Zobrazeno 1 - 10
of 366
pro vyhledávání: '"Méndez, A. H."'
Even after decades of usage as an extragalactic standard candle, the universal bright end of the planetary nebula luminosity function (PNLF) still lacks a solid theoretical explanation. Until now, models have modeled planetary nebulae (PNe) from arti
Externí odkaz:
http://arxiv.org/abs/2412.08702
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:
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:
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:
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
Autor:
Filippi, Leonardo S., Juárez Valieri, Rubén D., Gallina, Pablo A., Méndez, Ariel H., Gianechini, Federico A., Garrido, Alberto C.
Publikováno v:
In Cretaceous Research February 2024 154
Autor:
Garilli, B., McLure, R., Pentericci, L., Franzetti, P., Gargiulo, A., Carnall, A., Cucciati, O., Iovino, A., Amorin, R., Bolzonella, M., Bongiorno, A., Castellano, M., Cimatti, A., Cirasuolo, M., Cullen, F., Dunlop, J., Elbaz, D., Finkelstein, S., Fontana, A., Fontanot, F., Fumana, M., Guaita, L., Hartley, W., Jarvis, M., Juneau, S., Maccagni, D., McLeod, D., Nandra, K., Pompei, E., Pozzetti, L., Scodeggio, M., Talia, M., Calabro', A., Cresci, G., Fynbo, J. P. U., Hathi, N. P., Hibon, P., Koekemoer, A. M., Magliocchetti, M., Salvato, M., Vietri, G., Zamorani, G., Almaini, O., Balestra, I., Bardelli, S., Begley, R., Brammer, G., Bell, E. F., Bowler, R. A. A., Brusa, M., Buitrago, F., Caputi, C., Cassata, P., Charlot, S., Citro, A., Cristiani, S., Curtis-Lake, E., Dickinson, M., Fazio, G., Ferguson, H. C., Fiore, F., Franco, M., Georgakakis, A., Giavalisco, M., Grazian, A., Hamadouche, M., Jung, I., Kim, S., Khusanova, Y., Fevre, O. Le, Longhetti, M., Lotz, J., Mannucci, F., Maltby, D., Matsuoka, K., Mendez-Hernandez, H., Mendez-Abreu, J., Mignoli, M., Moresco, M., Nonino, M., Pannella, M., Papovich, C., Popesso, P., Roberts-Borsani, G., Rosario, D. J., Saldana-Lopez, A., Santini, P., Saxena, A., Schaerer, D., Schreiber, C., Stark, D., Tasca, L. A. M., Thomas, R., Vanzella, E., Wild, V., Williams, C., Zucca, E.
Publikováno v:
A&A 647, A150 (2021)
VANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high signal to noise, medium resolution spectra of galaxies at redshift between 1 and 6.5. Here we present the final Public Data Release of the VANDELS Survey, comprising 208
Externí odkaz:
http://arxiv.org/abs/2101.07645
Autor:
Méndez-Hernández, H., Ibar, E., Knudsen, K. K., Cassata, P., Aravena, M., Michałowski, M. J., Zhang, Zhi-Yu, Lara-López, M. A., Ivison, R. J., van der Werf, P., Villanueva, V., Herrera-Camus, R., Hughes, T. M.
We present Atacama Large Millimeter/sub-millimeter Array (ALMA) observations towards 27 low-redshift ($0.02< z<0.2$) star-forming galaxies taken from the Valpara\'iso ALMA/APEX Line Emission Survey (VALES). We perform stacking analyses of the $^{12}$
Externí odkaz:
http://arxiv.org/abs/2007.01182
Autor:
Fujimoto, S., Silverman, J. D., Bethermin, Matthieu, Ginolfi, M., Jones, G. C., Fèvre, O. Le, Dessauges-Zavadsky, M., Rujopakarn, W., Faisst, A. L., Fudamoto, Y., Cassata, P., Morselli, L., Maiolino, R., Schaerer, D., Capak, P., Yan, L., Vallini, L., Toft, S., Loiacono, F., Zamorani, G., Talia, M., Narayanan, D., Hathi, N. P., Lemaux, B. C., Boquien, Médéric, Amorin, R., Ibar, E., Koekemoer, A. M., Méndez-Hernández, H., Bardelli, Sandro, Vergani, D., Zucca, E., Romano, M., Cimatti, A.
We present the physical extent of [CII] 158um line-emitting gas from 46 star-forming galaxies at z=4-6 from the ALMA Large Program to INvestigate CII at Early Times (ALPINE). Using exponential profile fits, we measure the effective radius of the [CII
Externí odkaz:
http://arxiv.org/abs/2003.00013