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CORDIS - Risultati della ricerca dell’UE
CORDIS

Novel Evolutionary Model for the Early stages of Stars with Intelligent Systems

CORDIS fornisce collegamenti ai risultati finali pubblici e alle pubblicazioni dei progetti ORIZZONTE.

I link ai risultati e alle pubblicazioni dei progetti del 7° PQ, così come i link ad alcuni tipi di risultati specifici come dataset e software, sono recuperati dinamicamente da .OpenAIRE .

Risultati finali

Data Management Plan (si apre in una nuova finestra)

Data Management plan will address the relevant aspects of making data FAIR findable accessible interoperable and reusable including what data the project will generate whether and how it will be made accessible for verification and reuse and how it will be curated and preserved

Project internet portal online (si apre in una nuova finestra)

The project internet portal as a major gateway for communicating the major activities and results of the project will be created

Outreach module: visualization material of star forming regions (si apre in una nuova finestra)

We will create visualisation graphics and videos through online platforms such as ESASky WWT or the Milky Way 3D project We plan to combine our science data and produce colorcomposite images based on all starforming regions studiedIn addition we aimto use the parallax and kinematic information of Gaia together with Spitzer and Herschel data in order to render realistic 3D representations of starforming regions Due to their interoperability with other platforms for amateur telescopes and portable planetaria WWT modules are widely used to outreach activities worldwide To support these outreach actions we include 3 additional PhD months at UNIVIE

Communication of NEMESIS science to the public (si apre in una nuova finestra)

We will share and diffuse our fascination for our science to the wider public. We will develop an outreach module for school presentations, useful for teachers and scientists going into school classes. We will give public outreach talks locally, will diffuseour results via press releases to be picked up by the international media. The science addressed by NEMESIS is fascinating, the relevance of which is easy to explain to a very broad audience.

Novel evolutionary model of YSO formation, including formation timescales. (si apre in una nuova finestra)

We here aim to consolidate the results from all work packages in order to answer our central questions on the formation and early evolution of stars and the associated timescales. Based on the compiled observational data (WP 2) and the classification criteria produced with the use of ML techniques (WP 3) we will conclude on the main evolutionary transformations of YSO and will constrain the role, importance and duration for each phase. We will thus update the main YSO Classes, introducing when necessary new phases and classification criteria that will reflect the physical transformations revealed from the data. Most importantly, our compilation of the largest, most complete and unbiased sample of YSO will ensure that these criteria will be less affected by systematic errors.

Summary of organised international conference (si apre in una nuova finestra)

We will organize a scientific conference to share and discuss our results with the star and planet formation community. We include funds for the organization of this international conference in Hungary, under the lead of KONKOLY. These funds will help keep the registration fee low and fund registration waivers for participants requiring financialhelp. We will propose further sessions at large conferences of broader audience, such as EAS Annual Meetings. We will provide invited and contributed talks, and show posters, at major European/overseas conferences.A summary of the meeting including the most important results and contributions will be prepared as means of verification.

Determination of the influence of the environment in star formation (si apre in una nuova finestra)

The sample size will also determine the accuracy of the timescales describing the evolution, as such determinations are based on number statistics. This new evolutionary scenario will need to be placed into context with our current knowledge of the timescales for the formation at different scales in the solar system, from the families of solids in meteorites, up to the formation of gas giants and the rocky planets.

Dissemination of multi-wavelength datasets (si apre in una nuova finestra)

Dissemination at the end of the project of all compiled, panchromatic datasets.

Online dissemination of NEMESIS results (si apre in una nuova finestra)

We will put our data, including ML scripts and classification outputs, online for public access. A searchable database will be setup at UNIGE. We will further write papers describing the compiled data set properties, the ML techniques used and their outputs, the supervised and supervised classifications and associated attributes, and the novel evolutionary model. We expect to publish at least 10 papers in top-ranking journals.

Pubblicazioni

Gaia Data Release 3 Validating the classification of variable Young Stellar Object candidates (si apre in una nuova finestra)

Autori: Marton, Gábor ; Ábrahám, Péter ; Rimoldini, Lorenzo ; Audard, Marc search by orcid ; Kun, Mária ; Nagy, Zsófia search by orcid ; Kóspál, Ágnes ; Szabados, László ; Holl, Berry ; Gavras, Panagiotis ; Mowlavi, Nami search by orcid ; Nienartowicz, Krzysztof ; Jevardat de Fombelle, Grégory ; Lecoeur-Taïbi, Isabelle ; Karbevska, Lea ; Garcia-Lario, Pedro ; Eyer, Laurent
Pubblicato in: Astronomy & Astrophysics, Numero In press, 2022, ISSN 0004-6361
Editore: Springer Verlag
DOI: 10.1051/0004-6361/202243232

A deep neural network approach to compact source removal (si apre in una nuova finestra)

Autori: M. Madarász, G. Marton, I. Gezer, S. Lehner, J. Roquette, M. Audard, D. Hernandez, O. Dionatos
Pubblicato in: Astronomy & Astrophysics, Numero 696, 2025, Pagina/e A37, ISSN 0004-6361
Editore: Springer Verlag
DOI: 10.1051/0004-6361/202453262

Revisiting star and planet formation in the era of Big Data

Autori: Odysseas Dionatos
Pubblicato in: Hipparchos, 2022, ISSN 1790-9252
Editore: Hellenic Astronomical Society

Probing the global dust properties and cluster formation potential of the giant molecular cloud G148.24+00.41 (si apre in una nuova finestra)

Autori: Vineet Rawat, M R Samal, D L Walker, A Zavagno, A Tej, G Marton, D K Ojha, Davide Elia, W P Chen, J Jose, C Eswaraiah
Pubblicato in: Monthly Notices of the Royal Astronomical Society, Numero 521, 2023, Pagina/e 2786-2805, ISSN 0035-8711
Editore: Blackwell Publishing Inc.
DOI: 10.1093/mnras/stad639

Photometric and spectroscopic study of the burst-like brightening of two Gaia-alerted young stellar objects (si apre in una nuova finestra)

Autori: Zsófia Nagy; Péter Ábrahám; Ágnes Kóspál; Sunkyung Park; Michał Siwak; Fernando Cruz-Sáenz de Miera; Eleonora Fiorellino; David García-Álvarez; Zsófia Marianna Szabó; Simone Antoniucci; Teresa Giannini; Alessio Giunta; Levente Kriskovics; Mária Kun; Gábor Marton; Attila Moór; Brunella Nisini; Andras Pál; László Szabados; Paweł Zieliński; Łukasz Wyrzykowski
Pubblicato in: Monthly Notices of the Royal Astronomical Society, Numero Volume 515, Numero 2, September 2022, 2022, Pagina/e 1774–1787, ISSN 0035-8711
Editore: Blackwell Publishing Inc.
DOI: 10.48550/arxiv.2207.02341

SED modelling of young stellar objects in the Orion star formation complex (si apre in una nuova finestra)

Autori: Ilknur Gezer, Gábor Marton, Julia Roquette, Marc Audard, David Hernandez, Máté Madarász, Odysseas Dionatos
Pubblicato in: Astronomy & Astrophysics, 2025, ISSN 0004-6361
Editore: Springer Verlag
DOI: 10.1051/0004-6361/202453624

The enigma of Gaia18cjb: A possible rare hybrid of FUor and EXor properties (si apre in una nuova finestra)

Autori: Eleonora Fiorellino, Péter Ábrahám, Ágnes Kóspál, Mária Kun, Juan M. Alcalá, Alessio Caratti o Garatti, Fernando Cruz-Sáenz de Miera, David García-Álvarez, Teresa Giannini, Sunkyung Park, Michał Siwak, Máté Szilágyi, Elvira Covino, Gabor Marton, Zsófia Nagy, Brunella Nisini, Zsófia Marianna Szabó, Zsófia Bora, Borbála Cseh, Csilla Kalup, Máté Krezinger, Levente Kriskovics, Wa
Pubblicato in: Astronomy & Astrophysics, Numero 686, 2024, Pagina/e A160, ISSN 0004-6361
Editore: Springer Verlag
DOI: 10.1051/0004-6361/202347777

Identifying young stars in Star Forming Regions using Herschel

Autori: Pavlidou, Tatiana ; Dionatos, Odysseas ; Audard, Marc ; Marton, Gábor ; Roquette, Julia ; Gezer, Ilknur ; Hernandez, David
Pubblicato in: 44th COSPAR Scientific Assembly. Held 16-24 July, 2022, 2022
Editore: 44th COSPAR Scientific Assembly. Held 16-24 July, 2022

Star- and planet formation caught-in-the-act

Autori: Marton, Gábor ; Ábrahám, Péter ; Nagy, Zsófia ; Dionatos, Odysseas ; Audard, Mar ; Pavlidou, Tatiana ; Roquette, Julia ; Gezer, Ilknur ; Hernandez, David
Pubblicato in: 44th COSPAR Scientific Assembly. Held 16-24 July, 2022, 2022
Editore: 44th COSPAR Scientific Assembly. Held 16-24 July, 2022

The Orion Star-Formation Complex as a training set for machine learning techniques (si apre in una nuova finestra)

Autori: Roquette, Julia; Audard, Marc; Pavlidou, Tatiana; Marton, Gabor; Hernandez, David; Dionatos, Odysseas; Gezer, Ilknur
Pubblicato in: The 21st Cambridge workshop on Cool Stars, Stellar Systems, and the Sun, Numero 1, 2022
Editore: Conference Poster
DOI: 10.5281/zenodo.7589668

The Orion star-formation complex as a training set for machine learning techniques

Autori: Audard, Marc ; Roquette, Julia ; Dionatos, Odysseas ; Marton, Gábor ; Gezer, Ilknur ; Hernandez, David ; Pavlidou, Tatiana
Pubblicato in: 44th COSPAR Scientific Assembly. Held 16-24 July, 2022, 2022
Editore: 44th COSPAR Scientific Assembly. Held 16-24 July, 2022

The spin evolution of stars born in clusters (si apre in una nuova finestra)

Autori: Roquette, Julia; Matt, Sean; Winter, Andrew J.; Amard, Louis
Pubblicato in: The 21st Cambridge workshop on Cool Stars, Stellar Systems, and the Sun (CS21), Numero 1, 2022
Editore: Conference ePoster
DOI: 10.5281/zenodo.7590777

The NEMESIS Catalogue of Young Stellar Objects for the Orion Star Formation Complex. I. General description of data curation (si apre in una nuova finestra)

Autori: J. Roquette, M. Audard, D. Hernandez, I. Gezer, G. Marton, C. Mas, M. Madarász, O. Dionatos
Pubblicato in: Astronom & Astrophysics, 2025, ISSN 2331-8422
Editore: Cornell University, [1991]-
DOI: 10.48550/arxiv.2501.08486

Exploring Young Stellar Variability with Gaia DR3 light curves (si apre in una nuova finestra)

Autori: Chloé Mas, Julia Roquette, Marc Audard, Mate Madarász, Gabor Marton, David Hernandez, Ilknur Gezer, Odysseas Dionatos
Pubblicato in: Astronomy & Astrophysics, Numero submitted, under review, 2025, ISSN 2331-8422
Editore: Cornell University
DOI: 10.48550/arxiv.2503.23530

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