Artículo
Carnegie supernova project: classification of type Ia supernovae
Anthony, Lilian María; Baron, Edward; Ashall, Chris; Burns, Christopher R.; Morrell, Nidia Irene
; Stritzinger, Maximilian; Brown, Peter J.; Folatelli, Gaston
; Freedman, Wendy L.; Galbany, Lluís; Hoeflich, Peter; Hsiao, Eric; Krisciunas, Kevin; Phillips, M. M.; Piro, Anthony L.; Suntzeff, Nicholas B.; Uddin, Syed
Fecha de publicación:
10/2020
Editorial:
IOP Publishing
Revista:
Astrophysical Journal
ISSN:
0004-637X
Idioma:
Inglés
Tipo de recurso:
Artículo publicado
Clasificación temática:
Resumen
We use the spectroscopy and homogeneous photometry of 97 Type Ia supernovae (SNe Ia) obtained by the Carnegie Supernova Project as well as a subset of 36 SNe Ia presented by Zheng et al. to examine maximum-light correlations in a four-dimensional (4D) parameter space: B-band absolute magnitude, MB, Si II λ6355 velocity, vSi II, and Si II pseudo-equivalent widths pEW(Si II λ6355) and pEW(Si II λ5972). It is shown using Gaussian mixture models (GMMs) that the original four groups in the Branch diagram are well-defined and robust in this parameterization. We find three continuous groups that describe the behavior of our sample in [MB, vSi II] space. Extending the GMM into the full 4D space yields a grouping system that only slightly alters group definitions in the [MB, vSi II] projection, showing that most of the clustering information in [MB, vSi II] is already contained in the 2D GMM groupings. However, the full 4D space does divide group membership for faster objects between core-normal and broad-line objects in the Branch diagram. A significant correlation between MB and pseudo-equivalent width (Si II λ5972) is found, which implies that Branch group membership can be well-constrained by spectroscopic quantities alone. In general, we find that higher-dimensional GMMs reduce the uncertainty of group membership for objects between the originally defined Branch groups. We also find that the broad-line Branch group becomes nearly distinct with the inclusion of vSi II, indicating that this subclass of SNe Ia may be somehow different from the other groups.
Palabras clave:
Supernovae
,
Carnegie Supernova Project
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Colecciones
Articulos(IALP)
Articulos de INST.DE ASTROFISICA LA PLATA
Articulos de INST.DE ASTROFISICA LA PLATA
Citación
Anthony, Lilian María; Baron, Edward; Ashall, Chris; Burns, Christopher R.; Morrell, Nidia Irene; et al.; Carnegie supernova project: classification of type Ia supernovae; IOP Publishing; Astrophysical Journal; 901; 2; 10-2020; 154-179
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