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Authors:
Galbany, L
| Stanishev, V
| Barrera-Ballesteros, J
| Bland-Hawthorn, J
| Falcón-Barroso, J
| García-Lorenzo, B
| Gomes, J.M
| González Delgado, R.M
| Kehrig, C
| Lyubenova, M
| López-Sánchez, A.R
| de Lorenzo-Cáceres, A
| Mourão, A. M
| Marino, R.A
| Meidt, S
| Mollá, M
| Papaderos, P
| Pérez-Torres, M.A
| Rosales-Ortega, F.F
| van de Ven, G
| CALIFA Collaboration,
| Rodrigues, M
| Flores, H
| García-Benito, R
| Mast, D
| Mendoza, M. A
| Sánchez, S. F
| Badenes, C
Date: 2014
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/326367
Description:
We use optical integral field spectroscopy (IFS) of nearby supernova (SN) host galaxies (0.005 < z < 0.03) provided by the Calar Alto Legacy Integral Field Area (CALIFA) Survey with the goal of findin
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Authors:
Sanchez, S. F
| Kennicutt, R. C
| Alonso-Herrero, A
| Alves, J
| Bakos, J
| Bartáková, T
| Bland-Hawthorn, J
| Boselli, A
| Bomans, D. J
| Castillo-Morales, A
| Cortijo-Ferrero, C
| de Lorenzo-Cáceres, A
| Gil de Paz, A
| del Olmo, A
| Dettmar, R. - J
| Díaz, A
| Ellis, S
| Falcón-Barroso, J
| Flores, H
| Gallazzi, A
| García-Lorenzo, B
| González Delgado, R
| Gruel, N
| van de Ven, G
| Haines, T
| Hao, C
| Husemann, B
| Iglésias-Páramo, J
| Jahnke, K
| Johnson, B
| Jungwiert, B
| Kalinova, V
| Kehrig, C
| Kupko, D
| Vilchez, J. M
| López-Sánchez, Á. R
| Lyubenova, M
| Marino, R. A
| Mármol-Queraltó, E
| Márquez, I
| Masegosa, J
| Meidt, S
| Mendez-Abreu, J
| Monreal-Ibero, A
| Montijo, C
| Wisotzki, L
| Mourao, A. M
| Palacios-Navarro, G
| Papaderos, P
| Pasquali, A
| Peletier, R
| Pérez, E
| Pérez, I
| Quirrenbach, A
| Relaño, M
| Rosales-Ortega, F. F
| Walcher, C. J
| Roth, M. M
| Ruiz-Lara, T
| Sanchez-Blazquez, P
| Sengupta, C
| Singh, R
| Stanishev, V
| Trager, S. C
| Vazdekis, A
| Viironen, K
| Wild, V
| Mast, D
| Zibetti, S
| Ziegler, B
| Aguerri, J. A. L
| Albiol-Pérez, S
Date: 2012
Subject Keyword:
020100 Astronomical and Space Sciences
| galaxies: active
| galaxies: evolution
| galaxies: ISM
| galaxies: stellar content
| surveys; techniques
| spectroscopic
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/178171
Description:
The final product of galaxy evolution through cosmic time is the population of galaxies in the local universe. These galaxies are also those that can be studied in most detail, thus providing a string
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