Zobrazeno 1 - 10
of 191
pro vyhledávání: '"Espada, Daniel"'
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
Autor:
Furtak, Lukas J., Zitrin, Adi, Richard, Johan P., Eckert, Dominique, Sayers, Jack, Ebeling, Harald, Fujimoto, Seiji, Laporte, Nicolas, Lagattuta, David, Limousin, Marceau, Mahler, Guillaume, Meena, Ashish K., Andrade-Santos, Felipe, Frye, Brenda L., Jauzac, Mathilde, Koekemoer, Anton M., Kohno, Kotaro, Espada, Daniel, Lu, Harry, Massey, Richard, Niemiec, Anna
MACS J0600.1-2008 (MACS0600) is an X-ray luminous, massive galaxy cluster at $z_{\mathrm{d}}=0.43$, studied previously by the REionization LensIng Cluster Survey (RELICS) and ALMA Lensing Cluster Survey (ALCS) projects which revealed a complex, bimod
Externí odkaz:
http://arxiv.org/abs/2404.03286
Autor:
Uematsu, Ryosuke, Ueda, Yoshihiro, Kohno, Kotaro, Toba, Yoshiki, Yamada, Satoshi, Smail, Ian, Umehata, Hideki, Fujimoto, Seiji, Hatsukade, Bunyo, Ao, Yiping, Bauer, Franz Erik, Brammer, Gabriel, Dessauges-Zavadsky, Miroslava, Espada, Daniel, Jolly, Jean-Baptiste, Koekemoer, Anton M., Kokorev, Vasily, Magdis, Georgios E., Oguri, Masamune, Sun, Fengwu
Sub/millimeter galaxies are a key population for the study of galaxy evolution because the majority of star formation at high redshifts occurred in galaxies deeply embedded in dust. To search for this population, we have performed an extensive survey
Externí odkaz:
http://arxiv.org/abs/2402.05849
Autor:
Domínguez-Gómez, Jesús, Pérez, Isabel, Ruiz-Lara, Tomás, Peletier, Reynier F., Sánchez-Blázquez, Patricia, Lisenfeld, Ute, Bidaran, Bahar, Falcón-Barroso, Jesús, Alcázar-Laynez, Manuel, Argudo-Fernández, María, Blázquez-Calero, Guillermo, Courtois, Hélène, Puertas, Salvador Duarte, Espada, Daniel, Florido, Estrella, García-Benito, Rubén, Jiménez, Andoni, Kreckel, Kathryn, Relaño, Mónica, Sánchez-Menguiano, Laura, van der Hulst, Thijs, van de Weygaert, Rien, Verley, Simon, Zurita, Almudena
Publikováno v:
A&A 680, A111 (2023)
Void galaxies are essential for understanding the physical processes that drive galaxy evolution because they are less affected by external factors than galaxies in denser environments, that is, in filaments, walls, and clusters. The stellar metallic
Externí odkaz:
http://arxiv.org/abs/2310.11412
Autor:
Li, Zihao, Cai, Zheng, Sun, Fengwu, Richard, Johan, Trebitsch, Maxime, Helton, Jakob M., Diego, Jose M., Oguri, Masamune, Foo, Nicholas, Lin, Xiaojing, Bauer, Franz, Chen, Chian-Chou, Conselice, Christopher J., Espada, Daniel, Egami, Eiichi, Fan, Xiaohui, Frye, Brenda L., Fudamoto, Yoshinobu, Perez-Gonzalez, Pablo G., Hainline, Kevin, Hsiao, Tiger Yu-Yang, Ji, Zhiyuan, Jin, Xiangyu, Koekemoer, Anton M., Kokorev, Vasily, Kohno, Kotaro, Li, Mingyu, Lee, Minju, Magdis, Georgios E., Willmer, Christopher N. A., Windhorst, Rogier A., Wu, Yunjing, Yan, Haojing, Zhang, Haowen, Zitrin, Adi, Zou, Siwei, Bian, Fuyan, Cheng, Cheng, DeCoursey, Christa, Furtak, Lukas J., Steinhardt, Charles, Umehata, Hideki
We report galaxy MACS0416-Y3 behind the lensing cluster MACSJ0416.1--2403 as a tentative rotating disk at $z=8.34$ detected through its [OIII]$\lambda5007$ emission in JWST NIRCam wide-field slitless spectroscopic observations. The discovery is based
Externí odkaz:
http://arxiv.org/abs/2310.09327
Autor:
Guerrero, Andrea, Nagar, Neil, Kohno, Kotaro, Fujimoto, Seiji, Kokorev, Vasily, Brammer, Gabriel, Jolly, Jean-Baptiste, Knudsen, Kirsten, Sun, Fengwu, Bauer, Franz E., Caminha, Gabriel B., Caputi, Karina, Neumann, Gerald, Orellana-González, Gustavo, Cerulo, Pierluigi, González-López, Jorge, Laporte, Nicolas, Koekemoer, Anton M., Ao, Yiping, Espada, Daniel, Arancibia, Alejandra M. Muñoz
We develop new tools for continuum and spectral stacking of ALMA data, and apply these to the ALMA Lensing Cluster Survey (ALCS). We derive average dust masses, gas masses and star formation rates (SFR) from the stacked observed 260~GHz continuum of
Externí odkaz:
http://arxiv.org/abs/2309.16832
Autor:
Fujimoto, Seiji, Kohno, Kotaro, Ouchi, Masami, Oguri, Masamune, Kokorev, Vasily, Brammer, Gabriel, Sun, Fengwu, Gonzalez-Lopez, Jorge, Bauer, Franz E., Caminha, Gabriel B., Hatsukade, Bunyo, Richard, Johan, Smail, Ian, Tsujita, Akiyoshi, Ueda, Yoshihiro, Uematsu, Ryosuke, Zitrin, Adi, Coe, Dan, Kneib, Jean-Paul, Postman, Marc, Umetsu, Keiichi, Lagos, Claudia del P., Popping, Gergo, Ao, Yiping, Bradley, Larry, Caputi, Karina, Dessauges-Zavadsky, Miroslava, Egami, Eiichi, Espada, Daniel, Ivison, R. J., Jauzac, Mathilde, Knudsen, Kirsten K., Koekemoer, Anton M., Magdis, Georgios E., Mahler, Guillaume, Arancibia, A. M. Munoz, Rawle, Timothy, Shimasaku, Kazuhiro, Toft, Sune, Umehata, Hideki, Valentino, Francesco, Wang, Tao, Wang, Wei-Halo
We present a statistical study of 180 dust continuum sources identified in 33 massive cluster fields by the ALMA Lensing Cluster Survey (ALCS) over a total of 133 arcmin$^{2}$ area, homogeneously observed at 1.2 mm. ALCS enables us to detect extremel
Externí odkaz:
http://arxiv.org/abs/2303.01658