Zobrazeno 1 - 10
of 82
pro vyhledávání: '"Ikarashi, Soh"'
Autor:
Gillman, Steven, Smail, Ian, Gullberg, Bitten, Swinbank, A. M., Vijayan, Aswin P., Lee, Minju, Brammer, Gabe, Dudzevičiūtė, U., Greve, Thomas R., Almaini, Omar, Brinch, Malte, Chapman, Scott C., Chen, Chian-Chou, Ikarashi, Soh, Matsuda, Yuichi, Wang, Wei-Hao, Walter, Fabian, van der Werf, Paul P.
We present an analysis of the JWST NIRCam and MIRI morphological properties of 80 massive ($\log_{10}(M_\ast[M_{\odot}])$=11.2$\pm$0.1) dusty star-forming galaxies at $z$$=$2.7$^{+1.2}_{-0.7}$, identified as sub-millimetre galaxies (SMGs) by ALMA, th
Externí odkaz:
http://arxiv.org/abs/2406.03544
Autor:
Castillo, Marta Frias, Rybak, Matus, Hodge, Jacqueline A., Van der Werk, Paul, Smail, Ian, Butterworth, Joshua, Jansen, Jasper, Topkaras, Theodoros, Chen, Chian-Chou, Chapman, Scott C., Weiss, Axel, Algera, Hiddo, Birkin, Jack E., da Cunha, Elisabete, Chen, Jianhang, Dannerbauer, Helmut, Jiménez-Andrade, E. F., Ikarashi, Soh, Liao, Cheng-Lin, Murphy, Eric J., Swinbank, A. M., Walter, Fabian, Rivera, Gabriela Calistro, Ivison, R. J., Lagos, Claudia del P.
The CO(1--0) and [\ion{C}{1}](1--0) emission lines are well-established tracers of cold molecular gas mass in local galaxies. At high redshift, where the interstellar medium (ISM) is likely to be denser, there have been limited direct comparisons of
Externí odkaz:
http://arxiv.org/abs/2404.05596
We have obtained 1 and 3 mm spectral scans of ASXDF1100.053.1 using NOEMA. ASXDF1100.053.1 is an unlensed optically dark millimetre-bright SMG with $K_{\rm AB}>25.7$ ($2\sigma$), which was expected to lie at $z=$5-7 based on its radio-submm photo-$z$
Externí odkaz:
http://arxiv.org/abs/2112.09026
Autor:
Umehata, Hideki, Smail, Ian, Steidel, Charles C., Hayes, Matthew, Scott, Douglas, Swinbank, A. M., Ivison, R. J., Nagao, Toru, Kubo, Mariko, Nakanishi, Kouichiro, Matsuda, Yuichi, Ikarashi, Soh, Tamura, Yoichi, Geach, J. E.
We present observations of a giant Lyman-alpha blob in the SSA22 proto-cluster at z=3.1, SSA22-LAB1, taken with the Atacama Large Millimeter/submillimeter Array (ALMA). Dust continuum, along with [C II]158um, and CO(4-3) line emission have been detec
Externí odkaz:
http://arxiv.org/abs/2107.01162
Autor:
Izumi, Takuma, Matsuoka, Yoshiki, Fujimoto, Seiji, Onoue, Masafusa, Strauss, Michael A., Umehata, Hideki, Imanishi, Masatoshi, Kohno, Kotaro, Kawaguchi, Toshihiro, Kawamuro, Taiki, Baba, Shunsuke, Nagao, Tohru, Toba, Yoshiki, Inayoshi, Kohei, Silverman, John D., Inoue, Akio K., Ikarashi, Soh, Iwasawa, Kazushi, Kashikawa, Nobunari, Hashimoto, Takuya, Nakanishi, Kouichiro, Ueda, Yoshihiro, Schramm, Malte, Lee, Chien-Hsiu, Suh, Hyewon
We present ALMA [CII] 158 $\mu$m line and underlying far-infrared (FIR) continuum emission observations ($0''.70 \times 0''.56$ resolution) toward HSC J124353.93$+$010038.5 (J1243$+$0100) at $z = 7.07$, the only low-luminosity ($M_{\rm 1450} > -25$ m
Externí odkaz:
http://arxiv.org/abs/2104.05738
Autor:
Izumi, Takuma, Onoue, Masafusa, Matsuoka, Yoshiki, Strauss, Michael A., Fujimoto, Seiji, Umehata, Hideki, Imanishi, Masatoshi, Kawamuro, Taiki, Nagao, Tohru, Toba, Yoshiki, Kohno, Kotaro, Kashikawa, Nobunari, Inayoshi, Kohei, Kawaguchi, Toshihiro, Iwasawa, Kazushi, Inoue, Akio K., Goto, Tomotsugu, Baba, Shunsuke, Schram, Malte, Suh, Hyewon, Harikane, Yuichi, Ueda, Yoshihiro, Silverman, John D., Hashimoto, Takuya, Hashimoto, Yasuhiro, Ikarashi, Soh, Iono, Daisuke, Lee, Chien-Hsiu, Lee, Kianhong, Minezaki, Takeo, Nakanishi, Kouichiro, Nakano, Suzuka, Tamura, Yoichi, Tang, Ji-Jia
We present ALMA [C II] 158 $\mu$m line and far-infrared (FIR) continuum emission observations toward HSC J120505.09$-$000027.9 (J1205$-$0000) at $z = 6.72$ with the beam size of $\sim 0''.8 \times 0''.5$ (or 4.1 kpc $\times$ 2.6 kpc), the most distan
Externí odkaz:
http://arxiv.org/abs/2101.01199
Autor:
Mitsuhashi, Ikki, Matsuda, Yuichi, Smail, Ian, Hayatsu, Natsuki, Simpson, James, Swinbank, Mark, Umahata, Hideki, Dudzevičiūtė, Ugne, Birkin, Jack, Ikarashi, Soh, Chen, Chian-Chou, Tadaki, Ken-ichi, Yajima, Hidenobu, Harikane, Yuichi, Inami, Hanae, Chapman, Scott, Hatsukade, Bunyo, Iono, Daisuke, Bunker, Andrew, Ao, Yiping, Saito, Tomoki, Ueda, Junko, Sakamoto, Seiichi
We report the discovery of a 10 comoving Mpc-scale structure traced by massive submillimeter galaxies (SMGs) at z~4.6. These galaxies are selected from an emission line search of ALMA Band 7 observations targeting 184 luminous submillimeter sources (
Externí odkaz:
http://arxiv.org/abs/2011.09917
Autor:
Takekoshi, Tatsuya, Karatsu, Kenichi, Suzuki, Junya, Tamura, Yoichi, Oshima, Tai, Taniguchi, Akio, Asayama, Shin'ichiro, Bakx, Tom J. L. C., Baselmans, Jochem J. A., Bosma, Sjoerd, Bueno, Juan, Chin, Kah Wuy, Fujii, Yasunori, Fujita, Kazuyuki, Huiting, Robert, Ikarashi, Soh, Ishida, Tsuyoshi, Ishii, Shun, Kawabe, Ryohei, Klapwijk, Teun M., Kohno, Kotaro, Kouchi, Akira, Llombart, Nuria, Maekawa, Jun, Murugesan, Vignesh, Nakatsubo, Shunichi, Naruse, Masato, Ohtawara, Kazushige, Laguna, Alejandro Pascual, Suzuki, Koyo, Thoen, David J., Tsukagoshi, Takashi, Ueda, Tetsutaro, de Visser, Pieter J., van der Werf, Paul P., Yates, Stephen J. C., Yoshimura, Yuki, Yurduseven, Ozan, Endo, Akira
We are developing an ultra-wideband spectroscopic instrument, DESHIMA (DEep Spectroscopic HIgh-redshift MApper), based on the technologies of an on-chip filter-bank and Microwave Kinetic Inductance Detector (MKID) to investigate dusty star-burst gala
Externí odkaz:
http://arxiv.org/abs/2001.05151
Autor:
Endo, Akira, Karatsu, Kenichi, Tamura, Yoichi, Oshima, Tai, Taniguchi, Akio, Takekoshi, Tatsuya, Asayama, Shin'ichiro, Bakx, Tom J. L. C., Bosma, Sjoerd, Bueno, Juan, Chin, Kah Wuy, Fujii, Yasunori, Fujita, Kazuyuki, Huiting, Robert, Ikarashi, Soh, Ishida, Tsuyoshi, Ishii, Shun, Kawabe, Ryohei, Klapwijk, Teun M., Kohno, Kotaro, Kouchi, Akira, Llombart, Nuria, Maekawa, Jun, Murugesan, Vignesh, Nakatsubo, Shunichi, Naruse, Masato, Ohtawara, Kazushige, Laguna, Alejandro Pascual, Suzuki, Junya, Suzuki, Koyo, Thoen, David J., Tsukagoshi, Takashi, Ueda, Tetsutaro, de Visser, Pieter J., van der Werf, Paul P., Yates, Stephen J. C., Yoshimura, Yuki, Yurduseven, Ozan, Baselmans, Jochem J. A.
Ultra-wideband 3D imaging spectrometry in the millimeter-submillimeter (mm-submm) band is an essential tool for uncovering the dust-enshrouded portion of the cosmic history of star formation and galaxy evolution. However, it is challenging to scale u
Externí odkaz:
http://arxiv.org/abs/1906.10216
Autor:
Izumi, Takuma, Onoue, Masafusa, Matsuoka, Yoshiki, Nagao, Tohru, Strauss, Michael A., Imanishi, Masatoshi, Kashikawa, Nobunari, Fujimoto, Seiji, Kohno, Kotaro, Toba, Yoshiki, Umehata, Hideki, Goto, Tomotsugu, Ueda, Yoshihiro, Shirakata, Hikari, Silverman, John D., Greene, Jenny E., Harikane, Yuichi, Hashimoto, Yasuhiro, Ikarashi, Soh, Iono, Daisuke, Iwasawa, Kazushi, Lee, Chien-Hsiu, Minezaki, Takeo, Nakanishi, Kouichiro, Tamura, Yoichi, Tang, Ji-Jia, Taniguchi, Akio
We present ALMA [CII] line and far-infrared (FIR) continuum observations of three $z > 6$ low-luminosity quasars ($M_{\rm 1450} > -25$) discovered by our Subaru Hyper Suprime-Cam (HSC) survey. The [CII] line was detected in all three targets with lum
Externí odkaz:
http://arxiv.org/abs/1904.07345