Zobrazeno 1 - 10
of 5 449
pro vyhledávání: '"A. Delvecchio"'
Autor:
Traina, A., Magnelli, B., Gruppioni, C., Delvecchio, I., Parente, M., Calura, F., Bisigello, L., Feltre, A., Pozzi, F., Vallini, L.
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:
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
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:
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 ($>
Externí odkaz:
http://arxiv.org/abs/2405.18086
Autor:
Hansen, Samuel P., Lagos, Claudia D. P., Bonato, Matteo, Cook, Robin H. W., Davies, Luke J. M., Delvecchio, Ivan, Tompkins, Scott A.
We present a model of radio continuum emission associated with star formation (SF) and active galactic nuclei (AGN) implemented in the Shark semi-analytic model of galaxy formation. SF emission includes free-free and synchrotron emission, which depen
Externí odkaz:
http://arxiv.org/abs/2405.05586
Autor:
Cook, Robin H. W., Davies, Luke J. M., Rhee, Jonghwan, Hale, Catherine L., Bellstedt, Sabine, Thorne, Jessica E., Delvecchio, Ivan, Collier, Jordan D., Dodson, Richard, Driver, Simon P., Holwerda, Benne W., Jarvis, Matt J., Knowles, Kenda, Lagos, Claudia, Maddox, Natasha, Meyer, Martin, Robotham, Aaron S. G., Roychowdhury, Sambit, Rozgonyi, Kristof, Seymour, Nicholas, Siudek, Malgorzata, Whiting, Matthew, Whittam, Imogen
The tight relationship between infrared luminosity (L$_\mathrm{TIR}$) and 1.4 GHz radio continuum luminosity (L$_\mathrm{1.4GHz}$) has proven useful for understanding star formation free from dust obscuration. Infrared emission in star-forming galaxi
Externí odkaz:
http://arxiv.org/abs/2405.00337
Autor:
Adscheid, Sylvia, Magnelli, Benjamin, Liu, Daizhong, Bertoldi, Frank, Delvecchio, Ivan, Gruppioni, Carlotta, Schinnerer, Eva, Traina, Alberto, Béthermin, Matthieu, Gkogkou, Athanasia
Publikováno v:
A&A, 685, A1 (2024)
Galaxy submillimetre number counts are a fundamental measurement in our understanding of galaxy evolution models. Most early measurements are obtained via single-dish telescopes with substantial source confusion, whereas recent interferometric observ
Externí odkaz:
http://arxiv.org/abs/2403.03125
Autor:
Gentile, Fabrizio, Talia, Margherita, Daddi, Emanuele, Giulietti, Marika, Lapi, Andrea, Massardi, Marcella, Pozzi, Francesca, Zamorani, Giovanni, Behiri, Meriem, Enia, Andrea, Bethermin, Matthieu, Dallacasa, Daniele, Delvecchio, Ivan, Faisst, Andreas L., Gruppioni, Carlotta, Loiacono, Federica, Traina, Alberto, Vaccari, Mattia, Vallini, Livia, Vignali, Cristian, Smolcic, Vernesa, Cimatti, Andrea
Publikováno v:
A&A 687, A288 (2024)
We present the first spectroscopic ALMA follow-up for a pilot sample of nine Radio-Selected NIRdark galaxies in the COSMOS field. These sources were initially selected as radio-detected sources (S(3GHz)>12.65 uJy), lacking an optical/NIR counterpart
Externí odkaz:
http://arxiv.org/abs/2402.05994
Autor:
Zhou, Luwenjia, Wang, Tao, Daddi, Emanuele, Coogan, Rosemary, Sun, Hanwen, Xu, Ke, Arumugam, Vinodiran, Jin, Shuowen, Liu, Daizhong, Lu, Shiying, Sillassen, Nikolaj, Wang, Yijun, Shi, Yong, Zhang, Zhi-Yu, Tan, Qinghua, Gu, Qiusheng, Elbaz, David, Bail, Aurelien Le, Magnelli, Benjamin, Gómez-Guijarro, Carlos, d'Eugenio, Chiara, Magdis, Georgios E., Valentino, Francesco, Ji, Zhiyuan, Gobat, Raphael, Delvecchio, Ivan, Xiao, Mengyuan, Strazzullo, Veronica, Finoguenov, Alexis, Schinnerer, Eva, Rich, R. Michael, Huang, Jiasheng, Dai, Yu, Chen, Yanmei, Gao, Fangyou, Yang, Tiancheng, Hao, Qiaoyang
Publikováno v:
A&A, 684, A196 (2024)
The study of distant galaxy groups and clusters at the peak epoch of star formation is limited by the lack of a statistically and homogeneously selected and spectroscopically confirmed sample. Recent discoveries of concentrated starburst activities i
Externí odkaz:
http://arxiv.org/abs/2310.15925
Publikováno v:
Journal of Small Business and Enterprise Development, 2024, Vol. 31, Issue 4, pp. 679-704.
Externí odkaz:
http://www.emeraldinsight.com/doi/10.1108/JSBED-05-2023-0220
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