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: 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

The ALMA REBELS Survey: cosmic dust temperature evolution out to z~7

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

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 513(3), 3122-3135
Sommovigo, L, Ferrara, A, Pallottini, A, Dayal, P, Bouwens, R J, Smit, R, Da cunha, E, De looze, I, Bowler, R A A, Hodge, J, Inami, H, Oesch, P, Endsley, R, Gonzalez, V, Schouws, S, Stark, D, Stefanon, M, Aravena, M, Graziani, L, Riechers, D, Schneider, R, Van der werf, P, Algera, H, Barrufet, L, Fudamoto, Y, Hygate, A P S, Labbé, I, Li, Y, Nanayakkara, T & Topping, M 2022, ' The ALMA REBELS Survey : cosmic dust temperature evolution out to z ∼ 7 ', Monthly Notices of the Royal Astronomical Society, vol. 513, no. 3, pp. 3122-3135 . https://doi.org/10.1093/mnras/stac302
Monthly Notices of the Royal Astronomical Society, 513(3), 3122-3135. Oxford University Press
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

ALMA observations have revealed the presence of dust in the first generations of galaxies in the Universe. However, the dust temperature Td remains mostly unconstrained due to the few available FIR continuum data at redshift $z$ > 5. This introduces

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::339c1b75ed0983ce3f39e506dfd29829