7 THE GOAL OF THIS PROPOSAL IS TO USE THE LINE EMISSION FROM SECONDARY FE-PEAK ELEMENTS IN SUZAKU SPECTRA OF TYPE IA SUPERNOVA REMNANTS (SNRS) TO CONSTRAIN THE PHYSICS OF TYPE IA SUPERNOVAE (IA SNE) AND THE NATURE OF THEIR PROGENITORS. WE WILL RE-ANALYZE THE EXTANT SAMPLE OF SUZAKU OBSERVATIONS OF TYPE IA SNRS WITH PROMINENT FE K-SHELL LINES, AND SEARCH FOR EMISSION FROM MN, CR, AND NI. WE WILL USE LINE FLUXES AND UPPER LIMITS FROM THESE ELEMENTS TO DETERMINE THE REGIME OF THERMONUCLEAR COMBUSTION THAT SYNTHESIZED THE X-RAY EMITTING FE-GROUP EJECTA, AND MEASURE THE NEUTRON EXCESS OF THE SN PROGENITORS, WHICH IS CLOSELY RELATED TO THEIR METALLICITY. KNOWLEDGE OF THE COMBUSTION REGIME AND PROGENITOR METALLICITY CAN BE USED TO DETERMINE THE MASS OF THE EXPLODING WHITE DWARF, ESTIMATE THE AGE OF THE PROGENITOR SYSTEMS, AND VALIDATE SPECIFIC PROGENITOR EVOLUTION SCENARIOS. OUR WORK WILL YIELD THE FIRST SAMPLE OF METALLICITIES AND AGES FOR SN IA PROGENITORS IN DIFFERENT ENVIRONMENTS, A UNIQUE MEASUREMENT THAT CAN ONLY BE PERFORMED WITH THE SUZAKU DATA SET. Funding Only Action ($25) 11/18/19 Not listed THE GOAL OF THIS PROPOSAL IS TO USE THE LINE EMISSION FROM SECONDARY FE-PEAK ELEMENTS IN SUZAKU SPECTRA OF TYPE IA SUPERNOVA REMNANTS (SNRS) TO CONSTRAIN THE PHYSICS OF TYPE IA SUPERNOVAE (IA SNE) AND THE NATURE OF THEIR PROGENITORS. WE WILL RE-ANALYZE THE EXTANT SAMPLE OF SUZAKU OBSERVATIONS OF TYPE IA SNRS WITH PROMINENT FE K-SHELL LINES AND SEARCH FOR EMISSION FROM MN CR AND NI. WE WILL USE LINE FLUXES AND UPPER LIMITS FROM THESE ELEMENTS TO DETERMINE THE REGIME OF THERMONUCLEAR COMBUSTION THAT SYNTHESIZED THE X-RAY EMITTING FE-GROUP EJECTA AND MEASURE THE NEUTRON EXCESS OF THE SN PROGENITORS WHICH IS CLOSELY RELATED TO THEIR METALLICITY. KNOWLEDGE OF THE COMBUSTION REGIME AND PROGENITOR METALLICITY CAN BE USED TO DETERMINE THE MASS OF THE EXPLODING WHITE DWARF ESTIMATE THE AGE OF THE PROGENITOR SYSTEMS AND VALIDATE SPECIFIC PROGENITOR EVOLUTION SCENARIOS. OUR WORK WILL YIELD THE FIRST SAMPLE OF METALLICITIES AND AGES FOR SN IA PROGENITORS IN DIFFERENT ENVIRONMENTS A UNIQUE MEASUREMENT THAT CAN ONLY BE PERFORMED WITH THE SUZAKU DATA SET. ($25) 11/18/19 Not listed THE GOAL OF THIS PROPOSAL IS TO USE THE LINE EMISSION FROM SECONDARY FE-PEAK ELEMENTS IN SUZAKU SPECTRA OF TYPE IA SUPERNOVA REMNANTS (SNRS) TO CONSTRAIN THE PHYSICS OF TYPE IA SUPERNOVAE (IA SNE) AND THE NATURE OF THEIR PROGENITORS. WE WILL RE-ANALYZE THE EXTANT SAMPLE OF SUZAKU OBSERVATIONS OF TYPE IA SNRS WITH PROMINENT FE K-SHELL LINES AND SEARCH FOR EMISSION FROM MN CR AND NI. WE WILL USE LINE FLUXES AND UPPER LIMITS FROM THESE ELEMENTS TO DETERMINE THE REGIME OF THERMONUCLEAR COMBUSTION THAT SYNTHESIZED THE X-RAY EMITTING FE-GROUP EJECTA AND MEASURE THE NEUTRON EXCESS OF THE SN PROGENITORS WHICH IS CLOSELY RELATED TO THEIR METALLICITY. KNOWLEDGE OF THE COMBUSTION REGIME AND PROGENITOR METALLICITY CAN BE USED TO DETERMINE THE MASS OF THE EXPLODING WHITE DWARF ESTIMATE THE AGE OF THE PROGENITOR SYSTEMS AND VALIDATE SPECIFIC PROGENITOR EVOLUTION SCENARIOS. OUR WORK WILL YIELD THE FIRST SAMPLE OF METALLICITIES AND AGES FOR SN IA PROGENITORS IN DIFFERENT ENVIRONMENTS A UNIQUE MEASUREMENT THAT CAN ONLY BE PERFORMED WITH THE SUZAKU DATA SET. $0 5/30/18 6 THE GOAL OF THIS PROPOSAL IS TO USE THE LINE EMISSION FROM SECONDARY FE-PEAK ELEMENTS IN SUZAKU SPECTRA OF TYPE IA SUPERNOVA REMNANTS (SNRS) TO CONSTRAIN THE PHYSICS OF TYPE IA SUPERNOVAE (IA SNE) AND THE NATURE OF THEIR PROGENITORS. WE WILL RE-ANALYZE THE EXTANT SAMPLE OF SUZAKU OBSERVATIONS OF TYPE IA SNRS WITH PROMINENT FE K-SHELL LINES, AND SEARCH FOR EMISSION FROM MN, CR, AND NI. WE WILL USE LINE FLUXES AND UPPER LIMITS FROM THESE ELEMENTS TO DETERMINE THE REGIME OF THERMONUCLEAR COMBUSTION THAT SYNTHESIZED THE X-RAY EMITTING FE-GROUP EJECTA, AND MEASURE THE NEUTRON EXCESS OF THE SN PROGENITORS, WHICH IS CLOSELY RELATED TO THEIR METALLICITY. KNOWLEDGE OF THE COMBUSTION REGIME AND PROGENITOR METALLICITY CAN BE USED TO DETERMINE THE MASS OF THE EXPLODING WHITE DWARF, ESTIMATE THE AGE OF THE PROGENITOR SYSTEMS, AND VALIDATE SPECIFIC PROGENITOR EVOLUTION SCENARIOS. OUR WORK WILL YIELD THE FIRST SAMPLE OF METALLICITIES AND AGES FOR SN IA PROGENITORS IN DIFFERENT ENVIRONMENTS, A UNIQUE MEASUREMENT THAT CAN ONLY BE PERFORMED WITH THE SUZAKU DATA SET. Other Administrative Action $0 5/30/18 Not listed THE GOAL OF THIS PROPOSAL IS TO USE THE LINE EMISSION FROM SECONDARY FE-PEAK ELEMENTS IN SUZAKU SPECTRA OF TYPE IA SUPERNOVA REMNANTS (SNRS) TO CONSTRAIN THE PHYSICS OF TYPE IA SUPERNOVAE (IA SNE) AND THE NATURE OF THEIR PROGENITORS. WE WILL RE-ANALYZE THE EXTANT SAMPLE OF SUZAKU OBSERVATIONS OF TYPE IA SNRS WITH PROMINENT FE K-SHELL LINES AND SEARCH FOR EMISSION FROM MN CR AND NI. WE WILL USE LINE FLUXES AND UPPER LIMITS FROM THESE ELEMENTS TO DETERMINE THE REGIME OF THERMONUCLEAR COMBUSTION THAT SYNTHESIZED THE X-RAY EMITTING FE-GROUP EJECTA AND MEASURE THE NEUTRON EXCESS OF THE SN PROGENITORS WHICH IS CLOSELY RELATED TO THEIR METALLICITY. KNOWLEDGE OF THE COMBUSTION REGIME AND PROGENITOR METALLICITY CAN BE USED TO DETERMINE THE MASS OF THE EXPLODING WHITE DWARF ESTIMATE THE AGE OF THE PROGENITOR SYSTEMS AND VALIDATE SPECIFIC PROGENITOR EVOLUTION SCENARIOS. OUR WORK WILL YIELD THE FIRST SAMPLE OF METALLICITIES AND AGES FOR SN IA PROGENITORS IN DIFFERENT ENVIRONMENTS A UNIQUE MEASUREMENT THAT CAN ONLY BE PERFORMED WITH THE SUZAKU DATA SET. $43.2k 11/27/17