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.” Astrophysical Journal, vol. 938, no. 1, Oct. 2022, pp. 1–13. 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. Astrophysical Journal, 938(1), 1–13. 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.” Astrophysical Journal 938 (1): 1–13. doi:10.3847/1538-4357/ac8ea7.