High Cadence TESS and ground-based data of SN 2019esa, the less energetic sibling of SN 2006gy

MLA

Andrews, Jennifer E., et al. High Cadence TESS and Ground-Based Data of SN 2019esa, the Less Energetic Sibling of SN 2006gy. 2022. EBSCOhost, https://doi.org/10.3847/1538-4357/ac8ea7.

APA

Andrews, J. E., Pearson, J., Lundquist, M. J., Sand, D. J., Jencson, J. E., Bostroem, K. A., Hosseinzadeh, G., Valenti, S., Smith, N., Amaro, R. C., Dong, Y., Janzen, D., Meza, N., Wyatt, S., Burke, J., Hiramatsu, D., Howell, D. A., McCully, C., & Pellegrino, C. (2022). High Cadence TESS and ground-based data of SN 2019esa, the less energetic sibling of SN 2006gy. https://doi.org/10.3847/1538-4357/ac8ea7

Chicago

Andrews, Jennifer E., Jeniveve Pearson, M. J. Lundquist, David J. Sand, Jacob E. Jencson, K. Azalee Bostroem, Griffin Hosseinzadeh, et al. 2022. “High Cadence TESS and Ground-Based Data of SN 2019esa, the Less Energetic Sibling of SN 2006gy.” doi:10.3847/1538-4357/ac8ea7.