Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Bertoldi, Frank"'
Autor:
Decarli, Roberto, Walter, Fabian, Venemans, Bram P., Bañados, Eduardo, Bertoldi, Frank, Carilli, Chris, Fan, Xiaohui, Farina, Emanuele Paolo, Mazzucchelli, Chiara, Riechers, Dominik, Rix, Hans-Walter, Strauss, Michael A., Wang, Ran, Yang, Yujin
We present a survey of the [C II] 158 mu m line and underlying far-infrared (FIR) dust continuum emission in a sample of 27 greater than or similar to 6 quasars using the Atacama Large Millimeter Array (ALMA) at similar to 1 '' resolution. The [C II]
Externí odkaz:
http://hdl.handle.net/10150/627095
http://arizona.openrepository.com/arizona/handle/10150/627095
http://arizona.openrepository.com/arizona/handle/10150/627095
Autor:
Bădescu, Toma, Yang, Yujin, Bertoldi, Frank, Zabludoff, Ann, Karim, Alexander, Magnelli, Benjamin
Bright Ly alpha blobs (LABs)-extended nebulae with sizes of similar to 100 kpc and Ly alpha luminosities of similar to 10(44) erg s(-1)-often reside in overdensities of compact Ly alpha emitters (LAEs) that may be galaxy protoclusters. The number den
Externí odkaz:
http://hdl.handle.net/10150/625775
http://arizona.openrepository.com/arizona/handle/10150/625775
http://arizona.openrepository.com/arizona/handle/10150/625775
Autor:
Shao, Yali, Wang, Ran, Jones, Gareth C., Carilli, Chris L., Walter, Fabian, Fan, Xiaohui, Riechers, Dominik A., Bertoldi, Frank, Wagg, Jeff, Strauss, Michael A., Omont, Alain, Cox, Pierre, Jiang, Linhua, Narayanan, Desika, Menten, Karl M.
We present new Atacama Large Millimeter/submillimeter Array (ALMA) observations of the dust continuum and [C II] 158 mu m fine structure line emission toward a far-infrared-luminous quasar, ULAS J131911.29+095051.4 at z = 6.13, and combine the new Cy
Externí odkaz:
http://hdl.handle.net/10150/625774
http://arizona.openrepository.com/arizona/handle/10150/625774
http://arizona.openrepository.com/arizona/handle/10150/625774
Autor:
Walter, Fabian, Decarli, Roberto, Aravena, Manuel, Carilli, Chris, Bouwens, Rychard, Cunha, Elisabete da, Daddi, Emanuele, Ivison, R. J., Riechers, Dominik, Smail, Ian, Swinbank, Mark, Weiss, Axel, Anguita, Timo, Assef, Roberto, Bacon, Roland, Bauer, Franz, Bell, Eric F., Bertoldi, Frank, Chapman, Scott, Colina, Luis, Cortes, Paulo C., Cox, Pierre, Dickinson, Mark, Elbaz, David, Gónzalez-López, Jorge, Ibar, Edo, Inami, Hanae, Infante, Leopoldo, Hodge, Jacqueline, Karim, Alex, Fevre, Olivier Le, Magnelli, Benjamin, Neri, Roberto, Oesch, Pascal, Ota, Kazuaki, Popping, Gergö, Rix, Hans-Walter, Sargent, Mark, Sheth, Kartik, Wel, Arjen van der, Werf, Paul van der, Wagg, Jeff
We present the rationale for and the observational description of ASPECS: the ALMA SPECtroscopic Survey in the Hubble Ultra-Deep Field (UDF), the cosmological deep field that has the deepest multi-wavelength data available. Our overarching goal is to
Externí odkaz:
http://hdl.handle.net/10150/623953
http://arizona.openrepository.com/arizona/handle/10150/623953
http://arizona.openrepository.com/arizona/handle/10150/623953
Autor:
Decarli, Roberto, Walter, Fabian, Aravena, Manuel, Carilli, Chris, Bouwens, Rychard, da Cunha, Elisabete, Daddi, Emanuele, Ivison, R. J., Popping, Gergö, Riechers, Dominik, Smail, Ian R., Swinbank, Mark, Weiss, Axel, Anguita, Timo, Assef, Roberto J., Bauer, Franz E., Bell, Eric F., Bertoldi, Frank, Chapman, Scott, Colina, Luis, Cortes, Paulo C., Cox, Pierre, Dickinson, Mark, Elbaz, David, Gónzalez-López, Jorge, Ibar, Edo, Infante, Leopoldo, Hodge, Jacqueline, Karim, Alex, Fevre, Olivier Le, Magnelli, Benjamin, Neri, Roberto, Oesch, Pascal, Ota, Kazuaki, Rix, Hans-Walter, Sargent, Mark, Sheth, Kartik, van der Wel, Arjen, van der Werf, Paul, Wagg, Jeff
In this paper we use ASPECS, the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field in band. 3 and band. 6, to place blind constraints on the CO luminosity function and the evolution of the cosmic molecular gas density as a function of redshift
Externí odkaz:
http://hdl.handle.net/10150/623950
http://arizona.openrepository.com/arizona/handle/10150/623950
http://arizona.openrepository.com/arizona/handle/10150/623950
Autor:
Wang, Ran, Wu, Xue-Bing, Neri, Roberto, Fan, Xiaohui, Walter, Fabian, Carilli, Chris L., Momjian, Emmanuel, Bertoldi, Frank, Strauss, Michael A., Li, Qiong, Wang, Feige, Riechers, Dominik A., Jiang, Linhua, Omont, Alain, Wagg, Jeff, Cox, Pierre
We report new IRAM/PdBI, JCMT/SCUBA-2, and VLA observations of the ultraluminous quasar SDSS J010013.02+280225.8 (hereafter, J0100+2802) at z =. 6.3, which hosts the most massive supermassive black hole (SMBH), 1.24 x 10(10) M circle dot, that is kno
Externí odkaz:
http://hdl.handle.net/10150/624073
http://arizona.openrepository.com/arizona/handle/10150/624073
http://arizona.openrepository.com/arizona/handle/10150/624073