The Carnegie Supernova Project I : Third Photometry Data Release of Low-redshift Type Ia Supernovae and Other White Dwarf Explosions

We present final natural-system optical (<i>ugriBV</i>) and near-infrared (<i>YJH</i>) photometry of 134 supernovae (SNe) with probable white dwarf progenitors that were observed in 2004-2009 as part of the first stage of the Carnegie Supernova Project (CSP-I). The sample con...

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Detalles Bibliográficos
Autores: Krisciunas, K., Contreras, Carlos, Burns, Christopher R., Phillips, Mark M., Hamuy, Mario, Stritzinger, Maximilian, Anais, J., Boldt, Luis, Busta, Luis, Campillay, Abdo, Castellon, S., Folatelli, Gastón, Freedman, Wendy L., González, Consuelo, Hsiao, Eric Y., Krzeminski, Wojtek, Morrell, Nidia Irene, Persson, S. E., Roth, M., Salgado, Francisco, Serón, Jacqueline, Suntzeff, Nicholas B., Torres, Simón, Filippenko, Alexei V., Li, Weidong, Madore, Barry F., Depoy, D. L., Marshall, J. L., Rheault, J. P., Villanueva, Steven
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2017
País:Argentina
Institución:Universidad Nacional de La Plata
Repositorio:SEDICI (UNLP)
Idioma:inglés
OAI Identifier:oai:sedici.unlp.edu.ar:10915/87213
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/87213
Access Level:acceso abierto
Palabra clave:Ciencias Astronómicas
instrumentation: photometers
supernovae: general
surveys
techniques: photometric
Descripción
Sumario:We present final natural-system optical (<i>ugriBV</i>) and near-infrared (<i>YJH</i>) photometry of 134 supernovae (SNe) with probable white dwarf progenitors that were observed in 2004-2009 as part of the first stage of the Carnegie Supernova Project (CSP-I). The sample consists of 123 Type Ia SNe, 5 Type Iax SNe, 2 super-Chandrasekhar SN candidates, 2 Type Ia SNe interacting with circumstellar matter, and 2 SN 2006bt-like events. The redshifts of the objects range from to 0.0835; the median redshift is 0.0241. For 120 (90%) of these SNe, near-infrared photometry was obtained. Average optical extinction coefficients and color terms are derived and demonstrated to be stable during the five CSP-I observing campaigns. Measurements of the CSP-I near-infrared bandpasses are also described, and near-infrared color terms are estimated through synthetic photometry of stellar atmosphere models. Optical and near-infrared magnitudes of local sequences of tertiary standard stars for each supernova are given, and a new calibration of Y-band magnitudes of the Persson et al. standards in the CSP-I natural system is presented.

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