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pro vyhledávání: '"Wee, Jerrick"'
Autor:
Wee, Jerrick, Blagorodnova, Nadejda, Penprase, Bryan Edward, Facey, Jett Pierce, Morioka, Taiga, Corbett, Hank, Barlow, Brad N., Kupfer, Thomas, Law, Nicholas M., Ratzloff, Jeffrey K., Howard, Ward S., Chavez, Ramses Gonzalez, Glazier, Amy, Soto, Alan Vasquez, Horiuchi, Takashi
We present optical and infrared photometry of the classical nova V906 Car, also known as Nova Car 2018 and ASASSN-18fv, discovered by ASASS-SN survey on 16.32 March 2018 UT (MJD 58193.0). The nova reached its maximum on MJD 58222.56 at $V_{\rm{max}}
Externí odkaz:
http://arxiv.org/abs/2006.14336
Autor:
Perley, Daniel A., Mazzali, Paolo A., Yan, Lin, Cenko, S. Bradley, Gezari, Suvi, Taggart, Kirsty, Blagorodnova, Nadia, Fremling, Christoffer, Mockler, Brenna, Singh, Avinash, Tominaga, Nozomu, Tanaka, Masaomi, Watson, Alan M., Ahumada, Tomás, Anupama, G. C., Ashall, Chris, Becerra, Rosa L., Bersier, David, Bhalerao, Varun, Bloom, Joshua S., Butler, Nathaniel R., Copperwheat, Chris, Coughlin, Michael W., De, Kishalay, Drake, Andrew J., Duev, Dmitry A., Frederick, Sara, González, J. Jesús, Goobar, Ariel, Heida, Marianne, Ho, Anna Y. Q., Horst, John, Hung, Tiara, Itoh, Ryosuke, Jencson, Jacob E., Kasliwal, Mansi M., Kawai, Nobuyuki, Kulkarni, Shrinivas R., Kumar, Brajesh, Kumar, Harsh, Kutyrev, Alexander S., Khanam, Tanazza, Lee, William H., Maeda, Keiichi, Mahabal, Ashish, Murata, Katsuhiro L., Neill, James D., Ngeow, Chow-Choong, Penprase, Bryan, Pian, Elena, Quimby, Robert, Ramirez-Ruiz, Enrico, Richer, Michael, Román-Zúñiga, Carlos G., Srivastava, Shubham, Socia, Quentin, Sollerman, Jesper, Tachibana, Yutaro, Taddia, Francesco, Tinyanont, Samaporn, Troja, Eleonora, Ward, Charlotte, Wee, Jerrick
Wide-field optical surveys have begun to uncover large samples of fast (t_rise < 5d), luminous (M_peak < -18), blue transients. While commonly attributed to the breakout of a supernova shock into a dense wind, the great distances to the transients of
Externí odkaz:
http://arxiv.org/abs/1808.00969
On 2017 March 11, the DLT40 Transient Discovery Survey discovered SN 2017cbv in NGC5643, a Type 2 Seyfert Galaxy in the Lupus Constellation. SN 2017cbv went on to become a bright Type Ia supernova, with a $V_{max}$ of 11.51 $\pm$ 0.05 mag. We present
Externí odkaz:
http://arxiv.org/abs/1806.08794
Akademický článek
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Autor:
Wee, Jerrick, Blagorodnova, Nadejda, Penprase, Bryan Edward, Facey, Jett Pierce, Morioka, Taiga, Corbett, Hank, Barlow, Brad N., Kupfer, Thomas, Law, Nicholas M., Ratzloff, Jeffrey K., Howard, Ward S., Chavez, Ramses Gonzalez, Glazier, Amy, Soto, Alan Vasquez, Horiuchi, Takashi
Publikováno v:
Astrophysical Journal; 8/20/2020, Vol. 899 Issue 2, p1-10, 10p