id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
app01-2388	Maeda, Keiichi; Terada, Yukikatsu; Bamba, Aya	Expected Hard X-Ray and Soft Gamma-Ray from Supernovae	2014	5	.pdf	application/pdf	2734	95	59	The model DD2D asym 04 is for bright SNe Ia (resulting in ∼ 1M� of 56Ni), while 205 http://dx.doi.org/10.14311/APP.2014.01.0205 Keiichi Maeda, Yukikatsu Terada, Aya Bamba Figure 1: Examples of the delayed-detonation models (Kasen et al., 2009; see also Maeda et al., 2010b). Conditions for the ini- tial triggers have not been clarified from the first prin- ciple (e.g., Seitenzahl et al., 2013), thus Kasen et al. (2009) adopted various conditions (i.e., distribution of the sparks) and produced a range of the ejecta models.	cache/app01-2388.pdf	txt/app01-2388.txt
