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Integration of Near-Maximum-Light Type Ia Supernova Spectra as a Method of High-z Identification

Publication ,  Conference
Troxel, MA; Ketchum, WR; Branch, D; Garnavich, P; Baron, E; Wang, Y
Published in: American Astronomical Society Meeting Abstracts
December 2005

Duke Scholars

Published In

American Astronomical Society Meeting Abstracts

Publication Date

December 2005

Volume

207

Start / End Page

171.10 / 171.10
 

Citation

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Troxel, M. A., Ketchum, W. R., Branch, D., Garnavich, P., Baron, E., & Wang, Y. (2005). Integration of Near-Maximum-Light Type Ia Supernova Spectra as a Method of High-z Identification. In American Astronomical Society Meeting Abstracts (Vol. 207, pp. 171.10-171.10).
Troxel, M. A., W. R. Ketchum, D. Branch, P. Garnavich, E. Baron, and Y. Wang. “Integration of Near-Maximum-Light Type Ia Supernova Spectra as a Method of High-z Identification.” In American Astronomical Society Meeting Abstracts, 207:171.10-171.10, 2005.
Troxel MA, Ketchum WR, Branch D, Garnavich P, Baron E, Wang Y. Integration of Near-Maximum-Light Type Ia Supernova Spectra as a Method of High-z Identification. In: American Astronomical Society Meeting Abstracts. 2005. p. 171.10-171.10.
Troxel, M. A., et al. “Integration of Near-Maximum-Light Type Ia Supernova Spectra as a Method of High-z Identification.” American Astronomical Society Meeting Abstracts, vol. 207, 2005, pp. 171.10-171.10.
Troxel MA, Ketchum WR, Branch D, Garnavich P, Baron E, Wang Y. Integration of Near-Maximum-Light Type Ia Supernova Spectra as a Method of High-z Identification. American Astronomical Society Meeting Abstracts. 2005. p. 171.10-171.10.

Published In

American Astronomical Society Meeting Abstracts

Publication Date

December 2005

Volume

207

Start / End Page

171.10 / 171.10