First results from the nuclear astrophysics AMS program at the NSL using the MANTIS system in gas-filled mode

Nuclear Instruments and Methods in Physics Research, Section B: Beam Interactions with Materials and Atoms

Volumn 266, Issue 15, 2008, Pages 3481-3486

  Robertson, D ^a   Collon, P ^a   Henderson, D ^b   Kurtz, S ^a   Lamm, L ^a   Schmitt, C ^a   Shumard, B ^b   Webb, J ^c  

^a UNIVERSITY OF NOTRE DAME   (United States)

^b ARGONNE NATIONAL LABORATORY   (United States)

^c UNIVERSITY OF WATERLOO   (Canada)

Author keywords

AMS; Astrophysics; MANTIS; NSL; Spectrograph; Supernova

Indexed keywords

AMERICIUM; ATMOSPHERIC OPTICS; ATMOSPHERIC PRESSURE; CHEMICAL ELEMENTS; MASS SPECTROMETRY; NICKEL COMPOUNDS; PARTICLE ACCELERATORS; SEPARATION; SPECTROGRAPHS; SUPERNOVAE;

ACCELERATOR MASS SPECTROMETRY; ISOBAR SEPARATION; MANTIS; NUCLEAR ASTRO-PHYSICS; TANDEM ACCELERATORS; UNIVERSITY OF NOTRE DAME;

ASTROPHYSICS;

EID: 48049091362     PISSN: 0168583X     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.nimb.2008.05.009     Document Type: Article

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