Zobrazeno 1 - 10
of 1 344
pro vyhledávání: '"Solimano A"'
Autor:
Lopez, S., Afruni, A., Zamora, D., Tejos, N., Ledoux, C., Hernandez, J., Berg, T. A. M., Cortes, H., Urbina, F., Johnston, E. J., Barrientos, L. F., Bayliss, M. B., Cuellar, R., Krogager, J. K., Noterdaeme, P., Solimano, M.
We present VLT/MUSE integral-field spectroscopy ($R\approx 1\,800$) of four giant gravitational arcs exhibiting strong C IV absorption at 8 intervening redshifts, $z_{abs}\approx 2.0$--$2.5$. We detect C IV absorption in a total of 222 adjacent and s
Externí odkaz:
http://arxiv.org/abs/2410.03029
Autor:
Li, Juno, Da Cunha, Elisabete, González-López, Jorge, Aravena, Manuel, De Looze, Ilse, Schreiber, N. M. Förster, Herrera-Camus, Rodrigo, Spilker, Justin, Tadaki, Ken-ichi, Barcos-Munoz, Loreto, Battisti, Andrew J., Birkin, Jack E., Bowler, Rebecca A. A., Davies, Rebecca, Díaz-Santos, Tanio, Ferrara, Andrea, Fisher, Deanne B., Hodge, Jacqueline, Ikeda, Ryota, Killi, Meghana, Lee, Lilian, Liu, Daizhong, Lutz, Dieter, Mitsuhashi, Ikki, Naab, Thorsten, Posses, Ana, Relaño, Monica, Solimano, Manuel, Übler, Hannah, van der Giessen, Stefan Anthony, Villanueva, Vicente
Using a combination of HST, JWST, and ALMA data, we perform spatially resolved spectral energy distributions (SED) fitting of fourteen 4
Externí odkaz:
http://arxiv.org/abs/2409.10961
Autor:
Lines, N. E. P., Bowler, R. A. A., Adams, N. J., Fisher, R., Varadaraj, R. G., Nakazato, Y., Aravena, M., Assef, R. J., Birkin, J. E., Ceverino, D., da Cunha, E., Cullen, F., De Looze, I., Donnan, C. T., Dunlop, J. S., Ferrara, A., Grogin, N. A., Herrera-Camus, R., Ikeda, R., Koekemoer, A. M., Killi, M., Li, J., McLeod, D. J., McLure, R. J., Mitsuhashi, I., Pérez-González, P. G., Relano, M., Solimano, M., Spilker, J. S., Villanueva, V., Yoshida, N.
We present a spatially resolved analysis of four star-forming galaxies at $z = 4.44-5.64$ using data from the JWST PRIMER and ALMA-CRISTAL surveys to probe the stellar and inter-stellar medium properties on the sub-kpc scale. In the $1-5\,\mu{\rm m}$
Externí odkaz:
http://arxiv.org/abs/2409.10963
Autor:
Catán, V., González-López, J., Solimano, M., Barrientos, L. F., Afruni, A., Aravena, M., Bayliss, M., Hernández, J. A., Ledoux, C., Mahler, G., Tejos, N.
This study aims to investigate the molecular gas content of strongly magnified low-mass star-forming galaxies around the cosmic noon period ($z\sim2$) through observations of CO emission lines and dust continuum emission, both of which serve as trace
Externí odkaz:
http://arxiv.org/abs/2408.07849
Autor:
Ikeda, Ryota, Tadaki, Ken-ichi, Mitsuhashi, Ikki, Aravena, Manuel, De Looze, Ilse, Schreiber, Natascha M. Förster, González-López, Jorge, Herrera-Camus, Rodrigo, Spilker, Justin, Barcos-Muñoz, Loreto, da Cunha, Elisabete, Davies, Rebecca, Díaz-Santos, Tanio, Ferrara, Andrea, Killi, Meghana, Lee, Lilian L., Li, Juno, Lutz, Dieter, Smit, Renske, Solimano, Manuel, Telikova, Kseniia, Übler, Hannah, Veilleux, Sylvain, Villanueva, Vicente
We investigate the spatial extent of the [CII] line emission in a sample of 34 galaxies at $z=4-6$ from the ALMA-CRISTAL Survey. By modeling the [CII] line emission in the visibility data directly, we derive the effective radius of [CII] line emissio
Externí odkaz:
http://arxiv.org/abs/2408.03374
Autor:
Solimano, M., González-López, J., Aravena, M., Pampliega, B. Alcalde, Assef, R. J., Béthermin, M., Boquien, M., Bovino, S., Casey, C. M., Cassata, P., da Cunha, E., Davies, R. L., De Looze, I., Ding, X., Díaz-Santos, T., Faisst, A. L., Ferrara, A., Fisher, D. B., Förster-Schreiber, N. M., Fujimoto, S., Ginolfi, M., Gruppioni, C., Guaita, L., Hathi, N., Herrera-Camus, R., Ibar, E., Inami, H., Jones, G. C., Koekemoer, A. M., Lee, L., Li, J., Liu, D., Liu, Z., Molina, J., Ogle, P., Posses, A. C., Pozzi, F., Relaño, M., Riechers, D. A., Romano, M., Spilker, J., Sulzenauer, N., Telikova, K., Vallini, L., Vasan, K. G. C., Veilleux, S., Vergani, D., Villanueva, V., Wang, W., Yan, L., Zamorani, G.
We present new JWST/NIRSpec IFU observations of the J1000+0234 system at $z=4.54$, the dense core of a galaxy protocluster hosting a massive, dusty star forming galaxy (DSFG) with a low luminosity radio counterpart. The new data reveals two extended,
Externí odkaz:
http://arxiv.org/abs/2407.13020
Autor:
Villanueva, V., Herrera-Camus, R., Gonzalez-Lopez, J., Aravena, M., Assef, R. J., Baeza-Garay, Mauricio, Barcos-Muñoz, L., Bovino, S., Bowler, R. A. A., da Cunha, E., De Looze, I., Diaz-Santos, T., Ferrara, A., Foerster-Schreiber, N., Algera, H., Iked, R., Killi, M., Mitsuhashi, I., Naab, T., Relano, M., Spilker, J., Solimano, M., Palla, M., Price, S. H., Posses, A., Tadaki, K., Telikova, K., Übler, H.
We present new $\lambda_{\rm rest}=77$ $\mu$m dust continuum observations from the ALMA of HZ10 (CRISTAL-22), a dusty main-sequence galaxy at $z$=5.66 as part of the [CII] Resolved Ism in STar-forming Alma Large program, CRISTAL. The high angular res
Externí odkaz:
http://arxiv.org/abs/2407.09681
Autor:
Posses, A., Aravena, M., González-López, J., Schreiber, N. M. Förster, Liu, D., Lee, L., Solimano, M., Díaz-Santos, T., Assef, R. J., Barcos-Muñoz, L., Bovino, S., Bowler, R. A. A., Rivera, G. Calistro, da Cunha, E., Davies, R. L., Killi, M., De Looze, I., Ferrara, A., Fisher, D. B., Herrera-Camus, R., Ikeda, R., Lambert, T., Li, J., Lutz, D., Mitsuhashi, I., Palla, M., Relaño, M., Spilker, J., Naab, T., Tadaki, K., Telikova, K., Übler, H., van der Giessen, S., Villanueva, V.
The ALMA [CII] Resolved Ism in STar-forming gALaxies (CRISTAL) survey is a Cycle 8 ALMA Large Programme that studies the cold gas component of high-redshift galaxies. Its sub-arcsecond resolution observations are key to disentangling physical mechani
Externí odkaz:
http://arxiv.org/abs/2403.03379
Autor:
Welch, Brian, Olivier, Grace M., Hutchison, Taylor A., Rigby, Jane R., Berg, Danielle A., Aravena, Manuel, Bayliss, Matthew B., Birkin, Jack E., Chapman, Scott C., Dahle, Håkon, Khullar, Gourav, Kim, Keunho J., Mahler, Guillaume, Malkan, Matthew A., Narayanan, Desika, Phadke, Kedar A., Sharon, Keren, Smith, J. D. T., Solimano, Manuel, Spilker, Justin S., Viera, Joaquin D., Vizgan, David
Using integrated spectra for two gravitationally lensed galaxies from the JWST TEMPLATES Early Release Science program, we analyze faint auroral lines, which provide direct measurements of the gas-phase chemical abundance. For the brighter galaxy, SG
Externí odkaz:
http://arxiv.org/abs/2401.13046
Autor:
Solimano, M., González-López, J., Aravena, M., Herrera-Camus, R., De Looze, I., Schreiber, N. M. Förster, Spilker, J., Tadaki, K., Assef, R. J., Barcos-Muñoz, L., Davies, R. L., Díaz-Santos, T., Ferrara, A., Fisher, D. B., Guaita, L., Ikeda, R., Johnston, E. J., Lutz, D., Mitsuhashi, I., Moya-Sierralta, C., Relaño, M., Naab, T., Posses, A. C., Telikova, K., Übler, H., van der Giessen, S., Villanueva, V.
Publikováno v:
A&A 689, A145 (2024)
Massive star-forming galaxies in the high-redshift universe host large reservoirs of cold gas in their circumgalactic medium (CGM). Traditionally, these reservoirs have been linked to diffuse H I Lyman-$\alpha$ (Ly$\alpha)$ emission extending beyond
Externí odkaz:
http://arxiv.org/abs/2401.04919