Using Line Profiles to Test the Fraternity of Type Ia Supernovae at High and Low Redshifts
dc.contributor.author | Blondin, Stéphane | |
dc.contributor.author | Dessart, Luc | |
dc.contributor.author | Leibundgut, Bruno | |
dc.contributor.author | Branch, David | |
dc.contributor.author | Höflich, Peter | |
dc.contributor.author | Tonry, John L. | |
dc.contributor.author | Matheson, Thomas | |
dc.contributor.author | Foley, Ryan J. | |
dc.contributor.author | Chornock, Ryan | |
dc.contributor.author | Filippenko, Alexei V. | |
dc.contributor.author | Sollerman, Jesper | |
dc.contributor.author | Spyromilio, Jason | |
dc.contributor.author | Kirshner, Robert P. | |
dc.contributor.author | Wood-Vasey, W. Michael | |
dc.contributor.author | Clocchiatti, Alejandro | |
dc.contributor.author | Aguilera, Claudio | |
dc.contributor.author | Barris, Brian | |
dc.contributor.author | Becker, Andrew C. | |
dc.contributor.author | Challis, Peter | |
dc.contributor.author | Covarrubias, Ricardo | |
dc.contributor.author | Davis, Tamara M. | |
dc.contributor.author | Garnavich, Peter | |
dc.contributor.author | Hicken, Malcolm | |
dc.contributor.author | Jha, Saurabh | |
dc.contributor.author | Krisciunas, Kevin | |
dc.contributor.author | Li, Weidong | |
dc.contributor.author | Miceli, Anthony | |
dc.contributor.author | Miknaitis, Gajus | |
dc.contributor.author | Pignata, Giuliano | |
dc.contributor.author | Prieto, Jose Luis | |
dc.contributor.author | Rest, Armin | |
dc.contributor.author | Riess, Adam G. | |
dc.contributor.author | Salvo, Maria Elena | |
dc.contributor.author | Schmidt, Brian P. | |
dc.contributor.author | Smith, R. Chris | |
dc.contributor.author | Stubbs, Christopher W. | |
dc.contributor.author | Suntzeff, Nicholas B. | |
dc.date.accessioned | 2019-09-27T13:17:44Z | |
dc.date.issued | 2006 | |
dc.identifier.citation | Blondin, Stéphane, Luc Dessart, Bruno Leibundgut, David Branch, Peter Höflich, John L. Tonry, Thomas Matheson, et al. 2006. “Using Line Profiles to Test the Fraternity of Type Ia Supernovae at High and Low Redshifts.” The Astronomical Journal 131 (3): 1648–66. https://doi.org/10.1086/498724. | |
dc.identifier.issn | 0004-6256 | |
dc.identifier.issn | 1538-3881 | |
dc.identifier.uri | http://nrs.harvard.edu/urn-3:HUL.InstRepos:41417346 | * |
dc.language.iso | en_US | |
dc.publisher | American Astronomical Society | |
dash.license | LAA | |
dc.title | Using Line Profiles to Test the Fraternity of Type Ia Supernovae at High and Low Redshifts | |
dc.type | Journal Article | |
dc.description.version | Version of Record | |
dc.relation.journal | The Astronomical Journal | |
dash.depositing.author | Kirshner, Robert P.::0f07c3b6230f5e5a42326bcba12a1795::600 | |
dc.date.available | 2019-09-27T13:17:44Z | |
dash.workflow.comments | 1Science Serial ID 94643 | |
dc.identifier.doi | 10.1086/498724 | |
dash.source.volume | 131;3 | |
dash.source.page | 1648-1666 |
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