Host Galaxy Identification for Supernova Surveys

Host galaxy identification is a crucial step for modern supernova (SN) surveys such as the Dark Energy Survey (DES) and the Large Synoptic Survey Telescope (LSST), which will discover SNe by the thousands. Spectroscopic resources are limited, so in the absence of real-time SN spectra these surveys m...

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Veröffentlicht in:arXiv.org 2016-06
Hauptverfasser: Gupta, Ravi R, Kuhlmann, Steve, Kovacs, Eve, Spinka, Harold, Kessler, Richard, Goldstein, Daniel A, Liotine, Camille, Pomian, Katarzyna, D'Andrea, Chris B, Sullivan, Mark, Carretero, Jorge, Castander, Francisco J, Nichol, Robert C, Finley, David A, Fischer, John A, Foley, Ryan J, Kim, Alex G, Papadopoulos, Andreas, Sako, Masao, Scolnic, Daniel M, Smith, Mathew, Tucker, Brad E, Uddin, Syed, Wolf, Rachel C, Yuan, Fang, Abbott, Tim M C, Abdalla, Filipe B, Benoit-Levy, Aurelien, Bertin, Emmanuel, Brooks, David, Aurelio Carnero Rosell, Matias Carrasco Kind, Cunha, Carlos E, da Costa, Luiz N, Desai, Shantanu, Doel, Peter, Eifler, Tim F, Evrard, August E, Flaugher, Brenna, Fosalba, Pablo, Gaztanaga, Enrique, Gruen, Daniel, Gruendl, Robert, James, David J, Kuehn, Kyler, Kuropatkin, Nikolay, Maia, Marcio A G, Marshall, Jennifer L, Miquel, Ramon, Plazas, Andres A, Romer, A Kathy, Sanchez, Eusebio, Schubnell, Michael, Sevilla-Noarbe, Ignacio, Sobreira, Flavia, Suchyta, Eric, Swanson, Molly E C, Tarle, Gregory, Walker, Alistair R, Wester, William
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