Zobrazeno 1 - 10
of 901
pro vyhledávání: '"Kawabe R"'
Autor:
Mizukoshi, S., Kohno, K., Egusa, F., Hatsukade, B., Minezaki, T., Saito, T., Tamura, Y., Iono, D., Ueda, J., Matsuda, Y., Kawabe, R., Lee, M. M., Yun, M. S., Espada, D.
We present a detailed investigation of millimeter-wave line emitters ALMA J010748.3-173028 (ALMA-J0107a) and ALMA J010747.0-173010 (ALMA-J0107b), which were serendipitously uncovered in the background of the nearby galaxy VV114 with spectral scan obs
Externí odkaz:
http://arxiv.org/abs/2105.08894
Autor:
Kohno, K., Kawabe, R., Tamura, Y., Endo, A., Baselmans, J. J. A., Karatsu, K., Inoue, A. K., Moriwaki, K., Hayatsu, N. H., Yoshida, N., Yoshimura, Y., Hatsukade, B., Umehata, H., Oshima, T., Takekoshi, T., Taniguchi, A., Klaassen, P. D., Mroczkowski, T., Cicone, C., Bertoldi, F., Dannerbauer, H., Tosaki, T.
Publikováno v:
Proceedings Volume 11453, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X; 114530N (2020)
We present a conceptual study of a large format imaging spectrograph for the Large Submillimeter Telescope (LST) and the Atacama Large Aperture Submillimeter Telescope (AtLAST). Recent observations of high-redshift galaxies indicate the onset of earl
Externí odkaz:
http://arxiv.org/abs/2102.08280
Autor:
Kitayama, T., Ueda, S., Akahori, T., Komatsu, E., Kawabe, R., Kohno, K., Takakuwa, S., Tsutsumi, T., Takizawa, M., Yoshikawa, K.
We present measurements of the thermal Sunyaev-Zel'dovich effect (SZE) toward SPT-CL J2334-4243 (the Phoenix galaxy cluster) at z=0.597 by the Atacama Large Millimeter/submillimeter Array (ALMA) in Band 3. The SZE is imaged at 5" resolution (correspo
Externí odkaz:
http://arxiv.org/abs/2001.11239
Autor:
Yamagishi, M., Hara, C., Kawabe, R., Nakamura, F., Kamazaki, T., Takekoshi, T., Shimajiri, Y., Nomura, H., Takakuwa, S., Di Francesco, J.
We analyze $^{12}$CO($J$=2-1), $^{13}$CO($J$=2-1), C$^{18}$O ($J$=2-1), and 1.3 mm continuum maps of the $\rho$ Ophiuchi A photo-dissociation region (PDR) obtained with ALMA. Layered structures of the three CO isotopologues with an angular separation
Externí odkaz:
http://arxiv.org/abs/1903.02192
Autor:
Espada, D., Martin, S., Verley, S., Pettitt, A. R., Matsushita, S., Argudo-Fernandez, M., Randriamanakoto, Z., Hsieh, P. -Y., Saito, T., Miura, R. E., Kawana, Y., Sabater, J., Verdes-Montenegro, L., Ho, P. T. P., Kawabe, R., Iono, D.
Mergers of galaxies are an important mode for galaxy evolution because they serve as an efficient trigger of powerful starbursts. However, observational studies of the molecular gas properties during their early stages are scarce. We present interfer
Externí odkaz:
http://arxiv.org/abs/1809.04788
Autor:
Zeballos, M., Aretxaga, I., Hughes, D. H., Humphrey, A., Wilson, G. W., Austermann, J., Dunlop, J. S., Ezawa, H., Ferrusca, D., Hatsukade, B., Ivison, R. J., Kawabe, R., Kim, S., Kodama, T., Kohno, K., Montaña, A., Nakanishi, K., Plionis, M., Sánchez-Argüelles, D., Stevens, J. A., Tamura, Y., Velazquez, M., Yun, M. S.
We present observations at 1.1 mm towards 16 powerful radio galaxies and a radio-quiet quasar at 0.5
Externí odkaz:
http://arxiv.org/abs/1806.10291
Autor:
Saito, T., Iono, D., Ueda, J., Espada, D., Sliwa, K., Nakanishi, K., Lu, N., Xu, C. K., Michiyama, T., Kaneko, H., Yamashita, T., Ando, M., Yun, M. S., Motohara, K., Kawabe, R.
We present 0".97 $\times$ 0".53 (470 pc $\times$ 250 pc) resolution CO ($J$ = 2-1) observations toward the nearby luminous merging galaxy NGC 6240 with the Atacama Large Millimeter/submillimeter Array. We confirmed a strong CO concentration within th
Externí odkaz:
http://arxiv.org/abs/1712.07660
Autor:
Ao, Y., Matsuda, Y., Henkel, C., Iono, D., Alexander, D. M., Chapman, S. C., Geach, J., Hatsukade, B., Hayes, M., Hine, N. K., Kato, Y., Kawabe, R., Kohno, K., Kubo, M., Lehnert, M., Malkan, M., Menten, K. M., Nagao, T., Norris, R. P., Ouchi, M., Saito, T., Tamura, Y., Taniguchi, Y., Umehata, H., Weiss, A.
We study the heating mechanisms and Ly{\alpha} escape fractions of 35 Ly{\alpha} blobs (LABs) at z = 3.1 in the SSA22 field. Dust continuum sources have been identified in 11 of the 35 LABs, all with star formation rates (SFRs) above 100 Msun/yr. Lik
Externí odkaz:
http://arxiv.org/abs/1704.05101
Autor:
Hayatsu, N. H., Matsuda, Y., Umehata, H., Yoshida, N., Smail, I., Swinbank, A. M., Ivison, R., Kohno, K., Tamura, Y., Kubo, M., Iono, D., Hatsukade, B., Nakanishi, K., Kawabe, R., Nagao, T., Inoue, A. K., Takeuchi, T. T., Lee, M., Ao, Y., Fujimoto, S., Izumi, T., Yamaguchi, Y., Ikarashi, S., Yamada, T.
We report the identification of four millimeter line emitting galaxies with the Atacama Large Milli/submillimeter Array (ALMA) in SSA22 Field (ADF22). We analyze the ALMA 1.1 mm survey data, with an effective survey area of 5 arcmin$^2$, a frequency
Externí odkaz:
http://arxiv.org/abs/1702.07512
Autor:
Kitayama, T., Ueda, S., Takakuwa, S., Tsutsumi, T., Komatsu, E., Akahori, T., Iono, D., Izumi, T., Kawabe, R., Kohno, K., Matsuo, H., Ota, N., Suto, Y., Takizawa, M., Yoshikawa, K.
We present the first image of the thermal Sunyaev-Zel'dovich effect (SZE) obtained by the Atacama Large Millimeter/submillimeter Array (ALMA). Combining 7-m and 12-m arrays in Band 3, we create an SZE map toward a galaxy cluster RXJ1347.5-1145 with 5
Externí odkaz:
http://arxiv.org/abs/1607.08833