Marc J. Staley Fellow.
Berkeley Supernova Ia Program – III. Spectra near maximum brightness improve the accuracy of derived distances to Type Ia supernovae
Article first published online: 27 AUG 2012
© 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
Monthly Notices of the Royal Astronomical Society
Volume 425, Issue 3, pages 1889–1916, 21 September 2012
How to Cite
Silverman, J. M., Ganeshalingam, M., Li, W. and Filippenko, A. V. (2012), Berkeley Supernova Ia Program – III. Spectra near maximum brightness improve the accuracy of derived distances to Type Ia supernovae. Monthly Notices of the Royal Astronomical Society, 425: 1889–1916. doi: 10.1111/j.1365-2966.2012.21526.x
- Issue published online: 24 AUG 2012
- Article first published online: 27 AUG 2012
- Manuscript Accepted: 14 JUN 2012
- Manuscript Received: 4 MAY 2012
- Lick and Keck Observatories
- W. M. Keck Foundation
- NSF. Grant Number: AST-0908886
- DOE. Grant Numbers: DE-FC02-06ER41453, DE-FG02-08ER41563
- TABASGO Foundation
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