The Carnegie Supernova Project I

The first phase of the Carnegie Supernova Project (CSP-I) was a dedicated supernova follow-up program based at the Las Campanas Observatory that collected science data of young, low-redshift supernovae between 2004 and 2009. Presented in this paper is the CSP-I photometric data release of low-redshi...

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Published inAstronomy and astrophysics (Berlin) Vol. 609
Main Authors Stritzinger, M. D., Anderson, J. P., Contreras, C., Heinrich-Josties, E., Morrell, N., Phillips, M. M., Anais, J., Boldt, L., Busta, L., Burns, C. R., Campillay, A., Corco, C., Castellon, S., Folatelli, G., González, C., Holmbo, S., Hsiao, E. Y., Krzeminski, W., Salgado, F., Serón, J., Torres-Robledo, S., Freedman, W. L., Hamuy, M., Krisciunas, K., Madore, B. F., Persson, S. E., Roth, M., Suntzeff, N. B., Taddia, F., Li, W., Filippenko, A. V.
Format Journal Article
LanguageEnglish
Published Heidelberg EDP Sciences 2018
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ISSN0004-6361
1432-0746
DOI10.1051/0004-6361/201730842

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Abstract The first phase of the Carnegie Supernova Project (CSP-I) was a dedicated supernova follow-up program based at the Las Campanas Observatory that collected science data of young, low-redshift supernovae between 2004 and 2009. Presented in this paper is the CSP-I photometric data release of low-redshift stripped-envelope core-collapse supernovae. The data consist of optical (uBgVri) photometry of 34 objects, with a subset of 26 having near-infrared (YJH) photometry. Twenty objects have optical pre-maximum coverage with a subset of 12 beginning at least five days prior to the epoch of B-band maximum brightness. In the near-infrared, 17 objects have pre-maximum observations with a subset of 14 beginning at least five days prior to the epoch of J-band maximum brightness. Analysis of this photometric data release is presented in companion papers focusing on techniques to estimate host-galaxy extinction and the light-curve and progenitor star properties of the sample. The analysis of an accompanying visual-wavelength spectroscopy sample of ~150 spectra will be the subject of a future paper.
AbstractList The first phase of the Carnegie Supernova Project (CSP-I) was a dedicated supernova follow-up program based at the Las Campanas Observatory that collected science data of young, low-redshift supernovae between 2004 and 2009. Presented in this paper is the CSP-I photometric data release of low-redshift stripped-envelope core-collapse supernovae. The data consist of optical (uBgVri) photometry of 34 objects, with a subset of 26 having near-infrared (YJH) photometry. Twenty objects have optical pre-maximum coverage with a subset of 12 beginning at least five days prior to the epoch of B-band maximum brightness. In the near-infrared, 17 objects have pre-maximum observations with a subset of 14 beginning at least five days prior to the epoch of J-band maximum brightness. Analysis of this photometric data release is presented in companion papers focusing on techniques to estimate host-galaxy extinction and the light-curve and progenitor star properties of the sample. The analysis of an accompanying visual-wavelength spectroscopy sample of ~150 spectra will be the subject of a future paper.
Author Li, W.
Anais, J.
Taddia, F.
Boldt, L.
Persson, S. E.
Freedman, W. L.
Stritzinger, M. D.
Contreras, C.
Hsiao, E. Y.
Holmbo, S.
Corco, C.
Anderson, J. P.
Suntzeff, N. B.
Serón, J.
Madore, B. F.
Torres-Robledo, S.
Campillay, A.
Hamuy, M.
Burns, C. R.
Krzeminski, W.
Roth, M.
Krisciunas, K.
Heinrich-Josties, E.
Busta, L.
González, C.
Salgado, F.
Phillips, M. M.
Filippenko, A. V.
Castellon, S.
Folatelli, G.
Morrell, N.
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href:https://www.aanda.org/articles/aa/abs/2018/01/aa30842-17/aa30842-17.html
Deceased
Based on observations collected at Las Campanas Observatory.
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Snippet The first phase of the Carnegie Supernova Project (CSP-I) was a dedicated supernova follow-up program based at the Las Campanas Observatory that collected...
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SubjectTerms Brightness
Galaxies
Infrared photometry
Photometry
Red shift
Spectrum analysis
Supernovae
supernovae: general
Title The Carnegie Supernova Project I
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