Zobrazeno 1 - 10
of 9 483
pro vyhledávání: '"Magnelli A."'
Autor:
Ricci, G.
Publikováno v:
Il Foro Italiano, 2017 Mar 01. 140(3), 163/164-171/172.
Externí odkaz:
https://www.jstor.org/stable/44879135
Autor:
Xiao, Mengyuan, Williams, Christina C., Oesch, Pascal A., Elbaz, David, Dessauges-Zavadsky, Miroslava, Chaves, Rui Marques Coelho, Bing, Longji, Ji, Zhiyuan, Weibel, Andrea, Bezanson, Rachel, Brammer, Gabriel, Casey, Caitlin, Cloonan, Aidan P., Daddi, Emanuele, Dayal, Pratika, Faisst, Andreas L., Franx, Marijn, Glazebrook, Karl, Hutter, Anne, Kartaltepe, Jeyhan S., Labbe, Ivo, Lagache, Guilaine, Lim, Seunghwan, Magnelli, Benjamin, Martinez, Felix, Maseda, Michael V., Nanayakkara, Themiya, Schaerer, Daniel, Whitaker, Katherine E.
We report the discovery of an ultra-massive grand-design red spiral galaxy, named Zh\'ul\'ong (Torch Dragon), at $z_{\rm phot} = 5.2^{+0.3}_{-0.2}$ in the JWST PANORAMIC survey, identified as the most distant bulge+disk galaxy with spiral arms known
Externí odkaz:
http://arxiv.org/abs/2412.13264
Autor:
Sillassen, Nikolaj B., Jin, Shuowen, Magdis, Georgios E., Hodge, Jacqueline, Gobat, Raphael, Daddi, Emanuele, Knudsen, Kirsten, Finoguenov, Alexis, Schinnerer, Eva, Wang, Wei-Hao, Gao, Zhen-Kai, Weaver, John R., Algera, Hiddo, Andika, Irham T., Brinch, Malte, Chen, Chian-Chou, Cochrane, Rachel, Enia, Andrea, Faisst, Andreas, Gillman, Steven, Gomez-Guijarro, Carlos, Gozaliasl, Ghassem, Hayward, Chris, Kokorev, Vasily, Merchant, Maya, Rizzo, Francesca, Talia, Margherita, Valentino, Francesco, Blánquez-Sesé, David, Koekemoer, Anton M., Magnelli, Benjamin, Rich, Michael, Shuntov, Marko
Optically dark dusty star-forming galaxies (DSFGs) play an essential role in massive galaxy formation at early cosmic time, however their nature remains elusive. Here we present a detailed case study of all the baryonic components of a $z=4.821$ DSFG
Externí odkaz:
http://arxiv.org/abs/2412.09363
Autor:
Ciesla, L., Adscheid, S., Magnelli, B., Boquien, M., Laporte, N., Bethermin, M., Carvajal, C., Schinnerer, E., Liu, D.
[Abridged] Our view of dust in primordial galaxies is limited towards a few tens of z~7 galaxies, pre-selected from UV-optical observations, and are thus not necessarily representative of the bulk of the sources at these redshifts. In this work, we a
Externí odkaz:
http://arxiv.org/abs/2412.02557
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:
Karoumpis, C., Magnelli, B., Romano-Díaz, E., Garcia, K., Dev, A., Clarke, J., Wang, T. -M., Badescu, T., Riechers, D., Bertoldi, F.
Context. The Fred Young Submillimeter Telescope (FYST) line intensity mapping (LIM) survey will measure the power spectrum (PS) of the singly ionized carbon 158 $\rm \mu$m fine-structure line, [CII], to trace the appearance of the first galaxies that
Externí odkaz:
http://arxiv.org/abs/2410.17330
Autor:
Tan, Qing-Hua, Daddi, Emanuele, Magnelli, Benjamin, Correa, Camila A., Bournaud, Frédéric, Adscheid, Sylvia, Zhang, Shao-Bo, Elbaz, David, Gómez-Guijarro, Carlos, Kalita, Boris S., Liu, Daizhong, Liu, Zhaoxuan, Pety, Jérôme, Puglisi, Annagrazia, Schinnerer, Eva, Silverman, John D., Valentino, Francesco
The majority of stars in today's Universe reside within spheroids, which are bulges of spiral galaxies and elliptical galaxies. Their formation is still an unsolved problem. Infrared/submm-bright galaxies at high redshifts have long been suspected to
Externí odkaz:
http://arxiv.org/abs/2407.16578
Autor:
Traina, A., Magnelli, B., Gruppioni, C., Delvecchio, I., Parente, M., Calura, F., Bisigello, L., Feltre, A., Pozzi, F., Vallini, L.
Publikováno v:
A&A 690, A84 (2024)
Context. Although dust in galaxies represents only a few percent of the total baryonic mass, it plays a crucial role in the physical processes occurring in galaxies. Studying the dust content of galaxies, particularly at high$-z$, is therefore crucia
Externí odkaz:
http://arxiv.org/abs/2407.09607
Autor:
Jin, Shuowen, Sillassen, Nikolaj B., Hodge, Jacqueline, Magdis, Georgios E., Rizzo, Francesca, Casey, Caitlin, Koekemoer, Anton M., Valentino, Francesco, Kokorev, Vasily, Magnelli, Benjamin, Gobat, Raphael, Gillman, Steven, Franco, Maximilien, Faisst, Andreas, Kartaltepe, Jeyhan, Schinnerer, Eva, Toft, Sune, Algera, Hiddo S. B., Harish, Santosh, Lee, Minju, Liu, Daizhong, Shuntov, Marko, Talia, Margherita, Vijayan, Aswin
Publikováno v:
A&A 690, L16 (2024)
Photometric redshifts are widely used in studies of dusty star-forming galaxies (DSFGs), but catastrophic photo-$z$ failure can undermine all redshift-dependent results. Here we report the spectroscopic redshift confirmation of COSBO-7, a strongly le
Externí odkaz:
http://arxiv.org/abs/2407.07585
Autor:
Sillassen, Nikolaj B., Jin, Shuowen, Magdis, Georgios E., Daddi, Emanuele, Wang, Tao, Lu, Shiying, Sun, Hanwen, Arumugam, Vinod, Liu, Daizhong, Brinch, Malte, D'Eugenio, Chiara, Gobat, Raphael, Gómez-Guijarro, Carlos, Rich, Michael, Schinnerer, Eva, Strazzullo, Veronica, Tan, Qinghua, Valentino, Francesco, Wang, Yijun, Xiao, Mengyuan, Zhou, Luwenjia, Blánquez-Sesé, David, Cai, Zheng, Chen, Yanmei, Ciesla, Laure, Dai, Yu, Delvecchio, Ivan, Elbaz, David, Finoguenov, Alexis, Gao, Fangyou, Gu, Qiusheng, Hale, Catherine, Hao, Qiaoyang, Huang, Jiasheng, Jarvis, Matt, Kalita, Boris, Ke, Xu, Bail, Aurelien Le, Magnelli, Benjamin, Shi, Yong, Vaccari, Mattia, Whittam, Imogen, Yang, Tiancheng, Zhang, Zhiyu
Publikováno v:
A&A 690, A55 (2024)
The NOEMA formIng Cluster survEy (NICE) is a large program targeting 69 massive galaxy group candidates at $z>2$ in six deep fields. We report spectroscopic confirmation of eight groups at $1.65\leq z\leq3.61$ in COSMOS. Homogeneously selected as sig
Externí odkaz:
http://arxiv.org/abs/2407.02973