Three blue optical transients from CRTS

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dc.catalogadorpau
dc.contributor.authorDrake, A. J.
dc.contributor.authorDjorgovski, S. G.
dc.contributor.authorMahabal, A. A.
dc.contributor.authorGraham, M. J.
dc.contributor.authorWilliams, R.
dc.contributor.authorDonalek, C.
dc.contributor.authorPrieto, J.
dc.contributor.authorCatelan, Marcio
dc.contributor.authorChristensen, E.
dc.contributor.authorBeshore, E. C.
dc.contributor.authorLarson, S. M.
dc.contributor.authorMcNaught, R. H.
dc.date.accessioned2024-03-05T15:15:11Z
dc.date.available2024-03-05T15:15:11Z
dc.date.issued2011
dc.description.abstractDuring the course of the CRTS survey, observations of poorly understood transient sources were undertaken with the Palomar 5m+DBSP on May 7 and May 8 UT. In addition to many SNe (ATEL#3340), three events were found exhibiting very blue continua.
dc.fuente.origenORCID
dc.identifier.urihttps://ui.adsabs.harvard.edu/abs/2011ATel.3343....1D/abstract
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/84128
dc.information.autorucInstituto de Astrofísica; Catelan , Marcio; 0000-0001-6003-8877; 1001556
dc.language.isoen
dc.nota.accesocontenido parcial
dc.publisherThe SAO Astrophysics Data System
dc.rightsacceso abierto
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.titleThree blue optical transients from CRTS
dc.typecomentario
sipa.codpersvinculados1001556
sipa.trazabilidadORCID;2024-01-22
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