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pro vyhledávání: '"Aravena, Manuel"'
Akademický článek
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Autor:
Fasano Alessandro, Ade Peter, Aravena Manuel, Barria Emilio, Beelen Alexandre, Benoît Alain, Béthermin Matthieu, Bounmy Julien, Bourrion Olivier, Bres Guillaume, Calvo Martino, Catalano Andrea, De Breuck Carlos, Désert François-Xavier, Durán Carlos, Fenouillet Thomas, Garcia Jose, Garde Gregory, Goupy Johannes, Groppi Christopher, Hoarau Christophe, Hu Wenkai, Lagache Guilaine, Lambert Jean-Charles, Leggeri Jean-Paul, Levy-Bertrand Florence, Lundgren Andreas, Macías-Pérez Juan, Mani Hamdi, Marpaud Julien, Mauskopf Philip, Monfardini Alessandro, Pisano Giampaolo, Ponthieu Nicolas, Prieur Leo, Roni Samuel, Roudier Sebastien, Tourres Damien, Tucker Carol
Publikováno v:
EPJ Web of Conferences, Vol 293, p 00018 (2024)
CONCERTO (CarbON CII line in post-rEionization and ReionizaTiOn) is a low-resolution Fourier transform spectrometer dedicated to the study of star-forming galaxies and clusters of galaxies in the transparent millimeter windows from the ground. It is
Externí odkaz:
https://doaj.org/article/bbce0c35e8284994b95372ef89cf7ae2
Autor:
Brisbin, Drew, Aravena, Manuel, Daddi, Emanuele, Dannerbauer, Helmut, Decarli, Roberto, González-López, Jorge, Riechers, Dominik, Wagg, Jeff
Publikováno v:
A&A 628, A104 (2019)
We used the Plateau De Bure Interferometer to observe multiple CO and neutral carbon transitions in a z=2.2 main sequence disk galaxy, BX610. Our observation of CO(7-6), CO(4-3), and both far-infrared(FIR) [CI] lines complements previous observations
Externí odkaz:
http://arxiv.org/abs/1907.04936
Autor:
Jarugula, Sreevani, Vieira, Joaquin D., Spilker, Justin S., Apostolovski, Yordanka, Aravena, Manuel, Bethermin, Matthieu, de Breuck, Carlos, Chen, Chian-Chou, Cunningham, Daniel J. M., Dong, Chenxing, Greve, Thomas, Hayward, Christopher C., Hezaveh, Yashar, Litke, Katrina C., Mangian, Amelia C, Narayanan, Desika, Phadke, Kedar, Reuter, Cassie A., Van der Werf, Paul, ß, Axel Wei
Water ($\rm H_{2}O$), one of the most ubiquitous molecules in the universe, has bright millimeter-wave emission lines easily observed at high-redshift with the current generation of instruments. The low excitation transition of $\rm H_{2}O$, p$-$$\rm
Externí odkaz:
http://arxiv.org/abs/1906.05469
Autor:
Apostolovski, Yordanka, Aravena, Manuel, Anguita, Timo, Spilker, Justin, Weiss, Axel, Bethermin, Matthieu, Chapman, Scott C., Chen, Chian-Chou, Cunningham, Daniel, De Breuck, Carlos, Dong, Chenxing, Hayward, Christopher C., Hezaveh, Yashar, Jarugula, Sreevani, Litke, Katrina, Ma, Jingzhe, Marrone, Daniel P., Narayanan, Desika, Rotermund, Kaja, Vieira, Joaquin
Publikováno v:
A&A 628, A23 (2019)
Aims: We present and study spatially resolved imaging obtained with the Atacama Large Millimeter/submillimeter Array (ALMA) of multiple $^{12}$CO($J=$6$-$5, 8$-$7 and 9$-$8) and two H$_2$O(2$_{02}-$1$_{11}$ and 2$_{11}-$2$_{02}$) emission lines and c
Externí odkaz:
http://arxiv.org/abs/1905.12738
Autor:
Decarli, Roberto, Walter, Fabian, Gónzalez-López, Jorge, Aravena, Manuel, Boogaard, Leindert, Carilli, Chris, Cox, Pierre, Daddi, Emanuele, Popping, Gergö, Riechers, Dominik, Uzgil, Bade, Weiss, Axel, Assef, Roberto J., Bacon, Roland, Bauer, Franz Erik, Bertoldi, Frank, Bouwens, Rychard, Contini, Thierry, Cortes, Paulo C., da Cunha, Elisabete, Díaz-Santos, Tanio, Elbaz, David, Inami, Hanae, Hodge, Jacqueline, Ivison, Rob, Fèvre, Olivier Le, Magnelli, Benjamin, Novak, Mladen, Oesch, Pascal, Rix, Hans-Walter, Sargent, Mark T., Smail, Ian R., Swinbank, A. Mark, Somerville, Rachel S., van der Werf, Paul, Wagg, Jeff, Wisotzki, Lutz
We use the results from the ALMA large program ASPECS, the spectroscopic survey in the Hubble Ultra Deep Field (HUDF), to constrain CO luminosity functions of galaxies and the resulting redshift evolution of $\rho$(H$_2$). The broad frequency range c
Externí odkaz:
http://arxiv.org/abs/1903.09164
Autor:
Aravena, Manuel, Decarli, Roberto, Gónzalez-López, Jorge, Boogaard, Leindert, Walter, Fabian, Carilli, Chris, Popping, Gergö, Weiss, Axel, Assef, Roberto J., Bacon, Roland, Bauer, Franz Erik, Bertoldi, Frank, Bouwens, Richard, Contini, Thierry, Cortes, Paulo C., Cox, Pierre, da Cunha, Elisabete, Daddi, Emanuele, Díaz-Santos, Tanio, Elbaz, David, Hodge, Jacqueline, Inami, Hanae, Ivison, Rob, Fèvre, Olivier Le, Magnelli, Benjamin, Oesch, Pascal, Riechers, Dominik, Smail, Ian, Somerville, Rachel S., Swinbank, A. M., Uzgil, Bade, van der Werf, Paul, Wagg, Jeff, Wisotzki, Lutz
We analyze the interstellar medium properties of a sample of sixteen bright CO line emitting galaxies identified in the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS) Large Program. This CO$-$selected galaxy sample is complemented
Externí odkaz:
http://arxiv.org/abs/1903.09162
Autor:
Popping, Gergö, Pillepich, Annalisa, Somerville, Rachel S., Decarli, Roberto, Walter, Fabian, Aravena, Manuel, Carilli, Chris, Cox, Pierre, Nelson, Dylan, Riechers, Dominik, Weiss, Axel, Boogaard, Leindert, Bouwens, Richard, Contini, Thierry, Cortes, Paulo C., da Cunha, Elisabete, Daddi, Emanuele, Díaz-Santos, Tanio, Diemer, Benedikt, González-López, Jorge, Hernquist, Lars, Ivison, Rob, Fevre, Olivier Le, Marinacci, Federico, Rix, Hans-Walter, Swinbank, Mark, Vogelsberger, Mark, van der Werf, Paul, Wagg, Jeff, Yung, L. Y. Aaron
The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS) provides new constraints for galaxy formation models on the molecular gas properties of galaxies. We compare results from ASPECS to predictions from two cosmological galaxy formati
Externí odkaz:
http://arxiv.org/abs/1903.09158
Autor:
Boogaard, Leindert A., Decarli, Roberto, González-López, Jorge, van der Werf, Paul, Walter, Fabian, Bouwens, Rychard, Aravena, Manuel, Carilli, Chris, Bauer, Franz Erik, Brinchmann, Jarle, Contini, Thierry, Cox, Pierre, da Cunha, Elisabete, Daddi, Emanuele, Díaz-Santos, Tanio, Hodge, Jacqueline, Inami, Hanae, Ivison, Rob, Maseda, Michael, Matthee, Jorryt, Oesch, Pascal, Popping, Gergö, Riechers, Dominik, Schaye, Joop, Schouws, Sander, Smail, Ian, Weiss, Axel, Wisotzki, Lutz, Bacon, Roland, Cortes, Paulo C., Rix, Hans-Walter, Somerville, Rachel S., Swinbank, Mark, Wagg, Jeff
We discuss the nature and physical properties of gas-mass selected galaxies in the ALMA spectroscopic survey (ASPECS) of the Hubble Ultra Deep Field (HUDF). We capitalize on the deep optical integral-field spectroscopy from the MUSE HUDF Survey and m
Externí odkaz:
http://arxiv.org/abs/1903.09167
Autor:
González-López, Jorge, Decarli, Roberto, Pavesi, Ricardo, Walter, Fabian, Aravena, Manuel, Carilli, Chris, Boogaard, Leindert, Popping, Gergö, Weiss, Axel, Assef, Roberto J., Bauer, Franz Erik, Bertoldi, Frank, Bouwens, Richard, Contini, Thierry, Cortes, Paulo C., Cox, Pierre, da Cunha, Elisabete, Daddi, Emanuele, Díaz-Santos, Tanio, Inami, Hanae, Hodge, Jacqueline, Ivison, Rob, Fèvre, Olivier Le, Magnelli, Benjamin, esch, Pascal, Riechers, Dominik, Rix, Hans--Walter, Smail, Ian, Swinbank, A. M., Somerville, Rachel S., Uzgil, Bade, van der Werf, Paul
The ALMA SPECtroscopic Survey in the {\it Hubble} Ultra Deep Field is an ALMA large program that obtained a frequency scan in the 3\,mm band to detect emission lines from the molecular gas in distant galaxies. We here present our search strategy for
Externí odkaz:
http://arxiv.org/abs/1903.09161