Zobrazeno 1 - 10
of 200
pro vyhledávání: '"MANNUCCI, Filippo"'
Autor:
Ginolfi, Michele, Mannucci, Filippo, Belfiore, Francesco, Marconi, Alessandro, Boardman, Nicholas, Pozzetti, Lucia, Bolzonella, Micol, Di Teodoro, Enrico, Cresci, Giovanni, Wild, Vivienne, Rodrigues, Myriam, Maiolino, Roberto, Cirasuolo, Michele, Oliva, Ernesto
The era of large-scale astronomical surveys demands innovative approaches for rapid and accurate analysis of extensive spectral data, and a promising direction to address this challenge is offered by artificial intelligence (AI). Here we introduce a
Externí odkaz:
http://arxiv.org/abs/2410.22420
Autor:
Dou, Jing, Peng, Yingjie, Gu, Qiusheng, Renzini, Alvio, Ho, Luis C., Mannucci, Filippo, Daddi, Emanuele, Zhang, Chengpeng, Li, Jiaxuan, Shi, Yong, Wang, Tao, Zhao, Dingyi, Lyu, Cheqiu, Li, Di, Yuan, Feng, Maiolino, Roberto, Gao, Yulong
The cold interstellar medium (ISM) as the raw material for star formation is critical to understanding galaxy evolution. It is generally understood that galaxies stop making stars when, in one way or another, they run out of gas. However, here we pro
Externí odkaz:
http://arxiv.org/abs/2409.03168
Autor:
Zhao, Dingyi, Peng, Yingjie, Jing, Yipeng, Yang, Xiaohu, Ho, Luis C., Renzini, Alvio, Gallazzi, Anna R., Lyu, Cheqiu, Maiolino, Roberto, Dou, Jing, Gao, Zeyu, Gu, Qiusheng, Mannucci, Filippo, Mo, Houjun, Wang, Bitao, Wang, Enci, Wang, Kai, Wang, Yu-Chen, Xu, Bingxiao, Yuan, Feng, Zhu, Xingye
In $\Lambda$CDM cosmology, galaxies form and evolve in their host dark matter (DM) halos. Halo mass is crucial for understanding the halo-galaxy connection. The abundance matching (AM) technique has been widely used to derive the halo masses of galax
Externí odkaz:
http://arxiv.org/abs/2408.12442
Autor:
Gao, Zeyu, Peng, Yingjie, Wang, Kai, Ho, Luis C., Renzini, Alvio, Gallazzi, Anna R., Mannucci, Filippo, Mo, Houjun, Jing, Yipeng, Yang, Xiaohu, Wang, Enci, Zhao, Dingyi, Dou, Jing, Gu, Qiusheng, Lyu, Cheqiu, Maiolino, Roberto, Wang, Bitao, Wang, Yu-Chen, Xu, Bingxiao, Yuan, Feng, Zhu, Xingye
The spectral energy distribution (SED) of galaxies is essential for deriving fundamental properties like stellar mass and star formation history (SFH). However, conventional methods, including both parametric and non-parametric approaches, often fail
Externí odkaz:
http://arxiv.org/abs/2408.07749
Autor:
Lyu, Cheqiu, Peng, Yingjie, Jing, Yipeng, Yang, Xiaohu, Ho, Luis C., Renzini, Alvio, Zhao, Dingyi, Mannucci, Filippo, Mo, Houjun, Wang, Kai, Wang, Bitao, Xu, Bingxiao, Dou, Jing, Gallazzi, Anna R., Gu, Qiusheng, Maiolino, Roberto, Wang, Enci, Yuan, Feng
The properties of the galaxies are tightly connected to their host halo mass and halo assembly history. Accurate measurement of the halo assembly history in observation is challenging but crucial to the understanding of galaxy formation and evolution
Externí odkaz:
http://arxiv.org/abs/2407.03409
Autor:
Mainieri, Vincenzo, Anderson, Richard I., Brinchmann, Jarle, Cimatti, Andrea, Ellis, Richard S., Hill, Vanessa, Kneib, Jean-Paul, McLeod, Anna F., Opitom, Cyrielle, Roth, Martin M., Sanchez-Saez, Paula, Smiljanic, Rodolfo, Tolstoy, Eline, Bacon, Roland, Randich, Sofia, Adamo, Angela, Annibali, Francesca, Arevalo, Patricia, Audard, Marc, Barsanti, Stefania, Battaglia, Giuseppina, Aran, Amelia M. Bayo, Belfiore, Francesco, Bellazzini, Michele, Bellini, Emilio, Beltran, Maria Teresa, Berni, Leda, Bianchi, Simone, Biazzo, Katia, Bisero, Sofia, Bisogni, Susanna, Bland-Hawthorn, Joss, Blondin, Stephane, Bodensteiner, Julia, Boffin, Henri M. J., Bonito, Rosaria, Bono, Giuseppe, Bouche, Nicolas F., Bowman, Dominic, Braga, Vittorio F., Bragaglia, Angela, Branchesi, Marica, Brucalassi, Anna, Bryant, Julia J., Bryson, Ian, Busa, Innocenza, Camera, Stefano, Carbone, Carmelita, Casali, Giada, Casali, Mark, Casasola, Viviana, Castro, Norberto, Catelan, Marcio, Cavallo, Lorenzo, Chiappini, Cristina, Cioni, Maria-Rosa, Colless, Matthew, Colzi, Laura, Contarini, Sofia, Couch, Warrick, D'Ammando, Filippo, D., William d'Assignies, D'Orazi, Valentina, da Silva, Ronaldo, Dainotti, Maria Giovanna, Damiani, Francesco, Danielski, Camilla, De Cia, Annalisa, de Jong, Roelof S., Dhawan, Suhail, Dierickx, Philippe, Driver, Simon P., Dupletsa, Ulyana, Escoffier, Stephanie, Escorza, Ana, Fabrizio, Michele, Fiorentino, Giuliana, Fontana, Adriano, Fontani, Francesco, Sanchez, Daniel Forero, Franois, Patrick, Galindo-Guil, Francisco Jose, Gallazzi, Anna Rita, Galli, Daniele, Garcia, Miriam, Garcia-Rojas, Jorge, Garilli, Bianca, Grand, Robert, Guarcello, Mario Giuseppe, Hazra, Nandini, Helmi, Amina, Herrero, Artemio, Iglesias, Daniela, Ilic, Dragana, Irsic, Vid, Ivanov, Valentin D., Izzo, Luca, Jablonka, Pascale, Joachimi, Benjamin, Kakkad, Darshan, Kamann, Sebastian, Koposov, Sergey, Kordopatis, Georges, Kovacevic, Andjelka B., Kraljic, Katarina, Kuncarayakti, Hanindyo, Kwon, Yuna, La Forgia, Fiorangela, Lahav, Ofer, Laigle, Clotilde, Lazzarin, Monica, Leaman, Ryan, Leclercq, Floriane, Lee, Khee-Gan, Lee, David, Lehnert, Matt D., Lira, Paulina, Loffredo, Eleonora, Lucatello, Sara, Magrini, Laura, Maguire, Kate, Mahler, Guillaume, Majidi, Fatemeh Zahra, Malavasi, Nicola, Mannucci, Filippo, Marconi, Marcella, Martin, Nicolas, Marulli, Federico, Massari, Davide, Matsuno, Tadafumi, Mattheee, Jorryt, McGee, Sean, Merc, Jaroslav, Merle, Thibault, Miglio, Andrea, Migliorini, Alessandra, Minchev, Ivan, Minniti, Dante, Miret-Roig, Nuria, Ibero, Ana Monreal, Montano, Federico, Montet, Ben T., Moresco, Michele, Moretti, Chiara, Moscardini, Lauro, Moya, Andres, Mueller, Oliver, Nanayakkara, Themiya, Nicholl, Matt, Nordlander, Thomas, Onori, Francesca, Padovani, Marco, Pala, Anna Francesca, Panda, Swayamtrupta, Pandey-Pommier, Mamta, Pasquini, Luca, Pawlak, Michal, Pessi, Priscila J., Pisani, Alice, Popovic, Lukav C., Prisinzano, Loredana, Raddi, Roberto, Rainer, Monica, Rebassa-Mansergas, Alberto, Richard, Johan, Rigault, Mickael, Rocher, Antoine, Romano, Donatella, Rosati, Piero, Sacco, Germano, Sanchez-Janssen, Ruben, Sander, Andreas A. C., Sanders, Jason L., Sargent, Mark, Sarpa, Elena, Schimd, Carlo, Schipani, Pietro, Sefusatti, Emiliano, Smith, Graham P., Spina, Lorenzo, Steinmetz, Matthias, Tacchella, Sandro, Tautvaisiene, Grazina, Theissen, Christopher, Thomas, Guillaume, Ting, Yuan-Sen, Travouillon, Tony, Tresse, Laurence, Trivedi, Oem, Tsantaki, Maria, Tsedrik, Maria, Urrutia, Tanya, Valenti, Elena, Van der Swaelmen, Mathieu, Van Eck, Sophie, Verdiani, Francesco, Verdier, Aurelien, Vergani, Susanna Diana, Verhamme, Anne, Vernet, Joel, Verza, Giovanni, Viel, Matteo, Vielzeuf, Pauline, Vietri, Giustina, Vink, Jorick S., Vazquez, Carlos Viscasillas, Wang, Hai-Feng, Weilbacher, Peter M., Wendt, Martin, Wright, Nicholas, Ye, Quanzhi, Yeche, Christophe, Yu, Jiaxi, Zafar, Tayyaba, Zibetti, Stefano, Ziegler, Bodo, Zinchenko, Igor
The Wide-field Spectroscopic Telescope (WST) is proposed as a new facility dedicated to the efficient delivery of spectroscopic surveys. This white paper summarises the initial concept as well as the corresponding science cases. WST will feature simu
Externí odkaz:
http://arxiv.org/abs/2403.05398
Autor:
Lyu, Cheqiu, Peng, Yingjie, Jing, Yipeng, Yang, Xiaohu, Ho, Luis C., Renzini, Alvio, Wang, Bitao, Wang, Kai, Xu, Bingxiao, Zhao, Dingyi, Dou, Jing, Gu, Qiusheng, Maiolino, Roberto, Mannucci, Filippo, Yuan, Feng
The assembly of galaxies over cosmic time is tightly connected to the assembly of their host dark matter halos. We investigate the stellar mass growth history and the chemical enrichment history of central galaxies in SDSS-MaNGA. We find that the der
Externí odkaz:
http://arxiv.org/abs/2310.10733
Autor:
Hallakoun, Na'ama, Maoz, Dan, Istrate, Alina G., Badenes, Carles, Breedt, Elmé, Gänsicke, Boris T., Jha, Saurabh W., Leibundgut, Bruno, Mannucci, Filippo, Marsh, Thomas R., Nelemans, Gijs, Patat, Ferdinando, Rebassa-Mansergas, Alberto
Planets orbiting close to hot stars experience intense extreme-ultraviolet radiation, potentially leading to atmosphere evaporation and to thermal dissociation of molecules. However, this extreme regime remains mainly unexplored due to observational
Externí odkaz:
http://arxiv.org/abs/2306.08672
Autor:
Tozzi, Giulia, Maiolino, Roberto, Cresci, Giovanni, Piotrowska, Joanna M., Belfiore, Francesco, Curti, Mirko, Mannucci, Filippo, Marconi, Alessandro
Nebular HeII$\lambda$4686\AA~line emission is useful to unveil active galactic nuclei (AGN) residing in actively star-forming (SF) galaxies, typically missed by the standard BPT classification. Here we adopt the HeII diagnostic to identify hidden AGN
Externí odkaz:
http://arxiv.org/abs/2302.04282
Autor:
Cresci, Giovanni, Tozzi, Giulia, Perna, Michele, Brusa, Marcella, Marconcini, Cosimo, Marconi, Alessandro, Carniani, Stefano, Brienza, Marisa, Giroletti, Marcello, Belfiore, Francesco, Ginolfi, Michele, Mannucci, Filippo, Ulivi, Lorenzo, Scholtz, Jan, Venturi, Giacomo, Arribas, Santiago, Übler, Hanna, D'Eugenio, Francesco, Mingozzi, Matilde, Balmaverde, Barbara, Capetti, Alessandro, Parlanti, Eleonora, Zana, Tommaso
Publikováno v:
A&A 672, A128 (2023)
Quasar feedback in the form of powerful outflows is invoked as a key mechanism to quench star formation in galaxies, although direct observational evidence is still scarce and debated. Here we present Early Release Science JWST NIRSpec IFU observatio
Externí odkaz:
http://arxiv.org/abs/2301.11060