Newton STFC-NARIT: Thai-UK Python+Astronomy Summer Schools (ThaiPASS): A STEM outreach project on Python with applications to data-driven astronomy

Lead Research Organisation: University of Hull
Department Name: Mathematics

Abstract

Project ThaiPASS (Thai-UK Python+Astronomy Summer School) is a human-capacity building STEM outreach project proposed jointly by the E.A. Milne Centre for Astrophysics (University of Hull, UK) and the Institute of Fundamental Study (Naresuan University, Thailand), with partnership from the National Astronomical Research Institute of Thailand (NARIT). Each ThaiPASS is a full-board summer school aimed at Thai secondary school students age around 16-18. Students will receive training in scientific computing in Python, one of the fastest growing open-source programming languages and one of the most desirable from an employability perspective. Students will learn to use Python to handle data via the medium of astronomy, which is one of the most inspiring and high-impact STEM enablers. Over a 5-day course, professional astronomers from the UK will guide students through a series of lectures and hands-on tasks involving handling astronomical data and producing visual output such as astronomical images and videos. Students will leave the summer school with a new perspective on the role of data science in modern reserach, and will be inspired to continue to learn coding beyond the scope and time-scale of the summer school. The summer school will also include a "university and career" day to inform students on how STEM subjects can be taken further at university level and as a career.

The ThaiPASS project will address many of the challenges in science and ICT education in Thailand, which has fallen far behind other countries emerging out of the middle-income trap. At ThaiPASS, we will bring STFC-funded science to new audiences who may not have the opportunity to access such training otherwise. The skills developed at ThaiPASS are current, relevant and easily transferable to a wide range of industrial and academic applications. The UK team from Hull particularly understand the importance of high-quality STEM outreach: Hull is one of the most impoverished cities in the UK with a large proportion of under-performing schools. However, through our previous outreach work (over 150 science outreach events in the past 3 years, mostly in Hull and the Yorkshire region), we have witnessed first-hand the positive transformation STEM education can make for young people who might not have otherwise considered taking up science at University and as a career.

In recent years, Thailand has established itself as an emerging player in astrophysics research thanks to a new generation of internationally recognised researchers at NARIT, Naresuan. Chulalongkorn, Suranaree etc. Investment in the ThaiPASS project will be a small but significant step towards forging a strong and lasting Thai-UK synergy, which can easily spin off into future collaborations in astrophysics research and further outreach activities.

Planned Impact

The most important impacts that will be delivered by ThaiPASS are:
1) Using STFC-funded science to reach out to new audiences and build human capacity.
2) Training in programming and data-handling skills, which are highly transferable and employable.
3) STEM enabling via the medium of astronomy.
These impacts resonate strongly with the goals of Newton Fund, particularly those spelt out in the STFC-NARIT MOU.

Python is a highly desirable programming skill to a wide range of employers, especially those in the ICT and industrial sectors. The requirement for Python skills has grown rapidly in recent years, overtaking traditionally popular languages such as C++. Although the Python is the language of choice for ThaiPASS, it is used really as a medium to convey the main principles of scientific programming and data handling, so that skills learnt at ThaiPASS can be easily translated to any programming languages the participants may take up in the future.

A high-impact legacy of the ThaiPASS project is for a similar summer school to be held in the UK, particularly in Hull, which remains one of the most impoverished cities in the UK with a high number of underperforming schools. The teaching material developed for ThaiPASS can be adapted to organise a "UKPASS" targeting schools in the north of the UK and hosted by the University of Hull. The Physics group at Hull (particularly the Milne Centre) has a strong track-record of commitment to outreach within the Yorkshire region and beyond - with 150 outreach events held in the past 3 years, including outreach talks in schools, at science festivals and on BBC radio (see the full list at http://www.milne.hull.ac.uk/#events).

Another legacy of the ThaiPASS project is the establishment of a strong link between the E.A.Milne Centre and the Thai partner institutions, namely, Naresuan and NARIT, with a view to involve more Thai institutions in the future. Although ThaiPASS focuses purely on outreach, the synergy between the Thai and UK team could spin off into collaborative research projects in astrophysics, as there are shared research interests amongst researchers at Hull and Naresuan. The Thai-UK links forged via ThaiPASS also have the potential to develop into further joint workshops, conferences, outreach events and international teaching collaborations (e.g. postgraduate student exchanges or visiting lectureships).
 
Description We have understood how to bring astronomy and Python to an international audience, and how to create innovative tasks based on current astronomy research, that is accessible by non-UK high school students.
Exploitation Route Our workflow and organisation can be adapted to create an astronomy/programming outreach scheme for A-level students in the UK
Sectors Education

URL https://indico.narit.or.th/event/120/
 
Description It is used to address inequality and inequity in Thai education system, and to give high school students a head start for the modern data-based economy.
First Year Of Impact 2018
 
Description Project ThaiPASS: Thailand-UK Python+Astronomy Summer Schools 2020 and 2021.
Amount £66,677 (GBP)
Funding ID ST/T007141/1 
Organisation Science and Technologies Facilities Council (STFC) 
Sector Public
Country United Kingdom
Start 03/2020 
End 10/2021
 
Description Software Tools for Simulations in Nuclear Astrophysics: NuGrid/JINA/ChETEC - Conference grant
Amount € 20,400 (EUR)
Funding ID ECOST-TRAINING_SCHOOL-CA16117-170918-099956 
Organisation European Cooperation in Science and Technology (COST) 
Sector Public
Country Belgium
Start 09/2018 
End 10/2018
 
Description Stars, Supernovae and Nucleosynthesis V Annual BRIDGCE Meeting - APPLICATION FOR CONFERENCE AND SHORT COURSE SUPPORT
Amount £1,500 (GBP)
Organisation Science and Technologies Facilities Council (STFC) 
Sector Public
Country United Kingdom
Start 09/2018 
End 10/2018
 
Description COST Action - ChETEC - Chemical Elements as Tracers of the Evolution of the Cosmos 
Organisation Keele University
Country United Kingdom 
Sector Academic/University 
PI Contribution WP Lead, Nuclear astrophysics school organized (https://indico.cern.ch/event/719752/)
Collaborator Contribution To maximise the scientific and innovative return of these huge European investments it is essential: to coordinate research efforts in astronomy, astrophysics, and nuclear physics; to build pan-European inter-disciplinary bridges between these disciplines; and to link this blue skies research with SMEs who can provide the technological tools required for the exploitation of data, software and techniques and in return join the innovation cycle. These are the goals of our ChETEC (pronounced [ketek]) COST Action, which stands for Chemical Elements as Tracers of the Evolution of the Cosmos. The Action will also train a new generation of European scientists providing inter-disciplinary expertise and knowledge-transfer skills with the aim of strengthening the Innovation Union.
Impact Approved STSMs can be found here: https://docs.google.com/spreadsheets/d/1-I8qL-0fkdGqtLZ9JCn35D8bcJL3DlYLC0c1zlOPLEE/edit#gid=0 Approved workshop and training schools: http://www.chetec.eu/activities/training-schools
Start Year 2016
 
Description Chemical abundances in the ISM: the litmus test of stellar IMF variations in galaxies across cosmic time 
Organisation Nanjing University (NJU)
Country China 
Sector Academic/University 
PI Contribution Producing theoretical stellar simulations to make CNO. 2 invited talks at the ISSI meetings.
Collaborator Contribution With this proposal, we aim at building up an international team whose members have all the necessary expertise to (i) reduce significantly the uncertainties present in abundance measurements, (ii) extend the measurements to different types of galaxies, from dwarfs to ellipticals, at both high and low redshifts, (iii) improve -or develop from scratch- the theoretical tools that are necessary for a full exploitation and interpretation of the data. Our team is composed of ten scientists from five European countries and from China. It includes experts in numerical simulations, semi-analytical models of galaxy formation in a cosmological context, state-of-the-art hydro-dynamical simulations, stellar evolution and nucleosynthesis, chemical evolution, IGIMF theory, as well as experts in ISM physics, molecular line observations and data analysis. Because of the team composition, and to help self-supported external experts from both European countries and China to attend the meetings, our team would benefit from one 5-day meeting in ISSI, Bern, and one 5-day meeting in ISSI-BJ, Beijing.
Impact Ongoing meetings in Bern and Bejing. ISSI is covering accommodation costs at the meetings.
Start Year 2019
 
Description Chemical abundances in the ISM: the litmus test of stellar IMF variations in galaxies across cosmic time 
Organisation National Institute for Astrophysics
Country Italy 
Sector Academic/University 
PI Contribution Producing theoretical stellar simulations to make CNO. 2 invited talks at the ISSI meetings.
Collaborator Contribution With this proposal, we aim at building up an international team whose members have all the necessary expertise to (i) reduce significantly the uncertainties present in abundance measurements, (ii) extend the measurements to different types of galaxies, from dwarfs to ellipticals, at both high and low redshifts, (iii) improve -or develop from scratch- the theoretical tools that are necessary for a full exploitation and interpretation of the data. Our team is composed of ten scientists from five European countries and from China. It includes experts in numerical simulations, semi-analytical models of galaxy formation in a cosmological context, state-of-the-art hydro-dynamical simulations, stellar evolution and nucleosynthesis, chemical evolution, IGIMF theory, as well as experts in ISM physics, molecular line observations and data analysis. Because of the team composition, and to help self-supported external experts from both European countries and China to attend the meetings, our team would benefit from one 5-day meeting in ISSI, Bern, and one 5-day meeting in ISSI-BJ, Beijing.
Impact Ongoing meetings in Bern and Bejing. ISSI is covering accommodation costs at the meetings.
Start Year 2019
 
Description IF 
Organisation Naresuan University
Department Institute for Fundamental Study
Country Thailand 
Sector Public 
PI Contribution We have been working with IF staff on delivering the summer schools.
Collaborator Contribution Time of research staff (Dr Chantavat) over the course of the 2 year project.
Impact A research paper is in preparation.
Start Year 2018
 
Description IRENA - International Research Network for Nuclear Astrophysics 
Organisation Michigan State University
Country United States 
Sector Academic/University 
PI Contribution Focus area coordinator (FA6)
Collaborator Contribution The emergence of multi-messenger astronomy, where extreme astrophysical environments are observed using gravitational waves, X-rays, visible light, gamma-rays, radio waves, and neutrinos, opens up the opportunity to understand the formation of the elements and the nature of dense matter. IReNA connects this broad range of observations with the extraordinarily broad range of experimental and theoretical nuclear physics studies and advanced computational models needed to truly create new windows into the physics of the universe. IReNA is a US National Science Foundation AccelNet Network of Networks. It connects six interdisciplinary research networks across 17 countries to foster collaboration, complement and enhance research capabilities in the US and abroad, and thus greatly accelerate progress in science. An important component of IReNA is the training of students and other young researchers in an unique interdisciplinary, collaborative, and international environment that prepares them for a broad range of STEM careers in science, industry, government, and national laboratories.
Impact Direct support to workshops. In the UK: - Progress on the reaction rates and stellar modelling affecting the 26Al abundance in the Galaxy, 10-11 March 2020 (https://www.york.ac.uk/physics/news/events/groups/nuclear-physics/workshop-reaction-rates-stellar-modelling-galaxy/)
Start Year 2019
 
Description JINA-CEE 
Organisation Michigan State University
Country United States 
Sector Academic/University 
PI Contribution Associate institute, publications, organization of nuclear astrophysics school (https://indico.cern.ch/event/719752/)
Collaborator Contribution JINA-CEE is the successor of the successful Joint Institute for Nuclear Astrophysics (JINA), which was founded in 1999 between the University of Notre Dame, Michigan State University, and the University of Chicago. Since 2002 JINA has been supported as a NSF Physics Frontiers Center. Today, the JINA-CEE network includes 26 institutions in 9 countries and about 300 scientific participants, including about 240 students and postdocs. Michigan State University currently serves as lead institution, and forms - together with the University of Notre Dame, Arizona State University, and University of Washington - the core of the center. JINA-CEE includes partnerships with international centers for nuclear astrophysics that have been inspired by JINA-CEE.
Impact TBD
Start Year 2016
 
Description MoU NARIT 
Organisation National Astronomical Research Institute Of Thailand
Country Thailand 
Sector Public 
PI Contribution We worked with NARIT on delivering the summer schools. We signed an MOU with NARIT.
Collaborator Contribution NARIT team acted as the principal Local Organising Committee for the summer schools. Website hosting.
Impact MOU between Hull University and NARIT.
Start Year 2018
 
Description NuGRID 
Organisation Konkoly Observatory
Country Hungary 
Sector Academic/University 
PI Contribution PI, Project coordinator
Collaborator Contribution The Nucleosynthesis Grid (NuGrid) collaboration, formed in fall 2007, develops and maintains tools for large scale post-processing nucleosynthesis simulations with up-to-date and flexible nuclear physics input, and apply these to complete sets of quiescent and explosive nuclear production environments.
Impact Our science goal is to provide complete sets of stellar evolution sequences for low-mass and massive stars with compatible input physics, including explosion simulations, and calculate the complete nucleosynthesis with the same post-processing code. In this way we will obtain a high degree of internal consistency. We plan to generate yield sets covering the entire mass and metallicity space, in collaboration with teams working in galactic chemical evolution and near-field cosmology. The NuGrid approach is characterized by a commitment to forward modeling based on our physics understanding of the involved processes, verification and validation, and uncertainty quantification, including the important aspect of nuclear physics input. Here I highlight just 3 representative papers published in the past 5 years: - Keegans et al. 2019 MNRAS (DOI: 10.1093/mnras/stz368) - Ritter et al. 2018 MNRAS (10.1093/mnras/sty1729) - Pignatari et al. 2016, ApJS (DOI: 10.3847/0067-0049/225/2/24)
Start Year 2007
 
Description NuGRID 
Organisation University of Edinburgh
Country United Kingdom 
Sector Academic/University 
PI Contribution PI, Project coordinator
Collaborator Contribution The Nucleosynthesis Grid (NuGrid) collaboration, formed in fall 2007, develops and maintains tools for large scale post-processing nucleosynthesis simulations with up-to-date and flexible nuclear physics input, and apply these to complete sets of quiescent and explosive nuclear production environments.
Impact Our science goal is to provide complete sets of stellar evolution sequences for low-mass and massive stars with compatible input physics, including explosion simulations, and calculate the complete nucleosynthesis with the same post-processing code. In this way we will obtain a high degree of internal consistency. We plan to generate yield sets covering the entire mass and metallicity space, in collaboration with teams working in galactic chemical evolution and near-field cosmology. The NuGrid approach is characterized by a commitment to forward modeling based on our physics understanding of the involved processes, verification and validation, and uncertainty quantification, including the important aspect of nuclear physics input. Here I highlight just 3 representative papers published in the past 5 years: - Keegans et al. 2019 MNRAS (DOI: 10.1093/mnras/stz368) - Ritter et al. 2018 MNRAS (10.1093/mnras/sty1729) - Pignatari et al. 2016, ApJS (DOI: 10.3847/0067-0049/225/2/24)
Start Year 2007
 
Description NuGRID 
Organisation University of Hull
Country United Kingdom 
Sector Academic/University 
PI Contribution PI, Project coordinator
Collaborator Contribution The Nucleosynthesis Grid (NuGrid) collaboration, formed in fall 2007, develops and maintains tools for large scale post-processing nucleosynthesis simulations with up-to-date and flexible nuclear physics input, and apply these to complete sets of quiescent and explosive nuclear production environments.
Impact Our science goal is to provide complete sets of stellar evolution sequences for low-mass and massive stars with compatible input physics, including explosion simulations, and calculate the complete nucleosynthesis with the same post-processing code. In this way we will obtain a high degree of internal consistency. We plan to generate yield sets covering the entire mass and metallicity space, in collaboration with teams working in galactic chemical evolution and near-field cosmology. The NuGrid approach is characterized by a commitment to forward modeling based on our physics understanding of the involved processes, verification and validation, and uncertainty quantification, including the important aspect of nuclear physics input. Here I highlight just 3 representative papers published in the past 5 years: - Keegans et al. 2019 MNRAS (DOI: 10.1093/mnras/stz368) - Ritter et al. 2018 MNRAS (10.1093/mnras/sty1729) - Pignatari et al. 2016, ApJS (DOI: 10.3847/0067-0049/225/2/24)
Start Year 2007
 
Description NuGRID 
Organisation University of Victoria
Country Canada 
Sector Academic/University 
PI Contribution PI, Project coordinator
Collaborator Contribution The Nucleosynthesis Grid (NuGrid) collaboration, formed in fall 2007, develops and maintains tools for large scale post-processing nucleosynthesis simulations with up-to-date and flexible nuclear physics input, and apply these to complete sets of quiescent and explosive nuclear production environments.
Impact Our science goal is to provide complete sets of stellar evolution sequences for low-mass and massive stars with compatible input physics, including explosion simulations, and calculate the complete nucleosynthesis with the same post-processing code. In this way we will obtain a high degree of internal consistency. We plan to generate yield sets covering the entire mass and metallicity space, in collaboration with teams working in galactic chemical evolution and near-field cosmology. The NuGrid approach is characterized by a commitment to forward modeling based on our physics understanding of the involved processes, verification and validation, and uncertainty quantification, including the important aspect of nuclear physics input. Here I highlight just 3 representative papers published in the past 5 years: - Keegans et al. 2019 MNRAS (DOI: 10.1093/mnras/stz368) - Ritter et al. 2018 MNRAS (10.1093/mnras/sty1729) - Pignatari et al. 2016, ApJS (DOI: 10.3847/0067-0049/225/2/24)
Start Year 2007
 
Description NuGRID 
Organisation University of York
Country United Kingdom 
Sector Academic/University 
PI Contribution PI, Project coordinator
Collaborator Contribution The Nucleosynthesis Grid (NuGrid) collaboration, formed in fall 2007, develops and maintains tools for large scale post-processing nucleosynthesis simulations with up-to-date and flexible nuclear physics input, and apply these to complete sets of quiescent and explosive nuclear production environments.
Impact Our science goal is to provide complete sets of stellar evolution sequences for low-mass and massive stars with compatible input physics, including explosion simulations, and calculate the complete nucleosynthesis with the same post-processing code. In this way we will obtain a high degree of internal consistency. We plan to generate yield sets covering the entire mass and metallicity space, in collaboration with teams working in galactic chemical evolution and near-field cosmology. The NuGrid approach is characterized by a commitment to forward modeling based on our physics understanding of the involved processes, verification and validation, and uncertainty quantification, including the important aspect of nuclear physics input. Here I highlight just 3 representative papers published in the past 5 years: - Keegans et al. 2019 MNRAS (DOI: 10.1093/mnras/stz368) - Ritter et al. 2018 MNRAS (10.1093/mnras/sty1729) - Pignatari et al. 2016, ApJS (DOI: 10.3847/0067-0049/225/2/24)
Start Year 2007