Zobrazeno 1 - 10
of 165
pro vyhledávání: '"Gorski, Krzysztof"'
The cosmic microwave background (CMB) is a significant source of knowledge about the origin and evolution of our universe. However, observations of the CMB are contaminated by foreground emissions, obscuring the CMB signal and reducing its efficacy i
Externí odkaz:
http://arxiv.org/abs/2302.12378
Autor:
Aurlien, Ragnhild, Remazeilles, Mathieu, Belkner, Sebastian, Carron, Julien, Delabrouille, Jacques, Eriksen, Hans Kristian, Flauger, Raphael, Fuskeland, Unni, Galloway, Mathew, Gorski, Krzysztof M., Hanany, Shaul, Hensley, Brandon S., Hill, J. Colin, Lawrence, Charles R., van Engelen, Alexander, Wehus, Ingunn Kathrine
Publikováno v:
JCAP06(2023)034
PICO is a concept for a NASA probe-scale mission aiming to detect or constrain the tensor to scalar ratio $r$, a parameter that quantifies the amplitude of inflationary gravity waves. We carry out map-based component separation on simulations with fi
Externí odkaz:
http://arxiv.org/abs/2211.14342
Akademický článek
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Autor:
Green, Daniel, Amin, Mustafa A., Meyers, Joel, Wallisch, Benjamin, Abazajian, Kevork N., Abidi, Muntazir, Adshead, Peter, Ahmed, Zeeshan, Ansarinejad, Behzad, Armstrong, Robert, Baccigalupi, Carlo, Bandura, Kevin, Barron, Darcy, Battaglia, Nicholas, Baumann, Daniel, Bechtol, Keith, Bennett, Charles, Benson, Bradford, Beutler, Florian, Bischoff, Colin, Bleem, Lindsey, Bond, J. Richard, Borrill, Julian, Buckley-Geer, Elizabeth, Burgess, Cliff, Carlstrom, John E., Castorina, Emanuele, Challinor, Anthony, Chen, Xingang, Cooray, Asantha, Coulton, William, Craig, Nathaniel, Crawford, Thomas, Cyr-Racine, Francis-Yan, D'Amico, Guido, Demarteau, Marcel, Doré, Olivier, Yutong, Duan, Dunkley, Joanna, Dvorkin, Cora, Ellison, John, van Engelen, Alexander, Escoffier, Stephanie, Essinger-Hileman, Tom, Fabbian, Giulio, Filippini, Jeffrey, Flauger, Raphael, Foreman, Simon, Fuller, George, Garcia, Marcos A. G., García-Bellido, Juan, Gerbino, Martina, Gluscevic, Vera, Gontcho, Satya Gontcho A, Górski, Krzysztof M., Grin, Daniel, Grohs, Evan, Gudmundsson, Jon E., Hanany, Shaul, Handley, Will, Hill, J. Colin, Hirata, Christopher M., Hložek, Renée, Holder, Gilbert, Horiuchi, Shunsaku, Huterer, Dragan, Kadota, Kenji, Kamionkowski, Marc, Keeley, Ryan E., Khatri, Rishi, Kisner, Theodore, Kneib, Jean-Paul, Knox, Lloyd, Koushiappas, Savvas M., Kovetz, Ely D., L'Huillier, Benjamin, Lahav, Ofer, Lattanzi, Massimiliano, Lee, Hayden, Liguori, Michele, Lin, Tongyan, Loverde, Marilena, Madhavacheril, Mathew, Masui, Kiyoshi, McMahon, Jeff, McQuinn, Matthew, Meerburg, P. Daniel, Mirbabayi, Mehrdad, Motloch, Pavel, Mukherjee, Suvodip, Munõz, Julian B., Nagy, Johanna, Newburgh, Laura, Niemack, Michael D., Nomerotski, Andrei, Page, Lyman, Piacentni, Francesco, Pierpaoli, Elena, Pogosian, Levon, Pryke, Clement, Puglisi, Giuseppe, Stompor, Radek, Raveri, Marco, Reichardt, Christian L., Rose, Benjamin, Rossi, Graziano, Ruhl, John, Schaan, Emmanuel, Schubnell, Michael, Schutz, Katelin, Sehgal, Neelima, Senatore, Leonardo, Seo, Hee-Jong, Sherwin, Blake D., Simon, Sara, Slosar, Anže, Staggs, Suzanne, Stebbins, Albert, Suzuki, Aritoki, Switzer, Eric R., Timbie, Peter, Tristram, Matthieu, Trodden, Mark, Tsai, Yu-Dai, Umiltà, Caterina, Di Valentino, Eleonora, Vargas-Magaña, M., Vieregg, Abigail, Watson, Scott, Weiler, Thomas, Whitehorn, Nathan, Wu, W. L. K., Xu, Weishuang, Xu, Zhilei, Yasini, Siavash, Zaldarriaga, Matias, Zhao, Gong-Bo, Zhu, Ningfeng, Zuntz, Joe
The hot dense environment of the early universe is known to have produced large numbers of baryons, photons, and neutrinos. These extreme conditions may have also produced other long-lived species, including new light particles (such as axions or ste
Externí odkaz:
http://arxiv.org/abs/1903.04763
Autor:
Meerburg, P. Daniel, Green, Daniel, Abidi, Muntazir, Amin, Mustafa A., Adshead, Peter, Ahmed, Zeeshan, Alonso, David, Ansarinejad, Behzad, Armstrong, Robert, Avila, Santiago, Baccigalupi, Carlo, Baldauf, Tobias, Ballardini, Mario, Bandura, Kevin, Bartolo, Nicola, Battaglia, Nicholas, Baumann, Daniel, Bavdhankar, Chetan, Bernal, José Luis, Beutler, Florian, Biagetti, Matteo, Bischoff, Colin, Blazek, Jonathan, Bond, J. Richard, Borrill, Julian, Bouchet, François R., Bull, Philip, Burgess, Cliff, Byrnes, Christian, Calabrese, Erminia, Carlstrom, John E., Castorina, Emanuele, Challinor, Anthony, Chang, Tzu-Ching, Chaves-Montero, Jonas, Chen, Xingang, Yeche, Christophe, Cooray, Asantha, Coulton, William, Crawford, Thomas, Chisari, Elisa, Cyr-Racine, Francis-Yan, D'Amico, Guido, de Bernardis, Paolo, de la Macorra, Axel, Doré, Olivier, Duivenvoorden, Adri, Dunkley, Joanna, Dvorkin, Cora, Eggemeier, Alexander, Escoffier, Stephanie, Essinger-Hileman, Tom, Fasiello, Matteo, Ferraro, Simone, Flauger, Raphael, Font-Ribera, Andreu, Foreman, Simon, Friedrich, Oliver, Garcia-Bellido, Juan, Gerbino, Martina, Gluscevic, Vera, Goon, Garrett, Gorski, Krzysztof M., Gudmundsson, Jon E., Gupta, Nikhel, Hanany, Shaul, Handley, Will, Hawken, Adam J., Hill, J. Colin, Hirata, Christopher M., Hložek, Renée, Holder, Gilbert, Huterer, Dragan, Kamionkowski, Marc, Karkare, Kirit S., Keeley, Ryan E., Kinney, William, Kisner, Theodore, Kneib, Jean-Paul, Knox, Lloyd, Koushiappas, Savvas M., Kovetz, Ely D., Koyama, Kazuya, L'Huillier, Benjamin, Lahav, Ofer, Lattanzi, Massimiliano, Lee, Hayden, Liguori, Michele, Loverde, Marilena, Madhavacheril, Mathew, Maldacena, Juan, Marsh, M. C. David, Masui, Kiyoshi, Matarrese, Sabino, McAllister, Liam, McMahon, Jeff, McQuinn, Matthew, Meyers, Joel, Mirbabayi, Mehrdad, Dizgah, Azadeh Moradinezhad, Motloch, Pavel, Mukherjee, Suvodip, Muñoz, Julian B., Myers, Adam D., Nagy, Johanna, Naselsky, Pavel, Nati, Federico, Newburgh, Nicolis, Alberto, Niemack, Michael D., Niz, Gustavo, Nomerotski, Andrei, Page, Lyman, Pajer, Enrico, Padmanabhan, Hamsa, Palma, Gonzalo A., Peiris, Hiranya V., Percival, Will J., Piacentni, Francesco, Pimentel, Guilherme L., Pogosian, Levon, Prescod-Weinstein, Chanda, Pryke, Clement, Puglisi, Giuseppe, Racine, Benjamin, Stompor, Radek, Raveri, Marco, Remazeilles, Mathieu, Rocha, Gracca, Ross, Ashley J., Rossi, Graziano, Ruhl, John, Sasaki, Misao, Schaan, Emmanuel, Schillaci, Alessandro, Schmittfull, Marcel, Sehgal, Neelima, Senatore, Leonardo, Seo, Hee-Jong, Shan, Huanyuan, Shandera, Sarah, Sherwin, Blake D., Silverstein, Eva, Simon, Sara, Slosar, Anže, Staggs, Suzanne, Starkman, Glenn, Stebbins, Albert, Suzuki, Aritoki, Switzer, Eric R., Timbie, Peter, Tolley, Andrew J., Tomasi, Maurizio, Tristram, Matthieu, Trodden, Mark, Tsai, Yu-Dai, Uhlemann, Cora, Umilta, Caterina, van Engelen, Alexander, Vargas-Magaña, M., Vieregg, Abigail, Wallisch, Benjamin, Wands, David, Wandelt, Benjamin, Wang, Yi, Watson, Scott, Wise, Mark, Wu, W. L. K., Xianyu, Zhong-Zhi, Xu, Weishuang, Yasini, Siavash, Young, Sam, Yutong, Duan, Zaldarriaga, Matias, Zemcov, Michael, Zhao, Gong-Bo, Zheng, Yi, Zhu, Ningfeng
Our current understanding of the Universe is established through the pristine measurements of structure in the cosmic microwave background (CMB) and the distribution and shapes of galaxies tracing the large scale structure (LSS) of the Universe. One
Externí odkaz:
http://arxiv.org/abs/1903.04409
Autor:
Hanany, Shaul, Alvarez, Marcelo, Artis, Emmanuel, Ashton, Peter, Aumont, Jonathan, Aurlien, Ragnhild, Banerji, Ranajoy, Barreiro, R. Belen, Bartlett, James G., Basak, Soumen, Battaglia, Nick, Bock, Jamie, Boddy, Kimberly K., Bonato, Matteo, Borrill, Julian, Bouchet, François, Boulanger, François, Burkhart, Blakesley, Chluba, Jens, Chuss, David, Clark, Susan E., Cooperrider, Joelle, Crill, Brendan P., De Zotti, Gianfranco, Delabrouille, Jacques, Di Valentino, Eleonora, Didier, Joy, Doré, Olivier, Eriksen, Hans K., Errard, Josquin, Essinger-Hileman, Tom, Feeney, Stephen, Filippini, Jeffrey, Fissel, Laura, Flauger, Raphael, Fuskeland, Unni, Gluscevic, Vera, Gorski, Krzysztof M., Green, Dan, Hensley, Brandon, Herranz, Diego, Hill, J. Colin, Hivon, Eric, Hložek, Renée, Hubmayr, Johannes, Johnson, Bradley R., Jones, William, Jones, Terry, Knox, Lloyd, Kogut, Al, López-Caniego, Marcos, Lawrence, Charles, Lazarian, Alex, Li, Zack, Madhavacheril, Mathew, Melin, Jean-Baptiste, Meyers, Joel, Murray, Calum, Negrello, Mattia, Novak, Giles, O'Brient, Roger, Paine, Christopher, Pearson, Tim, Pogosian, Levon, Pryke, Clem, Puglisi, Giuseppe, Remazeilles, Mathieu, Rocha, Graca, Schmittfull, Marcel, Scott, Douglas, Shirron, Peter, Stephens, Ian, Sutin, Brian, Tomasi, Maurizio, Trangsrud, Amy, van Engelen, Alexander, Vansyngel, Flavien, Wehus, Ingunn K., Wen, Qi, Xu, Siyao, Young, Karl, Zonca, Andrea
The Probe of Inflation and Cosmic Origins (PICO) is an imaging polarimeter that will scan the sky for 5 years in 21 frequency bands spread between 21 and 799 GHz. It will produce full-sky surveys of intensity and polarization with a final combined-ma
Externí odkaz:
http://arxiv.org/abs/1902.10541
Autor:
Sutin, Brian, Alvarez, Marcelo, Battaglia, Nicholas, Bock, Jamie, Bonato, Matteo, Borrill, Julian, Chuss, David T., Cooperrider, Joelle, Crill, Brendan, Delabrouille, Jacques, Devlin, Mark, Essinger-Hileman, Thomas, Fissel, Laura, Flauger, Raphael, Gorski, Krzysztof, Green, Daniel, Hanany, Shaul, Hubmayr, Johannes, Johnson, Bradley, Jones, William C., Knox, Lloyd, Kogut, Alan, Lawrence, Charles, McMahon, Jeff, Matsumura, Tomotake, Negrello, Mattia, O'Brient, Roger, Paine, Christopher, Pryke, Clement, Shirron, Peter, Trangsrud, Amy, Wen, Qi, Young, Karl, de Zotti, Gianfranco
The Probe of Inflation and Cosmic Origins (PICO) is a NASA-funded study of a Probe-class mission concept. The top-level science objectives are to probe the physics of the Big Bang by measuring or constraining the energy scale of inflation, probe fund
Externí odkaz:
http://arxiv.org/abs/1808.01368
Autor:
Bills, Bruce G., Gorski, Krzysztof M.
Publikováno v:
In Planetary and Space Science June 2022 215
Publikováno v:
In Icarus April 2020 340
Akademický článek
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