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<ri:Resource created="2022-07-26T11:11:03Z" 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>The local universe with ZTF. I. Ca-rich gap transients</title><shortName>J/ApJ/905/58</shortName><identifier>ivo://CDS.VizieR/J/ApJ/905/58</identifier><altIdentifier>doi:10.26093/cds/vizier.19050058</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>De K.</name></creator><creator><name>Kasliwal M.M.</name></creator><creator><name>Tzanidakis A.</name></creator><creator><name>Fremling U.C.</name></creator><creator><name>Adams S.</name></creator><creator><name>Aloisi R.,Andreoni I.</name></creator><creator><name>Bagdasaryan A.</name></creator><creator><name>Bellm E.C.</name></creator><creator><name>Bildsten L.</name></creator><creator><name>Cannella C.,Cook D.O.</name></creator><creator><name>Delacroix A.</name></creator><creator><name>Drake A.</name></creator><creator><name>Duev D.</name></creator><creator><name>Dugas A.</name></creator><creator><name>Frederick S.,Gal-Yam A.</name></creator><creator><name>Goldstein D.</name></creator><creator><name>Golkhou V.Z.</name></creator><creator><name>Graham M.J.</name></creator><creator><name>Hale D.</name></creator><creator><name>Hankins M.,Helou G.</name></creator><creator><name>Ho A.Y.Q.</name></creator><creator><name>Irani I.</name></creator><creator><name>Jencson J.E.</name></creator><creator><name>Kaplan D.L.</name></creator><creator><name>Kaye S.,Kulkarni S.R.</name></creator><creator><name>Kupfer T.</name></creator><creator><name>Laher R.R.</name></creator><creator><name>Leadbeater R.</name></creator><creator><name>Lunnan R.</name></creator><creator><name>Masci F.J.,Miller A.A.</name></creator><creator><name>Neill J.D.</name></creator><creator><name>Ofek E.O.</name></creator><creator><name>Perley D.A.</name></creator><creator><name>Polin A.</name></creator><creator><name>Prince T.A.,Quataert E.</name></creator><creator><name>Reiley D.</name></creator><creator><name>Riddle R.L.</name></creator><creator><name>Rusholme B.</name></creator><creator><name>Sharma Y.</name></creator><creator><name>Shupe D.L.,Sollerman J.</name></creator><creator><name>Tartaglia L.</name></creator><creator><name>Walters R.</name></creator><creator><name>Yan L.</name></creator><creator><name>Yao Y.</name></creator><date role="Updated">2022-09-05T14:14:07Z</date><date role="Created">2022-07-26T11:11:03Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>spectroscopy</subject><subject>redshifted</subject><subject>absolute-magnitude</subject><subject>surveys</subject><description>Using the Zwicky Transient Facility alert stream, we are conducting a large spectroscopic campaign to construct a complete, volume-limited sample of transients brighter than 20mag, and coincident within 100" of galaxies in the Census of the Local Universe catalog. We describe the experiment design and spectroscopic completeness from the first 16 months of operations, which have classified 754 supernovae. We present results from a systematic search for calcium-rich gap transients in the sample of 22 low-luminosity (peak absolute magnitude M{&gt;}-17), hydrogen-poor events found in the experiment. We report the detection of eight new events, and constrain their volumetric rate to &gt;~15%+/-5% of the SN Ia rate. Combining this sample with 10 previously known events, we find a likely continuum of spectroscopic properties ranging from events with SN Ia-like features (Ca-Ia objects) to those with SN Ib/c-like features (Ca-Ib/c objects) at peak light. Within the Ca-Ib/c events, we find two populations distinguished by their red (g-r~1.5mag) or green (g-r~0.5mag) colors at the r-band peak, wherein redder events show strong line blanketing features and slower light curves (similar to Ca-Ia objects), weaker He lines, and lower [CaII]/[OI] in the nebular phase. We find that all together the spectroscopic continuum, volumetric rates, and striking old environments are consistent with the explosive burning of He shells on low-mass white dwarfs. We suggest that Ca-Ia and red Ca-Ib/c objects arise from the double detonation of He shells, while green Ca-Ib/c objects are consistent with low-efficiency burning scenarios like detonations in low-density shells or deflagrations.</description><source format="bibcode">2020ApJ...905...58D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/905/58</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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/195">VII/195 : Globular Clusters in the Milky Way (Harris, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/202">VII/202 : Globular Clusters in the Milky Way (Harris, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/281">VII/281 : GLADE v2.3 catalog (Dalya+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/560/566">J/ApJ/560/566 : K-band galaxy LF from 2MASS (Kochanek+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/696/870">J/ApJ/696/870 : Catalina Real-time Transient Survey (CRTS) (Drake+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/707/1449">J/ApJ/707/1449 : Local hosts of SNe Ia (Neill+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/741/97">J/ApJ/741/97 : Light curves of Ibc supernovae (Drout+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/412/1441">J/MNRAS/412/1441 : SNe luminosity functions (Li+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/425/1789">J/MNRAS/425/1789 : Berkeley supernova Ia program. 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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>Name</name><description>SN name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>n_Name</name><description>SN name (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Phase</name><description>[-8/265] Time since maximum</description><unit>d</unit><ucd>time.phase</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>V1</name><description>[3620/15010]? The HeI 5876{AA} velocity</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>W1</name><description>[5800/5876]? Wavelength of the measured V1 line</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>V2</name><description>[2470/11120]? The HeI 7065{AA}/SiII 6355{AA} velocity</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_V2</name><description>[20/760]? Uncertainty in V2</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>CLU</name><description>Display the properties for this SN presented in this paper (link to Table 1)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Fit</name><description>Display the spectral and LC fit parameters for this SN (link to Tables 4 and 5)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/905/58/table5</name><description>Light curve fit parameters for the Ca-rich gap transients presented in this paper, together with the fits for the literature sample of Ca-rich gap transients</description><column><name>Name</name><description>SN name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>tf0.5</name><description>[5/15.3]? Fall time from peak to half peak flux</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_tf0.5</name><description>[0.3/3.2]? Uncertainty in tf0.5</description><unit>d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Delm7</name><description>[0.09/0.8]? Magnitude drop after 7 days post peak</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Delm7</name><description>[0.02/0.5]? Uncertainty in Delm7</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ref</name><description>Reference (G2)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">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>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>Filt</name><description>[BVRIGgrizg'r' ] Filter used</description><ucd>instr.setup;instr.filter</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>tpk</name><description>[53387.15/58747.78] Modified Julian Date of peak time in Filt</description><unit>d</unit><ucd>time.epoch;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_tpk</name><description>[0.2/3.2]? Uncertainty in tpk</description><unit>d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>magpk</name><description>[16.2/20.3] Peak apparent magnitude in Filt (1)</description><unit>mag</unit><ucd>phot.mag;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_magpk</name><description>[0.01/0.3] Uncertainty in magpk</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>MAGpk</name><description>[-17.1/-13.42] Peak absolute magnitude in Filt</description><unit>mag</unit><ucd>phys.magAbs;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>tr0.5</name><description>[5.8/8.81]? Rise time to peak from half peak flux</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_tr0.5</name><description>[0.2/1.8]? Uncertainty in tr0.5</description><unit>d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>CLU</name><description>Display the properties for this SN presented in this paper (link to Table 1)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Fit</name><description>Display the spectral and LC fit parameters for this SN (link to Tables 4 and 5)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/905/58/fig5</name><description>Spectroscopic sequence of the Ca-rich gap transients presented in this paper</description><column><name>Date</name><description>Observation date</description><ucd>time.epoch;obs</ucd><flag>nullable</flag><flag>indexed</flag></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>ZTF</name><description>ZTF identifier (see the corresponding SN name in Table 1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Tel</name><description>Facility identifier (G1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>lambda</name><description>[3056.1/10309.4] Wavelength; Angstroms</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>[-0.045/1.8]? Flux density (1)</description><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/905/58/fig29</name><description>Photospheric and nebular phase spectrum of objects in the control that did not pass either the early nebular-phase transition criterion or the nebular-phase [CaII]/[OI] threshold</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>ZTF</name><description>ZTF identifier (see the corresponding SN name in Table 1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Date</name><description>Observation date</description><ucd>time.epoch;obs</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>Tel</name><description>Facility identifier (G1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>lambda</name><description>[3056/10499.8] Wavelength; Angstroms</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>[-1.3e-15/1.7e-14]? Flux density; in erg/s/cm^2^/{AA} units</description><unit>cW.m**-2.nm**-1</unit><ucd>meta.unit;phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>