Zobrazeno 1 - 10
of 323
pro vyhledávání: '"Elbaz, David"'
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:
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:
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
Autor:
Lyu, Yipeng, Magnelli, Benjamin, Elbaz, David, Pérez-González, Pablo G., Correa, Camila, Daddi, Emanuele, Gómez-Guijarro, Carlos, Dunlop, James S., Grogin, Norman A., Koekemoer, Anton M., McLeod, Derek J., Lu, Shiying
The stellar structures of star-forming galaxies (SFGs) undergo significant size growth during their mass assembly and must pass through a compaction phase as they evolve into quiescent galaxies (QGs). To shed light on the mechanisms behind this struc
Externí odkaz:
http://arxiv.org/abs/2406.11571
Autor:
Magnelli, Benjamin, Adscheid, Sylvia, Wang, Tsan-Ming, Ciesla, Laure, Daddi, Emanuele, Delvecchio, Ivan, Elbaz, David, Fudamoto, Yoshinobu, Fukushima, Shuma, Franco, Maximilien, Gómez-Guijarro, Carlos, Gruppioni, Carlotta, Jiménez-Andrade, Eric F., Liu, Daizhong, Oesch, Pascal, Schinnerer, Eva, Traina, Alberto
Publikováno v:
A&A 688, A55 (2024)
[Abridged] In recent years, conflicting results have provided an uncertain view of the dust-attenuated properties of $z>4$ star-forming galaxies (SFGs). To solve this, we used the deepest data publicly available in COSMOS to build a mass-complete ($>
Externí odkaz:
http://arxiv.org/abs/2405.18086
Autor:
Lu, Shiying, Daddi, Emanuele, Maraston, Claudia, Dickinson, Mark, Haro, Pablo Arrabal, Gobat, Raphael, Renzini, Alvio, Giavalisco, Mauro, Bagley, Micaela B., Calabrò, Antonello, Cheng, Yingjie, de la Vega, Alexander, D'Eugenio, Chiara, Elbaz, David, Finkelstein, Steven L., Gómez-Guijarro, Carlos, Gu, Qiusheng, Hathi, Nimish P., Huertas-Company, Marc, Kartaltepe, Jeyhan S., Koekemoer, Anton M., Bail, Aurélien Le, Lyu, Yipeng, Magnelli, Benjamin, Mobasher, Bahram, Papovich, Casey, Pirzkal, Nor, Rich, R. Michael, Tacchella, Sandro, Yung, L. Y. Aaron
Publikováno v:
2024, oct
Dating the ages and weighting the stellar populations in galaxies are essential steps when studying galaxy formation through cosmic times. Evolutionary population synthesis models with different input physics are used for this purpose. Moreover, the
Externí odkaz:
http://arxiv.org/abs/2403.07414
Autor:
Sun, Hanwen, Wang, Tao, Xu, Ke, Daddi, Emanuele, Gu, Qing, Kodama, Tadayuki, Zanella, Anita, Elbaz, David, Tanaka, Ichi, Gobat, Raphael, Guo, Qi, Han, Jiaxin, Lu, Shiying, Zhou, Luwenjia
Publikováno v:
ApJL, 967, L34 (2024)
Clusters and their progenitors (protoclusters) at z = 2-4, the peak epoch of star formation, are ideal laboratories to study the formation process of both the clusters themselves and their member galaxies. However, a complete census of their member g
Externí odkaz:
http://arxiv.org/abs/2403.05248
Autor:
Wang, Tao, Sun, Hanwen, Zhou, Luwenjia, Xu, Ke, Cheng, Cheng, Li, Zhaozhou, Chen, Yangyao, Mo, H. J., Dekel, Avishai, Zheng, Xianzhong, Cai, Zheng, Yang, Tiacheng, Dai, Y. -S., Elbaz, David, Huang, J. -S.
One of the main challenges in galaxy formation that has emerged recently is the early assembly of massive galaxies. The observed number density and the maximum stellar mass ($M_{\star}$) of massive galaxies in the early Universe appear to be higher t
Externí odkaz:
http://arxiv.org/abs/2403.02399
Autor:
Tan, Qing-Hua, Daddi, Emanuele, Magalhães, Victor de Souza, Gómez-Guijarro, Carlos, Pety, Jérôme, Kalita, Boris S., Elbaz, David, Liu, Zhaoxuan, Magnelli, Benjamin, Puglisi, Annagrazia, Rujopakarn, Wiphu, Silverman, John D., Valentino, Francesco, Zhang, Shao-Bo
Modern (sub)millimeter interferometers, such as ALMA and NOEMA, offer high angular resolution and unprecedented sensitivity. This provides the possibility to characterize the morphology of the gas and dust in distant galaxies. To assess the capabilit
Externí odkaz:
http://arxiv.org/abs/2312.05425
Autor:
Mérida, Rosa M., Gómez-Guijarro, Carlos, Pérez-González, Pablo G., Sánchez-Blázquez, Patricia, Elbaz, David, Franco, Maximilien, Leroy, Lucas, Magdis, Georgios E., Magnelli, Benjamin, Xiao, Mengyuan
Publikováno v:
A&A 686, A64 (2024)
Understanding the gas content in galaxies, its consumption and replenishment, remains pivotal in our comprehension of the evolution of the Universe. Numerous studies have addressed this, utilizing various observational tools and analytical methods. T
Externí odkaz:
http://arxiv.org/abs/2311.16279