Revealing the progenitor of SN 2021zby through analysis of the $TESS$ shock-cooling light curve

Qinan Wang(Johns Hopkins University), A. Zenteno(Cerro Tololo Inter-American Observatory), C. D. Kilpatrick(University of California, Santa Cruz), J. P. Anderson, D. O. Jones(University of Hawaii System), J. Lyman(Liverpool John Moores University), L. Galbany, M. Gromadzki(Astronomical Observatory), T. E. Müller-Bravo(Trinity College), C. Pellegrino(Las Cumbres Observatory Global Telescope Network), P. Armstrong(Australian National University), M. Fulton(Queen's University Belfast), A. Rest(Space Telescope Science Institute), Kyle W. Davis(University of California, Santa Cruz), J. Jencson(Space Telescope Science Institute), D. R. Young(Queen's University Belfast), D.H. O’Neill(University of Warwick), B. Tucker(Australian National University), Samaporn Tinyanont(University of California, Santa Cruz), J. Burke(Las Cumbres Observatory Global Telescope Network), Ken R. Smith(Huntsman Cancer Institute), Ryan Ridden-Harper(Johns Hopkins University), T. Killestein(University of Turku), Yossef Zenati(Space Telescope Science Institute), S. Rest(Johns Hopkins University), S. J. Smartt(University of Oxford), Kyle A. Dalrymple(Johns Hopkins University), Ting-wan Chen, Megan Newsome(Las Cumbres Observatory Global Telescope Network), N. Ihanec(European Southern Observatory), Melissa Shahbandeh(Space Telescope Science Institute), C. Lidman(Australian National University), M. Nicholl(Queen's University Belfast), C. Ashall(Virginia Tech), Shubham Srivastav(Queen's University Belfast), R. J. Foley(Center for Astrophysics Harvard & Smithsonian)
arXiv (Cornell University)
November 7, 2022
Cited by 0


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