<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>47</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Spetsieri, Z. T.</style></author><author><style face="normal" font="default" size="100%">Bonanos, A. Z.</style></author><author><style face="normal" font="default" size="100%">Bellas-Velidis, I.</style></author><author><style face="normal" font="default" size="100%">Hatzidimitriou, D.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Supernovae, transients and high amplitude variables in the Hubble Catalog of Variables</style></title><short-title><style face="normal" font="default" size="100%">Supernova Remnants: An Odyssey in Space after Stellar Death II</style></short-title></titles><dates><year><style  face="normal" font="default" size="100%">2019</style></year><pub-dates><date><style  face="normal" font="default" size="100%">2019/06/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/2019sros.confE..62S</style></url></web-urls></urls><pages><style face="normal" font="default" size="100%">62</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">We present an exceptionally deep catalog of supernovae, transients and high-amplitude variables included in the Hubble Catalog of Variables (HCV). The HCV contains all variable objects detected through a robust variability search of the light curves of all sources included in the Hubble Source Catalog version 3 (Whitmore et al. 2016). Taking this work one step further, we queried the HCV to detect all variable sources with an amplitude of variability &amp;gt; 1 mag, in more than one filter of observations. We cross-matched the sources with catalogs in CDS to check whether the highamplitude variable sources were previously reported. We proceeded to classify the newly identified high-amplitude variables based on their magnitude, light curve shape and position on the color magnitude diagram. The high-precision astrometry extracted from the HSC for all sources combined with the deep HST observations makes our catalog a powerful tool for further research on the environments and properties of high-amplitude variables observed by the Hubble Space Telescope. This work was supported by the European Space Agency (ESA) under the &quot;Hubble Catalog of Variables&quot; program, contract No. 4000112940.</style></abstract></record></records></xml>