Zobrazeno 1 - 10
of 425
pro vyhledávání: '"Krywult A."'
Autor:
Figueira, M., Siudek, M., Pollo, A., Krywult, J., Vergani, D., Bolzonella, M., Cucciati, O., Iovino, A.
How the quiescent galaxies evolve with redshift and the factors that impact their evolution are still debated. It is still unclear what the dominant mechanisms of passive galaxy growth are and what role is played by the environment in shaping their e
Externí odkaz:
http://arxiv.org/abs/2404.14103
Autor:
Hamed, M., Pistis, F., Figueira, M., Małek, K., Nanni, A., Buat, V., Pollo, A., Vergani, D., Bolzonella, M., Junais, Krywult, J., Takeuchi, T., Riccio, G., Moutard, T.
Publikováno v:
A&A 679, A26 (2023)
We aim to understand what drives the IRX-\beta dust attenuation relation at intermediate redshift (0.5 < z < 0.8) in star-forming galaxies. We investigate the role of various galaxy properties in shaping this observed relation. We use robust [O ii] {
Externí odkaz:
http://arxiv.org/abs/2309.01819
Autor:
Siudek, M., Lisiecki, K., Krywult, J., Donevski, D., Haines, C. P., Karska, A., Małek, K., Moutard, T., Pollo, A.
Red ultra-compact massive galaxies, called red nuggets were formed at high redshifts ($\rm{z\sim2-3}$). Survivors of red nuggets, known as relics, observed at lower redshifts ($\rm{z<2}$) are believed to remain almost unchanged since their formation.
Externí odkaz:
http://arxiv.org/abs/2306.03230
While we already seem to have a general scenario of the evolution of different types of galaxies, a complete and satisfactory understanding of the processes that led to the formation of all the variety of today's galaxy types is still beyond our reac
Externí odkaz:
http://arxiv.org/abs/2211.11792
Dwarf galaxies are ideal laboratories to study the relationship between the environment and AGN activity. However, the type of environments in which dwarf galaxies hosting AGN reside is still unclear and limited to low-redshift studies (z < 0.5). We
Externí odkaz:
http://arxiv.org/abs/2210.13486
Assessment of adipokines, adenine nucleotides and uric acid in the dynamics of coronary intervention
Autor:
Stygar D., Skrzep-Poloczek B., Slominska E., Dolezych B., Niedziela J., Nowak J., Wesolowski B., Kukla M., Krywult A., Długaszek M., Sawczyn T., Poloczek J., Zwirska-Korczala K.
Publikováno v:
Open Life Sciences, Vol 10, Iss 1 (2015)
Introduction: The association of vaspin and visfatin, with a myocardial infarction is still not fully understood. Reduced levels of adenine nucleotides are hallmarks of chronic heart failure. There is little data concerning the relationship between t
Externí odkaz:
https://doaj.org/article/db6ebd5553734f7b89ed03bb8d323c1a
Autor:
Cheng, Ting-Yun, Sánchez, H. Domínguez, Vega-Ferrero, J., Conselice, C. J., Siudek, M., Aragón-Salamanca, A., Bernardi, M., Cooke, R., Ferreira, L., Huertas-Company, M., Krywult, J., Palmese, A., Pieres, A., Malagón, A. A. Plazas, Rosell, A. Carnero, Gruen, D., Thomas, D., Bacon, D., Brooks, D., James, D. J., Hollowood, D. L., Friedel, D., Suchyta, E., Sanchez, E., Menanteau, F., Paz-Chinchón, F., Gutierrez, G., Tarle, G., Sevilla-Noarbe, I., Ferrero, I., Annis, J., Frieman, J., García-Bellido, J., Mena-Fernández, J., Honscheid, K., Kuehn, K., da Costa, L. N., Gatti, M., Raveri, M., Pereira, M. E. S., Rodriguez-Monroy, M., Smith, M., Kind, M. Carrasco, Aguena, M., Swanson, M. E. C., Weaverdyck, N., Doel, P., Miquel, R., Ogando, R. L. C., Gruendl, R. A., Allam, S., Hinton, S. R., Dodelson, S., Bocquet, S., Desai, S., Everett, S., Scarpine, V.
We compare the two largest galaxy morphology catalogues, which separate early and late type galaxies at intermediate redshift. The two catalogues were built by applying supervised deep learning (convolutional neural networks, CNNs) to the Dark Energy
Externí odkaz:
http://arxiv.org/abs/2209.06897
Autor:
Lisiecki, Krzysztof, Małek, Katarzyna, Siudek, Małgorzata, Pollo, Agnieszka, Krywult, Janusz, Karska, Agata, Junais
Publikováno v:
A&A 669, A95 (2023)
'Red nuggets' are a rare population of passive compact massive galaxies thought to be the first massive galaxies that formed in the Universe. First found at $z \sim 3$, they are even less abundant at lower redshifts, and it is believed that with time
Externí odkaz:
http://arxiv.org/abs/2208.04601
Autor:
Siudek, M., Malek, K., Pollo, A., Iovino, A., Haines, C. P., Bolzonella, M., Cucciati, O., Gargiulo, A., Granett, B., Krywult, J., Moutard, T., Scodeggio, M.
Publikováno v:
A&A 666, A131 (2022)
Aims. This study aims to explore the relationship between the physical properties of different galaxy subclasses and their environment based on the analysis of 31 631 VIMOS Public Extragalactic Redshift Survey (VIPERS) galaxies observed at 0.5 < z <
Externí odkaz:
http://arxiv.org/abs/2205.14736
Autor:
Turner, Sebastian, Siudek, Małgorzata, Salim, Samir, Baldry, Ivan K., Pollo, Agnieszka, Longmore, Steven N., Małek, Katarzyna, Collins, Chris A., Lisboa, Paulo J., Krywult, Janusz, Moutard, Thibaud, Vergani, Daniela, Fritz, Alexander
The colour bimodality of galaxies provides an empirical basis for theories of galaxy evolution. However, the balance of processes that begets this bimodality has not yet been constrained. A more detailed view of the galaxy population is needed, which
Externí odkaz:
http://arxiv.org/abs/2102.05056