S. Bisterzo

Istituto Nazionale di Fisica Nucleare — Italy

Physics and Astronomy · Physical Sciences

30h-index3.3kcitations110works0.02yr avg
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Research Topics

Stellar, planetary, and galactic studies(55), Astro and Planetary Science(46), Nuclear physics research studies(35), Nuclear Physics and Applications(29), Astronomy and Astrophysical Research(22)

Publications110 total

Enrichment of the Galactic disc with neutron capture elements: Sr
Monthly Notices of the Royal Astronomical Society·2019· 19 citedOpen Access
Corrigendum to “Simultaneous iron and nickel isotopic analyses of presolar silicon carbide grains” [Geochim. Cosmochim. Acta 221 (2018) 87–108]
Geochimica et Cosmochimica Acta·2018
VizieR Online Data Catalog: Solar s-process contributions with GCE model (Bisterzo+, 2014)
VizieR Online Data Catalog·2017
Simultaneous iron and nickel isotopic analyses of presolar silicon carbide grains
Geochimica et Cosmochimica Acta·2017· 36 citedOpen Access
Observing the metal-poor solar neighbourhood: a comparison of galactic chemical evolution predictions*†
Monthly Notices of the Royal Astronomical Society·2017· 30 citedOpen Access
Stellar Parameters, Chemical composition and Models of chemical evolution
Proceedings of the International Astronomical Union·2017
Neutron spectroscopy of 26Mg states: Constraining the stellar neutron source 22Ne(α,n)25Mg
Physics Letters B·2017· 45 citedOpen Access
Stellar (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>n</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi></mml:mrow></mml:math>) cross sections of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="bold">Na</mml:mi><mml:mprescripts/><mml:none/><mml:mn>23</mml:mn></mml:mmultiscripts></mml:math>
Physical review. C·2017· 9 citedOpen Access
GALACTIC CHEMICAL EVOLUTION: THE IMPACT OF THE <sup>13</sup>C-POCKET STRUCTURE ON THE s-PROCESS DISTRIBUTION
The Astrophysical Journal·2017· 57 citedOpen Access
Neutron spectroscopy of $^{26}$Mg states: constraining the stellar neutron source $^{22}$Ne($α, n$)$^{25}$Mg
Repository KITopen (Karlsruhe Institute of Technology)·2017Open Access
Stellar (n,.GAMMA.) cross sections of 23Na
Physical Review. C. Covering Nuclear Physics·2017
Mass and metallicity requirement in stellar models for galactic chemical evolution applications
Monthly Notices of the Royal Astronomical Society·2016· 34 citedOpen Access
Iron and Nickel Isotopic Compositions of Presolar Silicon Carbide Grains from AGB Stars Measured with CHILI
79th Annual Meeting of the Meteoritical Society·2016· 1 cited
Stellar neutron capture cross sections of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">K</mml:mi><mml:mrow/></mml:mrow><mml:mprescripts/><mml:none/><mml:mn>41</mml:mn></mml:mmultiscripts></mml:math>and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Sc</mml:mi><mml:mprescripts/><mml:none/><mml:mn>45</mml:mn></mml:mmultiscripts></mml:math>
Physical review. C·2016· 2 citedOpen Access
Probing astrophysically important states in the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Mg</mml:mi><mml:mprescripts/><mml:none/><mml:mn>26</mml:mn></mml:mmultiscripts></mml:math>nucleus to study neutron sources for the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>s</mml:mi></mml:math>process
Physical review. C·2016· 47 citedOpen Access
AGB yields and Galactic Chemical Evolution: last updated
Journal of Physics Conference Series·2016· 16 citedOpen Access
GCE AND SOLAR S-PROCESS ABUNDANCES: DEPENDENCE ON THE 13C-POCKET STRUCTURE
Proceedings of XIII Nuclei in the Cosmos — PoS(NIC XIII)·2015· 1 citedOpen Access
The 13C-pockets in AGB stars and their fingerprints in mainstream SiC grains
Proceedings of XIII Nuclei in the Cosmos — PoS(NIC XIII)·2015Open Access
Erratum: Stellar neutron capture cross sections of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">Ne</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>20</mml:mn><mml:mo>,</mml:mo><mml:mn>21</mml:mn><mml:mo>,</mml:mo><mml:mn>22</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>[Phys. Rev. C<b>90</b>, 045804 (2014)]
Physical Review C·2015Open Access
The branchings of the main s-process: their sensitivity to α-induced reactions on 13C and 22Ne and to the uncertainties of the nuclear network
Monthly Notices of the Royal Astronomical Society·2015· 101 citedOpen Access
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Frequent Co-authors

R. Gallino(42), F. Käppeler(25), M. Heil(15), A. Mengoni(15), M. Pignatari(14), C. Domingo‐Pardo(14), N. Colonna(13), J. Andrzejewski(13), F. Bečvář(13), E. Berthoumieux(13), F. Calviño(13), D. Cano‐Ott(13), G. Cortés(13), F. Gunsing(12), U. Abbondanno(12), G. Aerts(12), F. Álvarez‐Velarde(12), S. Andriamonje(12), G. Badurek(12), R. Capote(12)