What is an STSM?
Short-term Scientific Missions (STSMs) are exchange visits for researchers within their Action.
This exchange programme facilitates individuals to spend research time at an institution or laboratory based in a different country. STSMs are great opportunities for researchers to share techniques and gain skills that may not be available at their home institution or laboratory.
Who can apply?
Anyone officially participating in CosmoVerse can apply to STSMs grants but evaluation criteria (described in the dedicated section below) will matter for awarding the grants.
The Grantee must be affiliated to institutions within COST, Cooperating and Partner members countries, as listed in the COST web page.
The Grantee and the Host Institution must be in different countries.
Obligations of STSM Grantees
All applicants/grantees must be acquainted with rules and procedures described in the Annotated Rules in Section A2, and more specifically in subsection A2-2.3.
All the written outputs/deliverables derived from the STSM funds must properly acknowledge COST Action CA21136 CosmoVerse funding, as detailed in the COST acknowledgement guidelines. More specifically, the sentence “This article/publication is based upon work from COST Action CA21136 Addressing observational tensions in cosmology with systematics and fundamental physics (CosmoVerse) supported by COST (European Cooperation in Science and Technology).” in the Acknowledgement section is expected in any follow-up publications.
The STSM must happen within one Grant Period (between 1 November and 31 October the year after).
At the end of the STSM, the Grantee must submit in e-COST the following documents within at the latest 30 days after the end of the STSM, or 15 days after the end of the Grant Period, whichever date comes first:
- Scientific report on the work developed, main achievements of the STSM and planned future follow up activities.
- Host approval of the scientific report.
Financial support
The maximum grant that can be awarded is €2000 in total. STSM Grants do not necessarily cover all expenses related to undertaking a given mission.
STSM Grantees must make their own arrangements for all provisions related to personal security, health, taxation, social security, and pension matters.
The amount of the grant must be estimated by the applicants after the following criteria:
- The budget can cover a maximum of 6 nights, i.e., funding from 1 day before the start of the STSM to 1 day after the end of the STSM minimum length.
- The daily rate for accommodation, food, and local transport must be calculated based on the official COST table (link also available on the Annotated Rules).
- Long-distance travel expenses must follow general COST rules.
The effective STSM length may be longer than 5 days with the same budget. This is up to the candidate’s budget management.
Grants are processed only after the STSM ends, and after the reporting documents have been uploaded in the system, and if the STSM is approved.
The applicant can apply for a pre-payment of 50% of the Grant. The applicant must keep in mind that the transfer of the 50% of the Grant can only take place after the mission has started and will be decided by the Grant Holder (GH) Institution. When the STSM applicant requests and is granted a pre-payment of 50% of the grant, the STSM host receives a notification requesting her/him to confirm to the GH that the STSM started on schedule. Without the host confirmation, the prepayment cannot be done.
Timeline
For year 2, there are 3 calls:
- The third application was open from Tuesday 23 July until Sunday 11th August 2024, the selection process was conducted mid-August 2024, the decision communicated by end August, and the STSMs will have to happen in the period 15 July – 30 October 2024.
- The second application was open from Thursday 30th May until Monday 24th June 2024, the selection process was conducted end June 2024, the decision communicated beginning July, and the STSMs will have to happen in the period 15 July – 30 October 2024.
- The first application was open from 4 December 2023 until 6 January 2024, the selection process was conducted in January 2024, the decision communicated end January, and the STSMs will have to happen in the period February-June 2024.
For year 1, calls for STSM applications were open three times for 1 month:
- The first application was open from 7 December 2022 until 8 January 2023, the selection process was conducted in January 2023, the decision was communicated end January, and the STSMs happened in the period February-June 2023.
- The second application period was open from 15 May 2023 until 11 June 2023, the selection process was conducted in June 2023, the decision was communicated before 10 July 2023, and the STSMs happened in the period 17 July – 30 October 2023.
- The third application period was open between the 7 and 29 August 2023, the decision was communicated by 1 September 2023, and the STSMs took place in the period 28 August – 30 October 2023.
How to apply
It is the duty of the applicant to choose and contact the Host institution and the organisation of the application process. A Grant Awarding user guide is available.
- Applicants must register for an e-COST profile to be active.
- Applicants must complete the online application form.
- The following compulsory documents must be included in the online application:
- Title; start and end date; budget requested by the applicant; information about the host institution and contact person.
- STSM application form (template available on e-COST) describing (max 2 pages): Goals, description of the work to be carried out by the applicant, expected outcomes and description of the contribution to the Action MoU objectives.
- CV (No more than 3 pages – including a list of selected academic publications – if applicable).
- Letter of support from the home institution (in case of postgraduate students).
- Written agreement from the Host Institution that the STSM applicant can perform the activities detailed in the STSM work plan on the agreed dates.
Selection
The Grant Awarding Committee will be responsible for the selection of the Grantees. The scientific plan of the proposed STSM will be evaluated as for its quality, and connection and relevance to the goals and the topics of CosmoVerse.
Priority will be given in the following ranking order, as per COST Excellence and Inclusiveness Principles:
Postgraduate students and Young Researchers (i.e., < 40 years old) from Inclusiveness Target Countries (ITC)
Postgraduate students and Young Researchers (i.e., < 40 years old) from non-ITC
Senior researchers (i.e., > 40 years old) from ITC
Senior researchers (i.e., > 40 years old) from non-ITC
Gender equality will also be taken into consideration.
Applicants who did not receive an STSM from CosmoVerse will also be prioritised.
Evaluation Procedure
STSM & ITC conference grants committee composition:
The committee was formed by:
- 2 permanent members:
- Grant Coordinator: Vincenzo Salzano;
- Vice chair: Eleonora Di Valentino. Because of multiple conflicts of interest she has been substituted by a WG leader, Radosław Wojtak.
- 3 non-permanent members for 1 year term, randomly chosen from MC members.
Evaluation criteria
The committee has agreed to follow the scheme below to evaluate and rank the application.
This same scheme will be officially adopted for all future STSM grant calls.
- First shortlist with a “YES” or “NO”: to evaluate if a project generally agrees with the purposes and goals of an STSM and with the main scientific topics of CosmoVerse.
- The STSM projects are divided in three sections:
- “Goals”
- “Working plan”
- “Expected outputs and Contribution to the Action MoU objectives and deliverables”
- For each of the above sections the reviewers assign a score: “0”, “1” or “2”.
- After collecting all evaluations, the Grant Awarding Manager proceeds to average the marks.
- Finally, scores related to the age/ITC criteria (as described in the rules) are given following the scheme:
- “4”: Master, PhD students and Young Researchers (i.e., < 40 years old) from an ITC;
- “3”: Master, PhD student and Young Researchers (i.e., < 40 years old) from a non-ITC;
- “2”: Senior (i.e., > 40 years old) from ITC countries;
- “1”: Senior (i.e., > 40 years old) from non-ITC countries.
- On the final resulting ranking, the only threshold applied to decide which applications to be funded is the planned STSM budget.
For this second year, the total STSM budget amounts to 23,000€.
STSM Grantees
Recipient | Home Institution | Host Institution | Duration of stay (days) | Topic of project |
---|---|---|---|---|
Year 2 Grantees | ||||
Benjamin Bose | The University of Edinburgh, United Kingdom | NORDITA, Stockholm, Sweden | 8 | Addressing the Hubble Tension through Coupled Photon-Baryon Fluid Dynamics |
Biswajit Karmakar | University of Silesia in Katowice, Poland | Ruđer Bošković Institute, Zagreb, Croatia | 7 | Radiative neutrino mass and cosmological puzzles |
Charalampos Tzerefos | National Observatory of Athens, Greece | Scuola Superiore Meridionale, Naples, Italy | 8 | Gravitational waves induced by poisson fluctuations of primordial black holes in f(Q) gravity |
Chiara De Leo | SAPIENZA University of Rome, Italy | ESA-ESTEC, Noordwijk , Netherlands | 7 | Constraining Modified Gravity with Large Scale Structure and Gravitational Waves |
David Benisty | Stiftung Frankfurt Institute For Advanced Studies, Germany | Sissa (International School for Advanced Studies), Trieste, Italy | 8 | Galaxy groups constrains on dark matter models and the impact on the Hubble constant |
Elisa Fazzari | Università degli Studi di Roma La Sapienza, Italy | University of Sheffield, UK | 11 | Comparison between metric f(R)-gravity and other scenarios for the Hubble tension solution: the role of Cepheid and BAO data |
Elsa Teixeira | Universite De Montpellier, France | University of Sheffield, UK | 7 | Can a negative cosmological constant help address the cosmic tensions? |
Erik Jensko | University College, London, UK | Babeș-Bolyai University, Cluj-Napoca, Romania | 7 | Cosmological dynamics in geometrical gravitational theories |
Francesco Sorrenti | Universite De Geneve, Switzerland | Dipartimento di Fisica, Università di Torino, Italy | 19 | What peculiar velocities can tell us |
Gaspard Poulot | University of Sheffield, UK | Laboratoire Univers et Particules de Montpellier, France | 5 | Early dark energy and dark sector interactions to address the Hubble tension |
Gerardo García-Moreno | Instituto de Astrofísica de Andalucía (CSIC), Granada, Spain | Humbolt University of Berlin, Germany | 7 | Challenging homogeneity with both model dependent and independent approaches. |
Gergely Dálya | CNRS, Toulouse, France | Universiteit Gent, Belgium | 7 | New approaches to improve dark siren Hubble constant estimations |
Guilherme Franzmann | Stockholm University, Sweden | University of Edinburgh, UK | 8 | Addressing the Hubble tension beyond perturbation theory |
Konstantinos Dialektopoulos | Transilvania University of Brasov, Roumania | Rudjer Boskovic Institute, Zagreb, Croatia | 7 | Solving tensions with a gravitational θ-term in Symmetric Teleparallel gravity |
Laxmipriya Pati | University of Tartu, Estonia | Scuole Superiore Meridionale, University of Naples, Italy | 8 | The Hamiltonian Analysis of Symmetric Teleparallel Equivalent to General Relativity |
Marcin Postolak | Uniwersytet Wroclawski, Poland | University of Sheffield, UK | 8 | Axion-like (Scalar field) CDM interacting with the Standard Model particles as a possible solution to the H0 and σ8 (S8) tension |
Mateusz Rałowski | Jagiellonian University in Krakow, Poland | Università degli Studi di Firenze, Italy | 11 | Can the optical – infrared luminosity relation for quasars be used for cosmology? |
Miguel Pinto | Faculdade de Ciencias da Universidade de Lisboa, Portugal | INFN – Galileo Galilei Institute for Theoretical Physics, Florence, Italy | 11 | The role of non-minimally coupled scalar fields in f(R,T) gravity to address cosmic tensions |
Milan Dimitrijevic | Astronomical Observatory, Belgrade, Serbia | Faculty of Physics West University of Timisoara, Roumania | 7 | Stark broadening of O I spectral lines |
Oleksandr Zhuk | Helmholtz-Zentrum Dresden-Rossendorf, Germany | Department of Physics, Faculty of Science and Letters, Istanbul Technical University (ITU), Turkey | 9 | Observable tensions in cosmology in light of the LsCDM model: physical justification of the model. |
Oleksii Sokoliuk | National Academy Of Sciences Of Ukraine Nas Of Ukraine, Kyiv | Kavli Institute for Cosmology, University of Cambridge, UK | 7 | Possible detection of the cosmic web at z=2.48: Observations vs. Simulational data |
Pierros Ntelis | CNRS and Aix-Marseille University, France | Institute of Space Sciences and Astronomy, University of Malta | 6 | Non-Riemannian cosmologies: Addressing Tensions with Generalized Geometries |
Tiziano Schiavone | Galileo Galilei Institute for Theoretical Physics, Florence, Italy | University of Sheffield, UK | 10 | Constraining an effective Hubble constant in f(R) gravity with recent cosmological data |
Vitor da Fonseca | Faculdade De Ciencias Da Universidade De Lisboa | Universidade del País Vasco (Faculdad de Ciencia y Tecnologia), Bilbao, Spain | 9 | Seeking dark energy parametrization to address cosmological tensions |
Vitor da Fonseca | Faculdade De Ciencias Da Universidade De Lisboa, Portugal | Institute of Theoretical Astrophysics, University of Oslo, Norway | 7 | Connections in the dark sector |
Vladimir Sreckovic | Institute of Physics, Belgrade | Technical University in Sofia | 7 | Investigation of chemistry of lithium, hydrogen and helium molecular ions in the early Universe: dataset needed for modelling |
Year 1 Grantees | ||||
Aleksander Kozak | University of Wrocław | Facultad de Ciencias Físicas, Universidad Complutense Madrid | 8 | Investigating lithium-7 abundance problem in modified gravity: astrophysical and cosmological perspectives |
Aleksander Kozak | University of Wrocław | Institute of Space Sciences and Astronomy, University of Malta | 6 | Investigating light elements’ abundances in the Palatini-type theories of gravity |
Antonio Ferreiro | Radboud University Nijmegen | Instituto de Astrofísica Andalucía & Universidad de Granada | 5 | Vacuum polarization and backreaction of quantum fields in the expansion of the late time Universe |
David BENISTY | University of Cambirdge
| Bulgarian Academy of Sciences | 15
| Dark Energy in the Galactic Center
|
Débora Aguiar Gomes | Institute of Physics
| Institute of Space Sciences and Astronomy, University of Malta
| 5
| On the Lithium Cosmological Problem in Modified Gravity |
Denitsa Staicova | Bulgarian Academy of Sciences
| Complutense University of Madrid | 5
| Hubble tension in Lorentz Invariance Violation studies from GRB time-delays
|
Elsa Teixeira | School of Mathematics and Statistics, Sheffield | University of Rome Sapienza
| 7
| Addressing cosmological tensions with modified gravity
|
Emre Ozulker | Istanbul Technical University
| University of Sheffield
| 8
| Addressing major cosmological tensions with models beyond the standard LCDM model |
Enrico Specogna
| University of Sheffield
| Institute of Space Sciences and Astronomy, University of Malta | 7 | Exploring extended modified gravity models with current and future cosmological data
|
Enrico Specogna
| University of Sheffield
| La Sapienza University of Rome
| 8
| Investigating Phenomenological Extensions of the Standard Model through the Lens(ing) of CMB Data
|
Gabriele Barca
| La Sapienza University of Rome
| Instituto de Ciencias del Espacio – Consejo Superior de Investigaciones Cientificas (ICE-CSIC)
| 12
| Modified Gravity as a Paradigm for the Hubble Tension |
Gerardo García-Moreno | Instituto de Astrofísica de Andalucía, Granada
| Institute for Mathematics, Astrophysics, and Particle Physics (IMAPP) – Radboud University Nijmegen
| 7
| Reconsidering homogeneity and isotropy of the Universe
|
Ismael Ferrero
| Institute of Theoretical Astrophysics
| Instituto de Física Teórica (IFT) – Universidad Autónoma de Madrid (UAM)
| 7
| Enhancing Galaxy Mocks through Improved Galaxy Property Assignment”.
|
Konstantinos Dialektopoulos
| Aristotle University of Thessaloniki
| Institute of Space Sciences and Astronomy, University of Malta
| 7
| Reconstructing functions with Artificial Neural Networks
|
Laxmipriya Pati
| University of Tartu
| Institute of Astrophysics and Space Science , University of Lisbon
| 12
| Investigating the Hubble Constant Tension through Non-Trivial Connections in Extended Symmetric Teleparallel Gravity
|
Marco de Cesare | Università di Napoli “Federico II” | University of Sheffield
| 7
| Addressing the Hubble tension with diffusion
|
Matteo Forconi
| La Sapienza, University of Rome
| University of Oslo
| 7
| Investigating Physical Mechanisms for Depolarizing the Cosmic Microwave Background
|
Matteo Forconi
| La Sapienza University of Rome
| University of Sheffield
| 7
| Models beyond LCDM
|
Miguel Pinto
| Faculty of Sciences
| University of Valencia
| 7
| Addressing cosmological tensions with Palatini formulation of modified theories of gravity
|
Rebecca Briffa | University of Malta
| Università degli Studi di Torino
| 8
| Scalar tensor theories in Teleparallel Gravity
|
Ruchika Kaushik
| La Sapienza University of Rome
| Instituto de Fisica Corpuscular (IFIC)
| 7
| Addressing observational tensions in cosmology by allowing possible variations in fundamental physics. |
Ruchika Kaushik
| La Sapienza University of Rome
| University of Sheffield
| 8
| Cosmology with JWST and non-standard Lambda
|
Vasiliki Karanasou
| University of Tartu
| Center of Applied Space Technology and Microgravity (ZARM)
| 8
| Quasinormal Modes in New General Relativity
|
William Giarè
| University of Sheffield
| University of Trento
| 7
| New physics in light of the current tensions between Cosmic Microwave Background and Weak Lensing surveys
|
Yuejia Zhai
| School of Mathematics and Statistics, Sheffield
| Laboratoire Univers et Particules de Montpellier
| 7
| Exploring the cosmological tensions with EDE in extended cosmologies
|