<?xml version='1.0'?><?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?><ri:Resource created="2021-03-03T13:38:11Z" status="active" updated="2024-07-31T11:50:09" 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/RegistryInterface/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/RegistryInterface-v1.0.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource-v1.1.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService-v1.1.xsd" xsi:type="vs:DataService"><title>PSRFITS access link</title><shortName>PSRfitsaccess</shortName><identifier>ivo://astron.nl/arts_dr1/q/psrfitsaccess</identifier><curation><publisher>ASTRON</publisher><creator><name>Joeri van Leeuwen</name></creator><creator><name>Eric Kooistra</name></creator><creator><name>Leon Oostrum</name></creator><creator><name>Liam Connor</name></creator><creator><name>J. E. Hargreaves</name></creator><creator><name>Yogesh Maan</name></creator><creator><name>Inés Pastor-Marazuela</name></creator><creator><name>Emily Petroff</name></creator><creator><name>D. van der Schuur</name></creator><creator><name>Alessio Sclocco</name></creator><creator><name>Samayra M. Straal</name></creator><creator><name>Dany Vohl</name></creator><creator><name>Stefan J. Wijnholds</name></creator><creator><name>E. A. K. Adams</name></creator><creator><name>B. Adebahr</name></creator><creator><name>J. Attema</name></creator><creator><name>C. G. Bassa</name></creator><creator><name>J. E. Bast</name></creator><creator><name>Anna Bilous</name></creator><creator><name>O. M. Boersma</name></creator><creator><name>A. H. W. M. Coolen</name></creator><creator><name>H. Dénes</name></creator><creator><name>S. Damstra</name></creator><creator><name>J. P. R. de Reijer</name></creator><creator><name>D. W. Gardenier</name></creator><creator><name>Y. G. Grange</name></creator><creator><name>A. W. Gunst</name></creator><creator><name>K. M. Hess</name></creator><creator><name>H. A. Holties</name></creator><creator><name>B. Hut</name></creator><creator><name>A. Kutkin</name></creator><creator><name>G. Marcel Loose</name></creator><creator><name>D. M. Lucero</name></creator><creator><name>Á. Mika</name></creator><creator><name>K. Mikhailov</name></creator><creator><name>R. Morganti</name></creator><creator><name>V. A. Moss</name></creator><creator><name>H. Mulder</name></creator><creator><name>M. J. Norden</name></creator><creator><name>T. A. Oosterloo</name></creator><creator><name>Emaneula Orrú</name></creator><creator><name>Z. Paragi</name></creator><creator><name>A. P. Schoenmakers</name></creator><creator><name>K. J. C Stuurwold</name></creator><creator><name>S. ter Veen</name></creator><creator><name>W. A. van Cappellen</name></creator><creator><name>J. M. van der Hulst</name></creator><creator><name>G. N. J. van Diepen</name></creator><creator><name>Y. Y. Wang</name></creator><creator><name>A. W. Zanting</name></creator><creator><name>and J. Ziemke</name></creator><date role="updated">2024-07-31T11:50:09</date><contact><name>Michael Sipior</name><address>Oude Hoogeveensedijk 4, 7991PD Dwingeloo, the Netherlands</address><email>vo@astron.nl</email></contact></curation><content><subject>sky-surveys</subject><subject>fast-radio-bursts</subject><description> 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.</description><source format="bibcode">2023A&amp;A...672A.117V</source><referenceURL>https://vo.astron.nl/arts_dr1/q/psrfitsaccess/info</referenceURL><type>Survey</type><contentLevel>Research</contentLevel></content><rights rightsURI="http://creativecommons.org/licenses/by/3.0/">Licensed under CC-BY</rights></ri:Resource>