Explore the words cloud of the EHMVSIMF project. It provides you a very rough idea of what is the project "EHMVSIMF" about.
The following table provides information about the project.
|Coordinator Country||Netherlands [NL]|
|Total cost||165˙598 €|
|EC max contribution||165˙598 € (100%)|
1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
|Duration (year-month-day)||from 2017-01-23 to 2019-01-22|
Take a look of project's partnership.
|1||UNIVERSITEIT LEIDEN||NL (LEIDEN)||coordinator||165˙598.00|
One of the most important questions in the study of galaxy evolution is the assumption that stars formed within star clusters with a preferred mass distribution (IMF) independent of time and environment. Major advances in understanding mainly the low-mass IMF variations have been made in the past decade, however, relatively a little attention has been paid to the high-mass IMF. As such some critical questions remain: Does the high-mass IMF vary as a function of time and environment? Is it appropriate to describe the high-mass IMF with a single power-law as we do now? The multi-wavelength datasets that are becoming available now can address these questions.
My proposal will tackle this fundamental and long-standing issue to the limit of our current observing and theoretical capabilities. Spatial multi-wavelength data from the latest generation of surveys combined with up-to-date modeling tools and state-of-the-art hydrodynamical experiments will be used to shed light into potential variations of the IMF and their effects on galaxy evolution. The goals of the proposal are: 1. Investigate the spatial distribution and connection between star formation events within galaxies; 2. Identify reliable multi-wavelength high-mass IMF diagnostics; 3. Investigate the effects of IMF variations in moderating galaxy evolution using simulations. The proposed project is both high-impact and timely. The high quality data products need for this project are now available thanks to the latest sky surveys (e.g. GAMA) and multi-wavelength experiments (e.g. ESA's flagship mission Herschel). The timely implementation of the project will constitute to one of the most complete studies of the high-mass IMF variations over an unparalleled wavelength span using statistically significant samples. My expertise in data analysis and modeling combined with the world-leading expertise of my host, Leiden Observatory, in the same field provides exactly the right background to carry out this project.
|year||authors and title||journal||last update|
M. Paalvast, A. Verhamme, L. A. Straka, J. Brinchmann, E. C. Herenz, D. Carton, M. L. P. Gunawardhana, L. A. Boogaard, S. Cantalupo, T. Contini, B. Epinat, H. Inami, R. A. Marino, M. V. Maseda, L. Michel-Dansac, S. Muzahid, T. Nanayakkara, G. Pezzulli, J. Richard, J. Schaye, M. C. Segers, T. Urrutia, M. Wendt, L. Wisotzki
Properties and redshift evolution of star-forming galaxies with high [Oâ€¯III]/[Oâ€¯II] ratios with MUSE at 0.28Â <Â z Â <Â 0.85
published pages: A40, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201832866
|Astronomy & Astrophysics 618||2019-09-02|
M L P Gunawardhana, P Norberg, I Zehavi, D J Farrow, J Loveday, A M Hopkins, L J M Davies, L Wang, M Alpaslan, J Bland-Hawthorn, S Brough, B W Holwerda, M S Owers, A H Wright
Galaxy And Mass Assembly (GAMA): the signatures of galaxy interactions as viewed from small-scale galaxy clustering
published pages: 1433-1464, ISSN: 0035-8711, DOI: 10.1093/mnras/sty1638
|Monthly Notices of the Royal Astronomical Society 479/2||2019-09-02|
Nicholas Scott, Jesse vanÂ deÂ Sande, Scott M Croom, Brent Groves, Matt S Owers, Henry Poetrodjojo, Francesco Dâ€™Eugenio, Anne M Medling, Dilyar Barat, Tania M Barone, Joss Bland-Hawthorn, Sarah Brough, Julia Bryant, Luca Cortese, Caroline Foster, Andrew W Green, Sree Oh, Matthew Colless, Michael J Drinkwater, Simon P Driver, Michael Goodwin, Madusha L P Gunawardhana, Christoph Federrath, Lloyd Harischandra, Yifei Jin, J S Lawrence, Nuria P Lorente, Elizabeth Mannering, Simon Oâ€™Toole, Samuel N Richards, Sebastian F Sanchez, Adam L Schaefer, Katrina Sealey, Rob Sharp, Sarah M Sweet, Dan S Taranu, Mathew Varidel
The SAMI Galaxy Survey: Data Release Two with absorption-line physics value-added products
published pages: 2299-2319, ISSN: 0035-8711, DOI: 10.1093/mnras/sty2355
|Monthly Notices of the Royal Astronomical Society 481/2||2019-09-02|
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