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<ri:Resource created="2023-10-27T13:22:14Z" 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>Automated DASH classification for supernovae</title><shortName>J/ApJ/885/85</shortName><identifier>ivo://CDS.VizieR/J/ApJ/885/85</identifier><altIdentifier>doi:10.26093/cds/vizier.18850085</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Muthukrishna D.</name></creator><creator><name>Parkinson D.</name></creator><creator><name>Tucker B.E.</name></creator><date role="Updated">2023-12-14T01:23:35Z</date><date role="Created">2023-10-27T13:22:14Z</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>supernovae</subject><subject>redshifted</subject><subject>spectroscopy</subject><subject>visible-astronomy</subject><description>We present DASH (Deep Automated Supernova and Host classifier), a novel software package that automates the classification of the type, age, redshift, and host galaxy of supernova spectra. DASH makes use of a new approach that does not rely on iterative template-matching techniques like all previous software, but instead classifies based on the learned features of each supernova's type and age. It has achieved this by employing a deep convolutional neural network to train a matching algorithm. This approach has enabled DASH to be orders of magnitude faster than previous tools, being able to accurately classify hundreds or thousands of objects within seconds. We have tested its performance on 4yr of data from the Australian Dark Energy Survey (OzDES). The deep learning models were developed using TensorFlow and were trained using over 4000 supernova spectra taken from the CfA Supernova Program and the Berkeley SN Ia Program as used in SNID (Supernova Identification software). Unlike template-matching methods, the trained models are independent of the number of spectra in the training data, which allows for DASH's unprecedented speed. We have developed both a graphical interface for easy visual classification and analysis of supernovae and a Python library for the autonomous and quick classification of several supernova spectra. The speed, accuracy, user-friendliness, and versatility of DASH present an advancement to existing spectral classification tools. We have made the code publicly available on GitHub and PyPI (pip install astrodash) to allow for further contributions and development. The package documentation is available at http://astrodash.readthedocs.io/</description><source format="bibcode">2019ApJ...885...85M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/885/85</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/J/AJ/135/1598">J/AJ/135/1598 : Optical spectroscopy of type Ia supernovae (Matheson+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/143/126">J/AJ/143/126 : Spectroscopy of 462 nearby Type Ia supernovae (Blondin+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/425/1789">J/MNRAS/425/1789 : Berkeley supernova Ia program. I. (Silverman+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/99">J/AJ/147/99 : Spectroscopy of 73 stripped core-collapse SNe (Modjaz+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/827/90">J/ApJ/827/90 : Spectroscopy of SNe Ib, IIb and Ic (Liu+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/832/108">J/ApJ/832/108 : Spectral properties of Type Ic &amp; Ic-bl SNe (Modjaz+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/230/20">J/ApJS/230/20 : Machine learning technique for CoNFIG gal. (Aniyan+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/472/273">J/MNRAS/472/273 : OzDES DR1 (Childress+, 2017)</relatedResource><relatedResource>http://heracles.astro.berkeley.edu/sndb/info : SNDB home page</relatedResource><relatedResource>http://people.lam.fr/blondin.stephane/software/snid/index.html : SNID access</relatedResource><relatedResource>http://github.com/nyusngroup/SESNtemple/tree/master/SNIDtemplates : Liu &amp;</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/885/85</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/885/85</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/885/85</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/885/85</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/885/85</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/885/85</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/885/85/table2 (*Classification of supernovae released in the past 3yr of ATels by OzDES)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/885/85/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/885/85/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/885/85/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>36.9257389</ra><dec>-4.3149261</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/4422 4436 8868 8983 9026 6/17669 17671 17677 17679-17680 17682-17683 17686 17692 17694 17712 17735 17741 17750-17752 17756-17757 35383 35385 35387-35390 35476 35480 35926-35927 35931 35956-35957 36098 36128</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/885/85?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/885/85/table2</name><description>*Classification of supernovae released in the past 3yr of ATels by OzDES</description><column><name>Name</name><description>Supernova name (DESYYANaaaa)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></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>Cl-ATel</name><description>ATel classification given by OzDES (1)</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType></column><column><name>Cl-DASH</name><description>DASH classification</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>Prob</name><description>[0.34/1] DASH softmax regression probability</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rel</name><description>DASH reliability</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Match?</name><description>Agreement on the type of the SN by ATel and DASH? 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