Zobrazeno 1 - 10
of 594
pro vyhledávání: '"Inami H"'
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
Publikováno v:
Clinical Ophthalmology, Vol Volume 15, Pp 3687-3695 (2021)
Yuji Yoshikawa, Takuhei Shoji, Junji Kanno, Hisashi Ibuki, Kimitake Ozaki, Hirokazu Ishii, Hiromi Inami, Kei Shinoda Department of Ophthalmology, Saitama Medical University, Iruma, Saitama, JapanCorrespondence: Kei ShinodaDepartment of Ophthalmology,
Externí odkaz:
https://doaj.org/article/f84d009a542a4f1b806c9d9c2883cd94
Autor:
van Leeuwen, I. F., Bouwens, R. J., van der Werf, P. P., Hodge, J. A., Schouws, S., Stefanon, M., Algera, H. S. B., Aravena, M., Boogaard, L. A., Bowler, R. A . A., da Cunha, E., Dayal, P., Decarli, R., Gonzalez, V., Inami, H., de Looze, I., Sommovigo, L., Venemans, B. P., Walter, F., Barrufet, L., Ferrara, A., Graziani, L., Hygate, A. P. S., Oesch, P., Palla, M., Rowland, L., Schneider, R.
We present a new method to determine the star formation rate (SFR) density of the Universe at $z \gtrsim 5$ that includes the contribution of dust-obscured star formation. For this purpose, we use a [CII] (158 $\mu$m) selected sample of galaxies sere
Externí odkaz:
http://arxiv.org/abs/2409.11463
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.
Galaxy protoclusters are sites of rapid growth, with a high density of massive galaxies driving elevated rates of star formation and accretion onto supermassive black holes. Here, we present new JWST/NIRSpec IFU observations of the J1000+0234 group a
Externí odkaz:
http://arxiv.org/abs/2407.13020
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:
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
Autor:
Barrufet, L., Oesch, P. A., Bouwens, R., Inami, H., Sommovigo, L., Algera, H., da Cunha, E., Aravena, M., Dayal, P., Ferrara, A., Fudamoto, Y., Gonzalez, V., Graziani, L., Hygate, A., de Looze, I., Nanayakkara, T., Pallottini, A., Schneider, R., Stefanon, M., Topping, M., van Der Werf, P.
We present the first observational infrared luminosity function (IRLF) measurement in the Epoch of Reionization (EoR) based on a UV-selected galaxy sample with ALMA spectroscopic observations. Our analysis is based on the ALMA large program Reionizat
Externí odkaz:
http://arxiv.org/abs/2303.11321
Autor:
Rich, J., Aalto, S., Evans, A. S., Charmandaris, V., Privon, G. C., Lai, T., Inami, H., Linden, S., Armus, L., Diaz-Santos, T., Appleton, P., Barcos-Muñoz, L., Böker, T., Larson, K. L., Law, D. R., Malkan, M. A., Medling, A. M., Song, Y., U, V., van der Werf, P., Bohn, T., Brown, M. J. I., Finnerty, L., Hayward, C., Howell, J., Iwasawa, K., Kemper, F., Marshall, J., Mazzarella, J. M., McKinney, J., Muller-Sanchez, F., Murphy, E. J., Sanders, D., Soifer, B. T., Stierwalt, S., Surace, J.
We present results from the James Webb Space Telescope (JWST) Director's Discretionary Time Early Release Science (ERS) program 1328 targeting the nearby, Luminous Infrared Galaxy (LIRG), VV 114. We use the MIRI and NIRSpec instruments to obtain inte
Externí odkaz:
http://arxiv.org/abs/2301.02338
Autor:
Ciesla, L., Gómez-Guijarro, C., Buat, V., Elbaz, D., Jin, S., Béthermin, M., Daddi, E., Franco, M., Inami, H., Magdis, G., Magnelli, B.
Publikováno v:
A&A 672, A191 (2023)
Recently, a population of compact main sequence (MS) galaxies exhibiting starburst-like properties have been identified in the GOODS-ALMA blind survey at 1.1mm. Several evolution scenarios were proposed to explain their particular physical properties
Externí odkaz:
http://arxiv.org/abs/2211.02510