Zobrazeno 1 - 10
of 491
pro vyhledávání: '"Fudamoto Y."'
Autor:
Meyer, R. A., Oesch, P. A., Giovinazzo, E., Weibel, A., Brammer, G., Matthee, J., Naidu, R. P., Bouwens, R. J., Chisholm, J., Covelo-Paz, A., Fudamoto, Y., Maseda, M., Nelson, E., Shivaei, I., Xiao, M., Herard-Demanche, T., Illingworth, G. D., Kerutt, J., Kramarenko, I., Labbe, I., Leonova, E., Magee, D., Matharu, J., Lyon, G. Prieto, Reddy, N., Schaerer, D., Shapley, A., Stefanon, M., Wozniak, M. A., Wuyts, S.
We present the census of H$\beta$+[OIII] 4960,5008 \AA emitters at 6.8
Externí odkaz:
http://arxiv.org/abs/2405.05111
Autor:
Barrufet, L., Oesch, P., Marques-Chaves, R., Arellano-Cordova, K., Baggen, J. F. W., Carnall, A. C., Cullen, F., Dunlop, J. S., Gottumukkala, R., Fudamoto, Y., Illingworth, G. D., Magee, D., McLure, R. J., McLeod, D. J., Michałowski, M. J., Stefanon, M., van Dokkum, P. G., Weibel, A.
The advent of the JWST has revolutionised our understanding of high-redshift galaxies. In particular, the NIRCam instrument on-board JWST has revealed a population of Hubble Space Telescope (HST)-dark galaxies that had previously evaded optical detec
Externí odkaz:
http://arxiv.org/abs/2404.08052
Autor:
Fujimoto, S., Ouchi, M., Kohno, K., Valentino, F., Giménez-Arteaga, C., Brammer, G. B., Furtak, L. J., Kohandel, M., Oguri, M., Pallottini, A., Richard, J., Zitrin, A., Bauer, F. E., Boylan-Kolchin, M., Dessauges-Zavadsky, M., Egami, E., Finkelstein, S. L., Ma, Z., Smail, I., Watson, D., Hutchison, T. A., Rigby, J. R., Welch, B. D., Ao, Y., Bradley, L. D., Caminha, G. B., Caputi, K. I., Espada, D., Endsley, R., Fudamoto, Y., González-López, J., Hatsukade, B., Koekemoer, A. M., Kokorev, V., Laporte, N., Lee, M., Magdis, G. E., Ono, Y., Rizzo, F., Shibuya, T., Shimasaku, K., Sun, F., Toft, S., Umehata, H., Wang, T., Yajima, H.
Early galaxy formation, initiated by the dark matter and gas assembly, evolves through frequent mergers and feedback processes into dynamically hot, chaotic structures. In contrast, dynamically cold, smooth rotating disks have been observed in massiv
Externí odkaz:
http://arxiv.org/abs/2402.18543
Autor:
Béthermin, M., Accard, C., Guillaume, C., Dessauges-Zavadsky, M., Ibar, E., Cassata, P., Devereaux, T., Faisst, A., Freundlich, J., Jones, G. C., Kraljic, K., Algera, H., Amorin, R. O., Bardelli, S., Boquien, M., Buat, V., Donghia, E., Dubois, Y., Ferrara, A., Fudamoto, Y., Ginolfi, M., Guillard, P., Giavalisco, M., Gruppioni, C., Gururajan, G., Hathi, N., Hayward, C. C., Koekemoer, A. M., Lemaux, B. C., Magdis, G. E., Molina, J., Narayanan, D., Mayer, L., Pozzi, F., Rizzo, F., Romano, M., Tasca, L., Theulé, P., Vergani, D., Vallini, L., Zamorani, G., Zanella, A., Zucca, E.
The Kennicutt-Schmidt (KS) relation between the gas and the star formation rate (SFR) surface density ($\Sigma_{\rm gas}$-$\Sigma_{\rm SFR}$) is essential to understand star formation processes in galaxies. So far, it has been measured up to z~2.5 in
Externí odkaz:
http://arxiv.org/abs/2311.08474
Autor:
Gottumukkala, R., Barrufet, L., Oesch, P. A., Weibel, A., Allen, N., Pampliega, B. Alcalde, Nelson, E. J., Williams, C. C., Brammer, G., Fudamoto, Y., González, V., Heintz, K. E., Illingworth, G., Magee, D., Naidu, R. P., Shuntov, M., Stefanon, M., Toft, S., Valentino, F., Xiao, M.
With the advent of JWST, we can probe the rest-frame optical emission of galaxies at $z>3$ with high sensitivity and spatial resolution, making it possible to accurately characterise red, optically-faint galaxies and thus move towards a more complete
Externí odkaz:
http://arxiv.org/abs/2310.03787
Autor:
Bowler, R. A. A., Inami, H., Sommovigo, L., Smit, R., Algera, H. S. B., Aravena, M., Barrufet, L., Bouwens, R., da Cunha, E., Cullen, F., Dayal, P., de Looze, I., Dunlop, J. S., Fudamoto, Y., Mauerhofer, V., McLure, R. J., Stefanon, M., Schneider, R., Ferrara, A., Graziani, L., Hodge, J. A., Nanayakkara, T., Palla, M., Schouws, S., Stark, D. P., van der Werf, P. P.
We investigate the degree of dust obscured star formation in 49 massive (${\rm log}_{10}(M_{\star}/{\rm M}_{\odot})>9$) Lyman-break galaxies (LBGs) at $z = 6.5$-$8$ observed as part of the ALMA Reionization Era Bright Emission Line Survey (REBELS) la
Externí odkaz:
http://arxiv.org/abs/2309.17386
Autor:
Aravena, M., Heintz, K. E., Dessauges-Zavadsky, M., Oesch, P. A., Algera, H. S. B., Bouwens, R. J., Da Cunha, E., Dayal, P., De Looze, I., Ferrara, A., Fudamoto, Y., Gonzalez, V., Graziani, L., Inami, H., Pallottini, A., Schneider, R., Schouws, S., Sommovigo, L., Topping, M., van der Werf, P., Palla, M.
A key to understanding the formation of the first galaxies is to quantify the content of the molecular gas as the fuel for star formation activity through the epoch of reionization. In this paper, we use the 158$\mu$m [CII] fine-structure emission li
Externí odkaz:
http://arxiv.org/abs/2309.15948
Autor:
Fudamoto, Y., Oesch, P. A., Walter, F., Decarli, R., Carilli, C. L., Ferrara, A., Barrufet, L., Bouwens, R., Dessauges-Zavadsky, M., Nelson, E. J., Dannerbauer, H., Illingworth, G., Inoue, A. K., Marques-Chaves, R., Pérez-Fournon, I., Riechers, D. A., Schaerer, D., Smit, R., Sugahara, Y., van der Werf, P.
We present results of dust continuum and [CII]$\,158\,{\rm \mu m}$ emission line observations of a remarkably UV-luminous ($M_{\rm UV}=-21.6$) galaxy at $z=10.603$: GN-z11. Using the Northern Extended Millimeter Array (NOEMA), observations have been
Externí odkaz:
http://arxiv.org/abs/2309.02493
Autor:
Wang, Bingjie, Fujimoto, Seiji, Labbe, Ivo, Furtak, Lukas J., Miller, Tim B., Setton, David J., Zitrin, Adi, Atek, Hakim, Bezanson, Rachel, Brammer, Gabriel, Leja, Joel, Oesch, Pascal A., Price, Sedona H., Chemerynska, Iryna, Cutler, Sam E., Dayal, Pratika, van Dokkum, Pieter, Goulding, Andy D., Greene, Jenny E., Fudamoto, Y., Khullar, Gourav, Kokorev, Vasily, Marchesini, Danilo, Pan, Richard, Weaver, John R., Whitaker, Katherine E., Williams, Christina C.
Publikováno v:
The Astrophysical Journal Letters, 957, L34 (2023)
Observations of high-redshift galaxies provide a critical direct test to the theories of early galaxy formation, yet to date, only three have been spectroscopically confirmed at $z>12$. Due to strong gravitational lensing over a wide area, the galaxy
Externí odkaz:
http://arxiv.org/abs/2308.03745
Autor:
Hygate, A. P. S., Hodge, J. A., da Cunha, E., Rybak, M., Schouws, S., Inami, H., Stefanon, M., Graziani, L., Schneider, R., Dayal, P., Bouwens, R. J., Smit, R., Bowler, R. A. A., Endsley, R., Gonzalez, V., Oesch, P. A., Stark, D. P., Algera, H. S. B., Aravena, M., Barrufet, L., Ferrara, A., Fudamoto, Y., A, J. H., De Looze, I., Nanayakkara, T., Pallottin, A., Riechers, D. A., Sommovigo, L., Topping, M. W., van der Werf, P.
We present Atacama Large Millimeter/Submillimeter Array (ALMA) [CII] and $\sim158$ $\rm\mu m$ continuum observations of REBELS-25, a massive, morphologically complex ultra-luminous infrared galaxy (ULIRG; $L_{\rm IR}=1.5^{+0.8}_{-0.5}\times10^{12}$ L
Externí odkaz:
http://arxiv.org/abs/2304.09206