Zobrazeno 1 - 10
of 32
pro vyhledávání: '"Kalita, Boris S."'
Autor:
Tanaka, Takumi S., Silverman, John D., Nakazato, Yurina, Onoue, Masafusa, Shimasaku, Kazuhiro, Fudamoto, Yoshinobu, Fujimoto, Seiji, Ding, Xuheng, Faisst, Andreas L., Valentino, Francesco, Jin, Shuowen, Hayward, Christopher C., Kokorev, Vasily, Ceverino, Daniel, Kalita, Boris S., Casey, Caitlin M., Liu, Zhaoxuan, Kaminsky, Aidan, Fei, Qinyue, Andika, Irham T., Lambrides, Erini, Akins, Hollis B., Kartaltepe, Jeyhan S., Koekemoer, Anton M., McCracken, Henry Joy, Rhodes, Jason, Robertson, Brant E., Franco, Maximilien, Liu, Daizhong, Chartab, Nima, Gillman, Steven, Gozaliasl, Ghassem, Hirschmann, Michaela, Huertas-Company, Marc, Massey, Richard, Roy, Namrata, Sattari, Zahra, Shuntov, Marko, Sterling, Joseph, Toft, Sune, Trakhtenbrot, Benny, Yoshida, Naoki, Zavala, Jorge A.
The current paradigm for the co-evolution of galaxies and their supermassive black holes postulates that dust-obscured active galactic nuclei (AGNs) represent a transitional phase towards a more luminous and unobscured state. However, our understandi
Externí odkaz:
http://arxiv.org/abs/2410.00104
Autor:
McKinney, Jed, Casey, Caitlin M., Long, Arianna S., Cooper, Olivia R., Manning, Sinclaire M., Franco, Maximilien, Akin, Hollis, Lambrides, Erini, Gammon, Elaine, Silva, Camila, Gentile, Fabrizio, Zavala, Jorge A., Amvrosiadis, Aristeidis, Andika, Irma, Brinch, Malte, Champagne, Jaclyn B., Chartab, Nima, Drakos, Nicole E., Faisst, Andreas L., Fujimoto, Seiji, Gillman, Steven, Gozaliasl, Ghassem, Greve, Thomas R., Harish, Santosh, Hayward, Christopher C., Hirschmann, Michaela, Ilbert, Olivier, Kalita, Boris S., Kartaltepe, Jeyhan S., Koekemoer, Anton M., Kokorev, Vasily, Liu, Daizhong, Magdis, Georgios, McCracken, Henry Joy, Rhodes, Jason, Robertson, Brant E., Talia, Margherita, Valentino, Francesco, Vijayan, Aswin P.
JWST has enabled detecting and spatially resolving the heavily dust-attenuated stellar populations of sub-millimeter galaxies, revealing detail that was previously inaccessible. In this work we construct a sample of 289 sub-millimeter galaxies with d
Externí odkaz:
http://arxiv.org/abs/2408.08346
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:
Kalita, Boris S., Silverman, John D., Daddi, Emanuele, Mercier, Wilfried, Ho, Luis C., Ding, Xuheng
Resolved stellar morphology of z>1 galaxies was inaccessible before JWST. This limitation, due to the impact of dust on rest-frame UV light, had withheld major observational conclusions required to understand the importance of clumps in galaxy evolut
Externí odkaz:
http://arxiv.org/abs/2402.02679
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:
Liu, Zhaoxuan, Silverman, John D., Daddi, Emanuele, Puglisi, Annagrazia, Renzini, Alvio, Kalita, Boris S., Kartaltepe, Jeyhan S., Kashino, Daichi, Rodighiero, Giulia, Rujopakarn, Wiphu, Suzuki, Tomoko L., Tanaka, Takumi S., Valentino, Francesco, Andika, Irham Taufik, Casey, Caitlin M., Faisst, Andreas, Franco, Maximilien, Gozaliasl, Ghassem, Gillman, Steven, Hayward, Christopher C., Koekemoer, Anton M., Kokorev, Vasily, Lambrides, Erini, Lee, Minju M., Magdis, Georgios E., Harish, Santosh, McCracken, Henry Joy, Rhodes, Jason, Shuntov, Marko, Ding, Xuheng
We present observations and analysis of the starburst, PACS-819, at z=1.45 ($M_*=10^{10.7}$ M$_{ \odot}$), using high-resolution ($0^{\prime \prime}.1$; 0.8 kpc) ALMA and multi-wavelength JWST images from the COSMOS-Web program. Dissimilar to HST/ACS
Externí odkaz:
http://arxiv.org/abs/2311.14809
Autor:
Kalita, Boris S., Silverman, John D., Daddi, Emanuele, Bottrell, Connor, Ho, Luis C., Ding, Xuheng, Yang, Lilan
A key question in galaxy evolution has been the importance of the apparent `clumpiness' of high redshift galaxies. Until now, this property has been primarily investigated in rest-frame UV, limiting our understanding of their relevance. Are they shor
Externí odkaz:
http://arxiv.org/abs/2309.05737
Autor:
Bottrell, Connor, Yesuf, Hassen M., Popping, Gergö, Omori, Kiyoaki Christopher, Tang, Shenli, Ding, Xuheng, Pillepich, Annalisa, Nelson, Dylan, Eisert, Lukas, Gao, Hua, Goulding, Andy D., Kalita, Boris S., Luo, Wentao, Greene, Jenny E., Shi, Jingjing, Silverman, John D.
At fixed galaxy stellar mass, there is a clear observational connection between structural asymmetry and offset from the star forming main sequence, $\Delta$SFMS. Herein, we use the TNG50 simulation to investigate the relative roles of major mergers
Externí odkaz:
http://arxiv.org/abs/2308.14793
Autor:
Bail, Aurelien Le, Daddi, Emanuele, Elbaz, David, Dickinson, Mark, Giavalisco, Mauro, Magnelli, Benjamin, Gomez-Guijarro, Carlos, Kalita, Boris S., Koekemoer, Anton M., Holwerda, Benne W., Bournaud, Frederic, de la Vega, Alexander, Calabro, Antonello, Dekel, Avishai, Cheng, Yingjie, Bisigello, Laura, Franco, Maximilien, Costantin, Luca, Lucas, Ray A., Perez-Gonzalez, Pablo G., Lu, Shiying, Wilkins, Stephen M., Haro, Pablo Arrabal, Bagley, Micaela B., Finkelstein, Steven L., Kartaltepe, Jeyhan S., Papovich, Casey, Pirzkal, Nor, Yung, L. Y. Aaron
Publikováno v:
A&A 688, A53 (2024)
We investigate the morphology and resolved physical properties of a sample of 22 IR-selected DSFG at cosmic noon using the JWST/NIRCam images obtained in the EGS field for the CEERS survey. The resolution of the NIRCam images allowed to spatially res
Externí odkaz:
http://arxiv.org/abs/2307.07599
Autor:
Kalita, Boris S., Daddi, Emanuele, Bournaud, Frederic, Rich, R. Michael, Valentino, Francesco, Gómez-Guijarro, Carlos, Codis, Sandrine, Delvecchio, Ivan, Elbaz, David, Strazzullo, Veronica, Magalhaes, Victor de Sousa, Pety, Jérôme, Tan, Qinghua
Publikováno v:
A&A 666, A44 (2022)
We present well-resolved near-IR and sub-mm analysis of the three highly star-forming massive ($>10^{11}\,\rm M_{\odot}$) galaxies within the core of the RO-1001 galaxy group at $\rm z=2.91$. Each of them displays kpc-scale compact star-bursting core
Externí odkaz:
http://arxiv.org/abs/2206.05217