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<ri:Resource created="2020-08-27T08:51:38Z" status="active" updated="2025-05-19T09:50:00Z" 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>Follow-up obs. of the type IIn SN KISS15s</title><shortName>J/ApJ/872/135</shortName><identifier>ivo://CDS.VizieR/J/ApJ/872/135</identifier><altIdentifier>doi:10.26093/cds/vizier.18720135</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kokubo M.</name></creator><creator><name>Mitsuda K.</name></creator><creator><name>Morokuma T.</name></creator><creator><name>Tominaga N.</name></creator><creator><name>Tanaka M.</name></creator><creator><name>Moriya T.J.,Yoachim P.</name></creator><creator><name>Ivezic Z.</name></creator><creator><name>Sako S.</name></creator><creator><name>Doi M.</name></creator><date role="Updated">2020-11-26T11:35:57Z</date><date role="Created">2020-08-27T08:51:38Z</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>supernovae</subject><description>We report the discovery of an SN 1988Z-like type IIn supernova KISS15s found in a low-mass star-forming galaxy at redshift z=0.038 during the course of the Kiso Supernova Survey (KISS). KISS15s shows long-duration optical continuum and emission line light curves, indicating that KISS15s is powered by a continuous interaction between the expanding ejecta and dense circumstellar medium (CSM). The H{alpha} emission line profile can be decomposed into four Gaussians of narrow, intermediate, blueshifted intermediate, and broad velocity width components, with a full width at half maximum of &lt;~100, ~2000, and ~14000km/s for the narrow, intermediate, and broad components, respectively. The presence of the blueshifted intermediate component, of which the line-of-sight velocity relative to the systemic velocity is about -5000km/s, suggests that the ejecta-CSM interaction region has an inhomogeneous morphology and anisotropic expansion velocity. We found that KISS15s shows increasing infrared continuum emission, which can be interpreted as hot dust thermal emission of T~1200K from newly formed dust in a cool, dense shell in the ejecta-CSM interaction region. The progenitor mass-loss rate, inferred from bolometric luminosity, is dM/dt~0.4M_{sun}_/yr ({nu}_w_/40km/s), where {nu}_w_ is the progenitor's stellar wind velocity. This implies that the progenitor of KISS15s was a red supergiant star or a luminous blue variable that had experienced a large mass loss in the centuries before the explosion.</description><source format="bibcode">2019ApJ...872..135K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/872/135</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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/358">II/358 : SkyMapper Southern Sky Survey. 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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>Inst</name><description>Telescope/Instrument description</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType></column><column><name>Date</name><description>Observation date</description><ucd>time.epoch;obs</ucd><flag>nullable</flag></column><column><name>lambda</name><description>[3802.3/10359.6] Wavelength in the observed-frame; in Angstrom units</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>[-77.2/62] Flux in 10^-17^erg/cm^2^/s/{AA} units; corrected for Galactic extinction</description><unit>1e-17cW.m**-2.nm**-1</unit><ucd>meta.unit;phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Flux</name><description>[0.2/3.7] Error in Flux</description><unit>1e-17cW.m**-2.nm**-1</unit><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJ/872/135/photom</name><description>Optical and NIR photometry of KISS15s (Tables 1-7)</description><column><name>e_mag</name><description>[0.01/0.4] Error in mag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Inst</name><description>Instrument designation (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>MJD</name><description>[57234.7/58108.9] Modified Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Obs</name><description>[2015/2017] Year of the observation</description><ucd>time.epoch</ucd></column><column><name>Day2</name><description>? Second day of observation if any</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>mag</name><description>[16.9/22.7] Apparent magnitude in band; uncorrected for Galactic extinction</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Band</name><description>Bandpass of the observation (g, r, i, z, w; W1, W2 or H, J, Ks)</description><ucd>meta.code;instr.filter</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column></table><table><name>J/ApJ/872/135/fig6</name><description>Nayuta/LISS and ARC3.5-m/DIS low-resolution spectra of KISS15s</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Inst</name><description>Telescope/Instrument description</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType></column><column><name>Date</name><description>Observation date</description><ucd>time.epoch;obs</ucd><flag>nullable</flag></column><column><name>lambda</name><description>[3802.3/10359.6] Wavelength in the observed-frame; in Angstrom units</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>[-77.2/62] Flux in 10^-17^erg/cm^2^/s/{AA} units; corrected for Galactic extinction</description><unit>1e-17cW.m**-2.nm**-1</unit><ucd>meta.unit;phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Flux</name><description>[0.2/3.7] Error in Flux</description><unit>1e-17cW.m**-2.nm**-1</unit><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>