Zobrazeno 1 - 10
of 86
pro vyhledávání: '"Aussel, Herve'"'
Autor:
Scoville, Nick, Faisst, Andreas, Weaver, John, Toft, Sune, McCracken, Henry, Ilbert, Olivier, Diaz-Santos, Tanio, Staguhn, Johannes, Koda, Jin, Casey, Caitlin, Sanders, David, Mobasher, Bahram, Chartab, Nima, Sattari, Zahra, Capak, Peter, Bout, Paul Vanden, Bongiorno, Angela, Vlahakis, Catherine, Sheth, Kartik, Yun, Min, Aussel, Herve, Laigle, Clotilde, Masters, Dan
ALMA observations of the long wavelength dust continuum are used to estimate the gas masses in a sample of 708 star-forming (SF) galaxies at z = 0.3 to 4.5. We determine the dependence of gas masses and star formation efficiencies (SFE=SFR per unit g
Externí odkaz:
http://arxiv.org/abs/2211.07836
Autor:
Guy, Leanne P., Cuillandre, Jean-Charles, Bachelet, Etienne, Banerji, Manda, Bauer, Franz E., Collett, Thomas, Conselice, Christopher J., Eggl, Siegfried, Ferguson, Annette, Fontana, Adriano, Heymans, Catherine, Hook, Isobel M., Aubourg, Éric, Aussel, Hervé, Bosch, James, Carry, Benoit, Hoekstra, Henk, Kuijken, Konrad, Lanusse, Francois, Melchior, Peter, Mohr, Joseph, Moresco, Michele, Nakajima, Reiko, Paltani, Stéphane, Troxel, Michael, Allevato, Viola, Amara, Adam, Andreon, Stefano, Anguita, Timo, Bardelli, Sandro, Bechtol, Keith, Birrer, Simon, Bisigello, Laura, Bolzonella, Micol, Botticella, Maria Teresa, Bouy, Hervé, Brinchmann, Jarle, Brough, Sarah, Camera, Stefano, Cantiello, Michele, Cappellaro, Enrico, Carlin, Jeffrey L., Castander, Francisco J, Castellano, Marco, Chari, Ranga Ram, Chisari, Nora Elisa, Collins, Christopher, Courbin, Frédéric, Cuby, Jean-Gabriel, Cucciati, Olga, Daylan, Tansu, Diego, Jose M., Duc, Pierre-Alain, Fotopoulou, Sotiria, Fouchez, Dominique, Gavazzi, Raphaël, Gruen, Daniel, Hatfield, Peter, Hildebrandt, Hendrik, Landt, Hermine, Hunt, Leslie K., Ibata, Rodrigo, Ilbert, Olivier, Jasche, Jens, Joachimi, Benjamin, Joseph, Rémy, Kotak, Rubina, Laigle, Clotilde, Lançon, Ariane, Larsen, Søren S., Lavaux, Guilhem, Leclercq, Florent, Leonard, C. Danielle, von der Linden, Anja, Liu, Xin, Longo, Giuseppe, Magliocchetti, Manuela, Maraston, Claudia, Marshall, Phil, Martín, Eduardo L., Mattila, Seppo, Maturi, Matteo, McCracken, Henry Joy, Metcalf, R. Benton, Montes, Mireia, Mortlock, Daniel, Moscardini, Lauro, Narayan, Gautham, Paolillo, Maurizio, Papaderos, Polychronis, Pello, Roser, Pozzetti, Lucia, Radovich, Mario, Rejkuba, Marina, Román, Javier, Sánchez-Janssen, Rubén, Sarpa, Elena, Sartoris, Barbara, Schrabback, Tim, Sluse, Dominique, Smartt, Stephen J., Smith, Graham P., Snodgrass, Colin, Talia, Margherita, Tao, Charling, Toft, Sune, Tortora, Crescenzo, Tutusaus, Isaac, Usher, Christopher, van Velzen, Sjoert, Verma, Aprajita, Vernardos, Georgios, Voggel, Karina, Wandelt, Benjamin, Watkins, Aaron E., Weller, Jochen, Wright, Angus H, Yoachim, Peter, Yoon, Ilsang, Zucca, Elena
This report is the result of a joint discussion between the Rubin and Euclid scientific communities. The work presented in this report was focused on designing and recommending an initial set of Derived Data products (DDPs) that could realize the sci
Externí odkaz:
http://arxiv.org/abs/2201.03862
Autor:
van der Burg, Remco F. J., McGee, Sean, Aussel, Herve, Dahle, Hakon, Arnaud, Monique, Pratt, Gabriel W., Muzzin, Adam
We study the abundance of star-forming and quiescent galaxies in a sample of 21 massive clusters at 0.5
Externí odkaz:
http://arxiv.org/abs/1807.00820
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:
Adam, Remi, Adane, Amar, Ade, P. A. R., André, Philippe, Andrianasolo, Aina, Aussel, Herve, Beelen, Alexandre, Benoit, Alain, Bideaud, Aurelien, Billot, Nicolas, Bourrion, Olivier, Bracco, Andrea, Calvo, Martino, Catalano, Andrea, Coiffard, Gregoire, Comis, Barbara, De Petris, Marco, Désert, François-Xavier, Doyle, Simon, Driessen, E. F. C., Evans, Ruth, Goupy, Johannes, Kramer, Carsten, Lagache, Guilaine, Leclercq, Samuel, Leggeri, Jean-Paul, Lestrade, Jean-François, Macias-Perez, Juan-Francisco, Mauskopf, Philip, Mayet, Frederic, Maury, Anaelle, Monfardini, Alessandro, Navarro, Santiago, Pascale, Enzo, Perotto, Laurence, Pisano, Giampaolo, Ponthieu, Nicolas, Reveret, Vincent, Rigby, Andrew, Ritacco, Alessia, Romero, Charles, Roussel, Helene, Ruppin, Florian, Schuster, Karl, Sievers, Albrecht, Triqueneaux, Sebastien, Tucker, Carole, Zylka, Robert
Publikováno v:
A&A 609, A115 (2018)
Millimeter-wave continuum astronomy is today an indispensable tool for both general Astrophysics studies and Cosmology. General purpose, large field-of-view instruments are needed to map the sky at intermediate angular scales not accessible by the hi
Externí odkaz:
http://arxiv.org/abs/1707.00908
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:
McConnachie, Alan, Babusiaux, Carine, Balogh, Michael, Driver, Simon, Côté, Pat, Courtois, Helene, Davies, Luke, Ferrarese, Laura, Gallagher, Sarah, Ibata, Rodrigo, Martin, Nicolas, Robotham, Aaron, Venn, Kim, Villaver, Eva, Bovy, Jo, Boselli, Alessandro, Colless, Matthew, Comparat, Johan, Denny, Kelly, Duc, Pierre-Alain, Ellison, Sara, de Grijs, Richard, Fernandez-Lorenzo, Mirian, Freeman, Ken, Guhathakurta, Raja, Hall, Patrick, Hopkins, Andrew, Hudson, Mike, Johnson, Andrew, Kaiser, Nick, Koda, Jun, Konstantopoulos, Iraklis, Koshy, George, Lee, Khee-Gan, Nusser, Adi, Pancoast, Anna, Peng, Eric, Peroux, Celine, Petitjean, Patrick, Pichon, Christophe, Poggianti, Bianca, Schmid, Carlo, Shastri, Prajval, Shen, Yue, Willot, Chris, Croom, Scott, Lallement, Rosine, Schimd, Carlo, Smith, Dan, Walker, Matthew, Willis, Jon, Colless, Alessandro Bosselli Matthew, Goswami, Aruna, Jarvis, Matt, Jullo, Eric, Kneib, Jean-Paul, Konstantopoloulous, Iraklis, Newman, Jeff, Richard, Johan, Sutaria, Firoza, Taylor, Edwar, van Waerbeke, Ludovic, Battaglia, Giuseppina, Hall, Pat, Haywood, Misha, Sakari, Charli, Seibert, Arnaud, Thirupathi, Sivarani, Wang, Yuting, Wang, Yiping, Babas, Ferdinand, Bauman, Steve, Caffau, Elisabetta, Laychak, Mary Beth, Crampton, David, Devost, Daniel, Flagey, Nicolas, Han, Zhanwen, Higgs, Clare, Hill, Vanessa, Ho, Kevin, Isani, Sidik, Mignot, Shan, Murowinski, Rick, Pandey, Gajendra, Salmon, Derrick, Siebert, Arnaud, Simons, Doug, Starkenburg, Else, Szeto, Kei, Tully, Brent, Vermeulen, Tom, Withington, Kanoa, Arimoto, Nobuo, Asplund, Martin, Aussel, Herve, Bannister, Michele, Bhatt, Harish, Bhargavi, SS, Blakeslee, John, Bland-Hawthorn, Joss, Bullock, James, Burgarella, Denis, Chang, Tzu-Ching, Cole, Andrew, Cooke, Jeff, Cooper, Andrew, Di Matteo, Paola, Favole, Ginevra, Flores, Hector, Gaensler, Bryan, Garnavich, Peter, Gilbert, Karoline, Gonzalez-Delgado, Rosa, Guhathakurta, Puragra, Hasinger, Guenther, Herwig, Falk, Hwang, Narae, Jablonka, Pascale, Jarvis, Matthew, Kamath, Umanath, Kewley, Lisa, Borgne, Damien Le, Lewis, Geraint, Lupton, Robert, Martell, Sarah, Mateo, Mario, Mena, Olga, Nataf, David, Newman, Jeffrey, Pérez, Enrique, Prada, Francisco, Puech, Mathieu, Recio-Blanco, Alejandra, Robin, Annie, Saunders, Will, Smith, Daniel, Stalin, C. S., Tao, Charling, Thanjuvur, Karun, Tresse, Laurence, van Waerbeke, Ludo, Wang, Jian-Min, Yong, David, Zhao, Gongbo, Boisse, Patrick, Bolton, James, Bonifacio, Piercarlo, Bouchy, Francois, Cowie, Len, Cunha, Katia, Deleuil, Magali, de Mooij, Ernst, Dufour, Patrick, Foucaud, Sebastien, Glazebrook, Karl, Hutchings, John, Kobayashi, Chiaki, Kudritzki, Rolf-Peter, Li, Yang-Shyang, Lin, Lihwai, Lin, Yen-Ting, Makler, Martin, Narita, Norio, Park, Changbom, Ransom, Ryan, Ravindranath, Swara, Reddy, Bacham Eswar, Sawicki, Marcin, Simard, Luc, Srianand, Raghunathan, Storchi-Bergmann, Thaisa, Umetsu, Keiichi, Wang, Ting-Gui, Woo, Jong-Hak, Wu, Xue-Bing
MSE is an 11.25m aperture observatory with a 1.5 square degree field of view that will be fully dedicated to multi-object spectroscopy. More than 3200 fibres will feed spectrographs operating at low (R ~ 2000 - 3500) and moderate (R ~ 6000) spectral
Externí odkaz:
http://arxiv.org/abs/1606.00043
Autor:
Evans, Chris, Puech, Mathieu, Afonso, Jose, Almaini, Omar, Amram, Philippe, Aussel, Hervé, Barbuy, Beatriz, Basden, Alistair, Bastian, Nate, Battaglia, Giuseppina, Biller, Beth, Bonifacio, Piercarlo, Bouché, Nicholas, Bunker, Andy, Caffau, Elisabetta, Charlot, Stephane, Cirasuolo, Michele, Clenet, Yann, Combes, Francoise, Conselice, Chris, Contini, Thierry, Cuby, Jean-Gabriel, Dalton, Gavin, Davies, Ben, de Koter, Alex, Disseau, Karen, Dunlop, Jim, Epinat, Benoît, Fiore, Fabrizio, Feltzing, Sofia, Ferguson, Annette, Flores, Hector, Fontana, Adriano, Fusco, Thierry, Gadotti, Dimitri, Gallazzi, Anna, Gallego, Jesus, Giallongo, Emanuele, Gonçalves, Thiago, Gratadour, Damien, Guenther, Eike, Hammer, Francois, Hill, Vanessa, Huertas-Company, Marc, Ibata, Roridgo, Kaper, Lex, Korn, Andreas, Larsen, Søren, Fèvre, Olivier Le, Lemasle, Bertrand, Maraston, Claudia, Mei, Simona, Mellier, Yannick, Morris, Simon, Östlin, Göran, Paumard, Thibaut, Pello, Roser, Pentericci, Laura, Peroux, Celine, Petitjean, Patrick, Rodrigues, Myriam, Rodríguez-Muñoz, Lucía, Rouan, Daniel, Sana, Hugues, Schaerer, Daniel, Telles, Eduardo, Trager, Scott, Tresse, Laurence, Welikala, Niraj, Zibetti, Stefano, Ziegler, Bodo
This White Paper presents the scientific motivations for a multi-object spectrograph (MOS) on the European Extremely Large Telescope (E-ELT). The MOS case draws on all fields of contemporary astronomy, from extra-solar planets, to the study of the ha
Externí odkaz:
http://arxiv.org/abs/1501.04726
Autor:
Lee, Nicholas, Sanders, D. B., Casey, Caitlin M., Toft, Sune, Scoville, N. Z., Hung, Chao-Ling, Floc'h, Emeric Le, Ilbert, Olivier, Zahid, H. Jabran, Aussel, Herve, Capak, Peter, Kartaltepe, Jeyhan S., Kewley, Lisa J., Li, Yanxia, Schawinski, Kevin, Sheth, Kartik, Xiao, Quanbao
The relationship between galaxy star formation rates (SFR) and stellar masses ($M_\ast$) is re-examined using a mass-selected sample of $\sim$62,000 star-forming galaxies at $z \le 1.3$ in the COSMOS 2-deg$^2$ field. Using new far-infrared photometry
Externí odkaz:
http://arxiv.org/abs/1501.01080