Zobrazeno 1 - 10
of 66
pro vyhledávání: '"Albrecht, Marcus"'
Autor:
Brisbin, Drew, Miettinen, Oskari, Aravena, Manuel, Smolčić, Vernesa, Delvecchio, Ivan, Jiang, Chunyan, Magnelli, Benjamin, Albrecht, Marcus, Arancibia, Alejandra Muñoz, Aussel, Hervé, Baran, Nikola, Bertoldi, Frank, Béthermin, Matthieu, Capak, Peter, Casey, Caitlin M., Civano, Francesca, Hayward, Christopher C., Ilbert, Olivier, Karim, Alexander, Fevre, Olivier Le, Marchesi, Stefano, McCracken, Henry Joy, Navarrete, Felipe, Novak, Mladen, Riechers, Dominik, Padilla, Nelson, Salvato, Mara, Scott, Kimberly, Schinnerer, Eva, Sheth, Kartik, Tasca, Lidia
Publikováno v:
A&A 608, A15 (2017)
We carried out targeted ALMA observations of 129 fields in the COSMOS region at 1.25 mm, detecting 152 galaxies at S/N$\geq$5 with an average continuum RMS of 150 $\mu$Jy. These fields represent a S/N-limited sample of AzTEC / ASTE sources with 1.1 m
Externí odkaz:
http://arxiv.org/abs/1708.05748
Autor:
Miettinen, Oskari, Delvecchio, Ivan, Smolčić, Vernesa, Aravena, Manuel, Brisbin, Drew, Karim, Alexander, Magnelli, Benjamin, Novak, Mladen, Schinnerer, Eva, Albrecht, Marcus, Aussel, Hervé, Bertoldi, Frank, Capak, Peter L., Casey, Caitlin M., Hayward, Christopher C., Ilbert, Olivier, Intema, Huib T., Jiang, Chunyan, Fèvre, Olivier Le, McCracken, Henry J., Arancibia, Alejandra M. Muñoz, Navarrete, Felipe, Padilla, Nelson D., Riechers, Dominik A., Salvato, Mara, Scott, Kimberly S., Sheth, Kartik, Tasca, Lidia A. M.
Publikováno v:
A&A 606, A17 (2017)
We determine the physical properties of a sample of SMGs in the COSMOS field that were pre-selected at the observed wavelength of $\lambda_{\rm obs}=1.1$ mm, and followed up at $\lambda_{\rm obs}=1.3$ mm with ALMA. We used MAGPHYS to fit the panchrom
Externí odkaz:
http://arxiv.org/abs/1707.00637
Autor:
Miettinen, Oskari, Novak, Mladen, Smolčić, Vernesa, Delvecchio, Ivan, Aravena, Manuel, Brisbin, Drew, Karim, Alexander, Murphy, Eric J., Schinnerer, Eva, Albrecht, Marcus, Aussel, Hervé, Bertoldi, Frank, Capak, Peter L., Casey, Caitlin M., Civano, Francesca, Hayward, Christopher C., Ruiz, Noelia Herrera, Ilbert, Olivier, Jiang, Chunyan, Laigle, Clotilde, Fèvre, Olivier Le, Magnelli, Benjamin, Marchesi, Stefano, McCracken, Henry J., Middelberg, Enno, Arancibia, Alejandra M. Muñoz, Navarrete, Felipe, Padilla, Nelson D., Riechers, Dominik A., Salvato, Mara, Scott, Kimberly S., Sheth, Kartik, Tasca, Lidia A. M., Bondi, Marco, Zamorani, Gianni
We determine the radio size distribution of a large sample of 152 SMGs in COSMOS that were detected with ALMA at 1.3 mm. For this purpose, we used the observations taken by the VLA-COSMOS 3 GHz Large Project. One hundred and fifteen of the 152 target
Externí odkaz:
http://arxiv.org/abs/1702.07527
Autor:
Béthermin, Matthieu, Daddi, Emanuele, Magdis, Georgios, Lagos, Claudia, Sargent, Mark, Albrecht, Marcus, Aussel, Hervé, Bertoldi, Frank, Buat, Véronique, Galametz, Maud, Heinis, Sébastien, Karim, Alexander, Koekemoer, Anton, Lacey, Cedric, Floc'h, Emeric Le, Navarrete, Felipe, Pannella, Maurilio, Schreiber, Corentin, Symeonidis, Myrto, Viero, Marco
Publikováno v:
A&A 573, A113 (2015)
We aim to measure the average dust and molecular gas content of massive star-forming galaxies ($\rm > 3 \times 10^{10}\,M_\odot$) up to z=4 in the COSMOS field to determine if the intense star formation observed at high redshift is induced by major m
Externí odkaz:
http://arxiv.org/abs/1409.5796
Autor:
Thindlu Rudrappa, Manjunath1 (AUTHOR) manjunath.thindlu.rudrappa@fhr.fraunhofer.de, Albrecht, Marcus1 (AUTHOR), Knott, Peter1 (AUTHOR)
Publikováno v:
IET Radar, Sonar & Navigation (Wiley-Blackwell). Apr2024, Vol. 18 Issue 4, p620-634. 15p.
Autor:
Albrecht, Marcus.
Bochum, University, Diss., 2000.
Externí odkaz:
http://www-brs.ub.ruhr-uni-bochum.de/netahtml/HSS/Diss/AlbrechtMarcus/diss.pdf
http://deposit.ddb.de/cgi-bin/dokserv?idn=963688847
http://deposit.ddb.de/cgi-bin/dokserv?idn=963688847
Autor:
Oh, Semyeong, Woo, Jong-Hak, Bennert, Vardha N., Jungwiert, Bruno, Haas, Martin, Leipski, Christian, Albrecht, Marcus
We investigate the narrow-line region (NLR) of two radio-quiet QSOs, PG1012+008 and PG1307+085, using high signal-to-noise spatially resolved long-slit spectra obtained with FORS1 at the Very Large Telescope. Although the emission is dominated by the
Externí odkaz:
http://arxiv.org/abs/1303.6212
LABOCA observations of giant molecular clouds in the south west region of the Small Magellanic Cloud
Autor:
Bot, Caroline, Rubio, Monica, Boulanger, Francois, Albrecht, Marcus, Leroy, Adam, Bolatto, Alberto D., Bertoldi, Frank, Gordon, Karl, Engelbracht, Chad, Block, Miwa, Misselt, Karl
The amount of molecular gas is a key for understanding the future star formation in a galaxy. Because H2 is difficult to observe directly in dense and cold clouds, tracers like CO are used. However, at low metallicities especially, CO only traces the
Externí odkaz:
http://arxiv.org/abs/1009.0124
Autor:
Kishimoto, Makoto, Antonucci, Robert, Blaes, Omer, Lawrence, Andy, Boisson, Catherine, Albrecht, Marcus, Leipski, Christian
Publikováno v:
J.Phys.Conf.Ser.131:012039,2008
A crucial difficulty in understanding the nature of the putative accretion disk in AGNs is that some of its key intrinsic spectral signatures cannot be observed directly. The strong emissions from the broad-line region (BLR) and the obscuring torus,
Externí odkaz:
http://arxiv.org/abs/0810.1373