Zobrazeno 1 - 10
of 42 268
pro vyhledávání: '"A, Arango"'
Autor:
Shuntov, M., Ilbert, O., Toft, S., Arango-Toro, R. C., Akins, H. B., Casey, C. M., Franco, M., Harish, S., Kartaltepe, J. S., Koekemoer, A. M., McCracken, H. J., Paquereau, L., Laigle, C., Bethermin, M., Dubois, Y., Drakos, N. E., Faisst, A., Gozaliasl, G., Gillman, S., Hayward, C. C., Hirschmann, M., Huertas-Company, M., Jespersen, C. K., Jin, S., Kokorev, V., Lambrides, E., Borgne, D. Le, Liu, D., Magdis, G., Massey, R., McPartland, C. J. R., Mercier, W., McCleary, J. E., McKinney, J., Oesch, P. A., Rhodes, J. D., Rich, R. M., Robertson, B. E., Sanders, D., Trebitsch, M., Tresse, L., Valentino, F., Vijayan, A. P., Weaver, J. R., Weibel, A., Wilkins, S. M.
We study the stellar mass function (SMF) and the co-evolution with dark matter halos via abundance matching in the largest redshift range to date $0.25$, we find increas
Externí odkaz:
http://arxiv.org/abs/2410.08290
Autor:
Arango-Toro, R. C., Ilbert, O., Ciesla, L., Shuntov, M., Aufort, G., Mercier, W., Laigle, C., Franco, M., Bethermin, M., Borgne, D. Le, Dubois, Y., McCracken, H. J., Paquereau, L., Huertas-Company, M., Kartaltepe, J., Casey, C. M., Akins, H., Allen, N., Andika, I., Brinch, M., Drakos, N. E., Faisst, A., Gozaliasl, G., Harish, S., Kaminsky, A., Koekemoer, A., Kokorev, V., Liu, D., Magdis, G., Martin, C. L., Moutard, T., Rhodes, J., Rich, R. M., Robertson, B., Sanders, D. B., Sheth, K., Talia, M., Toft, S., Tresse, L., Valentino, F., Vijayan, A., Weaver, J.
The stellar mass-star formation rate (M$_\star$ - SFR) plane is essential for distinguishing galaxy populations, but how galaxies move within this plane over cosmic time remains unclear. This study aims to describe galaxy migrations in the M$_\star$
Externí odkaz:
http://arxiv.org/abs/2410.05375
Autor:
Arango, Sebastian Pineda, Janowski, Maciej, Purucker, Lennart, Zela, Arber, Hutter, Frank, Grabocka, Josif
Ensemble methods are known for enhancing the accuracy and robustness of machine learning models by combining multiple base learners. However, standard approaches like greedy or random ensembles often fall short, as they assume a constant weight acros
Externí odkaz:
http://arxiv.org/abs/2410.04520
Autor:
Aufort, G., Laigle, C., McCracken, H. J., Borgne, D. Le, Arango-Toro, R., Ciesla, L., Ilbert, O., Tresse, L., Dubois, Y.
We propose a novel method to reconstruct the full posterior distribution of the star formation histories (SFHs) of galaxies from broad-band photometry. Our method combines simulation-based inference (SBI) using a neural network trained with SFHs and
Externí odkaz:
http://arxiv.org/abs/2410.00795
In this work, we study the function $f_2(G)$ that counts the number of exact factorizations of a finite group $G$. We compute $f_2(G)$ for some well-known families of finite groups and use the results of Wiegold and Williamson \cite{WW} to derive an
Externí odkaz:
http://arxiv.org/abs/2409.10428
A proper subdomain $G$ of the unit disk $\mathbb{D}$ is horocyclically convex (horo-convex) if, for every $\omega \in \mathbb{D}\cap \partial G$, there exists a horodisk $H$ such that $\omega \in \partial H$ and $G\cap H=\emptyset$. In this paper we
Externí odkaz:
http://arxiv.org/abs/2407.21271
Energy system models are crucial for planning, supporting, and understanding energy transition pathways. Flexible energy modelling tools have emerged to provide practitioners, planners, and decision-makers with various alternatives to represent diver
Externí odkaz:
http://arxiv.org/abs/2407.05451
Autor:
Sierra-Botero, Daniel, Molina-Taborda, Ana, Valdés-Tresanco, Mario S., Hernández-Arango, Alejandro, Espinosa-Leal, Leonardo, Karpenko, Alexander, Lopez-Acevedo, Olga
In healthcare there is a pursuit for employing interpretable algorithms to assist healthcare professionals in several decision scenarios. Following the Predictive, Descriptive and Relevant (PDR) framework, the definition of interpretable machine lear
Externí odkaz:
http://arxiv.org/abs/2406.10213
The dissociation micro-states (DMS) of an $N$-protic acid are described using set theory notation. This facilitates the mathematical description of the dissociation micro-equilibrium (DME). In particular, the DME constants are easily obtained in term
Externí odkaz:
http://arxiv.org/abs/2405.09692
Autor:
Faisst, A. L., Brinch, M., Casey, C. M., Chartab, N., Dessauges-Zavadsky, M., Drakos, N. E., Gillman, S., Gonzaliasl, G., Hayward, C. C., Ilbert, O., Jablonka, P., Kartaltepe, J. S., Koekemoer, A. M., Kokorev, V., Lambrides, E., Liu, D., Maraston, C., Martin, C. L., Renzini, A., Robertson, B. E., Sanders, D. B., Sattari, Z., Scoville, N., Urry, C. M., Vijayan, A. P., Weaver, J. R., Akins, H. B., Allen, N., Arango-Toro, R. C., Cooper, O. R., Franco, M., Gentile, F., Harish, S., Hirschmann, M., Khostovan, A. A., Laigle, C., Larson, R. L., Lee, M., Liu, Z., Long, A. S., Magdis, G., Massey, R., McCracken, H. J., McKinney, J., Paquereau, L., Rhodes, J., Rich, R. M., Shuntov, M., Silverman, J. D., Talia, M., Toft, S., Zavala, J. A.
We study of the role of galaxy-galaxy interactions and disk instabilities in producing starburst activity in galaxies out to z=4. For this, we use a sample of 387 galaxies with robust total star formation rate measurements from Herschel, gas masses f
Externí odkaz:
http://arxiv.org/abs/2405.09619