Nearby supernova host galaxies from the CALIFA survey, I : sample, data analysis, and correlation to star-forming regions
- Galbany, L
- Stanishev, V
- Mourao, AM
- Rodrigues, M
- Flores, H
- Garcia-Benito, R
- Mast, D
- Mendoza, MA
- Sanchez, SF
- Badenes, C
- Barrera-Ballesteros, J
- Bland-Hawthorn, J
- Falcon-Barroso, J
- Garcia-Lorenzo, B
- Gomes, JM
- Gonzalez Delgado, RM
- Kehrig, C
- Lyubenova, M
- Lopez-Sanchez, AR
- de Lorenzo-Caceres, A
- Marino, RA
- van der Wel, Sharon Meidt
- Molla, M
- Papaderos, P
- Perez-Torres, MA
- Rosales-Ortega, FF
- van de Ven, G
DOIAbstract
We use optical integral field spectroscopy (IFS) of nearby supernova (SN) host galaxies (0.005 2.4 Gyr, respectively) than the massive SN Ia hosts (0.04%, 2.01%, and 97.95% in these intervals). We estimate that the low-mass galaxies produce ten times fewer SNe Ia and three times fewer CC SNe than the high-mass group. Therefore the ratio between the number of CC SNe and SNe Ia is expected to increase with decreasing galaxy mass. CC SNe tend to explode at positions with younger stellar populations than the galaxy average, but the galaxy properties at SNe Ia locations are one average the same as the global galaxy properties
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