<resource xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://datacite.org/schema/kernel-4" xsi:schemaLocation="http://datacite.org/schema/kernel-4 http://schema.datacite.org/meta/kernel-4.1/metadata.xsd"><identifier identifierType="DOI">10.34691/FK2/9SGXZG</identifier><creators><creator><creatorName nameType="Personal">Martínez Palomera, Jorge</creatorName><givenName>Jorge</givenName><familyName>Martínez Palomera</familyName><nameIdentifier SchemeURI="https://orcid.org/" nameIdentifierScheme="ORCID">0000-0002-7395-4935</nameIdentifier><affiliation>Universidad de Chile</affiliation></creator><creator><creatorName nameType="Personal">Förster, Francisco</creatorName><givenName>Francisco</givenName><familyName>Förster</familyName><nameIdentifier SchemeURI="https://orcid.org/" nameIdentifierScheme="ORCID">0000-0003-3459-2270</nameIdentifier><affiliation>Universidad de Chile</affiliation></creator></creators><titles><title>Replicar los datos para: The high cadence transient survey (Hits): Source, light-curve and classification catalogs</title></titles><publisher>Repositorio de datos de investigación de la Universidad de Chile</publisher><publicationYear>2019</publicationYear><subjects><subject>Astronomy and Astrophysics</subject><subject>Light-curve catalog</subject><subject>Variable stars</subject></subjects><contributors><contributor contributorType="ContactPerson"><contributorName nameType="Personal">Martínez Palomera, Jorge</contributorName><givenName>Jorge</givenName><familyName>Martínez Palomera</familyName><affiliation>Universidad de Chile</affiliation></contributor></contributors><dates><date dateType="Submitted">2019-06-19</date><date dateType="Updated">2023-04-04</date></dates><resourceType resourceTypeGeneral="Dataset"/><sizes><size>964800</size></sizes><formats><format>application/fits</format></formats><version>1.0</version><rightsList><rights rightsURI="info:eu-repo/semantics/openAccess"/><rights rightsURI="http://creativecommons.org/licenses/by/4.0">CC-BY 4.0</rights></rightsList><descriptions><description descriptionType="Abstract">The High Cadence Transient Survey (HiTS) aims to discover and study transient objects with characteristic timescales between hours and days, such as pulsating, eclipsing and exploding stars. This survey represents a unique laboratory to explore large etendue observations from cadences of about 0.1 days and to test new computational tools for the analysis of large data. This work follows a fully Data Science approach: from the raw data to the analysis and classification of variable sources. We compile a catalog of ~15 million object detections and a catalog of ~2.5 million light-curves classified by variability. The typical depth of the survey is 24.2, 24.3, 24.1 and 23.8 in u, g, r, and i bands, respectively. We classified all point-like non-moving sources by first extracting features from their light--curves and then applying a Random Forest classifier. For the classification, we used a training set constructed using a combination of cross-matched catalogs, visual inspection, transfer/active learning, and data augmentation. The classification model consists of several Random Forest classifiers organized in a hierarchical scheme. The classifier accuracy estimated on a test set is approximately 97%. In the unlabeled data, 3,485 sources were classified as variables, of which 1,321 were classified as periodic. Among the periodic classes we discovered with high confidence, 1 δ scuti, 39 eclipsing binaries, 48 rotational variables, and 90 RR-Lyrae. For the non-periodic classes we discovered 1 cataclysmic variables, 630 QSO, and 1 supernova candidate.</description></descriptions><geoLocations/></resource>