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<ri:Resource created="2024-04-26T14:47:22Z" 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 compilation of optical spectra from 361 SNe Ia</title><shortName>J/ApJ/930/70</shortName><identifier>ivo://CDS.VizieR/J/ApJ/930/70</identifier><altIdentifier>doi:10.26093/cds/vizier.19300070</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hu L.</name></creator><creator><name>Chen X.</name></creator><creator><name>Wang L.</name></creator><date role="Updated">2024-11-06T20:25:31Z</date><date role="Created">2024-04-26T14:47:22Z</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>visible-astronomy</subject><subject>spectroscopy</subject><subject>astronomical-reference-materials</subject><description>We present a data-driven method based on long short-term memory (LSTM) neural networks to analyze spectral time series of Type Ia supernovae (SNeIa). The data set includes 3091 spectra from 361 individual SNeIa. The method allows for accurate reconstruction of the spectral sequence of an SN Ia based on a single observed spectrum around maximum light. The precision of the spectral reconstruction increases with more spectral time coverages, but the significant benefit of multiple epoch data at around optical maximum is only evident for observations separated by more than a week. The method shows great power in extracting the spectral information of SNe Ia and suggests that the most critical information of an SN Ia can be derived from a single spectrum around the optical maximum. The algorithm we have developed is important for the planning of spectroscopic follow-up observations of future SN surveys with the LSST/Rubin and WFIRST/Roman telescopes.</description><source format="bibcode">2022ApJ...930...70H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/930/70</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/B/sn">B/sn : Asiago Supernova Catalogue (Barbon et al., 1999-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/1648">J/AJ/131/1648 : Type Ia SNe at high and low redshifts (Blondin+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/527">J/AJ/131/527 : UBVRI light curves of 44 type Ia supernovae (Jha+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/659/122">J/ApJ/659/122 : Improved distances to type Ia supernovae (Jha+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/686/749">J/ApJ/686/749 : Improved cosmological constraints from SNe (Kowalski+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/500/L17">J/A+A/500/L17 : Spectral flux ratio of SN Ia (Bailey+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/700/331">J/ApJ/700/331 : Light curves of type Ia supernovae (CfA3) (Hicken+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/183/109">J/ApJS/183/109 : Cepheids in 3 host galaxies (Riess+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/699/L139">J/ApJ/699/L139 : Spectral parameters of SNe Ia (Wang+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/716/712">J/ApJ/716/712 : HST light curves of six SNe and Union2 (Amanullah+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/406/782">J/MNRAS/406/782 : Type Ia supernovae luminosities (Sullivan+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/529/L4">J/A+A/529/L4 : Reddening law of type Ia supernovae (Chotard+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/156">J/AJ/142/156 : The CSP (DR2): photometry of SNe Ia (Stritzinger+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/143/126">J/AJ/143/126 : Spectroscopy of nearby Type Ia supernovae (Blondin+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/200/12">J/ApJS/200/12 : CfA4: light curves for 94 type Ia SNe (Hicken+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/425/1789">J/MNRAS/425/1789 : Berkeley supernova Ia program. 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