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<ri:Resource created="2021-04-30T08:58:31Z" 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>Most luminous SPIRITS IR transients follow-up obs.</title><shortName>J/ApJ/886/40</shortName><identifier>ivo://CDS.VizieR/J/ApJ/886/40</identifier><altIdentifier>doi:10.26093/cds/vizier.18860040</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Jencson J.E.</name></creator><creator><name>Kasliwal M.M.</name></creator><creator><name>Adams S.M.</name></creator><creator><name>Bond H.E.</name></creator><creator><name>De K.</name></creator><creator><name>Johansson J.,Karambelkar V.</name></creator><creator><name>Lau R.M.</name></creator><creator><name>Tinyanont S.</name></creator><creator><name>Ryder S.D.</name></creator><creator><name>Cody A.M.</name></creator><creator><name>Masci F.J.,Bally J.</name></creator><creator><name>Blagorodnova N.</name></creator><creator><name>Castellon S.</name></creator><creator><name>Fremling C.</name></creator><creator><name>Gehrz R.D.</name></creator><creator><name>Helou G.,Kilpatrick C.D.</name></creator><creator><name>Milne P.A.</name></creator><creator><name>Morrell N.</name></creator><creator><name>Perley D.A.</name></creator><creator><name>Phillips M.M.,Smith N.</name></creator><creator><name>van Dyk S.D.</name></creator><creator><name>Williams R.E.</name></creator><date role="Updated">2021-07-05T11:40:07Z</date><date role="Created">2021-04-30T08:58:31Z</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-sources</subject><subject>supernovae</subject><subject>surveys</subject><subject>extinction</subject><subject>infrared-photometry</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><subject>visible-astronomy</subject><description>We present a systematic study of the most luminous (MIR [Vega magnitudes] brighter than -14) infrared (IR) transients discovered by the SPitzer InfraRed Intensive Transients Survey (SPIRITS) between 2014 and 2018 in nearby galaxies (D&lt;35Mpc). The sample consists of nine events that span peak IR luminosities of M_[4.5],peak_ between -14 and -18.2, show IR colors between 0.2&lt;([3.6]-[4.5])&lt;3.0, and fade on timescales between 55d&lt;t_fade_&lt;480d. The two reddest events (A_V_&gt;12) show multiple, luminous IR outbursts over several years and have directly detected, massive progenitors in archival imaging. With analyses of extensive, multiwavelength follow-up, we suggest the following possible classifications: five obscured core-collapse supernovae (CCSNe), two erupting massive stars, one luminous red nova, and one intermediate-luminosity red transient. We define a control sample of all optically discovered transients recovered in SPIRITS galaxies and satisfying the same selection criteria. The control sample consists of eight CCSNe and one Type Iax SN. We find that 7 of the 13 CCSNe in the SPIRITS sample have lower bounds on their extinction of 2&lt;A_V_&lt;8. We estimate a nominal fraction of CCSNe in nearby galaxies that are missed by optical surveys as high as 38.5_-21.9_^+26.0^% (90% confidence). This study suggests that a significant fraction of CCSNe may be heavily obscured by dust and therefore undercounted in the census of nearby CCSNe from optical searches.</description><source format="bibcode">2019ApJ...886...40J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/886/40</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/ApJ/469/355">J/ApJ/469/355 : Teff, B-V and BC relation (Flower, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/1607">J/AJ/126/1607 : IRAS Revised Bright Galaxy Sample (Sanders+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/465/71">J/A+A/465/71 : 21cm observations of 452 galaxies (Theureau+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/705/1364">J/ApJ/705/1364 : MIR catalog of point sources in M33 (Thompson+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/408/181">J/MNRAS/408/181 : CN2002ch UBVRI and ugriz light curves (Pastorello+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/122/1397">J/PASP/122/1397 : Spitzer Survey of Stellar Structure in Gal. 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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>SPIRITS</name><description>SPIRITS name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>Date</name><description>Date of observation (UT)</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>MJD</name><description>[57095.1/58242.4] Modified Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Range</name><description>Wavelength range in {AA}</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>Exp</name><description>Integration time</description><unit>s</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column></table><table><name>J/ApJ/886/40/fig3</name><description>Optical spectra of SPIRITS transients</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>SPIRITS</name><description>SPIRITS name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>Tel/inst</name><description>Telescope and Instrument</description><ucd>instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Date</name><description>UT date or lower range of date of observation</description><ucd>time.epoch</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>lambda</name><description>Wavelength (observer frame) in {AA}</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flam</name><description>? Flux density (observer frame) in erg/s/cm^2^/{AA}</description><unit>cW.m**-2.nm**-1</unit><ucd>phot.flux.density</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/886/40/fig4</name><description>Near-infrared spectra of SPIRITS transients</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>SPIRITS</name><description>SPIRITS name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>Tel/inst</name><description>Telescope and Instrument</description><ucd>instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Date</name><description>UT date or lower range of date of observation</description><ucd>time.epoch</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>Date2</name><description>Upper range of UT date of observation (only for fig4)</description><ucd>time.epoch;stat.max</ucd><flag>nullable</flag></column><column><name>lambda</name><description>Wavelength (observer frame) in {AA}</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flam</name><description>? Flux density (observer frame) in erg/s/cm^2^/{AA}</description><unit>cW.m**-2.nm**-1</unit><ucd>phot.flux.density</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>