Supernova 2011cg
| dc.catalogador | dfo | |
| dc.contributor.author | Drake, A. J. | |
| dc.contributor.author | Djorgovski, S. G. | |
| dc.contributor.author | Mahabal, A. | |
| dc.contributor.author | Graham, M. J. | |
| dc.contributor.author | Williams, R. | |
| dc.contributor.author | Prieto, J. L. | |
| dc.contributor.author | Catelan, Marcio | |
| dc.contributor.author | Beshore, E. C. | |
| dc.contributor.author | Larson, S. M. | |
| dc.contributor.author | Christensen, E. | |
| dc.contributor.author | Marion, G. H. | |
| dc.contributor.author | Berlind, P. | |
| dc.date.accessioned | 2024-03-05T15:15:18Z | |
| dc.date.available | 2024-03-05T15:15:18Z | |
| dc.date.issued | 2011 | |
| dc.description.abstract | Report the Catalina Real-time Transient Survey's discovery of an apparent supernova in unfiltered Catalina Sky Survey images: SN 2011 UT R.A. (2000.0) Decl. Mag. Offset 2011cg Apr. 14.33 14 59 09.25 + 7 18 04.2 15.7 2" W, 1" S G. H. Marion, Harvard-Smithsonian Center for Astrophysics (CfA), on behalf of the CfA Supernova Group, report that a spectrum (range 340-740 nm) of 2011cg was obtained on May 5 UT by P. Berlind with the F. L. Whipple Observatory 1.5-m telescope (+ FAST). Cross-correlation with a library of supernova spectra using the "Supernova Identification" code (SNID; Blondin and Tonry 2007, Ap.J. 666, 1024) shows that 2011cg is a type-Ia supernova about two weeks after maximum light.... | |
| dc.fuente.origen | ORCID | |
| dc.identifier.uri | https://repositorio.uc.cl/handle/11534/84155 | |
| dc.information.autoruc | Instituto de Astrofísica; Catelan , Marcio; 0000-0001-6003-8877; 1001556 | |
| dc.language.iso | en | |
| dc.nota.acceso | contenido parcial | |
| dc.rights | acceso restringido | |
| dc.title | Supernova 2011cg | |
| dc.type | informe | |
| sipa.codpersvinculados | 1001556 | |
| sipa.trazabilidad | ORCID;2024-01-22 |