Zobrazeno 1 - 10
of 1 952
pro vyhledávání: '"A. Mendez-Hernandez"'
Autor:
Sawant, P., Nanni, A., Romano, M., Donevski, D., Bruzual, G., Ysard, N., Lemaux, B. C., Inami, H., Calura, F., Pozzi, F., Małek, K., Junais, Boquien, M., Faisst, A. L., Hamed, M., Ginolfi, M., Zamorani, G., Lorenzon, G., Molina, J., Bardelli, S., Ibar, E., Vergani, D., Di Cesare, C., Béthermin, M., Burgarella, D., Cassata, P., Dessauges-Zavadsky, M., D'Onghia, E., Dubois, Y., Magdis, G. E., Mendez-Hernandez, H.
Recent observations reveal a rapid dust build-up in high-redshift galaxies (z > 4), challenging current models of galaxy formation. While our understanding of dust production and destruction in the interstellar medium (ISM) is advancing, probing bary
Externí odkaz:
http://arxiv.org/abs/2412.02505
Autor:
Sifón, Cristóbal, Finoguenov, Alexis, Haines, Christopher P., Jaffé, Yara, Amrutha, B. M., Demarco, Ricardo, Lima, E. V. R., Lima-Dias, Ciria, Méndez-Hernández, Hugo, Merluzzi, Paola, Monachesi, Antonela, Teixeira, Gabriel S. M., Tejos, Nicolas, Araya-Araya, Pablo, Argudo-Fernández, Maria, Baier-Soto, Raúl, Bilton, Lawrence E., Bom, C. R., Calderón, Juan Pablo, Cassarà, Letizia P., Comparat, Johan, Courtois, H. M., D'Ago, Giuseppe, Dupuy, Alexandra, Fritz, Alexander, Haack, Rodrigo F., Herpich, Fabio R., Ibar, E., Kuchner, Ulrike, Lopes, Amanda R., Lopez, Sebastian, Lösch, Elismar, McGee, Sean, de Oliveira, C. Mendes, Morelli, Lorenzo, Moretti, Alessia, Pallero, Diego, Piraino-Cerda, Franco, Pompei, Emanuela, Rescigno, U., Smith, Rory, Castelli, Analía V. Smith, Sodré Jr, Laerte, Tempel, Elmo
CHANCES, the CHileAN Cluster galaxy Evolution Survey, will study the evolution of galaxies in and around ${\sim}$150 massive galaxy clusters, from the local universe out to z=0.45. CHANCES will use the new 4MOST Spectroscopic Survey Facility on the V
Externí odkaz:
http://arxiv.org/abs/2411.13655
Autor:
Killi, Meghana, Ginolfi, Michele, Popping, Gergö, Watson, Darach, Zamorani, Giovanni, Lemaux, Brian C., Fujimoto, Seiji, Faisst, Andreas, Bethermin, Matthieu, Romano, Michael, Fudamoto, Yoshinobu, Bardelli, Sandro, Boquien, Médéric, Carniani, Stefano, Dessauges-Zavadsky, Miroslava, Gruppioni, Carlotta, Hathi, Nimish, Ibar, Eduardo, Jones, Gareth C., Koekemoer, Anton M., Langan, Ivanna, Méndez-Hernández, Hugo, Sugahara, Yuma, Vallini, Livia, Vergani, Daniela
Galaxy morphology is shaped by stellar activity, feedback, gas and dust properties, and interactions with surroundings, and can therefore provide insight into these processes. In this paper, we study the spatial offsets between stellar and interstell
Externí odkaz:
http://arxiv.org/abs/2402.07982
Autor:
Cerdosino, M. C., O'Mill, A. L., Rodriguez, F., Taverna, A., Sodré Jr, L., Telles, E., Méndez-Hernández, H., Schoenell, W., Ribeiro, T., Kanaan, A., de Oliveira, C. Mendez
In this paper, we use photometric data from the S-PLUS DR4 survey to identify isolated galaxy pairs and analyse their characteristics and properties. Our results align with previous spectroscopic studies, particularly in luminosity function parameter
Externí odkaz:
http://arxiv.org/abs/2402.00120
Autor:
Devereaux, T., Cassata, P., Ibar, E., Accard, C., Guillaume, C., Béthermin, M., Dessauges-Zavadsky, M., Faisst, A., Jones, G. C., Zanella, A., Bardelli, S., Boquien, M., D'Onghia, E., Giavalisco, M., Ginolfi, M., Gobat, R., Hayward, C. C., Koekemoer, A. M., Lemaux, B., Magdis, G., Mendez-Hernandez, H., Molina, J., Pozzi, F., Romano, M., Tasca, L., Vergani, D., Zamorani, G., Zucca, E.
Publikováno v:
A&A 686, A156 (2024)
Context: From redshift 6 to redshift $\approx$ 4 galaxies grow rapidly from low mass galaxies towards the more mature massive galaxies we see at the cosmic noon. Growth via gas accretion and mergers undoubtedly shape this evolution - however, there c
Externí odkaz:
http://arxiv.org/abs/2311.11493
Autor:
Lima-Dias, Ciria, Monachesi, Antonela, Torres-Flores, Sergio, Cortesi, Arianna, Hernández-Lang, Daniel, Montaguth, Gissel P., Jiménez-Teja, Yolanda, Panda, Swayamtrupta, Menéndez-Delmestre, Karín, Gonçalves, Thiago S., Méndez-Hernández, Hugo, Telles, Eduardo, Dimauro, Paola, Bom, Clécio R., de Oliveira, Claudia Mendes, Kanaan, Antonio, Ribeiro, Tiago, Schoenell, William
When a galaxy falls into a cluster, its outermost parts are the most affected by the environment. In this paper, we are interested in studying the influence of a dense environment on different galaxy's components to better understand how this affects
Externí odkaz:
http://arxiv.org/abs/2311.09313
Autor:
Méndez-Hernández, H., Cassata, P., Ibar, E., Amorín, R, Aravena, M., Bardelli, S., Cucciati, O., Garilli, B., Giavalisco, M., Guaita, L., Hathi, N., Koekemoer, A., Brun, V. Le, Lemaux, B. C., Maccagni, D., Ribeiro, B., Tasca, L., Tejos, N., Thomas, R., Tresse, L., Vergani, D., Zamorani, G., Zucca, E.
Publikováno v:
A&A 666, A56 (2022)
The circumgalactic medium (CGM) is the location where the interplay between large-scale outflows and accretion onto galaxies occurs. Metals in different ionization states flowing between the circumgalactic and intergalactic mediums are affected by la
Externí odkaz:
http://arxiv.org/abs/2206.08923
Autor:
Chopra, Vianni, Fuentes-Velasco, Valeria, Nacif-Lopez, Samyr R., Melendez-Malpicca, Juliette, Mendez-Hernandez, Ana S., Ramos-Mendez-Iris, Luis F., Arroyo-Jimenez, Denev A., Reyes-Segura, Diana G., Gonzalez-Y-Mendoza, Pamela, Sanchez-Hernandez, K. Aline, Spinola-Corona, Estefania, Vazquez-del-Mercado-Pardiño, Jorge A., Chauhan, Gaurav
Publikováno v:
In Ceramics International 15 October 2024 50(20) Part B:38819-38840
Autor:
Romano, Michael, Morselli, L., Cassata, P., Ginolfi, M., Schaerer, D., Béthermin, M., Capak, P., Faisst, A., Fèvre, O. Le, Silverman, J. D., Yan, L., Bardelli, S., Boquien, M., Dessauges-Zavadsky, M., Fujimoto, S., Hathi, N. P., Jones, G. C., Koekemoer, A. M., Lemaux, B. C., Méndez-Hernández, H., Narayanan, D., Talia, M., Vergani, D., Zamorani, G., Zucca, E.
Publikováno v:
A&A 660, A14 (2022)
The [CII] 158$~\mu$m emission line represents so far one of the most profitable tools for the investigation of the high-redshift galaxies in the early Universe. Being one of the brightest cooling lines in the rest-frame far-infrared regime of star-fo
Externí odkaz:
http://arxiv.org/abs/2202.02334
Publikováno v:
In Journal of Non-Crystalline Solids 1 August 2024 637