tipa -- 12/14/2015

Exploring the Potential Diversity of Early Type Ia Supernova Light Curves

• Anthony L. Piro (Carnegie Observatories), Viktoriya S. Morozova (Caltech)

The interplay between chemistry and nucleation in the formation of carbonaceous dust in supernova ejecta

• Davide Lazzati (Oregon State), Alexander Heger (Monash)

Improved WIMP scattering limits from the LUX experiment

• LUX Collaboration

X-Ray Detection of Warm Ionized Matter in the Galactic Halo

• F. Nicastro (1,2,3), F. Senatore (1,4), A. Gupta (5,6), M. Guainazzi (7), S. Mathur (5,8), Y. Krongold (9), M. Elvis (2), L. Piro (10) ((1) Osservatorio Astronomico di Roma - INAF, Monte Porzio Catone, RM, Italy, (2) Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA, (3) University of Crete, Heraklion, Greece, (4) Universita' degli Studi di Roma Tor Vergata, Roma, Italy, (5) Ohio State University, Columbus, OH, USA, (6) Columbus State Community College, Columbus, OH, USA, (7) European Space Astronomy Center of ESA, Madrid, Spain, (8) Center for Cosmology and Astro-particle Physics, Columbus, OH, USA, (9) Instituto de Astronomia Universidad Nacional Autonoma de Mexico, Mexico City, Mexico, (10) Istituto di Astrofisica e Planetologia Spaziali - INAF, Roma, Italy)

High-Sensitivity 86GHz (3.5mm) VLBI Observations of M87: Deep Imaging of the Jet Base at a 10 Schwarzschild-Radius Resolution

• Kazuhiro Hada, Motoki Kino, Akihiro Doi, Hiroshi Nagai, Mareki Honma, Kazunori Akiyama, Fumie Tazaki, Rocco Lico, Marcello Giroletti, Gabriele Giovannini, Monica Orienti, Yoshiaki Hagiwara