Unveiling the nature of infrared bright, optically dark galaxies with early JWST data

Autor: L Barrufet, P A Oesch, A Weibel, G Brammer, R Bezanson, R Bouwens, Y Fudamoto, V Gonzalez, R Gottumukkala, G Illingworth, K E Heintz, B Holden, I Labbe, D Magee, R P Naidu, E Nelson, M Stefanon, R Smit, P van Dokkum, J R Weaver, C C Williams

Publikováno v: Barrufet, L, Oesch, P A, Weibel, A, Brammer, G, Bezanson, R, Bouwens, R, Fudamoto, Y, Gonzalez, V, Gottumukkala, R, Illingworth, G, Heintz, K E, Holden, B, Labbe, I, Magee, D, Naidu, R P, Nelson, E, Stefanon, M, Smit, R, Van dokkum, P, Weaver, J R & Williams, C C 2023, ' Unveiling the nature of infrared bright, optically dark galaxies with early JWST data ', Monthly Notices of the Royal Astronomical Society, vol. 522, no. 1, pp. 449-456 . https://doi.org/10.1093/mnras/stad947

Over the last few years, both ALMA and Spitzer/IRAC observations have revealed a population of likely massive galaxies at $z>3$ that was too faint to be detected in HST rest-frame ultraviolet imaging. However, due to the very limited photometry for i

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::68f0042ff79daee280306618a4ae3478
https://curis.ku.dk/portal/da/publications/unveiling-the-nature-of-infrared-bright-optically-dark-galaxies-with-early-jwst-data(4282a224-4e79-41c3-9991-940eaab2fcb0).html

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The ALMA REBELS Survey: discovery of a massive, highly star-forming, and morphologically complex ULIRG at z = 7.31

Autor: A P S Hygate, J A Hodge, E da Cunha, M Rybak, S Schouws, H Inami, M Stefanon, L Graziani, R Schneider, P Dayal, R J Bouwens, R Smit, R A A Bowler, R Endsley, V Gonzalez, P A Oesch, D P Stark, H S B Algera, M Aravena, L Barrufet, A Ferrara, Y Fudamoto, J H A Hilhorst, I De Looze, T Nanayakkara, A Pallottini, D A Riechers, L Sommovigo, M W Topping, P van der Werf

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: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6218f2d3be90e76d1f169ef55b122dcf
https://hdl.handle.net/11384/132062

The ALMA REBELS Survey: Average [CII] 158μm Sizes of Star-forming Galaxies from z~7 to z~4

Autor: Y. Fudamoto, R. Smit, R. A. A. Bowler, P. A. Oesch, R. Bouwens, M. Stefanon, H. Inami, R. Endsley, V. Gonzalez, S. Schouws, D. Stark, H. S. B. Algera, M. Aravena, L. Barrufet, E. da Cunha, P. Dayal, A. Ferrara, L. Graziani, J. A. Hodge, A. P. S. Hygate, A. K. Inoue, T. Nanayakkara, A. Pallottini, E. Pizzati, R. Schneider, L. Sommovigo, Y. Sugahara, M. Topping, P. van der Werf, M. Bethermin, P. Cassata, M. Dessauges-Zavadsky, E. Ibar, A. L. Faisst, S. Fujimoto, M. Ginolfi, N. Hathi, G. C. Jones, F. Pozzi, D. Schaerer

Publikováno v: Astrophysical Journal, 934(2):144. IOP PUBLISHING LTD
The Astrophysical Journal, 934(2):144
The Astrophysical Journal
The Astrophysical Journal, 2022, 934, ⟨10.3847/1538-4357/ac7a47⟩

We present the average [C ii] 158 μm emission line sizes of UV-bright star-forming galaxies at z ∼ 7. Our results are derived from a stacking analysis of [C ii] 158 μm emission lines and dust continua observed by the Atacama Large Millimeter/subm

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::73350a0467609f2a112d0f10968f10cf
https://research.rug.nl/en/publications/bc400b3b-c506-47f0-87ee-3c709bc327b8