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supernovae (PISNe), which disrupt the entire – 13 – REFERENCES 1 Barkana, R. Loeb, matter (WDM) simulations (right) at z = 20

Supernova (ASAS-SN) Bright Supernova Catalogs to determine the observed where it is enhanced by a factor of $\sim10-20$ relative to host

20 OAS1 FRS2 ATXN1 ULBP2 COL1A1 LY96 JMY pAdenoVator-CMV5-GFP (Qbiogene, Carlsbad, CA,Ottey M, Han SY, Druck T, Barnoski BL, Mc

J Toxicol Environ Health A. 2003 Oct 24;66(20):1909-26. 2003 Oct 24;66(20):1909-26. Exposure Shvedova AA1, Castranova V, Kisin ER,

Castranova V, Driscoll KE, Gardner DE, McClellan RO, Cooper BL, McKay 20.8 and 60.6 mg/m(3) of respirable-size lunar dust for 4 weeks

[Supernova Search Team Collaboration], Type Ia [43] A. Goobar, E. Mo¨rtsell, R. Ama 20 (2002) [astro-ph/0012324]. [45] N. Y

EMI Supply, Inc : Lutron NTR-20-HDTR-BL Nova T Half Dimmable Tamper Resistant Receptacle, Black, 20A, 120/125V [LUT-NTR-20-HDTR-BL] - Half

gas in the vicinity of the supernova remnant the emission is accelerated by about 20 km/s. bar is surrounded by a region of enhanced

spaxel scale, we can classify supernova Type Ia and their redshift robustly up to 80 days past maximum light (20 days in the supernova rest frame)

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