Zobrazeno 1 - 10
of 139
pro vyhledávání: '"Wilson, Grant W."'
Autor:
Pope, Alexandra, Montaña, Alfredo, Battisti, Andrew, Limousin, Marceau, Marchesini, Danilo, Wilson, Grant W., Alberts, Stacey, Aretxaga, Itziar, Avila-Reese, Vladimir, Bermejo-Climent, José Ramón, Brammer, Gabriel, Bravo-Alfaro, Hector, Calzetti, Daniela, Chary, Ranga-Ram, Cybulski, Ryan, Giavalisco, Mauro, Hughes, David, Kado-Fong, Erin, Keller, Erica, Kirkpatrick, Allison, Labbe, Ivo, Lange-Vagle, Daniel, Lowenthal, James, Murphy, Eric, Oesch, Pascal, Gonzalez, Daniel Rosa, Sánchez-Argüelles, David, Shipley, Heath, Stefanon, Mauro, Vega, Olga, Whitaker, Katherine, Williams, Christina C., Yun, Min, Zavala, Jorge A., Zeballos, Milagros
We directly detect dust emission in an optically detected, multiply imaged galaxy lensed by the Frontier Fields cluster MACSJ0717.5+3745. We detect two images of the same galaxy at 1.1 mm with the AzTEC camera on the Large Millimeter Telescope leavin
Externí odkaz:
http://hdl.handle.net/10150/623817
http://arizona.openrepository.com/arizona/handle/10150/623817
http://arizona.openrepository.com/arizona/handle/10150/623817
Autor:
Tang, Yuping, Wang, Q. Daniel, Wilson, Grant W., Heyer, Mark H., Gutermuth, Robert A., Schloerb, Peter, Yun, Min S., Bally, John, Loinard, Laurent, Silich, Sergiy, Chávez, Miguel, Haggard, Daryl, Montaña, Alfredo, Sánchez-Argüelles, David, Zeballos, Milagros, Zavala, Jorge A., León-Tavares, Jonathan
We present a large-scale survey of the central molecular zone (CMZ) of our Galaxy, as well as a monitoring program of Sgr A*, with the AzTEC/Large Millimeter Telescope (LMT) in the 1.1 mm continuum. Our 1.1 mm map covers the main body of the CMZ over
Externí odkaz:
http://arxiv.org/abs/2008.12351
The Central Molecular Zone (CMZ) of our Galaxy hosts an extreme environment analogous to that found in typical starburst galaxies in the distant universe. In order to understand dust properties in environments like our CMZ, we present results from a
Externí odkaz:
http://arxiv.org/abs/2008.12361
Autor:
Sayers, Jack, Montaña, Alfredo, Mroczkowski, Tony, Wilson, Grant W., Zemcov, Michael, Zitrin, Adi, Cibirka, Nathália, Golwala, Sunil, Hughes, David, Nagai, Daisuke, Reese, Erik D., Sánchez, David, Zuhone, John
We have imaged the Sunyaev-Zel'dovich (SZ) effect signals at 140 and 270 GHz towards ten galaxy clusters with Bolocam and AzTEC/ASTE. We also used Planck data to constrain the signal at large angular scales, Herschel-SPIRE images to subtract the brig
Externí odkaz:
http://arxiv.org/abs/1812.06926
Autor:
Brinkerink, Christiaan D., Müller, Cornelia, Falcke, Heino D., Issaoun, Sara, Akiyama, Kazunori, Bower, Geoffrey C., Krichbaum, Thomas P., Deller, Adam T., Castillo, Edgar, Doeleman, Sheperd S., Fraga-Encinas, Raquel, Goddi, Ciriaco, Hernández-Gómez, Antonio, Hughes, David H., Kramer, Michael, Léon-Tavares, Jonathan, Loinard, Laurent, Montaña, Alfredo, Mościbrodzka, Monika, Ortiz-León, Gisela N., Sanchez-Arguelles, David, Tilanus, Remo P. J., Wilson, Grant W., Zensus, J. Anton
Publikováno v:
A&A 621, A119 (2019)
The compact radio source Sagittarius~A$^*$ (Sgr~A$^*$)in the Galactic Center is the primary supermassive black hole candidate. General relativistic magnetohydrodynamical (GRMHD) simulations of the accretion flow around Sgr\,A$^*$ predict the presence
Externí odkaz:
http://arxiv.org/abs/1811.08394
Autor:
Takekoshi, Tatsuya, Minamidani, Tetsuhiro, Komugi, Shinya, Kohno, Kotaro, Tosaki, Tomoka, Sorai, Kazuo, Muller, Erik, Mizuno, Norikazu, Kawamura, Akiko, Onishi, Toshikazu, Fukui, Yasuo, Bot, Caroline, Rubio, Monica, Ezawa, Hajime, Oshima, Tai, Austermann, Jason E., Matsuo, Hiroshi, Aretxaga, Itziar, Hughes, David H., Kawabe, Ryohei, Wilson, Grant W., Yun, Min S.
We present a high-sensitivity ($1\sigma<1.6~\mathrm{mJy~beam^{-1}}$) continuum observation in a 343 arcmin$^2$ area of the northeast region in the Small Magellanic Cloud at a wavelength of 1.1 mm, conducted using the AzTEC instrument on the ASTE tele
Externí odkaz:
http://arxiv.org/abs/1809.09306
Autor:
Tadaki, Ken-ichi, Iono, Daisuke, Yun, Min S., Aretxaga, Itziar, Hatsukade, Bunyo, Hughes, David H., Ikarashi, So, Izumi, Takuma, Kawabe, Ryohei, Kohno, Kotaro, Lee, Minju, Matsuda, Yuichi, Nakanishi, Kohichiro, Saito, Toshiki, Tamura, Yoichi, Ueda, Junko, Umehata, Hideki, Wilson, Grant W., Michiyama, Tomonari, Ando, Misaki, Kamieneski, Patrick
Publikováno v:
Nature, 2018, Volume 560, Issue 7720
Submillimeter bright galaxies in the early Universe are vigorously forming stars at ~1000 times higher rate than the Milky Way. A large fraction of stars is formed in the central 1 kiloparsec region, that is comparable in size to massive, quiescent g
Externí odkaz:
http://arxiv.org/abs/1808.09592
Autor:
Hatsukade, Bunyo, Kohno, Kotaro, Yamaguchi, Yuki, Umehata, Hideki, Ao, Yiping, Aretxaga, Itziar, Caputi, Karina I., Dunlop, James S., Egami, Eicihi, Espada, Daniel, Fujimoto, Seiji, Hayatsu, Natsuki, Hughes, David H., Ikarashi, Soh, Iono, Daisuke, Ivison, Rob J., Kawabe, Ryohei, Kodama, Tadayuki, Lee, Minju, Matsuda, Yuichi, Nakanishi, Kouihiro, Ohta, Kouji, Ouchi, Masami, Rujopakarn, Wiphu, Suzuki, Tomoko, Tamura, Yocihi, Ueda, Yoshihiro, Wang, Tao, Wang, Wei-hao, Wilson, Grant W., Yoshimura, Yuki, Yun, Min S.
We present the survey design, data reduction, construction of images, and source catalog of the Atacama Large Millimeter/submillimeter Array (ALMA) twenty-six arcmin^2 survey of GOODS-S at one-millimeter (ASAGAO). ASAGAO is a deep (1sigma ~ 61 uJy/be
Externí odkaz:
http://arxiv.org/abs/1808.04502
Autor:
Jin, Shuowen, Daddi, Emanuele, Liu, Daizhong, Smolcic, Vernesa, Schinnerer, Eva, Calabrò, Antonello, Gu, Qiusheng, Delhaize, J., Delvecchio, Ivan, Gao, Yu, Salvato, Mara, Puglisi, Annagrazia, Dickinson, Mark, Bertoldi, Frank, Sargent, Mark, Novak, M., Magdis, G. E., Aretxaga, Itziar, Wilson, Grant W., Capak, Peter
We present a "super-deblended" far-infrared to (sub)millimeter photometric catalog in the Cosmic Evolution Survey (COSMOS), prepared with the method recently developed by Liu et al. 2018, with key adaptations. We obtain point spread function (PSF) fi
Externí odkaz:
http://arxiv.org/abs/1807.04697
Autor:
Rodríguez-Montoya, Iván, Sánchez-Argüelles, David, Aretxaga, Itziar, Bertone, Emanuele, Chávez-Dagostino, Miguel, Hughes, David H., Montaña, Alfredo, Wilson, Grant W., Zeballos, Milagros
We present an implementation of a blind source separation algorithm to remove foregrounds off millimeter surveys made by single-channel instruments. In order to make possible such a decomposition over single-wavelength data: we generate levels of art
Externí odkaz:
http://arxiv.org/abs/1711.08456