no code implementations • 20 Nov 2020 • A. Pastorello, G. Valerin, M. Fraser, N. Elias-Rosa, S. Valenti, A. Reguitti, P. A. Mazzali, R. C. Amaro, J. E. Andrews, Y. Dong, J. Jencson, M. Lundquist, D. E. Reichart, D. J. Sand, S. Wyatt, S. J. Smartt, K. W. Smith, S. Srivastav, Y. -Z. Cai, E. Cappellaro, S. Holmbo, A. Fiore, D. Jones, E. Kankare, E. Karamehmetoglu, P. Lundqvist, A. Morales-Garoffolo, T. M. Reynolds, M. D. Stritzinger, S. C. Williams, K. C. Chambers, T. J. L. de Boer, M. E. Huber, A. Rest, R. Wainscoat
A moderate-resolution spectrum of AT 2020hat taken at +37 d after maximum shows a forest of narrow P Cygni lines of metals with velocities of 180 km/s, along with an Halpha emission with a full-width at half-maximum velocity of 250 km/s.
Solar and Stellar Astrophysics
no code implementations • 23 Jan 2020 • S. C. Williams, D. Jones, P. Pessev, S. Geier, R. L. M. Corradi, I. M. Hook, M. J. Darnley, O. Pejcha, A. Núñez, S. Meingast, S. Moran
We present the most detailed optical light curve of an ILRT to date, with multi-band photometry starting around three weeks before peak brightness.
Solar and Stellar Astrophysics Astrophysics of Galaxies
