The ASAS-SN bright supernova catalogue - I. 2013-2014

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dc.contributor.authorHoloien, T. W. S.
dc.contributor.authorStanek, K. Z.
dc.contributor.authorKochanek, C. S.
dc.contributor.authorShappee, B. J.
dc.contributor.authorPrieto, J. L.
dc.contributor.authorBrimacombe, J.
dc.contributor.authorBersier, D.
dc.contributor.authorBishop, D. W.
dc.contributor.authorDong, Subo
dc.contributor.authorBrown, J. S.
dc.contributor.authorDanilet, A. B.
dc.contributor.authorSimonian, G. V.
dc.contributor.authorBasu, U.
dc.contributor.authorBeacom, J. F.
dc.contributor.authorFalco, E.
dc.contributor.authorPojmanski, G.
dc.contributor.authorSkowron, D. M.
dc.contributor.authorWozniak, P. R.
dc.contributor.authorAvila, C. G.
dc.contributor.authorConseil, E.
dc.contributor.authorContreras, C.
dc.contributor.authorCruz, I.
dc.contributor.authorFernandez, J. M.
dc.contributor.authorKoff, R. A.
dc.contributor.authorGuo, Zhen
dc.contributor.authorHerczeg, G. J.
dc.contributor.authorHissong, J.
dc.contributor.authorHsiao, E. Y.
dc.contributor.authorJose, J.
dc.contributor.authorKiyota, S.
dc.contributor.authorLong, Feng
dc.contributor.authorMonard, L. A. G.
dc.contributor.authorNicholls, B.
dc.contributor.authorNicolas, J.
dc.contributor.authorWiethoff, W. S.
dc.date.accessioned2024-01-10T13:43:44Z
dc.date.available2024-01-10T13:43:44Z
dc.date.issued2017
dc.description.abstractWe present basic statistics for all supernovae discovered by the All-Sky Automated Survey for SuperNovae (ASAS-SN) during its first year-and-a-half of operations, spanning 2013 and 2014. We also present the same information for all other bright (mV <= 17), spectroscopically confirmed supernovae discovered from 2014 May 1 through the end of 2014, providing a comparison to the ASAS-SN sample starting from the point where ASAS-SN became operational in both hemispheres. In addition, we present collected redshifts and near-UV through IR magnitudes, where available, for all host galaxies of the bright supernovae in both samples. This work represents a comprehensive catalogue of bright supernovae and their hosts from multiple professional and amateur sources, allowing for population studies that were not previously possible because the all-sky emphasis of ASAS-SN redresses many previously existing biases. In particular, ASAS-SN systematically finds bright supernovae closer to the centres of host galaxies than either other professional surveys or amateurs, a remarkable result given ASAS-SN's poorer angular resolution. This is the first of a series of yearly papers on bright supernovae and their hosts that will be released by the ASAS-SN team.
dc.description.funderNSF
dc.description.funderCenter for Cosmology and AstroParticle Physics at the Ohio State University
dc.description.funderMt. Cuba Astronomical Foundation
dc.description.funderDOE Computational Science Graduate Fellowship
dc.description.funderNASA
dc.description.funderFONDECYT
dc.description.funderMinistry of Economy, Development, and Tourism's Millennium Science Initiative
dc.description.funder'Strategic Priority Research Program-The Emergence of Cosmological Structures' of the Chinese Academy of Sciences
dc.description.funderNSFC
dc.description.funderUS Department of Energy as part of the Laboratory Directed Research and Development programme at LANL
dc.description.funderRobert Martin Ayers Sciences Fund
dc.description.funderSmithsonian Astrophysical Observatory
dc.description.funderNASA Office of Space Science
dc.description.funderAlfred P. Sloan Foundation
dc.description.funderNational Science Foundation
dc.description.funderU.S. Department of Energy Office of Science
dc.description.funderNASA through Hubble Fellowship - Space Telescope Science Institute
dc.description.funderScience and Technology Facilities Council
dc.description.funderDirect For Mathematical & Physical Scien
dc.description.funderDivision Of Physics
dc.fechaingreso.objetodigital2024-04-29
dc.format.extent15 páginas
dc.fuente.origenWOS
dc.identifier.doi10.1093/mnras/stw2273
dc.identifier.eissn1365-2966
dc.identifier.issn0035-8711
dc.identifier.urihttps://doi.org/10.1093/mnras/stw2273
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/78742
dc.identifier.wosidWOS:000393647600013
dc.information.autorucFísica;Fernandez J ;S/I;221915
dc.issue.numero3
dc.language.isoen
dc.nota.accesocontenido parcial
dc.pagina.final2686
dc.pagina.inicio2672
dc.publisherOXFORD UNIV PRESS
dc.revistaMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
dc.rightsacceso restringido
dc.subjectcatalogues
dc.subjectsurveys
dc.subjectsupernovae: general
dc.subjectGAMMA-RAYS
dc.subjectFOLLOW-UP
dc.subjectRATES
dc.subjectDISCOVERY
dc.subjectTIME
dc.subjectFREQUENCY
dc.subjectREDSHIFT
dc.subjectSEARCH
dc.subjectEVENT
dc.subjectFLARE
dc.subject.ods07 Affordable and Clean Energy
dc.subject.odspa07 Energía asequible y no contaminante
dc.titleThe ASAS-SN bright supernova catalogue - I. 2013-2014
dc.typeartículo
dc.volumen464
sipa.codpersvinculados221915
sipa.indexWOS
sipa.indexScopus
sipa.trazabilidadCarga SIPA;09-01-2024
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