Detected FRBivo://astron.nl/arts_dr1/q/det_coneASTRONJoeri van LeeuwenEric KooistraLeon OostrumLiam ConnorJ. E. HargreavesYogesh MaanInés Pastor-MarazuelaEmily PetroffD. van der SchuurAlessio ScloccoSamayra M. StraalDany VohlStefan J. WijnholdsE. A. K. AdamsB. AdebahrJ. AttemaC. G. BassaJ. E. BastAnna BilousO. M. BoersmaA. H. W. M. CoolenH. DénesS. DamstraJ. P. R. de ReijerD. W. GardenierY. G. GrangeA. W. GunstK. M. HessH. A. HoltiesB. HutA. KutkinG. Marcel LooseD. M. LuceroÁ. MikaK. MikhailovR. MorgantiV. A. MossH. MulderM. J. NordenT. A. OosterlooEmaneula OrrúZ. ParagiA. P. SchoenmakersK. J. C StuurwoldS. ter VeenW. A. van CappellenJ. M. van der HulstG. N. J. van DiepenY. Y. WangA. W. Zantingand J. Ziemke2024-07-31T11:50:09Michael Sipior

Oude Hoogeveensedijk 4, 7991PD Dwingeloo, the Netherlands

vo@astron.nlsky-surveysfast-radio-bursts This is the first release of data from the Apertif Radio Transient System (ARTS), a supercomputing radio-telescope instrument that performs real-time FRB detection and localisation on the Westerbork Synthesis Radio Telescope (WSRT) interferometer. It reaches coherent-addition sensitivity over the entire field of the view of the primary- dish beam. After commissioning results verified the system performed as planned, we initiated the Apertif FRB survey (ALERT). Over the first 5 weeks we observed at design sensitivity in 2019, we detected 5 new FRBs, and interferometrically localised each of these to 0.4−10 sq. arcmin. All detections are broad band and very narrow, of order 1 ms duration, and unscattered. Dispersion measures are generally high. Please note that the ARTS DR1 collection available from this end-point is superseded by the ARTS DR2 collection. DR2 includes all data from the DR1 collection that can be queried here. The ARTS DR2 FRB detection cone search can be reached at https://vo.astron.nl/arts_dr2/q/det_cone/form.2023A&A...672A.117Vhttps://vo.astron.nl/arts_dr1/q/det_cone/infoSurveyResearchserved-byThe VO @ ASTRON TAP serviceLicensed under CC-BYhttps://vo.astron.nl/arts_dr1/q/det_cone/scs.xml?GETapplication/x-votable+xmlRARight Ascension (ICRS decimal)degpos.eq.rarealDECDeclination (ICRS decimal)degpos.eq.decrealSRSearch radiusdegrealtargetName of the target. Matches also partial input (e.g. T1403+5324 or 1403+5324).chartime_mindtime.start;obs.exposurecharcompound_beamintegertied_array_beamintegerRESPONSEFORMATFile format requested for output.meta.code.mimecharMAXRECMaximum number of records returned. Pass 0 to retrieve service parameters.integerVERBExhaustiveness of column selection. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns.integer180100000true239.89549.01670.001https://vo.astron.nl/arts_dr1/q/det_cone/availabilityhttps://vo.astron.nl/arts_dr1/q/det_cone/capabilitieshttps://vo.astron.nl/arts_dr1/q/det_cone/tableMetadatahttps://vo.astron.nl/tapWSRTARTSRadioarts_dr1 This is the first release (DR1) of data from the Apertif Radio Transient System (ARTS), a supercomputing radio-telescope instrument that performs real-time FRB detection and localisation on the Westerbork Synthesis Radio Telescope (WSRT) interferometer. It reaches coherent-addition sensitivity over the entire field of the view of the primary- dish beam. After commissioning results verified the system performed as planned, we initiated the Apertif FRB survey (ALERT). Over the first 5 weeks we observed at design sensitivity in 2019, we detected 5 new FRBs, and interferometrically localised each of these to 0.4−10 sq. arcmin. All detections are broad band and very narrow, of order 1 ms duration, and unscattered. Dispersion measures are generally high. Please note that the ARTS DR1 collection available from this end-point is superseded by the ARTS DR2 collection. DR2 includes all data from the DR1 collection that can be queried here.arts_dr1.frb_det This is the first release (DR1) of data from the Apertif Radio Transient System (ARTS), a supercomputing radio-telescope instrument that performs real-time FRB detection and localisation on the Westerbork Synthesis Radio Telescope (WSRT) interferometer. It reaches coherent-addition sensitivity over the entire field of the view of the primary- dish beam. After commissioning results verified the system performed as planned, we initiated the Apertif FRB survey (ALERT). Over the first 5 weeks we observed at design sensitivity in 2019, we detected 5 new FRBs, and interferometrically localised each of these to 0.4−10 sq. arcmin. All detections are broad band and very narrow, of order 1 ms duration, and unscattered. Dispersion measures are generally high. Please note that the ARTS DR1 collection available from this end-point is superseded by the ARTS DR2 collection. DR2 includes all data from the DR1 collection that can be queried here.targetName of the observed targetcharnullableradegpos.eq.ra;meta.mainfloatindexednullabledecdegpos.eq.dec;meta.mainfloatindexednullabletime_mindtime.start;obs.exposuredoublenullabletime_maxdtime.end;obs.exposuredoublenullabledetection1 if an FRB was detected, 0 for a non-detection.intfrbName of the FRB if detected, linking to the FRB properties. None if non-detection.charnullableobs_titlemeta.id;meta.maincharnullableobsidID of the data setcharnullablecompound_beaminttied_array_beamintt_exptimestime.duration;obs.exposurefloatnullabletime_stepsintfilesizekbytephys.size;meta.fileintaccrefmeta.ref.urlAccess.Referencecharnullablefile_referencecharnullablemimetypemeta.code.mimecharnullablepub_didcharnullable