZhang Y.Xu J.Chen G.2026-07-22T07:44:42Z2026-07-22T08:13:08ZCDS support team

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

cds-question@unistra.frradio-sourcestransient-sourcesFast radio bursts (FRBs) are an extremely energetic cosmic phenomenon of short duration. Discovered only recently and with its origin still unknown, FRBs have already started to play a significant role in studying the distribution and evolution of matter in the Universe. FRBs can only be observed through radio telescopes, which produce petabytes of data, rendering the search for FRBs a challenging task. Traditional techniques are computationally expensive, time-consuming, and generally biased against weak signals. Various machine learning algorithms have been developed and employed, all of which require substantial data sets. Here, we introduce the FAST data set for FRBs EXploration, built upon the observations obtained by the Five-hundred-meter Aperture Spherical radio Telescope. Our data set comprises 600 positive samples of observed FRB signals from three sources and 1000 negative samples of noise and radio frequency interference. Furthermore, we provide a machine learning algorithm, Radio Single-Pulse Detection Algorithm Based on Visual Morphological Features (RaSPDAM), with significant improvements in efficiency and accuracy for FRB searches. We also employed the benchmark comparison between conventional single-pulse search software, namely, PRESTO and Heimdall, and RaSPDAM. RaSPDAMv2 achieves an average precision of 97% and an average recall of 83%, with notable enhancements in computational performance. Future machine learning algorithms can use this as a reference point to measure their performance and identify potential improvements. By enabling more accurate and efficient detection of transient radio events, our work facilitates the FRB and pulsars search pipeline, enhances the potential for discovering new astrophysical phenomena.2025ApJS..280...34Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/280/34CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/other/PASA/33.45 : FRBCAT: The Fast Radio Burst (FRB) Cat. (Petroff+, 2016)J/A+A/626/A104 : LOTAAS pulsar discoveries (Sanidas+, 2019)J/ApJS/257/59 : First CHIME FRB Cat. (CHIME/FRB Col.+, 2021)J/other/Nat/598.267 : List of radio bursts (Li+, 2021)J/MNRAS/509/1227 : Hidden repeating fast radio bursts (Chen+, 2022)J/MNRAS/511/1961 : New CHIME/FRB I cat. updates released (Hashimoto+, 2022)J/A+A/675/A99 : FRBs search with Fermi-LAT (Principe+, 2023)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/280/34https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/280/34http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/280/34https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/280/34https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/280/34http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/280/34GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapRadiodefaultJ/ApJS/280/34/table4Parameters of 600 positive samples in datasetrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintFileBurst file name (1)meta.id;meta.filecharSourceSource identifier (FRB20121102, FRB20180301 or FRB20201124)meta.id;meta.maincharMJD[58724.87/59485.83] Modified Julian Datedtime.epochdoubleDM[411.5/570] Dispersion Measurepc.cm**-3phys.dispMeasurefloatToA[0.0097/4.97] Time of Arrivalstime.epochfloatFWHM[0.34/78.52] Full Width at Half Maximummsspect.line.widthfloatBandwidth[16/500] BandwidthMHzinstr.bandwidthintFlux[0.0016/0.85] Peak flux densityJyphot.flux.density;em.radio.750-1500MHzdoubleFluence[0.0016/4.57] FluenceJy.msphot.fluencefloatFileIDFile ID at DOI:10.57760/sciencedb.15070; column added by CDSmeta.id;meta.filechar