BEGIN:VCALENDAR VERSION:2.0 PRODID:-//Plone.org//NONSGML plone.app.event//EN X-WR-TIMEZONE:Europe/Paris BEGIN:VEVENT SUMMARY:Period 4 main event DTSTART;VALUE=DATE:20200903 DTEND;VALUE=DATE:20200905 DTSTAMP;VALUE=DATE-TIME:20201230T131542Z UID:de3ea0afb63a4a0e8a37202f009c129d CONTACT:Raphael Hirschi\, r.hirschi@keele.ac.uk\, https://indico.cern.ch/e vent/942248/program CREATED;VALUE=DATE-TIME:20200825T170558Z DESCRIPTION:The ChETEC COST Action started in 2017 and is now in its fourt h year/period. In this meeting\, we will cover all the aspects of our Acti on and review all the achievements of the Action during the first three pe riods as well as plan period 4 and the future beyond the end of the Action . LAST-MODIFIED;VALUE=DATE-TIME:20200825T170613Z LOCATION:Virtual event (initially planned in Split) URL:http://www.chetec.eu/events/period-4-main-event END:VEVENT BEGIN:VEVENT SUMMARY:Zagreb Nucleosynthesis software pipeline training school DTSTART;VALUE=DATE:20200831 DTEND;VALUE=DATE:20200903 DTSTAMP;VALUE=DATE-TIME:20201230T131542Z UID:4770860e4d7441a4876281ffe1fde282 CONTACT:Raphael Hirschi\, r.hirschi@keele.ac.uk\, https://indico.cern.ch/e vent/937375/ CREATED;VALUE=DATE-TIME:20200825T170330Z DESCRIPTION:The ChETEC COST Action (CA16117)\, the IReNA NSF network of ne tworks\, and the NuGrid collaboration are organising a 3-day training scho ol event on the topic of nuclear reaction rates\, stellar nucleosynthesis\ , observations and implications for galactic chemical evolution. LAST-MODIFIED;VALUE=DATE-TIME:20200825T170340Z LOCATION:Virtual event (initially planned in Zagreb) URL:http://www.chetec.eu/events/zagreb-nucleosynthesis-software-pipeline-t raining-school END:VEVENT BEGIN:VEVENT SUMMARY:Reaction rates and stellar modelling affecting the 26 Al abundance in the Galaxy. (10-11 March\, 2020. York\, UK) DTSTART;TZID=Europe/Paris;VALUE=DATE-TIME:20200310T090000 DTEND;TZID=Europe/Paris;VALUE=DATE-TIME:20200311T130000 DTSTAMP;VALUE=DATE-TIME:20201230T131542Z UID:96203b454fbc4681804297a14ce25aae CONTACT:Alison Laird\, alison.laird@york.ac.uk CREATED;VALUE=DATE-TIME:20200120T143634Z LAST-MODIFIED;VALUE=DATE-TIME:20200128T164451Z LOCATION:York\, UK URL:http://www.chetec.eu/events/reaction-rates-and-stellar-modelling-affec ting-the-26-al-abundance-in-the-galaxy END:VEVENT BEGIN:VEVENT SUMMARY:Training School - Direct nuclear reaction methods. (19-21 February \, 2020. Orsay\, Paris\, France) DTSTART;TZID=Europe/Paris;VALUE=DATE-TIME:20200219T090000 DTEND;TZID=Europe/Paris;VALUE=DATE-TIME:20200221T170000 DTSTAMP;VALUE=DATE-TIME:20201230T131542Z UID:c901b4e4f18e4641b42e5ac392ae08ba CONTACT:Hammache Fairouz\, hammache@ipno.in2p3.fr CREATED;VALUE=DATE-TIME:20200120T143243Z DESCRIPTION:Various nuclear reaction methods such as transfer reactions at energies above or near the Coulomb barrier\, charge-exchange reactions\, ...etc\, are used to analyze experimental data and determine cross-section s or reaction rates of astrophysical interest. The theoretical formalism u sed goes from DWBA theory (Distorded wave born approximation) to coupled c hannels calculations (CRC\, CCBA\, CDCC\,...). An accurate and efficient u se of the reaction codes (e.g.FRESCO) to perform the aforementioned calcul ations require an understanding and a practical knowledge of the underlyin g concepts. For this purpose\, a four-day training school on direct nuclea r reaction methods will be organized in the winter of 2020 at IPN-Orsay (F rance). The speakers will first give lectures on the principles of direct nuclear reaction methods. Then\, they will show the students how to perfor m DWBA and coupled channel calculations using various codes\, such as FRES CO\, using specific practical examples. LAST-MODIFIED;VALUE=DATE-TIME:20200128T164401Z LOCATION:IPN-Orsay\, Paris\, France URL:http://www.chetec.eu/events/training-school-direct-nuclear-reaction-me thods END:VEVENT BEGIN:VEVENT SUMMARY:Extended Core Team Meeting and Dissemination Workshop. (3-6 Februa ry 2020. Barcelona\, Spain) DTSTART;VALUE=DATE:20200203 DTEND;VALUE=DATE:20200207 DTSTAMP;VALUE=DATE-TIME:20201230T131542Z UID:fcdd3fafd7c64374922eef4df8056878 CONTACT:Jordi Jose\, jordi.jose@upc.edu CREATED;VALUE=DATE-TIME:20200120T125929Z LAST-MODIFIED;VALUE=DATE-TIME:20200128T164543Z LOCATION:Barcelona\, Spain URL:http://www.chetec.eu/events/extended-core-team-meeting-and-disseminati on-workshop-barcelona-spain END:VEVENT BEGIN:VEVENT SUMMARY:Lithium in the Universe: to Be or not to Be? (Working Group Meetin g)\; (18-22 November\, 2019. Rome\, Italy) DTSTART;VALUE=DATE:20191118 DTEND;VALUE=DATE:20191123 DTSTAMP;VALUE=DATE-TIME:20201230T131542Z UID:bcc694ebc1a049e8a2cb8977d343a851 ATTENDEE;CN="INVITED SPEAKERS -";ROLE=REQ-PARTICIPANT:INVITED SPEAKERS - ATTENDEE;CN="Jerome Bouvier, ";ROLE=REQ-PARTICIPANT:Jerome Bouvier, ATTENDEE;CN="Sergio Cristallo, ";ROLE=REQ-PARTICIPANT:Sergio Cristallo , ATTENDEE;CN="Franca D’Antona, ";ROLE=REQ-PARTICIPANT:Franca D’Anton a, ATTENDEE;CN="Barry Davids, ";ROLE=REQ-PARTICIPANT:Barry Davids, ATTENDEE;CN="Brian Fields, ";ROLE=REQ-PARTICIPANT:Brian Fields, ATTENDEE;CN="Anibal Garcia-Hernandez, ";ROLE=REQ-PARTICIPANT:Anibal Garci a-Hernandez, ATTENDEE;CN="Nadege Lagarde, ";ROLE=REQ-PARTICIPANT:Nadeg e Lagarde, ATTENDEE;CN="Karin Lind, ";ROLE=REQ-PARTICIPANT :Karin Lind, ATTENDEE;CN="Jordi Jose, ";ROLE=REQ-PARTICIPA NT:Jordi Jose, ATTENDEE;CN="Francesca Matteucci, ";ROLE=REQ-PARTICIPANT:Frances ca Matteucci, ATTENDEE;CN="Jorge Melendez, ";ROLE=REQ-PARTICIPANT:Jor ge Melendez, ATTENDEE;CN="Paolo Molaro, ";ROLE=REQ-PARTICIPANT:P aolo Molaro, ATTENDEE;CN="Cyril Pitrou, ";ROLE=REQ-PARTICIPAN T:Cyril Pitrou, ATTENDEE;CN="Rafael Rebolo, ";ROLE=REQ-PARTICIPANT: Rafael Rebolo, ATTENDEE;CN="Matthias Steffen, ";ROLE=REQ-PARTICIPANT:Mat thias Steffen, ATTENDEE;CN="Aaron Steinhauer, ";ROLE=REQ-PARTICIPANT:Aaro n Steinhauer, ATTENDEE;CN="Rodolfo Smiljanic, ";ROLE=REQ-PARTICIPANT:Rodolfo Smiljanic, ATTENDEE;CN="Bruce Twarog ";ROLE=REQ-PARTICIPANT:Bruce Twa rog ATTENDEE;CN=;ROLE=REQ-PARTICIPANT: ATTENDEE;CN="- SOC -";ROLE=REQ-PARTICIPANT:- SOC - ATTENDEE;CN=;ROLE=REQ-PARTICIPANT: ATTENDEE;CN=" Gabriele Cescutti, ";ROLE=REQ-PARTICIPANT: Gabri ele Cescutti, ATTENDEE;CN=" Alain Coc, ";ROLE=REQ-PARTICIPANT: Alain Coc, ATTENDEE;CN=" Constantin Deliyannis,";ROLE=REQ-PARTICIPANT: Constantin Deliyannis, ATTENDEE;CN=" Margarita Hernanz, ";ROLE=REQ-PARTICIPANT: Margarit a Hernanz, ATTENDEE;CN=" Christian Iliaidis, ";ROLE=REQ-PARTICIPANT: Ch ristian Iliaidis, ATTENDEE;CN=" Andreas Korn (co-chair), ";ROLE=REQ-PARTICIPANT: Andreas Korn (co-chair), ATTENDEE;CN=" Karin Lind, ";ROLE=REQ-PARTICIPANT : Karin Lind, ATTENDEE;CN=" Ana Palacios, ";ROLE=REQ-PARTICIPANT: Ana Palacios, ATTENDEE;CN=" Paolo Ventura (co-chair), ";ROLE=REQ-PARTICIPANT: Paolo Ventura (co-chair), ATTENDEE;CN=" Maria Rosa Zapatero-Osorio ";ROLE=REQ-PARTICIPANT: Maria Rosa Zapatero-Osorio ATTENDEE;CN=;ROLE=REQ-PARTICIPANT: ATTENDEE;CN="- LOC -";ROLE=REQ-PARTICIPANT:- LOC - ATTENDEE;CN="Giuliana Giobbi (chair), ";ROLE=REQ-PARTICIPANT :Giuliana Giobbi (chair), ATTENDEE;CN="Marco Castellani, ";ROLE=REQ-PARTICIPA NT:Marco Castellani, ATTENDEE;CN="Flavia Dell'Agli, ";ROLE=REQ-PART ICIPANT:Flavia Dell'Agli, ATTENDEE;CN="Marcella Di Criscienzo, ";ROLE=REQ-PARTICIPANT:M arcella Di Criscienzo, ATTENDEE;CN="Maria Lugaro, ";ROLE=REQ-PARTIC IPANT:Maria Lugaro, ATTENDEE;CN="Ester Marini, ";ROLE=REQ-PARTI CIPANT:Ester Marini, ATTENDEE;CN="Vincenzo Testa ";ROLE=REQ-PARTICIPANT :Vincenzo Testa ATTENDEE;CN="- For an updated list of the participants: ";ROLE=REQ-PARTICI PANT:- For an updated list of the participants: ATTENDEE;CN="https://lithiumintheuniverse.wixsite.com/lithium2019/partecip ants";ROLE=REQ-PARTICIPANT:https://lithiumintheuniverse.wixsite.com/lithiu m2019/partecipants CONTACT:Gabriele Cescutti and Paolo Ventura\, cescutti.gabriele@gmail.com / paolo.ventura@oa-roma.inaf.it\, https://lithiumintheuniverse.wixsite.com /lithium2019 CREATED;VALUE=DATE-TIME:20190611T161435Z DESCRIPTION:Among all the chemical species present in the Universe\, lithi um is unique for being the protagonist in several astrophysical contexts\, spanning all epochs\, from the Big Bang to the present day\, and extendin g over distances from our Sun to remote regions in the Milky Way system an d beyond. Lithium is currently at the centre of two highly debated mys teries that catch the attention of astrophysicists. The expected primordia l value of 7Li is a factor of 3 higher than measured in warm halo dwarf st ars. This discrepancy is normally referred to as the cosmological lithium problem. Since the present lithium abundance as measured in meteorites or in young stars is A(Li)=3.3\, a Galactic source is required. The identifi cation of such sources is referred to as the Galactic lithium problem. LAST-MODIFIED;VALUE=DATE-TIME:20200128T164631Z LOCATION:The Observatory of Rome\, Monte Porzio Catone\, Italy URL:http://www.chetec.eu/events/lithium-in-the-universe-to-be-or-not-to-be -working-group-meeting END:VEVENT BEGIN:VEVENT SUMMARY:ChETEC follow-up in Horizon 2020 and Horizon Europe Programmes. (1 1-12 November 2019. Dresden\, Germany) DTSTART;TZID=Europe/Paris;VALUE=DATE-TIME:20191111T133000 DTEND;TZID=Europe/Paris;VALUE=DATE-TIME:20191112T123000 DTSTAMP;VALUE=DATE-TIME:20201230T131542Z UID:6761c1247b454ebc9a8f274507b1b1f5 ATTENDEE;CN="Aldo Serenelli; Andreas Korn; Arunas Kucinskas; Camilla Hanse n; Daniel Bemmerer; Felix Heim; Kathrin; Göbel; Livius; Trache; Maria Pet o; Raphael Hirschi; Richard Stancliffe; Rosanna Depalo; Tobias Fischer; Z solt Fülöp";ROLE=REQ-PARTICIPANT:Aldo Serenelli; Andreas Korn; Arunas Ku cinskas; Camilla Hansen; Daniel Bemmerer; Felix Heim; Kathrin; Göbel; Liv ius; Trache; Maria Peto; Raphael Hirschi; Richard Stancliffe; Rosanna Depa lo; Tobias Fischer; Zsolt Fülöp CONTACT:Daniel Bemmerer\, Daniel Bemmerer \, https://w ww.hzdr.de/db/Cms?pNid=874 CREATED;VALUE=DATE-TIME:20191022T093614Z LAST-MODIFIED;VALUE=DATE-TIME:20200616T072155Z LOCATION:Helmholtz-Zentrum Dresden-Rossendorf (HZDR)\, Bautzner Landstr. 4 00\, 01328 Dresden\, Germany\, Building 620\, room 021 (Klei) URL:http://www.chetec.eu/events/chetec-follow-up-in-horizon-2020-and-horiz on-europe-programmes-1 END:VEVENT BEGIN:VEVENT SUMMARY:MC meeting and Knowledge transfer workshop (Management Committee a nd Working Group Meetings). (September 18\, 2019. Frankfurt\, Germany) DTSTART;VALUE=DATE:20190918 DTEND;VALUE=DATE:20190919 DTSTAMP;VALUE=DATE-TIME:20201230T131543Z UID:3d73dde5d6f541bb8f1bf26ca3d039f2 ATTENDEE;CN="Aleksandra Cvetinovic; Alessandra Guglielmetti; Alison Laird; Andreas Korn; Ann-Cecilie Larsen; Anu Kankainen; Arūnas Kučinskas; Bran kica Kubátová; Camilla Juul Hansen; Daniel Bemmerer; Daniel Galaviz Redo ndo; Jerome Guilet; João Cruz; Livius Trache; Maria Lugaro; Maria Yavahch ova; Nalan Özkan Güray; Neven Soic; Pierre Descouvemont; Raphael Hirschi ; Robin Golser; Roland Diehl; Zsolt Fulop; György Gyürky; Konrad Schmidt ; Heinrich Wilsenach; Benoit Côté; Antonio Caciolli; Igor Gasparic; Frie drich-Karl Thielemann";ROLE=REQ-PARTICIPANT:Aleksandra Cvetinovic; Alessan dra Guglielmetti; Alison Laird; Andreas Korn; Ann-Cecilie Larsen; Anu Kank ainen; Arūnas Kučinskas; Brankica Kubátová; Camilla Juul Hansen; Danie l Bemmerer; Daniel Galaviz Redondo; Jerome Guilet; João Cruz; Livius Trac he; Maria Lugaro; Maria Yavahchova; Nalan Özkan Güray; Neven Soic; Pierr e Descouvemont; Raphael Hirschi; Robin Golser; Roland Diehl; Zsolt Fulop; György Gyürky; Konrad Schmidt; Heinrich Wilsenach; Benoit Côté; Antoni o Caciolli; Igor Gasparic; Friedrich-Karl Thielemann CONTACT:Raphael Hirschi and Rene Reifarth\, r.hirschi@keele.ac.uk / reifa rth@physik.uni-frankfurt.de CREATED;VALUE=DATE-TIME:20190611T161102Z LAST-MODIFIED;VALUE=DATE-TIME:20200128T164748Z LOCATION:Frankfurt\, Germany URL:http://www.chetec.eu/events/mc-meeting-and-knowledge-transfer-workshop -management-committee-and-working-group-meetings END:VEVENT BEGIN:VEVENT SUMMARY:CEMP Stars as Probes of First-Star Nucleosynthesis\, the IMF\, and Galactic Assembly (Working Group Meeting). (9-13 September\, Geneve\, Swi tzerland) DTSTART;VALUE=DATE:20190909 DTEND;VALUE=DATE:20190914 DTSTAMP;VALUE=DATE-TIME:20201230T131543Z UID:6a054df06c814837afde39afce5da7dd ATTENDEE;CN="Aldo Mura-Guzman The Australian National University ";ROLE= REQ-PARTICIPANT:Aldo Mura-Guzman The Australian National University ATTENDEE;CN="André Maeder Geneva Observatory ";ROLE=REQ-PARTICIPANT:And ré Maeder Geneva Observatory ATTENDEE;CN="Anish Amarsi Max Planck Institute for Astronomy ";ROLE=REQ- PARTICIPANT:Anish Amarsi Max Planck Institute for Astronomy ATTENDEE;CN="Anke Arentsen Leibniz-Institut für Astrophysik Potsdam ";R OLE=REQ-PARTICIPANT:Anke Arentsen Leibniz-Institut für Astrophysik Pots dam ATTENDEE;CN="Anne Verhamme anne.verhamme@unige.ch ";ROLE=REQ-PARTICIPANT :Anne Verhamme anne.verhamme@unige.ch ATTENDEE;CN=;ROLE=REQ-PARTICIPANT: ATTENDEE;CN="Arthur Choplin Konan University ";ROLE=REQ-PARTICIPANT:Arth ur Choplin Konan University ATTENDEE;CN="Arūnas Kučinskas Vilnius University, Lithuania ";ROLE=REQ -PARTICIPANT:Arūnas Kučinskas Vilnius University, Lithuania ATTENDEE;CN="Asa Skuladottir MPIA, Heidelberg ";ROLE=REQ-PARTICIPANT:Asa Skuladottir MPIA, Heidelberg ATTENDEE;CN="Avrajit Bandyopadhyay Indian Institute of Astrophysics, Ban galore ";ROLE=REQ-PARTICIPANT:Avrajit Bandyopadhyay Indian Institute of Astrophysics, Bangalore ATTENDEE;CN="Beatriz Barbuy Universidade de São Paulo ";ROLE=REQ-PARTIC IPANT:Beatriz Barbuy Universidade de São Paulo ATTENDEE;CN="Bing Du ";ROLE=REQ-PARTICIPANT:Bing Du ATTENDEE;CN="Birgitta Nordstrom Niels Bohr Institute, Copenhagen Univers ity, Denmark ";ROLE=REQ-PARTICIPANT:Birgitta Nordstrom Niels Bohr Instit ute, Copenhagen University, Denmark ATTENDEE;CN="Camilla Juul Hansen MPIA ";ROLE=REQ-PARTICIPANT:Camilla Juu l Hansen MPIA ATTENDEE;CN="Chiaki Kobayashi University of Hertfordshire ";ROLE=REQ-PAR TICIPANT:Chiaki Kobayashi University of Hertfordshire ATTENDEE;CN="Cristina Chiappini Leibniz Institute for Astrophysics Potsd am - AIP ";ROLE=REQ-PARTICIPANT:Cristina Chiappini Leibniz Institute for Astrophysics Potsdam - AIP ATTENDEE;CN="David Aguado University of Cambridge ";ROLE=REQ-PARTICIPANT :David Aguado University of Cambridge ATTENDEE;CN="David Yong Australian National University ";ROLE=REQ-PARTIC IPANT:David Yong Australian National University ATTENDEE;CN="Devin Whitten University of Notre Dame ";ROLE=REQ-PARTICIPA NT:Devin Whitten University of Notre Dame ATTENDEE;CN="Dogus Ozuyar Ankara University ";ROLE=REQ-PARTICIPANT:Dogus Ozuyar Ankara University ATTENDEE;CN="Else Starkenburg Leibniz Institute for Astrophysics Potsdam ";ROLE=REQ-PARTICIPANT:Else Starkenburg Leibniz Institute for Astrophys ics Potsdam ATTENDEE;CN="Falk Herwig University of Victoria ";ROLE=REQ-PARTICIPANT:F alk Herwig University of Victoria ATTENDEE;CN="Federico Sestito Observatoire Astronomique de Strasbourg "; ROLE=REQ-PARTICIPANT:Federico Sestito Observatoire Astronomique de Stras bourg ATTENDEE;CN="Friedrich Thielemann University of Basel and GSI Darmstadt ";ROLE=REQ-PARTICIPANT:Friedrich Thielemann University of Basel and GSI Darmstadt ATTENDEE;CN="Gabriele Cescutti I.N.A.F. Osservatorio Astronomico di Trie ste ";ROLE=REQ-PARTICIPANT:Gabriele Cescutti I.N.A.F. Osservatorio Astro nomico di Trieste ATTENDEE;CN="Gaël Buldgen University of Geneva ";ROLE=REQ-PARTICIPANT:G aël Buldgen University of Geneva ATTENDEE;CN="Georges Meynet Université de Genève ";ROLE=REQ-PARTICIPAN T:Georges Meynet Université de Genève ATTENDEE;CN="Jiannan Zhang NAOC ";ROLE=REQ-PARTICIPANT:Jiannan Zhang N AOC ATTENDEE;CN="Jinmi Yoon University of Notre Dame ";ROLE=REQ-PARTICIPANT: Jinmi Yoon University of Notre Dame ATTENDEE;CN="John Wise Georgia Institute of Technology ";ROLE=REQ-PARTIC IPANT:John Wise Georgia Institute of Technology ATTENDEE;CN="Joseph Zepeda University of Notre Dames ";ROLE=REQ-PARTICIP ANT:Joseph Zepeda University of Notre Dames ATTENDEE;CN="Kaitlin Rasmussen University of Notre Dame ";ROLE=REQ-PARTI CIPANT:Kaitlin Rasmussen University of Notre Dame ATTENDEE;CN="Krishna Choudhury University of Calcutta ";ROLE=REQ-PARTICI PANT:Krishna Choudhury University of Calcutta ATTENDEE;CN="kwame appiah ghana atomic energy commission ";ROLE=REQ-PART ICIPANT:kwame appiah ghana atomic energy commission ATTENDEE;CN="Laura Murphy Trinity College Dublin ";ROLE=REQ-PARTICIPANT: Laura Murphy Trinity College Dublin ATTENDEE;CN="Leah Cox ";ROLE=REQ-PARTICIPANT:Leah Cox ATTENDEE;CN="Lionel Haemmerlé Université de Genève ";ROLE=REQ-PARTICI PANT:Lionel Haemmerlé Université de Genève ATTENDEE;CN="Mahavir Sharma ICRAR, Curtin University ";ROLE=REQ-PARTICIP ANT:Mahavir Sharma ICRAR, Curtin University ATTENDEE;CN="Mattis Magg Insitute for Theoretical Astrophysics, Universi ty of Heidelberg ";ROLE=REQ-PARTICIPANT:Mattis Magg Insitute for Theoret ical Astrophysics, University of Heidelberg ATTENDEE;CN="Mohammad Mardini National Astronomical Observatories of Chi na ";ROLE=REQ-PARTICIPANT:Mohammad Mardini National Astronomical Observa tories of China ATTENDEE;CN="Myoungwon Jeon Kyung Hee University ";ROLE=REQ-PARTICIPANT: Myoungwon Jeon Kyung Hee University ATTENDEE;CN="Nial Tanvir University of Leicester ";ROLE=REQ-PARTICIPANT: Nial Tanvir University of Leicester ATTENDEE;CN="Ondrea Clarkson University of Victoria ";ROLE=REQ-PARTICIPA NT:Ondrea Clarkson University of Victoria ATTENDEE;CN="Piercarlo Bonifacio GEPI, Observatoire de Paris, PSL, CNRS ";ROLE=REQ-PARTICIPANT:Piercarlo Bonifacio GEPI, Observatoire de Paris, PSL, CNRS ATTENDEE;CN="Piyush Sharda Australian National University ";ROLE=REQ-PAR TICIPANT:Piyush Sharda Australian National University ATTENDEE;CN="Rana Ezzeddine Massachusetts Institute of Technology ";ROLE =REQ-PARTICIPANT:Rana Ezzeddine Massachusetts Institute of Technology ATTENDEE;CN="Raphael Hirschi Keele University ";ROLE=REQ-PARTICIPANT:Rap hael Hirschi Keele University ATTENDEE;CN="Roberto Gallino University of Torino(Italy) ";ROLE=REQ-PART ICIPANT:Roberto Gallino University of Torino(Italy) ATTENDEE;CN="Romain Lucchesi EPFL Laboratoire d'astrophysique, ESO ";ROL E=REQ-PARTICIPANT:Romain Lucchesi EPFL Laboratoire d'astrophysique, ESO ATTENDEE;CN="Sarah Dietz University of Notre Dame ";ROLE=REQ-PARTICIPANT :Sarah Dietz University of Notre Dame ATTENDEE;CN="Shingo Hirano Kyushu University ";ROLE=REQ-PARTICIPANT:Shin go Hirano Kyushu University ATTENDEE;CN="Silvia Rossi Universidade de São Paulo/IAG ";ROLE=REQ-PART ICIPANT:Silvia Rossi Universidade de São Paulo/IAG ATTENDEE;CN="stefania salvadori Florence University, Physics and Astrono my Department ";ROLE=REQ-PARTICIPANT:stefania salvadori Florence Univers ity, Physics and Astronomy Department ATTENDEE;CN="Susmitha Rani Antony Tata Institute of Fundamental Research , Mumbai, India ";ROLE=REQ-PARTICIPANT:Susmitha Rani Antony Tata Institu te of Fundamental Research, Mumbai, India ATTENDEE;CN="Sutirtha Sengupta Department of Applied Mathematics, UC San ta Cruz ";ROLE=REQ-PARTICIPANT:Sutirtha Sengupta Department of Applied M athematics, UC Santa Cruz ATTENDEE;CN="Sylvia Ekström Geneva University ";ROLE=REQ-PARTICIPANT:Sy lvia Ekström Geneva University ATTENDEE;CN="Sébastien Martinet University of Geneva ";ROLE=REQ-PARTICI PANT:Sébastien Martinet University of Geneva ATTENDEE;CN="Tadafumi Matsuno NAOJ/SOKENDAI ";ROLE=REQ-PARTICIPANT:Tadaf umi Matsuno NAOJ/SOKENDAI ATTENDEE;CN="Tejpreet Kaur Panjab University, Chandigarh ";ROLE=REQ-PART ICIPANT:Tejpreet Kaur Panjab University, Chandigarh ATTENDEE;CN="Theodora Xylakis-Dornbusch ZAH/LSW University of Heidelberg ";ROLE=REQ-PARTICIPANT:Theodora Xylakis-Dornbusch ZAH/LSW University of Heidelberg ATTENDEE;CN="Thomas Nordlander Australian National University ";ROLE=REQ -PARTICIPANT:Thomas Nordlander Australian National University ATTENDEE;CN="Tilman Hartwig University of Tokyo ";ROLE=REQ-PARTICIPANT:T ilman Hartwig University of Tokyo ATTENDEE;CN="Timothy Beers University of Notre Dame ";ROLE=REQ-PARTICIPA NT:Timothy Beers University of Notre Dame ATTENDEE;CN="Vanessa Hill UCA, Observatoire de la Côte d'Azur, CNRS, La boratoire Lagrange ";ROLE=REQ-PARTICIPANT:Vanessa Hill UCA, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange ATTENDEE;CN="Vinicius Placco University of Notre Dame ";ROLE=REQ-PARTICI PANT:Vinicius Placco University of Notre Dame ATTENDEE;CN="Volker Bromm University of Texas at Austin ";ROLE=REQ-PARTI CIPANT:Volker Bromm University of Texas at Austin ATTENDEE;CN="Wei-Ting Liao University of Illinois at Urbana-Champaign "; ROLE=REQ-PARTICIPANT:Wei-Ting Liao University of Illinois at Urbana-Cham paign ATTENDEE;CN="Zhen Yuan Shanghai Astronomical Observatory ";ROLE=REQ-PART ICIPANT:Zhen Yuan Shanghai Astronomical Observatory ATTENDEE;CN="Şeyma Çalışkan Ankara University";ROLE=REQ-PARTICIPANT: Şeyma Çalışkan Ankara University ATTENDEE;CN=;ROLE=REQ-PARTICIPANT: CONTACT:Georges Meynet and Timothy Beers\, +41 22 379 23 98\, georges.meyn et@unige.ch / tbeers@nd.edu\, https://indico.cern.ch/event/791509/overvi ew CREATED;VALUE=DATE-TIME:20190611T160456Z DESCRIPTION:The beginning of the stellar era in the Universe is a singular ly fascinating phase in the history of the Cosmos. The baryonic material f illing the Universe at that time\, having a composition inherited from Big Bang nucleosynthesis\, has its physical characteristics modified by the v ery first stars. Indeed\, the first stars will change the degree of ionize d material in their vicinity\, and\, through their winds and/or supernova explosion\, will inject energy\, momentum\, and newly-synthesized elements . Some pockets of gas\, enriched by the first stars\, will in turn form ne w stars\, whose initial composition is inherited from the first nucleosynt hetic events. These low-mass stars can live sufficiently long to be observ ed today in halo of the Galaxy\, providing the opportunity to obtain infor mation about the very high redshift Universe by the study of nearby stars. How did these processes happen? How were these processes different from similar ones occurring in the present Universe? What can they teach us ab out the infancy of the Universe during the reionization era? These are the questions that will be discussed during this workshop\, questions that ar e particularly topical at a time when new facilities\, such as SKA\, JWST\ , and the next generation of extremely large telescopes have as one of the ir prime objectives to probe this very period. At present\, observation al constraints on these first stars are scarce and/or indirect. Important constraints come from observations of the elemental abundances of very\, e xtremely\, and ultra iron-poor stars that likely formed from the ejecta of the first stellar generations. Of course the full story can be complex\, as some elements might be formed by more than one source\, and others may be somewhat altered by in-situ processes that occurred in the star that is observed today. Nevertheless\, through the accumulation of observational data\, progress made in numerical simulations\, and in our deeper understa nding of the physical processes involved\, a much more complete and detail ed story can be told. LAST-MODIFIED;VALUE=DATE-TIME:20200128T164843Z LOCATION:Geneva University\, 30 quai Ernest Ansermet in Auditorium A100 Sc iences II URL:http://www.chetec.eu/events/cemp-stars-as-probes-of-first-star-nucleos ynthesis-the-imf-and-galactic-assembly-working-group-meeting END:VEVENT BEGIN:VEVENT SUMMARY:Microphysics in Computational Relativistic Astrophysics. (12-16 Au gust\, 2019. Jena\, Germany) DTSTART;TZID=Europe/Paris;VALUE=DATE-TIME:20190812T090000 DTEND;TZID=Europe/Paris;VALUE=DATE-TIME:20190816T170000 DTSTAMP;VALUE=DATE-TIME:20201230T131543Z UID:cdcf7acf45b0491d8333a85052e6c0be CONTACT:Sebastiano Bernuzzi\, sebastiano.bernuzzi@uni-jena.de CREATED;VALUE=DATE-TIME:20200120T152400Z DESCRIPTION:MICRA is a workshop (and emphatically not a conference) that h eavily focuses the microphysics needs of computational simulations of astr ophysical systems\, neutrinos\, nucleosynthesis\, and nuclear density equa tions of state. The intention is to bring together active nuclear and neut rino theorists and astrophysicists with computational modelers to achieve improvements in the modeling of relativistic systems: stellar collapse\, c ore-collapse supernovae (CCSNe)\, binary mergers\, and gamma-ray bursts. B ased on previous MICRAs\, we envision ~40 participants from across the wor ld\, since this edition of MICRA is hosted in Europe\, we expect at least 50% European participation. LAST-MODIFIED;VALUE=DATE-TIME:20200128T164943Z LOCATION:Theoretisch-Physikalisches Institut at the University of Jena. JE NA\, GERMANY URL:http://www.chetec.eu/events/microphysics-in-computational-relativistic -astrophysics END:VEVENT BEGIN:VEVENT SUMMARY:Electron-Capture-Initiated Stellar Collapse. (20-24 May 2019\, Lei den\, Netherlands) DTSTART;TZID=Europe/Paris;VALUE=DATE-TIME:20190520T090000 DTEND;TZID=Europe/Paris;VALUE=DATE-TIME:20190524T170000 DTSTAMP;VALUE=DATE-TIME:20201230T131543Z UID:ee4da8e028144034a037fbf7d4a86613 ATTENDEE;CN="Dr Carolyn Doherty; Mr Dag Fahlin Strömberg; Dr Alina Istrat e; Prof Gabriel Martinez-Pinedo; Dr Mathieu Renzo; Dr Lionel Siess";ROLE=R EQ-PARTICIPANT:Dr Carolyn Doherty; Mr Dag Fahlin Strömberg; Dr Alina Istr ate; Prof Gabriel Martinez-Pinedo; Dr Mathieu Renzo; Dr Lionel Siess CREATED;VALUE=DATE-TIME:20190607T093522Z DESCRIPTION:One of the primary goals of stellar astrophysics is to connect the initial properties of stars to the remnants they leave behind. The ev olution of the subset of stellar systems that experience a collapse initia ted by electron-capture reactions is rich\, complex and uncertain. \; In particular\, this workshop aims to strengthen our theoretical understan ding of the type and properties of the remnants of electron-capture supern ovae and accretion-induced collapse. LAST-MODIFIED;VALUE=DATE-TIME:20200128T170138Z LOCATION:Lorentz center\, Leiden\, Netherlands URL:http://www.chetec.eu/events/electron-capture-initiated-stellar-collaps e END:VEVENT BEGIN:VEVENT SUMMARY:Nuclear and astrophysics aspects for the rapid neutron capture pro cess in the era of multi-messenger observations. (May 1\, 2019. Trento\, I taly) DTSTART;TZID=Europe/Paris;VALUE=DATE-TIME:20190501T090000 DTEND;TZID=Europe/Paris;VALUE=DATE-TIME:20190501T170000 DTSTAMP;VALUE=DATE-TIME:20201230T131543Z UID:1d46c9ee820041a9b37c0c73b0ffce14 ATTENDEE;CN="Dr Laetitia Canete; Dr Benoit Cote; Dr Marius Eichler; Dr Tob ias Fischer; Mr Stylianos Nikas; Mr Ante Ravlic";ROLE=REQ-PARTICIPANT:Dr L aetitia Canete; Dr Benoit Cote; Dr Marius Eichler; Dr Tobias Fischer; Mr S tylianos Nikas; Mr Ante Ravlic CREATED;VALUE=DATE-TIME:20200120T151926Z DESCRIPTION:The rapid-neutron capture process (r-process) is responsible f or producing around half of all nuclides heavier than iron. One site for t he r-process was recently confirmed: the advanced LIGO and Virgo detectors observed two neutron stars merging and immediate follow-up observations w ere fully compatible with a kilonova\, a thermal “afterglow” powered b y radioactive decay of newly synthesized r-process material. Moreover\, th e observations indicated that neutron-star mergers produce a blue lanthani de-free signal followed by a red lanthanide-rich component\, contrary to e xpectations. Although neutron-star mergers are now known to be r-process e lement factories\, this might not be the only r-process site\, and a compr ehensive understanding and description of the r-process is still lacking. This workshop will bring together theorists and experimentalists to addres s the many aspects of nuclear physics and astrophysics that must be consid ered and properly understood in order to model the r-process. LAST-MODIFIED;VALUE=DATE-TIME:20200128T165028Z LOCATION:ECT* (European Centre for Theoretical Studies in Nuclear Physics and Related Areas). Trento\, Italy URL:http://www.chetec.eu/events/nuclear-and-astrophysics-aspects-for-the-r apid-neutron-capture-process-in-the-era-of-multi-messenger-observations END:VEVENT BEGIN:VEVENT SUMMARY:ChETEC Working Group 3 Workshop 2019. (From February 27 to March 1\, 2019. Vilnius\, Lithuania) DTSTART;TZID=Europe/Paris;VALUE=DATE-TIME:20190227T094000 DTEND;TZID=Europe/Paris;VALUE=DATE-TIME:20190301T130000 DTSTAMP;VALUE=DATE-TIME:20201230T131543Z UID:101030068d7547a7bed68288b5ec9011 CONTACT:Arunas Kucinskas\, Vilnius University\, Lithuania\, arunas.kucinsk as@tfai.vu.lt CREATED;VALUE=DATE-TIME:20190316T142418Z DESCRIPTION:The main goal of the workshop is the preparation of two observ ing proposals aimed to investigate: (a) the origin and evolution of the r- process elements in the EMP stars\; (b) the origin of multiple stellar pop ulations (MPs) in the Galactic globular clusters (GGCs)\; and (c) to excha nge ideas regarding the possible future observing proposals related to the study of EMP stars\, as well as MPs in the GGCs. Several broader review talks will set up the stage for an in-depth discussions of the two observi ng proposals. Separate slots will be reserved for in-depth discussions to plan future observing proposals. The largest fraction of the workshop time will be devoted to hands-on activities for writing the two observing prop osals that will be submitted during the Period 104 call for proposals at E SO (March 2019). The detailed workshop program is provided below. LAST-MODIFIED;VALUE=DATE-TIME:20200128T165333Z LOCATION:National Center for Physical Sciences and Technology\, Vilnius\, Lithuania URL:http://www.chetec.eu/events/chetec-working-group-3-workshop-2019 END:VEVENT BEGIN:VEVENT SUMMARY:Chemical evolution and nucleosynthesis across the Galaxy & Low met allicity s-process. (26-30 November 2018. Heidelberg\, Germany) DTSTART;TZID=Europe/Paris;VALUE=DATE-TIME:20181126T090000 DTEND;TZID=Europe/Paris;VALUE=DATE-TIME:20181130T180000 DTSTAMP;VALUE=DATE-TIME:20201230T131543Z UID:2ca513ad01e94352979035dde356f04a CONTACT:Camilla Juul Hansen\, http://www2.mpia-hd.mpg.de/homes/cenag2018/ CREATED;VALUE=DATE-TIME:20181001T103245Z DESCRIPTION:Conference and satellite workshop (ChETEC) in Heidelberg\, Ger many. Abstract and details can be found on the listed web page. LAST-MODIFIED;VALUE=DATE-TIME:20200128T165531Z LOCATION:Heidelberg URL:http://www.chetec.eu/events/chemical-evolution-and-nucleosynthesis-acr oss-the-galaxy-low-metallicity-s-process END:VEVENT BEGIN:VEVENT SUMMARY:NuGrid/JINA-CEE/ChETEC School: Software Tools for Simulations in N uclear Astrophysics DTSTART;VALUE=DATE:20180917 DTEND;VALUE=DATE:20180920 DTSTAMP;VALUE=DATE-TIME:20201230T131543Z UID:78e934de44974804b8f41526ecbb8693 CONTACT:Marco Pignatari\, m.pignatari@gmail.com CREATED;VALUE=DATE-TIME:20180607T103232Z DESCRIPTION:NuGrid and the EA Milne Centre for Astrophysics in collaborati on organize a 3-day training school event on the topic of nuclear astrophy sics\, the 17th-19st September 2018\, at the University of Hull\, Hull\, U K. LAST-MODIFIED;VALUE=DATE-TIME:20180608T075606Z LOCATION:Hull\, United Kingdom URL:http://www.chetec.eu/activities/training-schools/nugrid-jina-cee-chete c-school-software-tools-for-simulations-in-nuclear-astrophysics END:VEVENT BEGIN:VEVENT SUMMARY:Technological challenges in Nuclear Astrophysics. (13 of September \, 2018. Debrecen\, Hungary) DTSTART;VALUE=DATE:20180913 DTEND;VALUE=DATE:20180914 DTSTAMP;VALUE=DATE-TIME:20201230T131543Z UID:a229f74459ad43dca1d2b7ff3ac4fc5b CONTACT:http://w3.atomki.hu/astro2018/#schedule CREATED;VALUE=DATE-TIME:20180910T154444Z DESCRIPTION:A 1-day meeting discussing the technological challenge in Nucl ear Astrophysics LAST-MODIFIED;VALUE=DATE-TIME:20200128T165657Z LOCATION:Debrecen\, Hungary URL:http://www.chetec.eu/events/technological-challenges-in-nuclear-astrop hysics END:VEVENT BEGIN:VEVENT SUMMARY:Knowledge Hubs workshop + period 2 MC meeting DTSTART;TZID=Europe/Paris;VALUE=DATE-TIME:20180627T123000 DTEND;TZID=Europe/Paris;VALUE=DATE-TIME:20180627T190000 DTSTAMP;VALUE=DATE-TIME:20201230T131543Z UID:f60c3e19bd374b4da53b577d8a0f9931 ATTENDEE;CN="MC members and workshop participants";ROLE=REQ-PARTICIPANT:MC members and workshop participants CONTACT:Raphael Hirschi\, +441782733324\, r.hirschi@keele.ac.uk CREATED;VALUE=DATE-TIME:20180605T111512Z DESCRIPTION:During the workshop\, we will review the "knowledge hubs" that we have assembled and discuss how we can improve them further. After the workshop\, we will have our period(year) 2 MC meeting. LAST-MODIFIED;VALUE=DATE-TIME:20180605T111840Z LOCATION:National Institute for Nuclear Physics - Gran Sasso National Labo ratory URL:http://www.chetec.eu/events/knowledge-hubs-workshop-period-2-mc-meetin g END:VEVENT BEGIN:VEVENT SUMMARY:Training School: "An experiment of Nuclear Physics for Astrophysic s using direct methods" DTSTART;VALUE=DATE:20180410 DTEND;VALUE=DATE:20180422 DTSTAMP;VALUE=DATE-TIME:20201230T131543Z UID:5e42032490bf418e945f7db1718efa33 CONTACT:Livius Trache & Mihai Straticiuc\, +40 21 404 2345\, chetec-school @nipne.ro\, http://www.nipne.ro/indico/conferenceDisplay.py?confId=354 CREATED;VALUE=DATE-TIME:20170627T153633Z LAST-MODIFIED;VALUE=DATE-TIME:20180203T185243Z LOCATION:IFIN-HH (ELI-NP)\, Bucharest\, Romania URL:http://www.chetec.eu/activities/training-schools/training-schools-an-e xperiment-of-nuclear-physics-for-astrophysics-using-direct-methods END:VEVENT BEGIN:VEVENT SUMMARY:ChETEC Working Group 3 Workshop 2018. (14-16 March\, 2018. Vilnius \, Lithuania) DTSTART;TZID=Europe/Paris;VALUE=DATE-TIME:20180314T093000 DTEND;TZID=Europe/Paris;VALUE=DATE-TIME:20180316T170000 DTSTAMP;VALUE=DATE-TIME:20201230T131543Z UID:43ec2e043e7b4016aeb5188ad201cf45 CONTACT:Arunas Kucinskas\, +37068587393\, arunas.kucinskas@tfai.vu.lt\, ht tps://docs.google.com/document/d/1DKDF4RFx4qvxGv9uQXCurVGyntO27jmGLF57NZ-5 NUQ/edit?usp=sharing CREATED;VALUE=DATE-TIME:20180306T145603Z DESCRIPTION:The aim of the meeting is to tackle the following questions: ( a) the preparation of the observing proposal to investigate evolution of E u and Ba in the EMP stars\; (b) discuss and take the necessary actions for the preparation of the Nuclear Astrophysics Database (NAD)\; and (c) disc uss and launch several science projects presented at the Keele meeting in October 2017. It is foreseen that the meeting will be heavily based on d iscussions and interactions. Several talks will set up the stage for an in -depth discussions\, with at least 10-15 min foreseen for questions and di scussion after each talk. Separate slots will be reserved for longer discu ssions to address various important issues in detail and\, ultimately\, to plan further steps and actions. The meeting program is available here: https://docs.google.com/document/d/1DKDF4RFx4qvxGv9uQXCurVGyntO27jmGLF57NZ -5NUQ/edit?usp=sharing LAST-MODIFIED;VALUE=DATE-TIME:20200128T165752Z LOCATION:Vilnius\, Lithuania URL:http://www.chetec.eu/events/chetec-working-group-3-workshop END:VEVENT BEGIN:VEVENT SUMMARY:Main Action Workshop DTSTART;TZID=Europe/Paris;VALUE=DATE-TIME:20171009T140000 DTEND;TZID=Europe/Paris;VALUE=DATE-TIME:20171011T170000 DTSTAMP;VALUE=DATE-TIME:20201230T131543Z UID:9caef9b2e4b848d3a690c8c108ee361f ATTENDEE;CN=tbc;ROLE=REQ-PARTICIPANT:tbc CONTACT:Raphael Hirschi\, 01782 733324\, r.hirschi_AT_keele.ac.uk CREATED;VALUE=DATE-TIME:20170615T100035Z DESCRIPTION:MC meeting + WG workshops LAST-MODIFIED;VALUE=DATE-TIME:20170927T115447Z LOCATION:Keele URL:http://www.chetec.eu/events/main-action-workshop END:VEVENT BEGIN:VEVENT SUMMARY:Training school: "R-matrix calculations for nuclear astrophysics" DTSTART;VALUE=DATE:20170913 DTEND;VALUE=DATE:20170916 DTSTAMP;VALUE=DATE-TIME:20201230T131543Z UID:6218c426e41548bc98d94c09adde096d ATTENDEE;CN="- ADSLEY Philip, IPN Orsay (France) ";ROLE= REQ-PARTICIPANT:- ADSLEY Philip, IPN Orsay (France) ATTENDEE;CN="- ALCINDOR Valérian, GANIL-Caen (France) "; ROLE=REQ-PARTICIPANT:- ALCINDOR Valérian, GANIL-Caen (France) ATTENDEE;CN="- BOWEN Jiang, TU Darmstadt (Germany) ";RO LE=REQ-PARTICIPANT:- BOWEN Jiang, TU Darmstadt (Germany) ATTENDEE;CN="- FRUET Guillaume , IPHC/CNRS Strasbourg (France) "; ROLE=REQ-PARTICIPANT:- FRUET Guillaume , IPHC/CNRS Strasbourg (France) ATTENDEE;CN="- GNECH Alex, Gran Sasso Science Institute (Italy)";ROLE=REQ -PARTICIPANT:- GNECH Alex, Gran Sasso Science Institute (Italy) ATTENDEE;CN="- HUBBARD Nicolas, University of York (United Kingdom) ";ROLE=REQ-PARTICIPANT:- HUBBARD Nicolas, University of York (Uni ted Kingdom) ATTENDEE;CN="- HORNYAK István, University of Debrecen (Hungary) "; ROLE=REQ-PARTICIPANT:- HORNYAK István, University of Debrecen (Hungary) ATTENDEE;CN="- MAUSS Benoît, GANIL-Caen (France) ";ROLE=R EQ-PARTICIPANT:- MAUSS Benoît, GANIL-Caen (France) ATTENDEE;CN="- MEYER Anne, IPN-Orsay (France) ";RO LE=REQ-PARTICIPANT:- MEYER Anne, IPN-Orsay (France) ATTENDEE;CN="- MRAZEK Jaromir, ASCR Rez (Czech Republic) ";R OLE=REQ-PARTICIPANT:- MRAZEK Jaromir, ASCR Rez (Czech Republic) ATTENDEE;CN="- STOECKEL Klaus, HZDR (Germany)";ROLE=REQ-PARTICIPANT:- STOE CKEL Klaus, HZDR (Germany) ATTENDEE;CN="- STUART Perrie, University of Birmingham (United kingdom) ";ROLE=REQ-PARTICIPANT:- STUART Perrie, University of Birmingham (United kingdom) ATTENDEE;CN="- SWARTZ Jacobus Andreas, Aarhus University (Denmark)";ROLE=R EQ-PARTICIPANT:- SWARTZ Jacobus Andreas, Aarhus University (Denmark) ATTENDEE;CN="- THÖER Rémy, CSNSM-Orsay (France) ";ROLE=REQ-PARTICIPANT:- THÖER Rémy, CSNSM-Orsay (France) ATTENDEE;CN="- VUKMAN Nikola, Ruđer Bošković Institute (Croatia)";ROLE= REQ-PARTICIPANT:- VUKMAN Nikola, Ruđer Bošković Institute (Croatia) CONTACT:Fairouz Hammache\, hammache _AT_ ipno.in2p3.fr CREATED;VALUE=DATE-TIME:20170627T153432Z DESCRIPTION:The main goal of the R-matrix method\, which was developed by Lane and Thomas in the fifties\, is to parametrize known experimental obse rvables such as cross-sections of nuclear reactions of astrophysical inte rest or phase shifts with a small number of parameters\, and then use thes e parameters to extrapolate data measured at higher energies down to stel lar energies. R-matrix codes\, easy to use\, were developed these last 20 years such as DREAM of P. Descouvemont et al. and AZURE of Azuma et al.. These codes allow to analyze complex cases including multiple resonances w hich can interfere and non-resonant contributions. In this training schoo l\, the lecturers Pierre Descouvemont (Universiy ULB of Brussels) and Edw ard Simpson (University of Canberra) will show the participants how to use the two R-matrix codes after giving an introduction on the R-matrix forma lism. LAST-MODIFIED;VALUE=DATE-TIME:20170824T085943Z LOCATION:IPN\, Orsay\, France URL:http://www.chetec.eu/activities/training-schools/training-school-r-mat rix-calculations-for-nuclear-astrophysics END:VEVENT BEGIN:VTIMEZONE TZID:Europe/Paris X-LIC-LOCATION:Europe/Paris BEGIN:STANDARD DTSTART;VALUE=DATE-TIME:20171029T020000 TZNAME:CET TZOFFSETFROM:+0200 TZOFFSETTO:+0100 END:STANDARD BEGIN:DAYLIGHT DTSTART;VALUE=DATE-TIME:20170326T030000 TZNAME:CEST TZOFFSETFROM:+0100 TZOFFSETTO:+0200 END:DAYLIGHT BEGIN:STANDARD DTSTART;VALUE=DATE-TIME:20181028T020000 TZNAME:CET TZOFFSETFROM:+0200 TZOFFSETTO:+0100 END:STANDARD BEGIN:DAYLIGHT DTSTART;VALUE=DATE-TIME:20180325T030000 TZNAME:CEST TZOFFSETFROM:+0100 TZOFFSETTO:+0200 END:DAYLIGHT BEGIN:STANDARD DTSTART;VALUE=DATE-TIME:20191027T020000 TZNAME:CET TZOFFSETFROM:+0200 TZOFFSETTO:+0100 END:STANDARD BEGIN:DAYLIGHT DTSTART;VALUE=DATE-TIME:20190331T030000 TZNAME:CEST TZOFFSETFROM:+0100 TZOFFSETTO:+0200 END:DAYLIGHT END:VTIMEZONE END:VCALENDAR