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<ri:Resource created="2023-11-22T08:22:44Z" status="active" updated="2026-07-02T11:58:21Z" 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>Fast-evolving SNIbn with LCO LCs &amp; FLOYDS sp.</title><shortName>J/ApJ/926/125</shortName><identifier>ivo://CDS.VizieR/J/ApJ/926/125</identifier><altIdentifier>doi:10.26093/cds/vizier/ba-wy-3x</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pellegrino C.</name></creator><creator><name>Howell D.A.</name></creator><creator><name>Vinko J.</name></creator><creator><name>Gangopadhyay A.</name></creator><creator><name>Xiang D.,Arcavi I.</name></creator><creator><name>Brown P.</name></creator><creator><name>Burke J.</name></creator><creator><name>Hiramatsu D.</name></creator><creator><name>Hosseinzadeh G.</name></creator><creator><name>Li Z.,McCully C.</name></creator><creator><name>Misra K.</name></creator><creator><name>Newsome M.</name></creator><creator><name>Gonzalez E.P.</name></creator><creator><name>Pritchard T.A.,Valenti S.</name></creator><creator><name>Wang X.</name></creator><creator><name>Zhang T.</name></creator><date role="Updated">2026-07-02T11:58:21Z</date><date role="Created">2023-11-22T08:22:44Z</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>transient-sources</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>spectroscopy</subject><subject>redshifted</subject><description>Rapidly evolving transients, or objects that rise and fade in brightness on timescales two to three times shorter than those of typical Type Ia or Type II supernovae (SNe), have uncertain progenitor systems and powering mechanisms. Recent studies have noted similarities between rapidly evolving transients and Type Ibn SNe, which are powered by ejecta interacting with He-rich circumstellar material (CSM). In this work we present multiband photometric and spectroscopic observations from Las Cumbres Observatory and Swift of four fast-evolving Type Ibn SNe. We compare these observations with those of rapidly evolving transients identified in the literature. We discuss several common characteristics between these two samples, including their light curve and color evolution as well as their spectral features. To investigate a common powering mechanism we construct a grid of analytical model light curves with luminosity inputs from CSM interaction as well as ^56^Ni radioactive decay. We find that models with ejecta masses of ~1-3M_{sun}_, CSM masses of ~0.2-1M_{sun}_, and CSM radii of ~20-65au can explain the diversity of peak luminosities, rise times, and decline rates observed in Type Ibn SNe and rapidly evolving transients. This suggests that a common progenitor system-the core collapse of a high-mass star within a dense CSM shell-can reproduce the light curves of even the most luminous and fast-evolving objects, such as AT 2018cow. This work is one of the first to reproduce the light curves of both SNe Ibn and other rapidly evolving transients with a single model.</description><source format="bibcode">2022ApJ...926..125P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/926/125</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/II/183">II/183 : UBVRI Photometric Standards (Landolt 1992)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/109/874">J/AJ/109/874 : Kinematics of MKW and AWM Poor Clusters (Beers+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Sci/337.444">J/other/Sci/337.444 : RV curves of Galactic massive O stars (Sana+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/555/A10">J/A+A/555/A10 : Light curves of 5 type IIn supernovae (Taddia+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/213/19">J/ApJS/213/19 : Optical and near-IR light curves of 64 SNe (Bianco+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/794/23">J/ApJ/794/23 : Pan-STARRS1 transients optical photometry (Drout+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/789/104">J/ApJ/789/104 : SNe IIn observations and properties (Ofek+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/574/A60">J/A+A/574/A60 : Light curve templates of SNe Ib/c from SDSS (Taddia+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/819/35">J/ApJ/819/35 : LCs of four transients from PTF &amp; SNLS (Arcavi+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/459/3939">J/MNRAS/459/3939 : Type II supernova light curves (Valenti+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/481/894">J/MNRAS/481/894 : Rapidly evolving transients in the DES (Pursiainen+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/895/L23">J/ApJ/895/L23 : Radio obs. of the transient CSS161010 (Coppejans+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/895/32">J/ApJ/895/32 : Zwicky Transient Facility BTS. 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