Zobrazeno 1 - 10
of 1 018
pro vyhledávání: '"Suzuki, Tomoko"'
Autor:
Tang, Shenli, Silverman, John D., Liu, Zhaoxuan, Banerji, Manda, Suzuki, Tomoko, Fujimoto, Seiji, Goulding, Andy, Imanishi, Masatoshi, Kawaguchi, Toshihiro, Bottrell, Connor, Hartwig, Tilman, Jahnke, Knud, Onoue, Masafusa, Schramm, Malte, Ueda, Yoshihiro
We present a study of the molecular gas in five closely-spaced ($R_{\perp}<20$ kpc) dual quasars ($L_{\rm bol}\gtrsim10^{44}~\mathrm{erg~s}^{-1}$) at redshifts $0.4
Externí odkaz:
http://arxiv.org/abs/2407.09399
Autor:
Daikuhara, Kazuki, Kodama, Tadayuki, Pérez-Martínez, Jose M., Shimakawa, Rhythm, Suzuki, Tomoko L., Tadaki, Ken-ichi, Koyama, Yusei, Tanaka, Ichi
Low-mass galaxies at high redshifts are the building blocks of more massive galaxies at later times and are thus key populations for understanding galaxy formation and evolution. We have made deep narrow-band observations for two protoclusters and th
Externí odkaz:
http://arxiv.org/abs/2405.20663
Autor:
Pérez-Martínez, Jose Manuel, Kodama, Tadayuki, Koyama, Yusei, Shimakawa, Rhythm, Suzuki, Tomoko L., Daikuhara, Kazuki, Adachi, Kota, Onodera, Masato, Tanaka, Ichi
We use K-band multi-object near-infrared spectroscopy with Keck/MOSFIRE to search for environmental imprints on the gas properties of 27 narrow-band selected H$\alpha$ emitters (HAEs) across the three major clumps of the assembling USS1558--003 proto
Externí odkaz:
http://arxiv.org/abs/2312.03574
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:
Tadaki, Ken-ichi, Kodama, Tadayuki, Koyama, Yusei, Suzuki, Tomoko L., Mitsuhashi, Ikki, Ikeda, Ryota
We present the results of 0.6"-resolution observations of CO J=3-2 line emission in 10 massive star-forming galaxies at z=2.2-2.5 with the Atacama Large Millimeter/submillimeter Array (ALMA). We compare the spatial extent of molecular gas with those
Externí odkaz:
http://arxiv.org/abs/2309.02703
Sub-millimeter observations reveal the star-formation activity obscured by dust in the young Universe. It still remains unclear how galaxies detected at sub-millimeter wavelengths are related to ultraviolet/optical-selected galaxies in terms of their
Externí odkaz:
http://arxiv.org/abs/2309.02625
Autor:
Kakimoto, Takumi, Tanaka, Masayuki, Onodera, Masato, Shimakawa, Rhythm, Wu, Po-Feng, Gould, Katriona M. L., Ito, Kei, Jin, Shuowen, Kubo, Mariko, Suzuki, Tomoko L., Toft, Sune, Valentino, Francesco, Yabe, Kiyoto
We report on the spectroscopic confirmation of a massive quiescent galaxy at $z_\mathrm{spec}=4.53$ in the COSMOS field. The object was first identified as a galaxy with suppressed star formation at $z_\mathrm{phot}\sim4.65$ from the COSMOS2020 catal
Externí odkaz:
http://arxiv.org/abs/2308.15011
Autor:
Casey, Caitlin M., Kartaltepe, Jeyhan S., Drakos, Nicole E., Franco, Maximilien, Harish, Santosh, Paquereau, Louise, Ilbert, Olivier, Rose, Caitlin, Cox, Isabella G., Nightingale, James W., Robertson, Brant E., Silverman, John D., Koekemoer, Anton M., Massey, Richard, McCracken, Henry Joy, Rhodes, Jason, Akins, Hollis B., Amvrosiadis, Aristeidis, Arango-Toro, Rafael C., Bagley, Micaela B., Bongiorno, Angela, Capak, Peter L., Champagne, Jaclyn B., Chartab, Nima, Ortiz, Oscar A. Chavez, Chworowsky, Katherine, Cooke, Kevin C., Cooper, Olivia R., Darvish, Behnam, Ding, Xuheng, Faisst, Andreas L., Finkelstein, Steven L., Fujimoto, Seiji, Gentile, Fabrizio, Gillman, Steven, Gould, Katriona M. L., Gozaliasl, Ghassem, Hayward, Christopher C., He, Qiuhan, Hemmati, Shoubaneh, Hirschmann, Michaela, Jahnke, Knud, Jin, Shuowen, Khostovan, Ali Ahmad, Kokorev, Vasily, Lambrides, Erini, Laigle, Clotilde, Larson, Rebecca L., Leung, Gene C. K., Liu, Daizhong, Liaudat, Tobias, Long, Arianna S., Magdis, Georgios, Mahler, Guillaume, Mainieri, Vincenzo, Manning, Sinclaire M., Maraston, Claudia, Martin, Crystal L., McCleary, Jacqueline E., McKinney, Jed, McPartland, Conor J. R., Mobasher, Bahram, Pattnaik, Rohan, Renzini, Alvio, Rich, R. Michael, Sanders, David B., Sattari, Zahra, Scognamiglio, Diana, Scoville, Nick, Sheth, Kartik, Shuntov, Marko, Sparre, Martin, Suzuki, Tomoko L., Talia, Margherita, Toft, Sune, Trakhtenbrot, Benny, Urry, C. Megan, Valentino, Francesco, Vanderhoof, Brittany N., Vardoulaki, Eleni, Weaver, John R., Whitaker, Katherine E., Wilkins, Stephen M., Yang, Lilan, Zavala, Jorge A.
We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hour treasury program conducted by the James Webb Space Telescope in its first cycle of observations. COSMOS-Web is a contiguous 0.54 deg$^2$ NIRCam imaging survey in fou
Externí odkaz:
http://arxiv.org/abs/2211.07865
Autor:
Pérez-Martínez, Jose Manuel, Dannerbauer, Helmut, Kodama, Tadayuki, Koyama, Yusei, Shimakawa, Rhythm, Suzuki, Tomoko L., Calvi, Rosa, Chen, Zhengyi, Daikuhara, Kazuki, Hatch, Nina A., Laza-Ramos, Andrés, Sobral, David, Stott, John P., Tanaka, Ichi
We use multi-object near-infrared (NIR) spectroscopy with VLT/KMOS to investigate the role of the environment in the evolution of the ionized gas properties of narrow-band selected H$\alpha$ emitters (HAEs) in the Spiderweb protocluster at $z=2.16$.
Externí odkaz:
http://arxiv.org/abs/2209.13069
Autor:
Mao, Zhiying, Kodama, Tadayuki, Pérez-Martínez, Jose Manuel, Suzuki, Tomoko L., Yamamoto, Naoaki, Adachi, Kouta
Publikováno v:
A&A 666, A141 (2022)
Galaxy quenching is a critical step in galaxy evolution. In this work, we present a statistical study of galaxy quenching in 17 cluster candidates at 0.5
Externí odkaz:
http://arxiv.org/abs/2208.00722