Zobrazeno 1 - 10
of 20 500
pro vyhledávání: '"Espada, A"'
Autor:
Jolly, Jean-Baptiste, Knudsen, Kirsten, Laporte, Nicolas, Guerrero, Andrea, Fujimoto, Seiji, Kohno, Kotaro, Kokorev, Vasily, Lagos, Claudia del P., Schirmer, Thiébaut-Antoine, Bauer, Franz, Dessauge-Zavadsky, Miroslava, Espada, Daniel, Hatsukade, Bunyo, Koekemoer, Anton M., Richard, Johan, Sun, Fengwu, Wu, John F.
Understanding the dust content of galaxies, its evolution with redshift and its relationship to stars and star formation is fundamental for our understanding of galaxy evolution. Using the ALMA Lensing Cluster Survey (ALCS) wide-area band-6 continuum
Externí odkaz:
http://arxiv.org/abs/2411.11212
Autor:
Argudo-Fernández, M., Hernández, C. Gómez, Verley, S., Zurita, A., Puertas, S. Duarte, Calero, G. Blázquez, Domínguez-Gómez, J., Espada, D., Florido, E., Pérez, I., Sánchez-Menguiano, L.
Publikováno v:
A&A 692, A258 (2024)
In this work we investigate the effects of the environment on the evolution of void galaxies. In particular, we study their morphology and explore its dependence with their location within the void where the galaxies reside, as well as with propertie
Externí odkaz:
http://arxiv.org/abs/2411.02129
Autor:
Rodríguez, M. I., Lisenfeld, U., Puertas, S. Duarte, Espada, D., Domínguez-Gómez, J., Sánchez-Portal, M., Bongiovanni, A., Alcázar-Laynez, M., Argudo-Fernández, M., Bidaran, B., De Daniloff, S. B., Falcón-Barroso, J., Florido, E., García-Benito, R., Jimenez, A., Kreckel, K., Peletier, R. F., Pérez, I., Ruiz-Lara, T., Sánchez-Menguiano, L., Torres-Ríos, G., Villalba-González, P., Verley, S., Zurita, A.
Publikováno v:
A&A 692, A125 (2024)
Cosmic voids, distinguished by their low-density environment, provide a unique opportunity to explore the interplay between the cosmic environment and the processes of galaxy formation and evolution. Data on the molecular gas has been scarce so far.
Externí odkaz:
http://arxiv.org/abs/2410.18078
Autor:
García-Benito, Rubén, Jiménez, Andoni, Sánchez-Menguiano, Laura, Ruiz-Lara, Tomás, Puertas, Salvador Duarte, Domínguez-Gómez, Jesús, Bidaran, Bahar, Torres-Ríos, Gloria, Argudo-Fernández, María, Espada, Daniel, Pérez, Isabel, Verley, Simon, Conrado, Ana M., Florido, Estrella, Rodríguez, Mónica I., Zurita, Almudena, Alcázar-Laynez, Manuel, De Daniloff, Simon B., Lisenfeld, Ute, van de Weygaert, Rien, Courtois, Hélène M., Falcón-Barroso, Jesús, Ferré-Mateu, Anna, Galbany, Lluís, Delgado, Rosa M. González, del Moral-Castro, Ignacio, Peletier, Reynier F., Román, Javier, Sánchez, Sebastián F., Sánchez-Alarcón, Pablo M., Sánchez-Blázquez, Patricia, Villalba-González, Pedro, Azzaro, Marco, Blazek, Martín, Fernández, Alba, Gallego, Julia, Góngora, Samuel, Guijarro, Ana, de Guindos, Enrique, Hermelo, Israel, Hernández, Ricardo, de Juan, Enrique, Linares, José Ignacio Vico
The Calar Alto Void Integral-field Treasury surveY (CAVITY) is a legacy project aimed at characterising the population of galaxies inhabiting voids, which are the most under-dense regions of the cosmic web, located in the Local Universe. This paper d
Externí odkaz:
http://arxiv.org/abs/2410.08265
Autor:
Torres-Ríos, G., Pérez, I., Verley, S., Domínguez-Gómez, J., Argudo-Fernández, M., Puertas, S. Duarte, Jiménez, A., Ruiz-Lara, T., Zurita, A., Bidaran, B., Conrado, A., Espada, D., García-Benito, R., Delgado, R. M. González, Falcón-Barroso, J., Florido, E., Sánchez-Blázquez, P., Sánchez-Menguiano, L.
Publikováno v:
A&A 691, A341 (2024)
We aim to investigate how the local environment influences the star formation history (SFH) of galaxies residing in various large-scale environments. We categorise a sample of 9384 galaxies into the three primary large scale structures (voids, walls
Externí odkaz:
http://arxiv.org/abs/2410.00959
Autor:
Pérez, I., Verley, S., Sánchez-Menguiano, L., Ruiz-Lara, T., García-Benito, R., Puertas, S. Duarte, Jiménez, A., Domínguez-Gómez, J., Espada, D., Peletier, R. F., Román, J., Rodríguez, M. I., Alarcón, P. Sánchez, Argudo-Fernández, M., Torres-Ríos, G., Bidaran, B., Alcázar-Laynez, M., van de Weygaert, R., Sánchez, S. F., Lisenfeld, U., Zurita, A., Florido, E., van der Hulst, J. M., Blázquez-Calero, G., Villalba-González, P., del Moral-Castro, I., Lugo-Aranda, A., Walo-Martín, D., Conrado, A., Delgado, R. González, Falcón-Barroso, J., Ferré-Mateu, A., Hernández-Sánchez, M., Awad, P., Kreckel, K., Courtois, H., Espada-Miura, R., Relaño, M., Galbany, L., Sánchez-Blázquez, P., Pérez-Montero, E., Sánchez-Portal, M., Bongiovanni, A., Planelles, S., Quilis, V., Aubert, M., Guinet, D., Pomaréde, D., Weijmans, A. M., Raj, M. A., Aragón-Calvo, M. A., Azzaro, M., Bergond, G., Blazek, M., Cikota, S., Fernández-Martín, A., Gardini, A., Guijarro, A., Hermelo, I., Martín, P., Linares, J. I. Vico
Publikováno v:
A&A 689, A213 (2024)
We have learnt in the last decades that the majority of galaxies belong to high density regions interconnected in a sponge-like fashion. This large-scale structure is characterised by clusters, filaments, walls, where most galaxies concentrate, but a
Externí odkaz:
http://arxiv.org/abs/2405.04217
Autor:
Tsujita, Akiyoshi, Kohno, Kotaro, Huang, Shuo, Oguri, Masamune, Tadaki, Ken-ichi, Smail, Ian, Umehata, Hideki, Gao, Zhen-Kai, Wang, Wei-Hao, Sun, Fengwu, Fujimoto, Seiji, Wang, Tao, Uematsu, Ryosuke, Espada, Daniel, Valentino, Francesco, Ao, Yiping, Bauer, Franz E., Hatsukade, Bunyo, Egusa, Fumi, Nishimura, Yuri, Koekemoer, Anton M., Schaerer, Daniel, Lagos, Claudia, Dessauges-Zavadsky, Miroslava, Brammer, Gabriel, Caputi, Karina, Egami, Eiichi, González-López, Jorge, Jolly, Jean-Baptiste, Knudsen, Kirsten K., Kokorev, Vasily, Magdis, Georgios E., Ouchi, Masami, Toft, Sune, Wu, John F., Zitrin, Adi
We present results from Atacama Large Millimeter/submillimeter Array (ALMA) spectral line-scan observations at 3-mm and 2-mm bands of three near-infrared-dark (NIR-dark) galaxies behind two massive lensing clusters MACS J0417.5-1154 and RXC J0032.1+1
Externí odkaz:
http://arxiv.org/abs/2406.09890
Autor:
Ma, Zhiyuan, Sun, Bangzheng, Cheng, Cheng, Yan, Haojing, Sun, Fengwu, Foo, Nicholas, Egami, Eiichi, Diego, Jose M., Cohen, Seth H., Jansen, Rolf A., Summers, Jake, Windhorst, Rogier A., D'Silva, Jordan C. J., Koekemoer, Anton M., Coe, Dan, Conselice, Christopher J., Driver, Simon P., Frye, Brenda, Grogin, Norman A., Marshall, Madeline A., Nonino, Mario, Ortiz III, Rafael, Pirzkal, Nor, Robotham, Aaron, Ryan, Jr., Russell E., Willmer, Christopher N. A., Adams, Nathan J., Hathi, Nimish P., Dole, Herve, Willner, S. P., Espada, Daniel, Furtak, Lukas J., Hsiao, Tiger Yu-Yang, Li, Qiong, Chen, Wenlei, Jolly, Jean-Baptiste, Chen, Chian-Chou
New JWST/NIRCam wide-field slitless spectroscopy provides redshifts for four z>8 galaxies located behind the lensing cluster MACS J0416.1-2403. Two of them, "Y1" and "JD", have previously reported spectroscopic redshifts based on ALMA measurements of
Externí odkaz:
http://arxiv.org/abs/2406.04617
Autor:
Conrado, Ana M., Delgado, Rosa M. González, García-Benito, Rubén, Pérez, Isabel, Verley, Simon, Ruiz-Lara, Tomás, Sánchez-Menguiano, Laura, Puertas, Salvador Duarte, Jiménez, Andoni, Domínguez-Gómez, Jesús, Espada, Daniel, Argudo-Fernández, María, Alcázar-Laynez, Manuel, Blázquez-Calero, Guillermo, Bidaran, Bahar, Zurita, Almudena, Peletier, Reynier, Torres-Ríos, Gloria, Florido, Estrella, Martínez, Mónica Rodríguez, del Moral-Castro, Ignacio, van de Weygaert, Rien, Falcón-Barroso, Jesús, Lugo-Aranda, Alejandra Z., Sánchez, Sebastián F., van der Hulst, Thijs, Courtois, Hélène M., Ferré-Mateu, Anna, Sánchez-Blázquez, Patricia, Román, Javier, Aceituno, Jesús
Publikováno v:
A&A 687, A98 (2024)
The Universe is shaped as a web-like structure, formed by clusters, filaments, and walls that leave large volumes in between named voids. Galaxies in voids have been found to be of a later type, bluer, less massive, and to have a slower evolution tha
Externí odkaz:
http://arxiv.org/abs/2404.10823
Autor:
Fudamoto, Yoshinobu, Sun, Fengwu, Diego, Jose M., Dai, Liang, Oguri, Masamune, Zitrin, Adi, Zackrisson, Erik, Jauzac, Mathilde, Lagattuta, David J., Egami, Eiichi, Iani, Edoardo, Windhorst, Rogier A., Abe, Katsuya T., Bauer, Franz Erik, Bian, Fuyan, Bhatawdekar, Rachana, Broadhurst, Thomas J., Cai, Zheng, Chen, Chian-Chou, Chen, Wenlei, Cohen, Seth H., Conselice, Christopher J., Espada, Daniel, Foo, Nicholas, Frye, Brenda L., Fujimoto, Seiji, Furtak, Lukas J., Golubchik, Miriam, Hsiao, Tiger Yu-Yang, Jolly, Jean-Baptiste, Kawai, Hiroki, Kelly, Patrick L., Koekemoer, Anton M., Kohno, Kotaro, Kokorev, Vasily, Li, Mingyu, Li, Zihao, Lin, Xiaojing, Magdis, Georgios E., Meena, Ashish K., Nabizadeh, Armin, Richard, Johan, Steinhardt, Charles L., Wu, Yunjing, Zhu, Yongda, Zou, Siwei
Strong gravitational magnification by massive galaxy clusters enable us to detect faint background sources, resolve their detailed internal structures, and in the most extreme cases identify and study individual stars in distant galaxies. Highly magn
Externí odkaz:
http://arxiv.org/abs/2404.08045