Zobrazeno 1 - 10
of 104
pro vyhledávání: '"Bechtol, Keith"'
Autor:
Demirbozan, Umut, Nadathur, Seshadri, Ferrero, Ismael, Fosalba, Pablo, Kovacs, Andras, Miquel, Ramon, Davies, Christopher T., Pandey, Shivam, Adamow, Monika, Bechtol, Keith, Drlica-Wagner, Alex, Gruendl, Robert, Hartley, Will, Pieres, Adriano, Ross, Ashley, Rykoff, Eli, Sheldon, Erin, Yanny, Brian, Abbott, Tim, Aguena, Michel, Allam, Sahar, Alves, Otavio, Bacon, David, Bertin, Emmanuel, Bocquet, Sebastian, Brooks, David, Rosell, Aurelio Carnero, Carretero, Jorge, Cawthon, Ross, da Costa, Luiz, Pereira, Maria Elidaiana da Silva, De Vicente, Juan, Desai, Shantanu, Doel, Peter, Everett, Spencer, Flaugher, Brenna, Friedel, Douglas, Frieman, Josh, Gatti, Marco, Gaztanaga, Enrique, Giannini, Giulia, Gutierrez, Gaston, Hinton, Samuel, Hollowood, Devon L., James, David, Jeffrey, Niall, Kuehn, Kyler, Lahav, Ofer, Lee, Sujeong, Marshall, Jennifer, Mena-Fernández, Juan, Mohr, Joe, Myles, Justin, Ogando, Ricardo, Malagón, Andrés Plazas, Roodman, Aaron, Sanchez, Eusebio, Sevilla, Ignacio, Smith, Mathew, Soares-Santos, Marcelle, Suchyta, Eric, Swanson, Molly, Tarle, Gregory, Weaverdyck, Noah, Weller, Jochen, Wiseman, Philip
$ $Low density cosmic voids gravitationally lens the cosmic microwave background (CMB), leaving a negative imprint on the CMB convergence $\kappa$. This effect provides insight into the distribution of matter within voids, and can also be used to stu
Externí odkaz:
http://arxiv.org/abs/2404.18278
Autor:
Martinez, Michael N., Gordon, Yjan A., Bechtol, Keith, Cartwright, Gillian, Ferguson, Peter S., Gorsuch, Miranda
Radio observations of strongly lensed objects are valuable as cosmological probes. Lensed radio sources have proven difficult to identify in large part due to the limited depth and angular resolution of the previous generation of radio sky surveys, a
Externí odkaz:
http://arxiv.org/abs/2404.09954
Autor:
Gordon, Yjan A., O'Dea, Christopher P., Baum, Stefi A., Bechtol, Keith, Duggal, Chetna, Ferguson, Peter S.
Compact Steep Spectrum (CSS) radio sources are active galactic nuclei that have radio jets propagating only on galactic scales, defined as having projected linear sizes (LS) of up to $20\,$kpc. CSS sources are generally hosted by massive early-type g
Externí odkaz:
http://arxiv.org/abs/2304.10538
Autor:
Simon, Joshua D., Brown, Thomas M., Mutlu-Pakdil, Burçin, Ji, Alexander P., Drlica-Wagner, Alex, Avila, Roberto J., Martínez-Vázquez, Clara E., Li, Ting S., Balbinot, Eduardo, Bechtol, Keith, Frebel, Anna, Geha, Marla, Hansen, Terese T., James, David J., Pace, Andrew B., Aguena, M., Alves, O., Andrade-Oliveira, F., Annis, J., Bacon, D., Bertin, E., Brooks, D., Burke, D. L., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Costanzi, M., da Costa, L. N., De Vicente, J., Desai, S., Doel, P., Everett, S., Ferrero, I., Frieman, J., García-Bellido, J., Gatti, M., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Kuehn, K., Kuropatkin, N., Marshall, J. L., Mena-Fernández, J., Miquel, R., Palmese, A., Paz-Chinchón, F., Pereira, M. E. S., Pieres, A., Malagón, A. A. Plazas, Raveri, M., Rodriguez-Monroy, M., Sanchez, E., Santiago, B., Scarpine, V., Sevilla-Noarbe, I., Smith, M., Suchyta, E., Swanson, M. E. C., Tarle, G., To, C., Vincenzi, M., Weaverdyck, N., Wilkinson, R. D.
The ultra-faint dwarf galaxy Reticulum II (Ret II) exhibits a unique chemical evolution history, with 72 +10/-12% of its stars strongly enhanced in r-process elements. We present deep Hubble Space Telescope photometry of Ret II and analyze its star f
Externí odkaz:
http://arxiv.org/abs/2212.00810
Autor:
Drlica-Wagner, Alex, Prescod-Weinstein, Chanda, Yu, Hai-Bo, Albert, Andrea, Amin, Mustafa, Banerjee, Arka, Baryakhtar, Masha, Bechtol, Keith, Bird, Simeon, Birrer, Simon, Bringmann, Torsten, Caputo, Regina, Chakrabarti, Sukanya, Chen, Thomas Y., Croon, Djuna, Cyr-Racine, Francis-Yan, Dawson, William A., Dvorkin, Cora, Gluscevic, Vera, Gilman, Daniel, Grin, Daniel, Hložek, Renée, Leane, Rebecca K., Li, Ting S., Mao, Yao-Yuan, Meyers, Joel, Mishra-Sharma, Siddharth, Muñoz, Julian B., Munshi, Ferah, Nadler, Ethan O., Parikh, Aditya, Perez, Kerstin, Peter, Annika H. G., Profumo, Stefano, Schutz, Katelin, Sehgal, Neelima, Simon, Joshua D., Sinha, Kuver, Valluri, Monica, Wechsler, Risa H.
Cosmological and astrophysical observations currently provide the only robust, positive evidence for dark matter. Cosmic probes of dark matter, which seek to determine the fundamental properties of dark matter through observations of the cosmos, have
Externí odkaz:
http://arxiv.org/abs/2209.08215
Autor:
Guy, Leanne P., Bechtol, Keith, Carlin, Jeffrey L., Dennihy, Erik, Ferguson, Peter S., Krughoff, K. Simon, Lupton, Robert H., Slater, Colin T., Findeisen, Krzysztof, Kannawadi, Arun, Kelvin, Lee S., Lust, Nate B., MacArthur, Lauren A., Martinez, Michael N., Reed, Sophie L., Taranu, Dan S., Wood-Vasey, W. Michael
The Vera C. Rubin Observatory will advance many areas of astronomy over the next decade with its unique wide-fast-deep multi-color imaging survey, the Legacy Survey of Space and Time (LSST). The LSST will produce approximately 20TB of raw data per ni
Externí odkaz:
http://arxiv.org/abs/2206.15447
Autor:
Dvorkin, Cora, Mishra-Sharma, Siddharth, Nord, Brian, Villar, V. Ashley, Avestruz, Camille, Bechtol, Keith, Ćiprijanović, Aleksandra, Connolly, Andrew J., Garrison, Lehman H., Narayan, Gautham, Villaescusa-Navarro, Francisco
Methods based on machine learning have recently made substantial inroads in many corners of cosmology. Through this process, new computational tools, new perspectives on data collection, model development, analysis, and discovery, as well as new comm
Externí odkaz:
http://arxiv.org/abs/2203.08056
Autor:
Bechtol, Keith, Birrer, Simon, Cyr-Racine, Francis-Yan, Schutz, Katelin, Adhikari, Susmita, Amin, Mustafa, Banerjee, Arka, Bird, Simeon, Blinov, Nikita, Boddy, Kimberly K., Boehm, Celine, Bundy, Kevin, Buschmann, Malte, Chakrabarti, Sukanya, Curtin, David, Dai, Liang, Drlica-Wagner, Alex, Dvorkin, Cora, Erickcek, Adrienne L., Gilman, Daniel, Heeba, Saniya, Kim, Stacy, Iršič, Vid, Leauthaud, Alexie, Lovell, Mark, Lukić, Zarija, Mao, Yao-Yuan, Mau, Sidney, Mitridate, Andrea, Mocz, Philip, Muñoz, Julian B., Nadler, Ethan O., Peter, Annika H. G., Price-Whelan, Adrian, Robertson, Andrew, Sabti, Nashwan, Sehgal, Neelima, Shipp, Nora, Simon, Joshua D., Singh, Rajeev, Van Tilburg, Ken, Wechsler, Risa H., Widmark, Axel, Yu, Hai-Bo
The non-linear process of cosmic structure formation produces gravitationally bound overdensities of dark matter known as halos. The abundances, density profiles, ellipticities, and spins of these halos can be tied to the underlying fundamental parti
Externí odkaz:
http://arxiv.org/abs/2203.07354
Autor:
Mao, Yao-Yuan, Peter, Annika H. G., Adhikari, Susmita, Bechtol, Keith, Bird, Simeon, Birrer, Simon, Blazek, Jonathan, Carlin, Jeffrey L., Chamba, Nushkia, Cohen-Tanugi, Johann, Cyr-Racine, Francis-Yan, Daylan, Tansu, Dhanasingham, Birendra, Drlica-Wagner, Alex, Dvorkin, Cora, Fassnacht, Christopher, Gawiser, Eric, Giannotti, Maurizio, Gluscevic, Vera, Gonzalez-Morales, Alma, Hlozek, Renee, Jee, M. James, Kim, Stacy, Mahmood, Akhtar, Mandelbaum, Rachel, Mishra-Sharma, Siddharth, Moniez, Marc, Nadler, Ethan O., Prescod-Weinstein, Chanda, Tyson, J. Anthony, Wechsler, Risa H., Yu, Hai-Bo, Zaharijas, Gabrijela
Establishing that Vera C. Rubin Observatory is a flagship dark matter experiment is an essential pathway toward understanding the physical nature of dark matter. In the past two decades, wide-field astronomical surveys and terrestrial laboratories ha
Externí odkaz:
http://arxiv.org/abs/2203.07252
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