Zobrazeno 1 - 10
of 1 949
pro vyhledávání: '"OBSCURED STAR-FORMATION"'
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:
Tarrasse, Maxime, Gómez-Guijarro, Carlos, Elbaz, David, Magnelli, Benjamin, Dickinson, Mark, Henry, Aurélien, Franco, Maximilien, Lyu, Yipeng, Billand, Jean-Baptiste, Bhatawdekar, Rachana, Cheng, Yingjie, Fontana, Adriano, Finkelstein, Steven L., Gandolfi, Giovanni, Hathi, Nimish, Hirschmann, Michaela, Holwerda, Benne W., Koekemoer, Anton M., Lucas, Ray A., Seillé, Lise-Marie, Wilkins, Stephen, Yung, L. Y. Aaron
During the last decade, studies about highly attenuated and massive red star-forming galaxies (RedSFGs) at $z \sim 4$ have suggested that they could constitute a crucial population for unraveling the mechanisms driving the transition from vigorous st
Externí odkaz:
http://arxiv.org/abs/2411.00279
Autor:
Zhang, Y. H., Dannerbauer, H., Pérez-Martínez, J. M., Koyama, Y., Zheng, X. Z., D'Eugenio, C., Emonts, B. H. C., Calvi, R., Chen, Z., Daikuhara, K., De Breuck, C., Jin, S., Kodama, T., Lehnert, M. D., Naufal, A., Shimakawa, R.
Publikováno v:
A&A 692, A22 (2024)
We report the results of the deep and wide Atacama Large Millimeter/submillimeter Array (ALMA) 1.2 mm mapping of the Spiderweb protocluster at $z=2.16$. The observations were divided into six contiguous fields covering a survey area of 19.3\,arcmin$^
Externí odkaz:
http://arxiv.org/abs/2410.10169
We explore the cosmic evolution of the fraction of dust obscured star formation predicted by the \textsc{simba} cosmological hydrodynamic simulations featuring an on-the-fly model for dust formation, evolution, and destruction. We find that up to $z=
Externí odkaz:
http://arxiv.org/abs/2401.06719
Autor:
Mitsuhashi, Ikki, Tadaki, Ken-ichi, Ikeda, Ryota, Herrera-Camus, Rodrigo, Aravena, Manuel, De Looze, Ilse, Schreiber, Natascha M. Förster, González-López, Jorge, Spilker, Justin, Assef, Roberto J., Bouwens, Rychard, Barcos-Munoz, Loreto, Birkin, Jack, Bowler, Rebecca A. A., Rivera, Gabriela Calistro, Davies, Rebecca, Da Cunha, Elisabete, Díaz-Santos, Tanio, Ferrara, Andrea, Fisher, Deanne, Lee, Lilian L., Li, Juno, Lutz, Dieter, Relaño, Monica, Naab, Thorsten, Palla, Marco, Posses, Ana, Solimano, Manuel, Tacconi, Linda, Übler, Hannah, van der Giessen, Stefan, Veilleux, Sylvain
Publikováno v:
A&A 690, A197 (2024)
We present the morphological parameters and global properties of dust-obscured star formation in typical star-forming galaxies at z=4-6. Among 26 galaxies composed of 20 galaxies observed by the Cycle-8 ALMA Large Program, CRISTAL, and six galaxies f
Externí odkaz:
http://arxiv.org/abs/2311.17671
Autor:
Smail, Ian
Clusters of galaxies at z>1 are expected to be increasingly active sites of star formation. To test this, an 850um survey was undertaken of eight high-redshift clusters at z=1.6-2.0 using SCUBA-2 on the James Clerk Maxwell Telescope. Mid-infrared pro
Externí odkaz:
http://arxiv.org/abs/2401.08761
Akademický článek
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Autor:
Bowler, R. A. A., Inami, H., Sommovigo, L., Smit, R., Algera, H. S. B., Aravena, M., Barrufet, L., Bouwens, R., da Cunha, E., Cullen, F., Dayal, P., de Looze, I., Dunlop, J. S., Fudamoto, Y., Mauerhofer, V., McLure, R. J., Stefanon, M., Schneider, R., Ferrara, A., Graziani, L., Hodge, J. A., Nanayakkara, T., Palla, M., Schouws, S., Stark, D. P., van der Werf, P. P.
We investigate the degree of dust obscured star formation in 49 massive (${\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:
Traina, A., Gruppioni, C., Delvecchio, I., Calura, F., Bisigello, L., Feltre, A., Magnelli, B., Schinnerer, E., Liu, D., Adscheid, S., Behiri, M., Gentile, F., Pozzi, F., Talia, M., Zamorani, G., Algera, H., Gillman, S., Lambrides, E., Symeonidis, M.
Aims: We leverage the largest available Atacama Large Millimetre/submillimetre Array (ALMA) survey from the archive (A$^3$COSMOS) to study to study infrared luminosity function and dust-obscured star formation rate density of sub-millimeter/millimete
Externí odkaz:
http://arxiv.org/abs/2309.15150
Autor:
Hill, Ryley, Scott, Douglas, McLeod, Derek J., McLure, Ross J., Chapman, Scott C., Dunlop, James S.
We combine archival ALMA data targeting the Hubble Ultra Deep Field (HUDF) to produce the deepest currently attainable 1-mm maps of this key region. Our deepest map covers 4.2arcmin^2, with a beamsize of 1.49''x1.07'' at an effective frequency of 243
Externí odkaz:
http://arxiv.org/abs/2309.10988