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<ri:Resource created="2026-02-23T10:29:01Z" status="active" updated="2026-07-02T12:00:59Z" version="1.2" 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/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>SN 2022joj optical and UV photometry follow-up</title><shortName>J/ApJ/958/178</shortName><identifier>ivo://CDS.VizieR/J/ApJ/958/178</identifier><altIdentifier>doi:10.26093/cds/vizier/ba-xy-5j</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Liu C.</name></creator><creator><name>Miller A.A.</name></creator><creator><name>Boos S.J.</name></creator><creator><name>Shen K.J.</name></creator><creator><name>Townsley D.M.</name></creator><creator><name>Schulze S.,Harvey L.</name></creator><creator><name>Maguire K.</name></creator><creator><name>Johansson J.</name></creator><creator><name>Brink T.G.</name></creator><creator><name>Burgaz U.,Dimitriadis G.</name></creator><creator><name>Filippenko A.V.</name></creator><creator><name>Hall S.</name></creator><creator><name>Hinds K.-R.</name></creator><creator><name>Hoffman A.,Karambelkar V.</name></creator><creator><name>Kilpatrick C.D.</name></creator><creator><name>Perley D.</name></creator><creator><name>Pichay N.</name></creator><creator><name>Sears H.,Sollerman J.</name></creator><creator><name>Stein R.</name></creator><creator><name>Terwel J.H.</name></creator><creator><name>Zheng W.</name></creator><creator><name>Graham M.J.</name></creator><creator><name>Kasliwal M.M.,Lacroix L.</name></creator><creator><name>Purdum J.</name></creator><creator><name>Rusholme B.</name></creator><creator><name>Wold A.</name></creator><date role="Updated">2026-07-02T12:00:59Z</date><date role="Created">2026-02-23T10:29:01Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>ultraviolet-astronomy</subject><description>We present observations of SN 2022joj, a peculiar Type Ia supernova discovered by the Zwicky Transient Facility. SN 2022joj exhibits an unusually red gZTF-rZTF color at early times and a rapid blueward evolution afterward. Around maximum brightness, SN 2022joj shows a high luminosity (M_gZTF,max_~-19.7mag), a blue broadband color (gZTF-rZTF~-0.2mag), and shallow SiII absorption lines, consistent with those of overluminous, SN 1991T-like events. The maximum-light spectrum also shows prominent absorption around 4200{AA}, which resembles the TiII features in subluminous, SN 1991bg-like events. Despite the blue optical-band colors, SN 2022joj exhibits extremely red ultraviolet minus optical colors at maximum luminosity (u-v~0.6mag and uvw1-v~2.5mag), suggesting a suppression of flux at ~2500-4000{AA}. Strong CII lines are also detected at peak. We show that these unusual spectroscopic properties are broadly consistent with the helium-shell double detonation of a sub-Chandrasekhar mass (M~1M_{sun}_) carbon/oxygen white dwarf from a relatively massive helium shell (Ms~0.04-0.1M_{sun}_), if observed along a line of sight roughly opposite to where the shell initially detonates. None of the existing models could quantitatively explain all the peculiarities observed in SN 2022joj. The low flux ratio of [NiII]{lambda}7378 to [FeII]{lambda}7155 emission in the late-time nebular spectra indicates a low yield of stable Ni isotopes, favoring a sub-Chandrasekhar mass progenitor. The significant blueshift measured in the [FeII]{lambda}7155 line is also consistent with an asymmetric chemical distribution in the ejecta, as is predicted in double-detonation models.</description><source format="bibcode">2023ApJ...958..178L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/958/178</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>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/MNRAS/425/1789">J/MNRAS/425/1789 : Berkeley supernova Ia program. I. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MJD</name><description>[59707.2/59804.2] Observation date (JD-2400000.5)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Filter</name><description>Filter (1)</description><ucd>meta.id;instr.filter</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>omag</name><description>[15.8/21] Observed magnitude in Filter (2)</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_omag</name><description>[0.005/0.9] Uncertainty in omag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>n_omag</name><description>Magnitude System, AB or Vega</description><ucd>meta.note;phot.mag</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Tel</name><description>Telescope used (3)</description><ucd>meta.id;instr.tel</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column></table></schema></tableset></ri:Resource>