no code implementations • 4 Dec 2020 • Thavisha E. Dharmawardena, M. J. Barlow, J. E. Drew, A. Seales, S. E. Sale, D. Jones, A. Mampaso, Q. A. Parker, L. Sabin, R. Wesson
Distances to the PNe were then estimated using three different 3D interstellar dust extinction mapping methods, including the IPHAS-based H-MEAD algorithm of Sale (2014).
Astrophysics of Galaxies Solar and Stellar Astrophysics
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
