Short Term Scientific Missions

Short Term Scientific Missions

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.

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.

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.

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.

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.

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.

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.

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