Kitayama, Tetsu, Komatsu, Eiichiro, Ota, Naomi, Kuwabara, Takeshi, Suto, Yasushi, Yoshikawa, Kohji, Hattori, Makoto, Matsuo, Hiroshi (2004) Exploring Cluster Physics with High-Resolution Sunyaev-Zel’dovich Effect Images and X-Ray Data: The Case of the Most X-Ray-Luminous Galaxy Cluster RX J1347—1145. Publications of the Astronomical Society of Japan, 56 (1). 17-28 doi:10.1093/pasj/56.1.17

See Also

These are possibly similar items as determined by title/reference text matching only.

	Komatsu, Eiichiro, Matsuo, Hiroshi, Kitayama, Tetsu, Hattori, Makoto, Kawabe, Ryohei, Kohno, Kotaro, Kuno, Nario, Schindler, Sabine, Suto, Yasushi, Yoshikawa, Kohji (2001) Substructures Revealed by the Sunyaev–Zel’dovich Effect at 150 GHz in a High-Resolution Map of RX J1347$-$1145. Publications of the Astronomical Society of Japan, 53 (1). 57-62 doi:10.1093/pasj/53.1.57
	Komatsu, Eiichiro, Kitayama, Tetsu, Suto, Yasushi, Hattori, Makoto, Kawabe, Ryohei, Matsuo, Hiroshi, Schindler, Sabine, Yoshikawa, Kohji (1999) Submillimeter Detection of the Sunyaev-Zeldovich Effect toward the Most Luminous X-Ray Cluster at [CLC][ITAL]z[/ITAL][/CLC] = 0.45. The Astrophysical Journal, 516 (1). doi:10.1086/311983
	Kitayama, Tetsu, Ueda, Shutaro, Takakuwa, Shigehisa, Tsutsumi, Takahiro, Komatsu, Eiichiro, Akahori, Takuya, Iono, Daisuke, Izumi, Takuma, Kawabe, Ryohei, Kohno, Kotaro, Matsuo, Hiroshi, Ota, Naomi, Suto, Yasushi, Takizawa, Motozaku, Yoshikawa, Kohji (2016) The Sunyaev–Zel'dovich effect at 5″: RX J1347.5−1145 imaged by ALMA. Publications of the Astronomical Society of Japan, 68 (5). 88pp. doi:10.1093/pasj/psw082
	Kitayama, Tetsu, Ueda, Shutaro, Akahori, Takuya, Komatsu, Eiichiro, Kawabe, Ryohei, Kohno, Kotaro, Takakuwa, Shigehisa, Takizawa, Motokazu, Tsutsumi, Takahiro, Yoshikawa, Kohji (2020) Deeply cooled core of the Phoenix galaxy cluster imaged by ALMA with the Sunyaev–Zel’dovich effect. Publications of the Astronomical Society of Japan, 72 (2) doi:10.1093/pasj/psaa009
	Yamada, Kenkichi, Kitayama, Tetsu, Takakuwa, Shigehisa, Iono, Daisuke, Tsutsumi, Takahiro, Kohno, Kotaro, Takizawa, Motokazu, Yoshikawa, Kohji, Akahori, Takuya, Komatsu, Eiichiro, Suto, Yasushi, Matsuo, Hiroshi, Kawabe, Ryohei (2012) Imaging Simulations of the Sunyaev–Zel'dovich Effect for ALMA. Publications of the Astronomical Society of Japan, 64 (5). 102pp. doi:10.1093/pasj/64.5.102
	Suto, Yasushi, Kitayama, Tetsu, Komatsu, Eiichiro, Hattori, Makoto, Kawabe, Ryohei, Matsuo, Hiroshi, Schindler, Sabine, Yoshikawa, Kohji (2000) Cosmological implications of galaxy clusters in X-ray, millimeter, and submillimeter bands. Advances in Space Research, 25. 771-780 doi:10.1016/s0273-1177(99)00838-8
	Ueda, Shutaro, Kitayama, Tetsu, Oguri, Masamune, Komatsu, Eiichiro, Akahori, Takuya, Iono, Daisuke, Izumi, Takumi, Kawabe, Ryohei, Kohno, Kotaro, Matsuo, Hiroshi, Ota, Naomi, Suto, Yasushi, Takakuwa, Shigehisa, Takizawa, Motokazu, Tsutsumi, Takahiro, Yoshikawa, Kohji (2018) A Cool Core Disturbed: Observational Evidence for the Coexistence of Subsonic Sloshing Gas and Stripped Shock-heated Gas around the Core of RX J1347.5–1145. The Astrophysical Journal, 866 (1). 48pp. doi:10.3847/1538-4357/aadd9d
	Shimizu, Mamoru, Kitayama, Tetsu, Sasaki, Shin, Suto, Yasushi (2004) Monte Carlo Modeling of Non-Gravitational Heating Processes in Galaxy Clusters. Publications of the Astronomical Society of Japan, 56 (1). 1-16 doi:10.1093/pasj/56.1.1
	Tsuboi, Masato, Miyazaki, Atsushi, Kasuga, Takashi, Kuno, Nario, Sakamoto, Akihiro, Matsuo, Hiroshi (2004) Sunyaev-Zel’dovich Effect toward Distant Galaxy Clusters at 43 GHz; Observation and Data. Publications of the Astronomical Society of Japan, 56 (5). 711-721 doi:10.1093/pasj/56.5.711
	Kitayama, Tetsu, Sasaki, Shin, Suto, Yasushi (1998) Cosmological Implications of Number Counts of Clusters of Galaxies: logN–logSin X-Ray and Submm Bands. Publications of the Astronomical Society of Japan, 50 (1). 1-11 doi:10.1093/pasj/50.1.1
	Pointecouteau, E., Giard, M., Benoit, A., Desert, F. X., Bernard, J. P., Coron, N., Lamarre, J. M. (2001) Extended Sunyaev‐Zeldovich Map of the Most Luminous X‐Ray Cluster, RX J1347−1145. The Astrophysical Journal, 552 (1). 42-48 doi:10.1086/320447